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Sensing Out-of-Equilibrium and Quantum Non-Gaussian environments via induced Time-Reversal Symmetry Breaking on the quantum-probe dynamics

Martin Kuffer Centro Atómico Bariloche, CONICET, CNEA, S. C. de Bariloche, 8400, Argentina Instituto de Nanociencia y Nanotecnologia, CNEA, CONICET, S. C. de Bariloche, 8400, Argentina Instituto Balseiro, CNEA, Universidad Nacional de Cuyo, S. C. de Bariloche, 8400, Argentina    Analia Zwick Centro Atómico Bariloche, CONICET, CNEA, S. C. de Bariloche, 8400, Argentina Instituto de Nanociencia y Nanotecnologia, CNEA, CONICET, S. C. de Bariloche, 8400, Argentina Instituto Balseiro, CNEA, Universidad Nacional de Cuyo, S. C. de Bariloche, 8400, Argentina    Gonzalo A. Álvarez [email protected] Centro Atómico Bariloche, CONICET, CNEA, S. C. de Bariloche, 8400, Argentina Instituto de Nanociencia y Nanotecnologia, CNEA, CONICET, S. C. de Bariloche, 8400, Argentina Instituto Balseiro, CNEA, Universidad Nacional de Cuyo, S. C. de Bariloche, 8400, Argentina
Abstract

Advancing quantum sensing tools for investigating systems at atomic and nanoscales is crucial for the progress of quantum technologies. While numerous protocols employ quantum probes to extract information from stationary or weakly coupled environments, the challenges intensify at atomic- and nano-scales where the environment is inherently out-of-equilibrium or strongly coupled with the sensor. We here prove that the time-reversal symmetry in the quantum-sensor control dynamics is broken, when partial information is probed from an environment that is out-of-equilibrium with non-stationary fluctuations or is described by quantum non-Gaussian, strongly coupled environmental correlations. We exploit this phenomenon as a quantum sensing paradigm with proof-of-principle experimental quantum simulations using solid-state nuclear magnetic resonance (NMR). This introduces a signal contrast on a qubit-probe that quantifies how far the sensed environment is from equilibrium or its quantum non-Gaussian nature. Protocols are also presented to discern and filter a variety of environmental properties including stationary, non-stationary and non-Gaussian quantum noise fluctuations as a step toward sensing the ubiquitous environments of a quantum-sensor at atomic and nanoscales.

I Introduction

The progress on controlling single quantum systems at atomic and nanometric scales has lead to the development of quantum technologies [1, 2, 3]. Both the storage and processing of quantum information in quantum devices suffer from decoherence, the loss of quantum information as a function of time, that distorts the encoded information [4]. Nevertheless, decoherence effects are a key information resource about the environment that is exploited for designing novel quantum sensors with important applications in geology, archaeology, material science, biology and medicine [5, 6, 7] .

These quantum probes have strong potential to enable measurement of physical properties with unprecedented sensitivity, but more importantly they allow probing spatial scales that are not accessible by classical means, such as the atomic and nanoscales [6, 5]. They have already enabled the magnetometry of single neurons [8] and magnetic biomarkers with subcellular resolution [9], microscale and nanoscale detection of single molecules [10, 11], and the probing of temperature-dependent biological processes in cells and small organisms [12].

In the context of these scales, particularly when employing single quantum sensors, environmental systems either manifest intrinsic out-of-equilibrium features or can be unavoidable driven out-of-equilibrium via the quantum feedback induced by the probe, both inducing non-stationary environmental fluctuations [13, 14, 15, 16, 17, 18]. Moreover, quantum probes at these scales can be strongly coupled to its environment generating what is known as non-Gaussian effects [19, 20, 21, 22, 23, 24, 25]. Conventional frameworks to describe the quantum open nature of these sensors do not account for non-stationary environmental features and/or non-Gaussian effects [26, 27, 4, 5]. Only recently, due to progress in quantum sensing technologies, frameworks for sensing out-of-equilibrium and/or non-Gaussian environments with quantum sensors have been introduced [20, 21, 17, 23, 24, 18, 25].

In this article, we delve into the realm of time reversal symmetry to design quantum control sensing-paradigms of the ubiquitous environments found at atomic and nanoscales. We demonstrate the time reversal symmetry breaking in the quantum control of a qubit-sensor, specifically when coupled to quantum non-Gaussian and/or out-of-equilibrium environmental interactions. Leveraging this characteristic, arising from the partial information observed by a quantum-probe, we present a novel quantum sensing paradigm rooted in the design of time-asymmetric dynamical control of the sensor. We name this technique SENSIT (Sensing of Environmental Non-Symmetric Information due to T-symmetry breaking) and demonstrate it through experimental quantum simulations using solid-state NMR.

In this context, we illustrate how the distance of the quantum environmental state from equilibrium can be encoded onto a qubit-probe signal contrast. Furthermore, we showcase the selective filtration of non-stationary features with respect to stationary noise fluctuations. Additionally, we introduce protocols that leverage this contrast to selectively quantify quantum non-Gaussian features and non-equilibrium characteristics of the environment. Overall, our work marks a step forward in the practical application of quantum sensing technology, offering valuable insights into the ubiquitous out-of-equilibrium and quantum non-Gaussian environments encountered by quantum sensors.

II Decoding Environmental Information through Dynamically Controlled Qubit-Sensor

To demonstrate the quantum sensing paradigm based on the time reversal symmetry breaking, we consider a dynamically controlled qubit-sensor coupled to an environment that induces pure dephasing. This quantum sensor platform is found in a variety of systems as in electrons in diamonds [28, 29, 11], electronic spins in nanoscale nuclear spin baths [30], quantum dots [31], donors in silicon [32], superconducting qubits [27], trapped atoms [33], and solid-, liquid- and gas-state NMR systems [26, 7].

Control on the qubit-sensor via dynamical decoupling effectively modulates the strength of the qubit-environment interaction and can thus be used to selectively encode environmental information on the signal decay of the qubit-sensor [26, 27]. In the interaction picture with respect to the environmental evolution and control of the qubit, the qubit-environment Hamiltonian is

HSE(t)=f(t)SzB(t),H_{SE}(t)=f(t)S_{z}B(t)\,, (1)

where SzS_{z} is the qubit-probe spin operator in the zz direction, B(t)B(t) is the noise operator representing the environmental fluctuating degrees of freedom that induce dephasing on the qubit-probe, and f(t)f(t) is the qubit-environment interaction whose time dependence is only due to the modulation induced by dynamical decoupling [34, 35, 36, 37, 27, 26] (Fig. 1a). The fluctuating noise operator is given by B(t)=eiHEtBeiHEtB(t)=\mathrm{e}^{iH_{E}t}B\mathrm{e}^{-iH_{E}t}, where HEH_{E} is the environmental Hamiltonian and BB is the environmental degree of freedom coupled to the qubit-probe.

Refer to caption
Figure 1: (a) Schematic illustration of the dynamically modulated interaction f(t)f(t), enabling the qubit-probe to sense its environment. Realizations of a stochastic process of (b) a stationary fluctuating field B(t)B(t) as a function of time and (c,d) stochastic processes representing an out-of-equilibrium environment due to a quench by a change in the dynamics of the process at t=0t=0. In (c), prior to t=0t=0, the fluctuating field remains fixed at 0, evolving stochastically for t0t\geq 0 and reaching a stationary regime for tt\to\infty. Notably, around t0t\sim 0, the field exhibits a smaller variance than at equilibrium, resulting in a comparatively less impact of the qubit control on its signal. In (d) preceding t=0t=0, the fluctuating field has a greater variance than for tt\to\infty, evolving stochastically for t0t\geq 0 and attaining a stationary regime for tt\to\infty. Around t0t\sim 0, the field has a greater variance than at equilibrium, leading to a more pronounced impact of the qubit control on its signal compared to the equilibrium state. (e) Qubit-sensor signal M(Ts)M(T_{s}) as a function of the sensing time TsT_{s} for the fluctuating field displayed in panels (b-d). Distinctions emerge at shorter times, yet the signals converge to the same decay rate upon reaching the stationary regime. The decay-shift from the stationary curve reflects the influence of an out-of-equilibrium environment during the earlier times.

The evolution operator of the qubit-probe is thus U(Ts)=𝒯ei0Tsdtf(t)SzB(t)U(T_{s})=\mathcal{T}\mathrm{e}^{-i\int_{0}^{T_{s}}\mathrm{d}t\,f(t)S_{z}B(t)}, where 𝒯\mathcal{T} is the time-order superoperator and TsT_{s} is the sensing time, the time during which the qubit-sensor dephases due to sensing the environmental fluctuations. The probe observable is the in-plane qubit-polarization that decays as M(Ts)=S+𝕀Eρ(Ts)S+𝕀Eρ(0)=e𝒥(Ts)M(T_{s})=\frac{\left\langle S_{+}\otimes\mathbb{I}_{E}\,\rho(T_{s})\right\rangle}{\left\langle S_{+}\otimes\mathbb{I}_{E}\,\rho(0)\right\rangle}=\mathrm{e}^{-\mathcal{J}(T_{s})} due to the environment with the decoherence factor 𝒥\mathcal{J}, where ρ(Ts)\rho(T_{s}) is the density matrix of the full qubit-environment system after the qubit has sensed the environment, =tr[]\left\langle\cdot\right\rangle=\text{tr}\left[\cdot\right], and S+=Sx+iSyS_{+}=S_{x}+iS_{y} the up spin operator.

We assume that, in the quantum sensing protocol, the qubit-environment system is initially in a separable state when the probe is brought into contact with the environment. Specifically, we consider the initial state ρ(0)=ρ0=pSxρE\rho(0)=\rho_{0}=pS_{x}\otimes\rho_{E} with the qubit polarized in the xx direction. We do not explicitly write terms proportional to the qubit identity 𝕀S\mathbb{I}_{S} in the density matrix, as they do not contribute to the qubit-probe signal.

We perform a cumulant expansion of the decoherence factor 𝒥\mathcal{J} on the SE interaction coupling strength with the environment

𝒥(Ts)=ninn!0Tsdt10Tsdtnf(t1)f(tn)Wn(t1,,tn)\begin{array}[]{cc}\mathcal{J}(T_{s})=&-\sum_{n}\frac{i^{n}}{n!}\int_{0}^{T_{s}}\mathrm{d}t_{1}\dots\int_{0}^{T_{s}}\mathrm{d}t_{n}\\ &f(t_{1})\dots f(t_{n})W_{n}(t_{1},\dots,t_{n})\end{array} (2)

where WnW_{n} are the cumulants that completely characterize the environment fluctuations felt by the qubit-sensor. They are defined based on the environmental correlation functions

Gn(t1,,tn)=12n1{B(t1),{B(t2),{,B(tn)}}}ρEG_{n}(t_{1},\dots,t_{n})=\\ \frac{1}{2^{n-1}}\left\langle\left\{B(t_{1}),\left\{B(t_{2}),\left\{\dots,B(t_{n})\right\}\dots\right\}\right\}\rho_{\text{E}}\right\rangle (3)

for t1t2tnt_{1}\leq t_{2}\leq\dots\leq t_{n} with {,}\left\{\cdot,\cdot\right\} the anti-commutator (see SI A).

III Environment-Induced Time-reversal Symmetry Breaking

In quantum mechanics, the evolution operator U(t)U(t) is unitary, meaning it is invertible (U(t)=U1(t)U^{\dagger}(t)=U^{-1}(t)). When a quantum system exhibits time-reversal symmetry, this is typically expressed through the time reversal operator TT, which is an anti-unitary operator. Time reversal symmetry implies that TT commutes with the system Hamiltonian [T,H]=0[T,H]=0 and thus satisfies T1U(t)T=U1(t)T^{-1}U(t)T=U^{-1}(t) [38].

At first glance, one might expect this symmetry to result in a corresponding symmetry on the control operation of the qubit-probe dynamics. However, we here demonstrate that when a dynamically controlled qubit-sensor probes an environment, the partial information accessible to the sensor, obtained through the partial trace of environmental degrees of freedom, can unveil a breaking in the time-reversal symmetry of the control function. In particular, we illustrate that the symmetry is disrupted, when the noise operators of the environment, denoted as B(t)B(t), fail to commute at different times. This breakdown occurs explicitly when the decoherence factor involves cumulants of order n3n\geq 3. Moreover, we also show that the symmetry is always broken if the environmental fluctuations are non-stationary, indicative of non-equilibrium features (Proof in SI C).

Quantum non-Gaussian noises thus induce time-reversal symmetry breaking in the quantum control of the qubit-sensor. These noises are characteristic of quantum environments strongly coupled to the sensor and operating at low temperatures. The manifestation of symmetry breaking is absent when the environment is weakly coupled validating the Gaussian approximation, or at the high-temperature limit leading to the semiclassical field approximation (see SI C.2). Furthermore, in the latter scenario, if the environmental fluctuations are non-Gaussian but can be effectively described by classical fields, the time-reversal symmetry remains protected.

A nonstationary environment does not have cumulants invariant under time translation Δt\Delta t, i.e. Wn(t1,,tn)Wn(t1+Δt,,tn+Δt)W_{n}(t_{1},\dots,t_{n})\neq W_{n}(t_{1}+\Delta t,\dots,t_{n}+\Delta t). In this case, for quantum or classical noise operators, the time-reversal symmetry of the control is broken. Notice that time translation symmetry is achieved when the environment reaches a stationary state, including when it is in equilibrium. This is illustrated in Fig. 1, which compares stationary fluctuations of the field B(t)B(t) (panel b) with non-stationary fluctuations induced by quenches (panels c and d). Time-reversal symmetry –in the control– is broken in the latter cases.

This asymmetry in time evolution is reflected in the dephasing of the qubit-probe (Fig. 1e), where the dephasing near the quench decays slower or faster compared to the stationary case, depending on whether the noise fluctuation variance just before the quench is lower or higher than in the stationary regime. This exemplifies how one can exploit the manifestation of the time reversal symmetry breaking of the environment on the qubit-probe dephasing.

The qubit-probe signal has time-reversal symmetry in the control function if the cumulants in Eq. (2) satisfy the symmetry condition Wn(t1,,tn)=(±1)nWn(Tst1,,Tstn)W_{n}(t_{1},\dots,t_{n})=(\pm 1)^{n}W_{n}(T_{s}-t_{1},\dots,T_{s}-t_{n}). The sign (±1)n(\pm 1)^{n} depends on the nature of the noise, i.e. when the noise operator BB is an electric charge, electric field, gate potential, etc. the sign corresponds to 11, and in cases where it is a magnetic field, magnetization, electric current, etc. corresponds to 1-1. We thus call these cases of the electric- and magnetic-type, respectively (details and proof in SI C.2). The cumulants exhibit this symmetry if and only if they possess time translation symmetry, and the noise operators commute at different times or their non-commutation is negligible.

Under these conditions, we prove that the qubit-probe signal satisfies time-reversal symmetry in the control function

Mf=e𝒥f={MfT=e𝒥fTelectric-typeMfT=e𝒥fTmagnetic-type,M_{f}=e^{-\mathcal{J}_{f}}=\begin{cases}M_{f_{T}}=e^{-\mathcal{J}_{f_{T}}}&\text{electric-type}\\ M_{f_{T}}^{*}=e^{-\mathcal{J}_{f_{T}}^{*}}&\text{magnetic-type}\end{cases}\,, (4)

where MfM_{f} is the signal measured when using the control function ff and MfTM_{f_{T}} is that measured when using as control the time reversal of ff, i.e. fT(t)=f(Tst)f_{T}(t)=f(T_{s}-t) (proof in SI C.3). This demonstrates that the polarization of the qubit-probe remains invariant, up to conjugation, under time reversal of the control sequence determined by the control function ff, when the cumulants exhibit time-reversal symmetry. This time-reversal symmetry is a consequence of stationary correlation functions of an environment plus negligible quantum noncommutativity effects guaranteed only by classical fields, weak coupling, high temperature or Gaussianity. When either of these conditions fails, the symmetry is broken, thus enabling the measurement of quantum non-Gaussianity and/or non-stationary phenomena due to out-of-equilibrium dynamics.

Therefore the argument Δ𝒥=𝒥f𝒥fT()\Delta\mathcal{J}=\mathcal{J}_{f}-\mathcal{J}_{f_{T}}^{(*)} of the ratio between the corresponding qubit-probe signals Mf/MfT()=exp{Δ𝒥}M_{f}/M_{f_{T}}^{(*)}=\exp\left\{-\Delta\mathcal{J}\right\} is proportional to the degree of environmental time-reversal symmetry breaking and/or the breaking of the time translation symmetry of the environmental correlation functions (see SI B and C). Here (∗) corresponds to the complex conjugation applied only for magnetic-type cases. The ratio Mf/MfT()M_{f}/M_{f_{T}}^{(*)} is in general a complex number, where its modulus is given by the even cumulants and the phase by the odd cumulants (see SI C.3). Thus the modulus defines the SENSIT qubit-signal contrast, and the phase, the SENSIT qubit-phase contrast (see SI B). In this article, our emphasis is on the SENSIT qubit-signal contrast due to its greater accessibility and robustness in experiments. However, in principle, either quantity can be employed.

The SENSIT qubit-signal contrast is

ReΔ𝒥=n=0(1)n(2n)!0Tsdt1f(t1)0Tsdt2nf(t2n)ΔW2n(t1,,t2n),\text{Re}\Delta\mathcal{J}=-\sum_{n=0}^{\infty}\frac{\left(-1\right)^{n}}{\left(2n\right)!}\int_{0}^{T_{s}}\mathrm{d}t_{1}f(t_{1})\dots\int_{0}^{T_{s}}\mathrm{d}t_{2n}f(t_{2n})\,\Delta W_{2n}(t_{1},\dots,t_{2n})\,, (5)

where

ΔW2n(t1,,t2n)=W2n(t1,,t2n)W2n(Tst1,,Tst2n)\Delta W_{2n}(t_{1},\dots,t_{2n})=\\ W_{2n}(t_{1},\dots,t_{2n})-W_{2n}(T_{s}-t_{1},\dots,T_{s}-t_{2n}) (6)

is the difference between the 2n2n-th cumulant at forward times tit_{i} and at the time reversed ones from the sensing time TstiT_{s}-t_{i}. These quantities serve as order parameters, gauging the extent of time-reversal symmetry breaking in the qubit-control. The SENSIT contrast, therefore, acts as a probe for these order parameters, with weights determined by the control function f(t)f(t). Notice that in Eq. (5), we performed a change in the time variables to convert the reversed control fT(t)f_{T}(t) into f(t)f(t), and this change the arrow of time in the cumulants W2n(Tst1,,Tst2n)W_{2n}(T_{s}-t_{1},\dots,T_{s}-t_{2n}).

The key to utilizing this quantification lies in its resilience against any noise contribution to qubit-probe dephasing that does not induce a time-reversal symmetry breaking, i.e. a contribution that is stationary and such that the noise operators either commute at different times or their non-commutation is negligible. This robustness is ensured as the terms from W2n(t1,,t2n)W_{2n}(t_{1},\dots,t_{2n}) cancel out with those in W2n(Tst1,,Tst2n)W_{2n}(T_{s}-t_{1},\dots,T_{s}-t_{2n}) and similarly for the phase term (proof in SI C.3). This means that if the sensed environment can be separated into two independent parts, aa and bb, such that only aa induces a time-reversal symmetry breaking on the control, then the SENSIT contrast will exclusively sense properties of aa; while remaining completely independent of bb. Consequently, the SENSIT contrast exclusively responds to noise sources that induce the time-reversal symmetry breaking of the qubit-probe control (SI D). This may set an avenue for pump and probe experiments, where a qubit that interacts with a complex environment is used to sense just a part of it by first driving the desired target subsystem out of equilibrium (pump) and then use SENSIT to selectively detect just that subsystem (probe).

To give an example, the SENSIT contrast provides information about the distance to equilibrium. In the simple but general case when the environment state ρE=ρE(0)+ϵρE(1)\rho_{E}=\rho_{E}^{(0)}+\epsilon\rho_{E}^{(1)} is near to a stationary state ρE(0)\rho_{E}^{(0)}, with ρE(1)\rho_{E}^{(1)} a constant perturbation, we demonstrate that Δ𝒥ϵ\Delta\mathcal{J\propto\epsilon} thus quantifying the distance to equilibrium (see SI E). In the particular cases illustrated in Fig. 1, the SENSIT contrast ReΔ𝒥(σσ0)\text{Re}\Delta\mathcal{J}\propto\left(\sigma-\sigma_{0}\right), where σ\sigma the variance of the noise fluctuation before the quench, and σ0\sigma_{0} the variance at the stationary regime achieved at long times after the quench (see SI F). This thus sets a paradigmatic example about how the SENSIT contrast is proportional to the distance (σσ0)\left(\sigma-\sigma_{0}\right) of the initial state of the environment to its stationary state at equilibrium.

IV Experimental detection of out-of-equilibrium states

One of our main results is that the SENSIT contrast, being a readily available quantity in experimental setups, serves as a sensing protocol for detecting and characterizing out-of-equilibrium and/or quantum non-Gaussian environments. To provide a concrete illustration of the underlying principles of SENSIT and enhance the clarity of the introduced general results, we experimentally performed solid-state NMR quantum simulations on a Bruker Avance III HD 9.4T WB NMR spectrometer with a H1{}^{1}\text{H} resonance frequency of 400.15400.15 MHz and a C13{}^{13}\text{C} resonance frequency of 100.61100.61 MHz. The C13{}^{13}C nucleus plays the role of the qubit-probe, and the surrounding H1{}^{1}H nuclei are considered the environment. Since C13{}^{13}C is in natural abundance, it is present in low concentration and all interaction between C13{}^{13}C nuclei are negligible on the performed experiments (see SI G.1 for details on the experimental setup).

The system is initially in thermal equilibrium, as represented in the first step of the sensing protocol in Fig. 2a. We induce an out-of-equilibrium state in the environment to generate non-stationary noise fluctuations on the qubit-sensor. To achieve this, we initially employ the qubit-probe to build up quantum correlations between the qubit and the environmental spins during a preparation time TpT_{p}, ensuring a localized spread of information near the sensor (Fig. 2a,b).

Refer to caption
Figure 2: Illustration of nonequilibrium sensing with SENSIT. (a) Experimental protocol diagram implemented to induce nonequilibrium in the qubit environment and its detection using the SENSIT technique. (b) Schematic representation of the out-of-time-order commutator KK, a well-established measure quantifying the correlation of environmental spins with the qubit during preparation. (c) Correlated spins KK and SENSIT contrast, measured by the qubit, as a function of the preparation time TpT_{p}. Error bars for KK are obtained from a fit, while those for the SENSIT contrast account for the NMR detection sensitivity. The SENSIT contrast 0N1NdxReΔ𝒥(x)\int_{0}^{\frac{N-1}{N}}\mathrm{d}x\,\text{Re}\Delta\mathcal{J}(x) quantifies the environmental non-equilibrium degree by integrating the difference of ReΔ𝒥(x)\text{Re}\Delta\mathcal{J}(x) between SDR and TSDR sequences over the parameter xx. Insets show the signals measured by SDR and TSDR control sequences for various preparation times (indicated by geometrical symbols). Using N=12N=12 pulses in our experiments, the curves match at equilibrium (Tp=0T_{p}=0), and diverge as the environment deviates from equilibrium. This experimental demonstration highlights the utilization of time-reversal symmetry breaking for measuring nonequilibrium environments.

Then we performed a quantum nondemolition measurement on the qubit-probe state mimicked by induced dephasing to erase the probe-environment correlations [39, 7]. This procedure leaves the environment in a correlated out-of-equilibrium state (see third step of Fig. 2a and SI G.2). All these steps constitute the preparation of a nonequilibrium state in the environment.

Subsequently, we initialize the qubit-probe state in a separable state with the environment ρ0=pSxρE\rho_{0}=pS_{x}\otimes\rho_{E} by the application of a π/2\pi/2 pulse on the qubit. After the initialization, we proceed to implement non-equidistant dynamical decoupling sequences to manipulate the time-reversal symmetry of the sequence. We observe the decay of the qubit signal at the sensing time TsT_{s}, representing the duration of the dynamical decoupling sequence, to quantify the SENSIT contrast. This process is illustrated in the last two steps of Fig. 2a.

We employed the Selective Dynamical Recoupling (SDR) sequence [40, 41], chosen for its simplicity in constructing a time-asymmetric sequence using only π\pi-pulses, along with the flexibility of having a single parameter that can be adjusted without changing TsT_{s}. This makes SDR the most straightforward choice for our purposes. It consists of a concatenation of a CPMG spin-echo train with N1N-1 rapid, spin-echo train π\pi-pulses between the times t=0t=0 and t=xTst=xT_{s}, and a Hahn spin-echo sequence consisting of a single echo π\pi-pulse at the center between the times xTsxT_{s} and TsT_{s}. The SDR modulation f(t)f(t) is shown with the blue curve in Fig. 2a. Here xx is a dimensionless parameter, that defines the asymmetry of the SDR sequence interpolating between a single Hahn echo at x=0x=0 and a CPMG sequence of NN equidistant pulses at x=N1Nx=\frac{N-1}{N}. The time-reversed SDR (TSDR) sequence contains the inverse succession in time of the π\pi-pulses, consisting first of the single Hahn-echo sequence between times 0 and (1x)Ts(1-x)T_{s}, followed by the N1N-1 CPMG pulses between the times (1x)Ts(1-x)T_{s} and TsT_{s} (see the orange curve for fT(t)f_{T}(t) in Fig. 2a and SI G.2).

The insets in Fig. 2c illustrate the qubit-probe signal following the SDR and TSDR modulations as a function of xx, for a fixed total sensing time and varying preparation times TpT_{p} for the initial out-of-equilibrium state in the environment. The results demonstrate that the SDR and TSDR signals are indistinguishable at Tp=0T_{p}=0 when the environment is stationary at equilibrium. Subsequently, they showcase how the signals progressively increase their contrast as the environment is shifted further out of equilibrium producing non-stationary noise fluctuations.

To get a single SENSIT-contrast quantification of the non-equilibrium degree of the environmental state, we integrate the attenuation factors of the qubit signals 0N1NdxReΔ𝒥(x)\int_{0}^{\frac{N-1}{N}}\mathrm{d}x\,\text{Re}\Delta\mathcal{J}(x) over the parameter xx (main panel of Fig. 2c). This contrast is proportional to the distance of the initial environmental state from equilibrium, consequently increasing as a function of the preparation time, with a greater number of environmental spins becoming correlated (see SI C).

These experiments were performed at room temperature that represents a high-temperature limit as the thermal energy is much larger than the Zeeman energy of the spins (see SI G.1), therefore the time-reversal symmetry for quantum control described in Eq. (4) will only be broken if the environment is out-of-equilibrium manifesting non-stationary noise fluctuations. Thus here we demonstrate how the SENSIT contrast probes a quenched state on the environment and determines how far from equilibrium it is [13, 24, 25].

V Comparing SENSIT Contrast and Out-of-Time-Order Correlation Metrics for Out-of-Equilibrium States

To have an alternative method for quantifying the out-of-equilibrium degree, we employed a more established approach based on out-of-time-order correlations (OTOC) measured with multiple quantum coherences [15, 42]. This method assesses the non-commutation degree of the evolved density matrix during the preparation time in relation to the initial state of the environment before preparation, as depicted in Fig. 2b. This OTOC approach quantifies the effective number KK of environmental spins that were correlated during the preparation step [13, 43] (see SI G.3 for details).

Figure 2c compares the number KK of correlated environmental spins to the qubit-probe during preparation, and the SENSIT contrast measured from the qubit-probe. Both quantities increase with the preparation time, manifesting a monotonous relation between the established OTOC measure KK of non-equilibrium degree and the proposed SENSIT contrast. Measuring the OTOC involves experimental control over the environment, necessitating the ability to apply collective rotations to environmental spins and reverse the many-body evolution resulting from environmental spin-spin interaction (see SI G.3). Consequently, while OTOC measurements are feasible in e.g. NMR experiments, they are not readily available for most systems. In contrast, assessing the SENSIT contrast only requires control over the qubit-probe, specifically without the need for any control over the sensed environment.

VI Probing quantum information scrambling with SENSIT contrast

To illustrate how the SENSIT contrast, reliant on time-reversal symmetry breaking, can selectively captures information about out-of-equilibrium or quantum non-Gaussian environmental fluctuations over stationary noise fluctuations, we measure the effect of environmental scrambling [15, 42]. In this context, we examine how the quenched state information is erased due to scrambling, consequently impacting the SENSIT contrast (Fig. 3).

Quantum information scrambling is the encoding of an initial local information into non-local degrees of freedom, in this case due to the environmental dynamics driven by the Hamiltonian of the environment HEH_{E} (Fig. 3b) [15, 42]. This in turn renders the information inaccessible by local measurements, and it is related to the autothermalization and quantum information dynamics of the environment [13, 44, 45, 16, 15, 46, 43, 42]. Since the qubit-probe performs a local measurement, the measurements after scrambling should match those found at equilibrium. The key control source in this context involves introducing a waiting period, denoted as the environmental scrambling time TET_{E}, before implementing the detection of the SENSIT contrast following the quenching of the environment (Fig. 3a). In the case of a non-Gaussian environment that is stationary, the cumulant expansion terms exhibit time translation symmetry, rendering the SENSIT contrast invariant with respect to the waiting time. Conversely, an out-of-equilibrium environment relaxes towards equilibrium as a function of the waiting—scrambling—time.

Refer to caption
Figure 3: Sensing environmental scrambling with SENSIT. (a) Experimental protocol diagram implemented to induce nonequilibrium in the qubit environment, followed by scrambling and measurement using the SENSIT technique. (b) Schematic representation of scrambling, the process encoding localized information into non-local degrees of freedom, rendering it inaccessible by local measurements. In the limit of large environmental scrambling times TET_{E} , the qubit’s ability to sense non-equilibrium conditions diminishes. (c) Qubit-measured SENSIT contrast as a function of the scrambling time TET_{E}, enabling the distinction between non-stationary environmental dynamics (experimental violet curve) and non-Gaussian stationary noise (illustrative dashed yellow curve), which should remain invariant under TET_{E}. Error bars are due to the NMR detection sensitivity. Insets display signals measured by the SDR and TSDR control sequences for different scrambling times (marked by geometrical symbols). N=12N=12 pulses were used in our experiments. Note the separation of curves at low scrambling times converging as the quench is scrambled away.

The decay of the SENSIT contrast, observed in Fig. 3c, is presented as a function of the environmental scrambling time TET_{E}. The insets provide the SDR and TSDR signals for three distinct scrambling times. The contrast between the SDR and TSDR curves diminishes as the quenched state is progressively scrambled away. These results thus effectively showcase SENSIT’s ability to selectively quantify the extent to which the environment of the qubit-probe is departing from equilibrium and evolving towards equilibrium. Importantly, SENSIT enables the measurement of quantum information scrambling without relying on environmental time reversions, a requirement typical need in measurements based on OTOCs [15, 42].

VII Summary and outlook

While most quantum systems exhibit time reversal symmetry [38], our research unveils a fundamental breakdown of time reversal symmetry when a quantum sensor probes partial information from environments, characterized by out-of-equilibrium, non-stationary dynamics or with interactions containing quantum non-Gaussian correlations. This opens a quantum sensing paradigm, offering a lens to explore ubiquitous environments at the quantum level, where intrinsic out-of-equilibrium dynamics prevail, driven either by inherent fluctuations or quantum feedback induced by the probe [17, 24, 18, 25]. Moreover, it offers a tool for single sensors at atomic or nanoscales that can be strongly coupled with the environment, thus generating quantum non-Gaussian effects on the dephasing of the qubit-probe [25].

Our findings gain practical significance in the realm of quantum sensing. Specifically, within pump and probe schemes [47], our results open avenues for tailored measurements using qubit-probes, enabling selective detection of the environmental degrees of freedom being selectively pumped out of equilibrium. Moreover, our results holds promise for characterizing noise of time crystals [48] or Floquet systems [49], specially those with partially broken time translation symmetry induced by external driving forces. This offers insights into the dynamics of such systems, providing a means to understand and quantify the intricate interplay between the quantum probe and environments with complex, time-varying characteristics [14, 24, 25].

An additional strength of our work lies in its ability to capture information scrambling of local operators, like the OTOCS, but notably without requiring environmental time reversions [15, 42]. This unique feature positions our research as a valuable tool for detecting persistent states characterized by long-lasting temporal features, such as localized modes [50]. In essence, our study not only contributes theoretical insights but also introduces practical methodologies that can be harnessed to explore and manipulate quantum systems in diverse and dynamic environments.

In conclusion, our study not only contributes fundamental insights into the breakdown of control function time reversal symmetry in quantum sensing but also presents a platform for practical applications. From tailored measurements in complex samples to probing intriguing phenomena in time crystal and Floquet systems, the potential impact of our findings offers an alternative avenue in the realm of quantum sensing technologies. This work paves the way for future research directions and applications, emphasizing the dynamic interplay between quantum sensors and complex, out-of-equilibrium environments.

ACKNOWLEDGMENTS

This work was supported by CNEA; CONICET; ANPCyT-FONCyT PICT-2017-3156, PICT-2017-3699, PICT-2018-4333, PICT-2021-GRF-TI-00134, PICT-2021-I-A-00070; PIP-CONICET (11220170100486CO); UNCUYO SIIP Tipo I 2019-C028, 2022-C002, 2022-C030; Instituto Balseiro; Collaboration programs between the MINCyT (Argentina) and, MAECI (Italy) and MOST (Israel).

Appendix A Cumulant expansion for the qubit-probe signal decay

In this section we derive the cumulant expansion of the decoherence factor 𝒥\mathcal{J} given by Eq. (2) in the main text. Initially, we describe the signal decay of a controlled qubit-probe that dephases due to the influence of an arbitrary quantum environment. We then express it as a function of the correlation functions of the environmental fluctuation, subsequently deriving the cumulant expansion representation.

A.1 Qubit-probe dephasing in terms of the environmental correlation functions

We denote the initial state of the full system as ρ(t=0)=ρ0\rho(t=0)=\rho_{0} and we assume it is separable

ρ0=pSxρE,\rho_{0}=pS_{x}\otimes\rho_{E}, (A.1)

where pp is the polarization of the qubit and the qubit-probe state SxS_{x} is in the xx direction. Notice that, we do not explicitly write terms proportional to the qubit identity 𝕀S\mathbb{I}_{S} in the density matrix, as they do not contribute to the qubit-probe signal. We calculate the decay of in-plane polarization M=2pS+𝕀EU(Ts)ρ0U(Ts)M=\frac{2}{p}\left\langle S_{+}\otimes\mathbb{I}_{E}U(T_{s})\rho_{0}U^{\dagger}(T_{s})\right\rangle of the qubit sensor after dephasing

M=2pS+𝕀EU(Ts)ρ0U(Ts)=2pS+𝕀EU(Ts)pSxρEU(Ts)M=\frac{2}{p}\left\langle S_{+}\otimes\mathbb{I}_{E}U(T_{s})\rho_{0}U^{\dagger}(T_{s})\right\rangle=\frac{2}{p}\left\langle S_{+}\otimes\mathbb{I}_{E}U(T_{s})pS_{x}\otimes\rho_{E}U^{\dagger}(T_{s})\right\rangle (A.2)

where 𝕀E\mathbb{I}_{E} is the environmental identity matrix and U(Ts)U(T_{s}) is the evolution operator. As described in the maintext, U(Ts)=𝒯ei0Tsdtf(t)SzB(t)U(T_{s})=\mathcal{T}\mathrm{e}^{-i\int_{0}^{T_{s}}\mathrm{d}t\,f(t)S_{z}B(t)}, and evaluating the trace over the qubit-degrees of freedom in Eq. (A.2), we find

M=(𝒯ei20Tsdtf(t)B(t))ρE(𝒯ei20Tsdtf(t)B(t))=(𝒯ei20Tsdtf(t)B(t))ρE(𝒯~ei20Tsdtf(t)B(t)),\begin{array}[]{cc}M&=\left\langle\left(\mathcal{T}\mathrm{e}^{\frac{i}{2}\int_{0}^{T_{s}}\mathrm{d}t\,f(t)B(t)}\right)\rho_{E}\left(\mathcal{T}\mathrm{e}^{-\frac{i}{2}\int_{0}^{T_{s}}\mathrm{d}t\,f(t)B(t)}\right)^{\dagger}\right\rangle\\ &=\left\langle\left(\mathcal{T}\mathrm{e}^{\frac{i}{2}\int_{0}^{T_{s}}\mathrm{d}t\,f(t)B(t)}\right)\rho_{E}\left(\tilde{\mathcal{T}}\mathrm{e}^{\frac{i}{2}\int_{0}^{T_{s}}\mathrm{d}t\,f(t)B(t)}\right)\right\rangle\,,\end{array} (A.3)

where 𝒯~\tilde{\mathcal{T}} is the anti-time-order superoperator. Considering MM as a functional of ff, we can perform a functional Taylor expansion in ff to obtain

M=n1n!dt1dtnf(t1)f(tn)[δδf(t1)δδf(tn)M]|f=0,M=\sum_{n}\frac{1}{n!}\int\mathrm{d}t_{1}\dots\int\mathrm{d}t_{n}\,f(t_{1})\dots f(t_{n})\left.\left[\frac{\delta}{\delta f(t_{1})}\dots\frac{\delta}{\delta f(t_{n})}M\right]\right|_{f=0}\,, (A.4)

where δδf(t)\frac{\delta}{\delta f(t)} represents functional differentiation with respect to f(t)f(t). Defining the environmental correlation functions as

Gn(t1,,tn)=\displaystyle G_{n}(t_{1},\dots,t_{n})= (i)n[δδf(t1)δδf(tn)M]|f=0\displaystyle\left.\left(-i\right)^{n}\left[\frac{\delta}{\delta f(t_{1})}\dots\frac{\delta}{\delta f(t_{n})}M\right]\right|_{f=0} (A.5)
=\displaystyle= (i)n[δδf(t1)δδf(tn)(𝒯ei20Tsdtf(t)B(t))ρE(𝒯ei20Tsdtf(t)B(t))]|f=0,\displaystyle\left.\left(-i\right)^{n}\left[\frac{\delta}{\delta f(t_{1})}\dots\frac{\delta}{\delta f(t_{n})}\left\langle\left(\mathcal{T}\mathrm{e}^{\frac{i}{2}\int_{0}^{T_{s}}\mathrm{d}t\,f(t)B(t)}\right)\rho_{E}\left(\mathcal{T}\mathrm{e}^{-\frac{i}{2}\int_{0}^{T_{s}}\mathrm{d}t\,f(t)B(t)}\right)^{\dagger}\right\rangle\right]\right|_{f=0}, (A.6)

we find that

M=ninn!0Tsdt1dtnf(t1)f(tn)Gn(t1,,tn).M=\sum_{n}\frac{i^{n}}{n!}\int_{0}^{T_{s}}\mathrm{d}t_{1}\dots\mathrm{d}t_{n}\,f(t_{1})\dots f(t_{n})G_{n}(t_{1},\dots,t_{n})\,. (A.7)

Notice that the correlation functions Gn(t1,,tn)G_{n}(t_{1},\dots,t_{n}) are symmetric under exchange of their arguments, i.e. Gn(t1,ti,,tj,,tn)=Gn(t1,tj,,ti,,tn)G_{n}(t_{1},\dots t_{i},\dots,t_{j},\dots,t_{n})=G_{n}(t_{1},\dots t_{j},\dots,t_{i},\dots,t_{n}). They depend solely on the environmental time-dependent noise operator B(t)B(t) and initial state ρE\rho_{E} as

Gn(t1,,tn)=12n1{B(t1),{B(t2),{,B(tn)}}}ρE,G_{n}(t_{1},\dots,t_{n})=\frac{1}{2^{n-1}}\left\langle\left\{B(t_{1}),\left\{B(t_{2}),\left\{\dots,B(t_{n})\right\}\dots\right\}\right\}\rho_{E}\right\rangle, (A.8)

for t1t2tnt_{1}\leq t_{2}\leq\dots\leq t_{n}. These correlation functions are the mean value of the nested anti-commutators {,}\left\{\cdot,\cdot\right\} of the noise operator in the environmental state ρE\rho_{E}. The lowest order ones are

G0=\displaystyle G_{0}= 1,\displaystyle 1\,,
G1(t1)=\displaystyle G_{1}(t_{1})= B(t1)ρE,\displaystyle\left\langle B(t_{1})\rho_{E}\right\rangle\,,
G2(t1,t2)=\displaystyle G_{2}(t_{1},t_{2})= 12{B(t1),B(t2)}ρE,\displaystyle\frac{1}{2}\left\langle\left\{B(t_{1}),B(t_{2})\right\}\rho_{E}\right\rangle\,,
G3(t1,t2,t3)=\displaystyle G_{3}(t_{1},t_{2},t_{3})= 14{B(t1),{B(t2),B(t3)}}ρE,\displaystyle\frac{1}{4}\left\langle\left\{B(t_{1}),\left\{B(t_{2}),B(t_{3})\right\}\right\}\rho_{E}\right\rangle\,,

for t1t2t3t_{1}\leq t_{2}\leq t_{3}. While this procedure is perturbative, the knowledge of the correlation functions completely determines the decay of the qubit even in the non-perturbative regime.

A.2 The cumulant expansion for the qubit-signal decay

The correlation functions GnG_{n} completely describe the decay of the qubit-probe. However, certain effects can be more easily described using the cumulants, e.g. non-Gaussianity, separability of the effects of independent processes, exponential signal decay and quantification of the control time-reversal symmetry breaking. Expanding in a perturbation series the decoherence factor 𝒥\mathcal{J} with M=e𝒥M=\mathrm{e}^{-\mathcal{J}}, we obtain Eq. (2) of the main text

𝒥=ninn!0Tsdt10Tsdtnf(t1)f(tn)Wn(t1,,tn),\mathcal{J}=-\sum_{n}\frac{i^{n}}{n!}\int_{0}^{T_{s}}\mathrm{d}t_{1}\dots\int_{0}^{T_{s}}\mathrm{d}t_{n}\,f(t_{1})\dots f(t_{n})W_{n}(t_{1},\dots,t_{n})\,, (A.9)

where WnW_{n} are the cumulants of the environmental correlation functions. Then by expanding M=n(1)nn!𝒥nM=\sum_{n}\frac{(-1)^{n}}{n!}\mathcal{J}^{n}, we find the connection between the cumulants WnW_{n} and the correlation functions GnG_{n}

W0=\displaystyle W_{0}= 0\displaystyle 0
W1(t1)=\displaystyle W_{1}(t_{1})= G1(t1)\displaystyle G_{1}(t_{1})
W2(t1,t2)=G2(t1\displaystyle W_{2}(t_{1},t_{2})=G_{2}(t_{1} ,t2)W1(t1)W1(t2)\displaystyle,t_{2})-W_{1}(t_{1})W_{1}(t_{2})
W3(t1,t2,t3)=G3(t1,t2,t3)W2(t1,t2)W1(t3)\displaystyle W_{3}(t_{1},t_{2},t_{3})=G_{3}(t_{1},t_{2},t_{3})-W_{2}(t_{1},t_{2})W_{1}(t_{3})- W1(t1)W2(t2,t3)W1(t2)W2(t3,t1)W1(t1)W1(t2)W1(t3).\displaystyle W_{1}(t_{1})W_{2}(t_{2},t_{3})-W_{1}(t_{2})W_{2}(t_{3},t_{1})-W_{1}(t_{1})W_{1}(t_{2})W_{1}(t_{3})\,.

The general guideline for constructing the nn-th order cumulant WnW_{n}, involves subtracting from GnG_{n} all possible combinations of functions generated by taking products of cumulants with orders less than nn [51]. Specifically, for a Gaussian environment, Wick’s theorem dictates that Wn=0W_{n}=0 for n>2n>2 [51].

Since the correlation functions GnG_{n} are real, the cumulants WnW_{n} are also real. Therefore the cumulants of odd order contribute to the qubit signal phase argM=Im(𝒥)\text{arg}M=-\text{Im}\left(\mathcal{J}\right) based on Eq. (A.9)

Im(𝒥)=n(1)n(2n+1)!0Tsdt10Tsdt2n+1f(t1)f(t2n+1)W2n+1(t1,,t2n+1),\text{Im}\left(\mathcal{J}\right)=-\sum_{n}\frac{\left(-1\right)^{n}}{\left(2n+1\right)!}\int_{0}^{T_{s}}\mathrm{d}t_{1}\dots\int_{0}^{T_{s}}\mathrm{d}t_{2n+1}\,f(t_{1})\dots f(t_{2n+1})W_{2n+1}(t_{1},\dots,t_{2n+1}), (A.10)

and the cumulants of even order to the absolute value of the qubit-signal |M|=eRe(𝒥)\left|M\right|=\mathrm{e}^{-\text{Re}\left(\mathcal{J}\right)}, with

Re(𝒥)=n(1)n(2n)!0Tsdt10Tsdt2nf(t1)f(t2n)W2n(t1,,t2n).\text{Re}\left(\mathcal{J}\right)=-\sum_{n}\frac{\left(-1\right)^{n}}{\left(2n\right)!}\int_{0}^{T_{s}}\mathrm{d}t_{1}\dots\int_{0}^{T_{s}}\mathrm{d}t_{2n}\,f(t_{1})\dots f(t_{2n})W_{2n}(t_{1},\dots,t_{2n})\,. (A.11)

Appendix B SENSIT Contrast

We here calculate the SENSIT contrast based on the comparison between the qubit-probe signal MfM_{f}, when the control modulating function is f(t)f(t), with the signal MfTM_{f_{T}}, for the time reversed control fT(t)=f(Tst)f_{T}(t)=f(T_{s}-t). The corresponding decoherence factors based on Eq. (A.9) are

𝒥f=\displaystyle\mathcal{J}_{f}= ninn!0Tsdt10Tsdtnf(t1)f(tn)Wn(t1,,tn),\displaystyle-\sum_{n}\frac{i^{n}}{n!}\int_{0}^{T_{s}}\mathrm{d}t_{1}\dots\int_{0}^{T_{s}}\mathrm{d}t_{n}\,f(t_{1})\dots f(t_{n})W_{n}(t_{1},\dots,t_{n})\,,
𝒥fT=\displaystyle\mathcal{J}_{f_{T}}= ninn!0Tsdt10TsdtnfT(t1)fT(tn)Wn(t1,,tn),\displaystyle-\sum_{n}\frac{i^{n}}{n!}\int_{0}^{T_{s}}\mathrm{d}t_{1}\dots\int_{0}^{T_{s}}\mathrm{d}t_{n}\,f_{T}(t_{1})\dots f_{T}(t_{n})W_{n}(t_{1},\dots,t_{n})\,,

respectively. Changing variables we can rewrite the last equation as 𝒥fT=n(i)nn!0Tsdt10Tsdtnf(t1)f(tn)Wn(Tst1,,Tstn)\mathcal{J}_{f_{T}}=-\sum_{n}\frac{\left(-i\right)^{n}}{n!}\int_{0}^{T_{s}}\mathrm{d}t_{1}\dots\int_{0}^{T_{s}}\mathrm{d}t_{n}\,f(t_{1})\dots f(t_{n})W_{n}(T_{s}-t_{1},\dots,T_{s}-t_{n}).

Then the difference between the attenuation factors is Δ𝒥=𝒥f𝒥fT()\Delta\mathcal{J}=\mathcal{J}_{f}-\mathcal{J}_{f_{T}}^{(*)}, where (∗) is complex conjugation applied only for magnetic-type cases. The distinction between electric- and magnetic-type cases is described in SI C. In terms of the cumulant differences, we obtain

Δ𝒥=nin(n)!0Tsdt10Tsdtnf(t1)f(tn)ΔWn(t1,,tn),\Delta\mathcal{J}=-\sum_{n}\frac{i^{n}}{\left(n\right)!}\int_{0}^{T_{s}}\mathrm{d}t_{1}\dots\int_{0}^{T_{s}}\mathrm{d}t_{n}\,f(t_{1})\dots f(t_{n})\,\Delta W_{n}(t_{1},\dots,t_{n})\,, (A.12)

where the cumulant differences are

ΔWn(t1,,tn)=Wn(t1,,tn)(±1)nWn(Tst1,,Tstn),\Delta W_{n}(t_{1},\dots,t_{n})=W_{n}(t_{1},\dots,t_{n})-\left(\pm 1\right)^{n}W_{n}(T_{s}-t_{1},\dots,T_{s}-t_{n})\,,

with ±1\pm 1 being 11 for electric- and 1-1 for magnetic-type cases. For cumulants of even order, this distinction is irrelevant as (±1)2n=1\left(\pm 1\right)^{2n}=1, leading to Eq. (6) in the main text.

As stated in the main text, they measure the degree of time reversal symmetry breaking of the control operations of the qubit-probe, acting as a kind of order parameters. As shown in SI A.2, (i)nWn(-i)^{n}W_{n} is real for nn and imaginary for nn odd. Consequently, Δ𝒥\Delta\mathcal{J} separates into real and imaginary components. The real (resp. imaginary) component is influenced only by cumulants of even (resp. odd) order, corresponding to a difference in the magnitude (resp. phase) of the qubit-probe signals MfM_{f} and MfTM_{f_{T}}. Explicitly real component

ReΔ𝒥=ln|MfTMf()|=ln|MfTMf|=n(1)n(2n)!0Tsdt10Tsdt2nf(t1)f(t2n)ΔW2n(t1,,t2n)\text{Re}\Delta\mathcal{J}=\ln\left|\frac{M_{f_{T}}}{M_{f}^{(*)}}\right|=\ln\left|\frac{M_{f_{T}}}{M_{f}}\right|=-\sum_{n}\frac{\left(-1\right)^{n}}{\left(2n\right)!}\int_{0}^{T_{s}}\mathrm{d}t_{1}\dots\int_{0}^{T_{s}}\mathrm{d}t_{2n}\,f(t_{1})\dots f(t_{2n})\Delta W_{2n}(t_{1},\dots,t_{2n})\,

corresponds to a difference in the magnitude of the qubit-probe signals, and it is defined by cumulant differences of even order ΔW2n\Delta W_{2n}. This thus demonstrates Eq. (5) of the main text. Analogously, the imaginary component

ImΔ𝒥=arg(MfTMf())=n=0(1)n(2n+1)!0Tsdt1f(t1)0Tsdt2n+1f(t2n+1)ΔW2n+1(t1,,t2n)\text{Im}\Delta\mathcal{J}=\text{arg}\left(\frac{M_{f_{T}}}{M_{f}^{(*)}}\right)=-\sum_{n=0}^{\infty}\frac{\left(-1\right)^{n}}{\left(2n+1\right)!}\int_{0}^{T_{s}}\mathrm{d}t_{1}f(t_{1})\dots\int_{0}^{T_{s}}\mathrm{d}t_{2n+1}f(t_{2n+1})\Delta W_{2n+1}(t_{1},\dots,t_{2n})

corresponds to a difference in the phases of the qubit signals, and it is defined by the cumulant differences of odd order ΔW2n+1\Delta W_{2n+1}.

Appendix C Conditions in the environment for attaining time-reversal symmetry of the qubit-probe control

In this Section, we analyze the conditions required on the environment to satisfy the time-reversal symmetry of the control on the qubit-probe. Based on the expression for the SENSIT contrast of Eq. (A.12) and Eq. (5) of the maintext, the cumulant difference ΔWn(t1,,t2n)=0\Delta W_{n}(t_{1},\dots,t_{2n})=0 should vanish.

To obtain ΔWn(t1,,tn)=0\Delta W_{n}(t_{1},\dots,t_{n})=0 for all sensing times TsT_{s}, it is required for the cumulant functions to have time translation symmetry and that Wn(t1,,t2n)=(±1)nWn(t1,,t2n)W_{n}(t_{1},\dots,t_{2n})=\left(\pm 1\right)^{n}W_{n}(-t_{1},\dots,-t_{2n}), where the sign (±1)n\left(\pm 1\right)^{n} depends on the nature of the noise operator and will be explained later in this section. The first condition is attained if the environmental noise operator fluctuations are stationary. The second one if they have time-reversal symmetry. In Sec. C.1 we thus evaluate the effects of the time translation symmetry of stationary environments and in Sec. C.2 we determine the effects of time-reversal symmetry in the environment.

C.1 Time translation symmetry of the correlation functions and cumulants: a stationary environment

To obtain ΔWn(t1,,tn)=0\Delta W_{n}(t_{1},\dots,t_{n})=0, we need the cumulants to have time translation symmetry

Wn(t1+Δt,,tn+Δt)=Wn(t1,,tn).W_{n}(t_{1}+\Delta t,\dots,t_{n}+\Delta t)=W_{n}(t_{1},\dots,t_{n})\,.

As the cumulants are written in terms of the environment correlation functions GnG_{n} of Eq. (A.8), we thus need them to have time translation symmetry Gn(t1+Δt,,tn+Δt)=Gn(t1,,tn)G_{n}(t_{1}+\Delta t,\dots,t_{n}+\Delta t)=G_{n}(t_{1},\dots,t_{n}). As the noise operators are defined by B(t)=eitHEBeitHEB(t)=\mathrm{e}^{itH_{E}}B\mathrm{e}^{-itH_{E}}, where HEH_{E} is the environment Hamiltonian, we obtain

Gn(t1+Δt,,tn+\displaystyle G_{n}(t_{1}+\Delta t,\dots,t_{n}+ Δt)=12n1{B(t1+Δt),{B(t2+Δt),{,B(tn+Δt)}}}ρE\displaystyle\Delta t)=\frac{1}{2^{n-1}}\left\langle\left\{B(t_{1}+\Delta t),\left\{B(t_{2}+\Delta t),\left\{\dots,B(t_{n}+\Delta t)\right\}\dots\right\}\right\}\rho_{E}\right\rangle
=12n1\displaystyle=\frac{1}{2^{n-1}} {eiΔtHEB(t1)eiΔtHE,{eiΔtHEB(t2)eiΔtHE,{,eiΔtHEB(tn)eiΔtHE}}}ρE\displaystyle\left\langle\left\{\mathrm{e}^{i\Delta tH_{E}}B(t_{1})\mathrm{e}^{-i\Delta tH_{E}},\left\{\mathrm{e}^{i\Delta tH_{E}}B(t_{2})\mathrm{e}^{-i\Delta tH_{E}},\left\{\dots,\mathrm{e}^{i\Delta tH_{E}}B(t_{n})\mathrm{e}^{-i\Delta tH_{E}}\right\}\dots\right\}\right\}\rho_{E}\right\rangle
=12n1\displaystyle=\frac{1}{2^{n-1}} eiΔtHE{B(t1),{B(t2),{,B(tn)}}}eiΔtHEρE\displaystyle\left\langle\mathrm{e}^{i\Delta tH_{E}}\left\{B(t_{1}),\left\{B(t_{2}),\left\{\dots,B(t_{n})\right\}\dots\right\}\right\}\mathrm{e}^{-i\Delta tH_{E}}\rho_{E}\right\rangle
=12n1\displaystyle=\frac{1}{2^{n-1}} {B(t1),{B(t2),{,B(tn)}}}eiΔtHEρEeiΔtHE.\displaystyle\left\langle\left\{B(t_{1}),\left\{B(t_{2}),\left\{\dots,B(t_{n})\right\}\dots\right\}\right\}\mathrm{e}^{-i\Delta tH_{E}}\rho_{E}\mathrm{e}^{i\Delta tH_{E}}\right\rangle.

Therefore we need the environment to be in a stationary state such that eiΔtHEρEeiΔtHE=ρE\mathrm{e}^{-i\Delta tH_{E}}\rho_{E}\mathrm{e}^{i\Delta tH_{E}}=\rho_{E} for all translation times Δt\Delta t. Then

Gn(t1+Δt,,tn+Δt)=\displaystyle G_{n}(t_{1}+\Delta t,\dots,t_{n}+\Delta t)= 12n1{B(t1),{B(t2),{,B(tn)}}}eiΔtHEρEeiΔtHE\displaystyle\frac{1}{2^{n-1}}\left\langle\left\{B(t_{1}),\left\{B(t_{2}),\left\{\dots,B(t_{n})\right\}\dots\right\}\right\}\mathrm{e}^{-i\Delta tH_{E}}\rho_{E}\mathrm{e}^{i\Delta tH_{E}}\right\rangle
=\displaystyle= 12n1{B(t1),{B(t2),{,B(tn)}}}ρE\displaystyle\frac{1}{2^{n-1}}\left\langle\left\{B(t_{1}),\left\{B(t_{2}),\left\{\dots,B(t_{n})\right\}\dots\right\}\right\}\rho_{E}\right\rangle
=\displaystyle= Gn(t1,,tn).\displaystyle G_{n}(t_{1},\dots,t_{n})\,.

The cumulants thus have time translation symmetry if and only if the environment is in a stationary state.

C.2 Time reversal symmetry of the correlation functions and cumulants of the environment

To satisfy the second condition Wn(t1,,t2n)=(±1)nWn(t1,,t2n)W_{n}(t_{1},\dots,t_{2n})=\left(\pm 1\right)^{n}W_{n}(-t_{1},\dots,-t_{2n}), we need the cumulants to have time-reversal symmetry. We thus require our full system with time-reversal symmetry. Time reversal symmetry in simple terms involves reversing the direction of time in the equations that describe the evolution of a system. If these equations remain unchanged when time is reversed, the system is said to exhibit time reversal symmetry. Quantum mechanics is unitary, i.e. the evolution operator U(t)U(t) is unitary and thus invertible U(t)=U1(t)U^{\dagger}(t)=U^{-1}(t). When a quantum system has time-reversal symmetry, this can be expressed with the time reversal operator TT, an anti-unitary operator that commutes with the system Hamiltonian [T,H]=0[T,H]=0 and such that T1U(t)T=U1(t)T^{-1}U(t)T=U^{-1}(t) [38].

In our particular case, to have time-reversal symmetry there exists some anti-unitarian operator T=TSTET=T_{S}\otimes T_{E} such that the full Hamiltonian HH is TT-invariant, i.e. T1HT=HT^{-1}HT=H. This implies in particular that TS1SzTS=±SzT_{S}^{-1}S_{z}T_{S}=\pm S_{z}, and TE1BTE=±BT_{E}^{-1}BT_{E}=\pm B, as the qubit-environment interaction SzB\propto S_{z}B must be TT-invariant. We call the cases when BB commutes with the time reversal operator [B,Tenv]=0[B,T_{\text{env}}]=0 of the electric-type, as it is the case when BB represents gate charges, voltages, electric fields, polarizations, etc. Analogously, we call the case when BB anticommutes with the time reversal operator {B,Tenv}=0\{B,T_{\text{env}}\}=0 of the magnetic-type, as it is the case when BB represents currents, magnetic fields, magnetizations, etc. In our experimental realization the noise operator is a magnetic field, therefore we performed experiments in a magnetic-type case.

The time reversal operator TET_{E} must satisfy TE2=±1T_{E}^{2}=\pm 1 [38], therefore TE1=±TET_{E}^{-1}=\pm T_{E}. This in turn implies

TE1UE(t)TE\displaystyle T_{E}^{-1}U_{E}(t)T_{E} =UE(t),\displaystyle=U_{E}^{\dagger}(t)\,,
TE1UE(t)TE\displaystyle T_{E}^{-1}U_{E}^{\dagger}(t)T_{E} =UE(t),\displaystyle=U_{E}(t)\,,
TEUE(t)TE1\displaystyle T_{E}U_{E}(t)T_{E}^{-1} =UE(t),\displaystyle=U_{E}^{\dagger}(t)\,,
TEUE(t)TE1\displaystyle T_{E}U_{E}^{\dagger}(t)T_{E}^{-1} =UE(t),\displaystyle=U_{E}(t)\,,

where UE(t)=eiHEtU_{E}(t)=\mathrm{e}^{-iH_{E}t} is the environmental evolution operator. This thus implies that TE1B(t)TE=TE1UE(t)BUE(t)TE=±B(t)T_{E}^{-1}B(t)T_{E}=T_{E}^{-1}U_{E}^{\dagger}(t)BU_{E}(t)T_{E}=\pm B(-t).

Based on this properties of the time-reversal operator, we analyze the behavior of the cumulants under the time-reversal. As the cumulants are written in terms of the environment correlation functions GnG_{n} of Eq. (A.8), for the cumulants to have time-reversal symmetry it is necessary and sufficient for the correlation functions to have time reversal symmetry Gn(t1,,tn)=(±1)nGn(t1,,tn)G_{n}(t_{1},\dots,t_{n})=(\pm 1)^{n}G_{n}(-t_{1},\dots,-t_{n}). Without loss of generality we consider t1t2tnt_{1}\leq t_{2}\leq\dots\leq t_{n}, and thus tntn1t1-t_{n}\leq-t_{n-1}\leq\dots\leq-t_{1}. Therefore

Gn(t1,,tn)=(±1)n2n1{B(tn),{B(tn1),{,B(t1)}}}ρE.G_{n}(-t_{1},\dots,-t_{n})=\frac{(\pm 1)^{n}}{2^{n-1}}\left\langle\left\{B(-t_{n}),\left\{B(-t_{n-1}),\left\{\dots,B(-t_{1})\right\}\dots\right\}\right\}\rho_{E}\right\rangle\,.

We can now achieve to this expression using TET_{E} as

Gn(t1,,tn)=(±1)n2n1{TE1B(tn)TE,{TE1B(tn1)TE,{,TE1B(t1)TE}}}ρE.G_{n}(-t_{1},\dots,-t_{n})=\frac{(\pm 1)^{n}}{2^{n-1}}\left\langle\left\{T_{E}^{-1}B(t_{n})T_{E},\left\{T_{E}^{-1}B(t_{n-1})T_{E},\left\{\dots,T_{E}^{-1}B(t_{1})T_{E}\right\}\dots\right\}\right\}\rho_{E}\right\rangle\,.

The product of the operators TET_{E} and TE1T_{E}^{-1} is the identity and we get

Gn(t1,,tn)=(±1)n2n1{B(tn),{B(tn1),{,B(t1)}}}TEρETE1.G_{n}(-t_{1},\dots,-t_{n})=\frac{(\pm 1)^{n}}{2^{n-1}}\left\langle\left\{B(t_{n}),\left\{B(t_{n-1}),\left\{\dots,B(t_{1})\right\}\dots\right\}\right\}T_{E}\rho_{E}T_{E}^{-1}\right\rangle\,.

We thus obtain that for the cumulants to have time-reversal symmetry, we need the environmental state ρE\rho_{E} to be TET_{E}-invariant, i.e. TEρETE1=ρET_{E}\rho_{E}T_{E}^{-1}=\rho_{E}. If we assume this, we obtain

Gn(t1,,tn)=(±1)n2n1{B(tn),{B(tn1),{,B(t1)}}}ρE.G_{n}(-t_{1},\dots,-t_{n})=\frac{(\pm 1)^{n}}{2^{n-1}}\left\langle\left\{B(t_{n}),\left\{B(t_{n-1}),\left\{\dots,B(t_{1})\right\}\dots\right\}\right\}\rho_{E}\right\rangle. (A.13)

This differs from (±1)nGn(t1,,tn)(\pm 1)^{n}G_{n}(t_{1},\dots,t_{n}) in the ordering of the noise operators in the anticommutators. For G1G_{1} and G2G_{2}, Eq. (A.13) becomes G1(t1)=±G1(t1)G_{1}(t_{1})=\pm G_{1}(-t_{1}) and G2(t1,t2)=G2(t1,t2)G_{2}(t_{1},t_{2})=G_{2}(-t_{1},-t_{2}). However from n=3n=3 and forth, Gn(t1,,tn)G_{n}(t_{1},\dots,t_{n}) differs from (±1)nGn(t1,,tn)(\pm 1)^{n}G_{n}(-t_{1},\dots,-t_{n}).

For example for t1t2t3t_{1}\leq t_{2}\leq t_{3},

G3(t1,t2,t3)=14{B(t1),{B(t2),B(t3)}}ρE=14[B(t1)B(t2)B(t3)+B(t1)B(t3)B(t2)+B(t2)B(t3)B(t1)+B(t3)B(t2)B(t1)]ρE,G_{3}(t_{1},t_{2},t_{3})=\frac{1}{4}\left\langle\left\{B(t_{1}),\left\{B(t_{2}),B(t_{3})\right\}\right\}\rho_{E}\right\rangle\\ =\frac{1}{4}\left\langle\left[B(t_{1})B(t_{2})B(t_{3})+B(t_{1})B(t_{3})B(t_{2})+B(t_{2})B(t_{3})B(t_{1})+B(t_{3})B(t_{2})B(t_{1})\right]\rho_{E}\right\rangle\,,

and

±Gn(t1,t2,t3)=14{B(t3),{B(t2),B(t1)}}ρE=14[B(t3)B(t2)B(t1)+B(t3)B(t1)B(t2)+B(t2)B(t1)B(t3)+B(t1)B(t2)B(t3)]ρE.\pm G_{n}(-t_{1},-t_{2},-t_{3})=\frac{1}{4}\left\langle\left\{B(t_{3}),\left\{B(t_{2}),B(t_{1})\right\}\right\}\rho_{E}\right\rangle\\ =\frac{1}{4}\left\langle\left[B(t_{3})B(t_{2})B(t_{1})+B(t_{3})B(t_{1})B(t_{2})+B(t_{2})B(t_{1})B(t_{3})+B(t_{1})B(t_{2})B(t_{3})\right]\rho_{E}\right\rangle\,.

Therefore

G3(t1,t2,t3)\displaystyle G_{3}(t_{1},t_{2},t_{3}) Gn(t1,t2,t3)=\displaystyle\mp G_{n}(-t_{1},-t_{2},-t_{3})=
=\displaystyle= 14[B(t1)B(t3)B(t2)+B(t2)B(t3)B(t1)B(t3)B(t1)B(t2)B(t2)B(t1)B(t3)]ρE\displaystyle\frac{1}{4}\left\langle\left[B(t_{1})B(t_{3})B(t_{2})+B(t_{2})B(t_{3})B(t_{1})-B(t_{3})B(t_{1})B(t_{2})-B(t_{2})B(t_{1})B(t_{3})\right]\rho_{E}\right\rangle
=\displaystyle= 14{[B(t1)B(t3)B(t3)B(t1)]B(t2)+B(t2)[B(t3)B(t1)B(t1)B(t3)]}ρE\displaystyle\frac{1}{4}\left\langle\left\{\left[B(t_{1})B(t_{3})-B(t_{3})B(t_{1})\right]B(t_{2})+B(t_{2})\left[B(t_{3})B(t_{1})-B(t_{1})B(t_{3})\right]\right\}\rho_{E}\right\rangle
=\displaystyle= 14{[B(t1),B(t3)]B(t2)+B(t2)[B(t3),B(t1)]}ρE\displaystyle\frac{1}{4}\left\langle\left\{\left[B(t_{1}),B(t_{3})\right]B(t_{2})+B(t_{2})\left[B(t_{3}),B(t_{1})\right]\right\}\rho_{E}\right\rangle
=\displaystyle= 14[[B(t1),B(t3)],B(t2)]ρE.\displaystyle\frac{1}{4}\left\langle\left[\left[B(t_{1}),B(t_{3})\right],B(t_{2})\right]\rho_{E}\right\rangle\,.

This thus shows an example on how the time reversal symmetry of higher order correlation functions is broken and the breaking is proportional to commutators of the noise operator at different times.

Nevertheless, if the environment is classical or it is at the high temperature limit, one can make a semiclassical approximation of the noise operators and replace

{B(t1),B(t2)}2B(t1)B(t2)2B(t2)B(t1).\left\{B(t_{1}),B(t_{2})\right\}\sim 2B(t_{1})B(t_{2})\sim 2B(t_{2})B(t_{1})\,.

In these cases, the correlation functions become

Gn(t1,,tn)=B(t1)B(t2)B(tn)ρE=(±1)nGn(t1,,tn),G_{n}(t_{1},\dots,t_{n})=\left\langle B(t_{1})B(t_{2})\dots B(t_{n})\rho_{E}\right\rangle=(\pm 1)^{n}G_{n}(-t_{1},\dots,-t_{n}),

and therefore also the cumulants satisfy

Wn(t1,,tn)=(±1)nWn(t1,,tn),W_{n}(t_{1},\dots,t_{n})=(\pm 1)^{n}W_{n}(-t_{1},\dots,-t_{n})\,,

thus satisfying the time-reversal symmetry in the cumulants.

When the environment is Gaussian, either quantum or classical, the only non-zero cumulants are W1W_{1} and W2W_{2}. Since G1(t1)=±G1(t1)G_{1}(t_{1})=\pm G_{1}(-t_{1}) and G2(t1,t2)=G2(t1,t2)G_{2}(t_{1},t_{2})=G_{2}(-t_{1},-t_{2}), then W1(t1)=±W1(t1)W_{1}(t_{1})=\pm W_{1}(-t_{1}) and W2(t1,t2)=W2(t1,t2)W_{2}(t_{1},t_{2})=W_{2}(-t_{1},-t_{2}). Analogously, when the qubit is weakly coupled to its environment, then the phase is dominated by W1W_{1} and the decay by W2W_{2}, and the environment can be well approximated as a Gaussian environment even if it is a quantum environment.

The cumulants thus only have time-reversal symmetry when the contributions of noise operators commute at different times, if the environment is quantum and non-Gaussian in the sense that is described with cumulants of order higher than 2.

Summarizing, the results presented here mean that the time-reversal symmetry is only attained when all the relevant cumulants to the qubit-probe dephasing satisfy

Wn(t1,,tn)=(±1)nWn(t1,,tn).W_{n}(t_{1},\dots,t_{n})=(\pm 1)^{n}W_{n}(-t_{1},\dots,-t_{n})\,. (A.14)

Instead, the time-reversal symmetry is broken when the environment is quantum, at low temperature, non-Gaussian, and strongly coupled to the qubit.

C.3 Time reversal symmetry of the decoherence factor

When the environment is in a stationary state, and satisfies Eq. (A.14), this means that

𝒥fT=n(±1)ninn!0Tsdt10Tsdtnf(t1)f(tn)Wn(t1,,tn),\mathcal{J}_{f_{T}}=-\sum_{n}(\pm 1)^{n}\frac{i^{n}}{n!}\int_{0}^{T_{s}}\mathrm{d}t_{1}\dots\int_{0}^{T_{s}}\mathrm{d}t_{n}\,f(t_{1})\dots f(t_{n})W_{n}(t_{1},\dots,t_{n})\,,

or, equivalently,

Re(𝒥fT)=\displaystyle\text{Re}\left(\mathcal{J}_{f_{T}}\right)= Re(𝒥fT),\displaystyle\text{Re}\left(\mathcal{J}_{f_{T}}\right)\,,
Im(𝒥fT)=\displaystyle\text{Im}\left(\mathcal{J}_{f_{T}}\right)= ±Im(𝒥fT),\displaystyle\pm\text{Im}\left(\mathcal{J}_{f_{T}}\right)\,,

where ±=+\pm=+ for electric-type noise and ±=\pm=- for magnetic-type noise. This means that for electric-type noise MfT=MfM_{f_{T}}=M_{f}, and for magnetic noise MfT=MfM_{f_{T}}=M_{f}^{*}.

Appendix D Filter out of stationary environmental noise sources by the SENSIT contrast

We here demonstrate the selective property of the SENSIT contrast to filter in environmental sources that leads to the breaking of the time reversed symmetry of the qubit-control, i.e. nonstationary or quantum non-Gaussian noise sources. The SENSIT control filters out the noise sources that induce decoherence on the qubit-probe, but do not induce a breaking in the control time-reversal symmetry. Formally, we consider an environment containing two separated subsystems aa and bb, such that aa is either out of equilibrium inducing non-stationary noise sources or it is quantum non-Gaussian and bb is an environment that is stationary and effectively Gaussian or classical. This means both aa and bb induce decoherence on the qubit-probe, but only aa induces time-reversal symmetry breaking on the control. We write the environment Hilbert space as E=ab\mathcal{H}_{E}=\mathcal{H}_{a}\otimes\mathcal{H}_{b}, the noise operator B=Ba𝕀b+𝕀aBbB=B_{a}\otimes\mathbb{I}_{b}+\mathbb{I}_{a}\otimes B_{b}, the environmental Hamiltonian HE=Ha𝕀b+𝕀aHbH_{E}=H_{a}\otimes\mathbb{I}_{b}+\mathbb{I}_{a}\otimes H_{b} and the initial environmental state as ρE=ρaρb\rho_{E}=\rho_{a}\otimes\rho_{b}. The environments have thus an independent initial state, evolve independently and each of them adds a separated noise contribution to the qubit-probe. For example, in the experiments we carried out on this work, the environment aa would be the spin network of H1{}^{1}H nuclei, while bb would be any other sources of decoherence, e.g. the electrons and phonons of the sample, cosmic rays and radiation going trough it, the current fluctuations in the magnet, the noise induced by electrical installations, etc. Since the environmental subsystems do not interact with each other, the evolution of the noise operator with respect to the environmental Hamiltonian is B(t)=Ba(t)𝕀b+𝕀aBb(t)B(t)=B_{a}(t)\otimes\mathbb{I}_{b}+\mathbb{I}_{a}\otimes B_{b}(t), where Bi(t)=eiHitBieiHitB_{i}(t)=\mathrm{e}^{iH_{i}t}B_{i}\mathrm{e}^{-iH_{i}t} for i=a,bi=a,b. The evolution operator 𝒯ei20Tsdtf(t)B(t)\mathcal{T}\mathrm{e}^{\frac{i}{2}\int_{0}^{T_{s}}\mathrm{d}t\,f(t)B(t)} in Eq. (A.3) is also separable

𝒯ei20Tsdtf(t)B(t)=𝒯ei20Tsdtf(t)Ba(t)𝒯ei20Tsdtf(t)Bb(t).\mathcal{T}\mathrm{e}^{\frac{i}{2}\int_{0}^{T_{s}}\mathrm{d}t\,f(t)B(t)}=\mathcal{T}\mathrm{e}^{\frac{i}{2}\int_{0}^{T_{s}}\mathrm{d}t\,f(t)B_{a}(t)}\otimes\mathcal{T}\mathrm{e}^{\frac{i}{2}\int_{0}^{T_{s}}\mathrm{d}t\,f(t)B_{b}(t)}.

The decay of the qubit magnetization thus becomes

M=(𝒯ei20Tsdtf(t)Ba(t))ρa(𝒯ei20Tsdtf(t)Ba(t))×(𝒯ei20Tsdtf(t)Bb(t))ρb(𝒯ei20Tsdtf(t)Bb(t)).M=\left\langle\left(\mathcal{T}\mathrm{e}^{\frac{i}{2}\int_{0}^{T_{s}}\mathrm{d}t\,f(t)B_{a}(t)}\right)\rho_{a}\left(\mathcal{T}\mathrm{e}^{-\frac{i}{2}\int_{0}^{T_{s}}\mathrm{d}t\,f(t)B_{a}(t)}\right)^{\dagger}\right\rangle\times\left\langle\left(\mathcal{T}\mathrm{e}^{\frac{i}{2}\int_{0}^{T_{s}}\mathrm{d}t\,f(t)B_{b}(t)}\right)\rho_{b}\left(\mathcal{T}\mathrm{e}^{-\frac{i}{2}\int_{0}^{T_{s}}\mathrm{d}t\,f(t)B_{b}(t)}\right)^{\dagger}\right\rangle\,.

We now define the cumulants Wna/bW_{n}^{a/b} of the subsystems as the cumulants of the respective noise operators Ba/b(t)B^{a/b}(t). We can thus write the contributions to the decay in terms of

(𝒯ei20Tsdtf(t)Bi(t))ρi(𝒯ei20Tsdtf(t)Bi(t))=exp[n(i)nn!0Tsdt10Tsdtnf(t1)f(tn)Wni(t1,,tn),]\left\langle\left(\mathcal{T}\mathrm{e}^{\frac{i}{2}\int_{0}^{T_{s}}\mathrm{d}t\,f(t)B_{i}(t)}\right)\rho_{i}\left(\mathcal{T}\mathrm{e}^{-\frac{i}{2}\int_{0}^{T_{s}}\mathrm{d}t\,f(t)B_{i}(t)}\right)^{\dagger}\right\rangle=\exp\left[\sum_{n}\frac{\left(i\right)^{n}}{n!}\int_{0}^{T_{s}}\mathrm{d}t_{1}\dots\int_{0}^{T_{s}}\mathrm{d}t_{n}\,f(t_{1})\dots f(t_{n})W_{n}^{i}(t_{1},\dots,t_{n})\,,\right]

and we obtain the decoherence factor as

𝒥=n(i)nn!0Tsdt10Tsdtnf(t1)f(tn)[Wna(t1,,tn)+Wnb(t1,,tn)],\mathcal{J}=-\sum_{n}\frac{\left(i\right)^{n}}{n!}\int_{0}^{T_{s}}\mathrm{d}t_{1}\dots\int_{0}^{T_{s}}\mathrm{d}t_{n}\,f(t_{1})\dots f(t_{n})\left[W_{n}^{a}(t_{1},\dots,t_{n})+W_{n}^{b}(t_{1},\dots,t_{n})\right]\,,

and compare with Eq. (A.9), we obtain that the cumulants of the environment Wn=Wna+WnbW_{n}=W_{n}^{a}+W_{n}^{b} are the sum of the cumulants of each subsystem. Since the environment bb is neither non-stationary nor quantum non-Gaussian, the cumulants WnbW_{n}^{b} are symmetric under time reversed control. Therefore, the SENSIT contrast is

Δ𝒥=nin(n)!0Tsdt10Tsdtnf(t1)f(tn)ΔWna(t1,,tn),\Delta\mathcal{J}=-\sum_{n}\frac{i^{n}}{\left(n\right)!}\int_{0}^{T_{s}}\mathrm{d}t_{1}\dots\int_{0}^{T_{s}}\mathrm{d}t_{n}\,f(t_{1})\dots f(t_{n})\,\Delta W_{n}^{a}(t_{1},\dots,t_{n})\,,

where ΔWna(t1,,t2n)=Wna(t1,,t2n)Wna(Tst1,,Tst2n)\Delta W_{n}^{a}(t_{1},\dots,t_{2n})=W_{n}^{a}(t_{1},\dots,t_{2n})-W_{n}^{a}(T_{s}-t_{1},\dots,T_{s}-t_{2n}). This thus shows how the SENSIT contrast is independent of all properties of bb, and is in fact the same as what would be obtained if aa were the entire environment of the qubit-probe. This shows that SENSIT is filtering out all noise sources leading to time-reversal symmetry on the qubit control, while maintaining sensitivity to those out of equilibrium or quantum non-Gaussian.

Appendix E SENSIT contrast with an environment near to a stationary state

To give an example on how the distance to equilibrium is encoded in the SENSIT contrast, we consider a simple but general case where the environment is near to a stationary state ρE(0)\rho_{E}^{(0)}. We consider that quantum non-Gaussian contributions to the cumulants are negligible. That is, ρE(0)\rho_{E}^{(0)} is a state where the cumulants have time reversal symmetry in the qubit-probe control ΔWn=0\Delta W_{n}=0. We consider the environmental sate to be ρE=ρE(0)+ϵρE(1)\rho_{E}=\rho_{E}^{(0)}+\epsilon\rho_{E}^{(1)}, where ρE(1)\rho_{E}^{(1)} is a constant perturbation to the environmental state with ϵ\epsilon quantifying the distance to equilibrium. Under these conditions, the cumulants can be expanded in the distance ϵ\epsilon as Wn=Wn(0)+ϵWn(1)+𝒪(ϵ2)W_{n}=W_{n}^{(0)}+\epsilon W_{n}^{(1)}+\mathcal{O}\left(\epsilon^{2}\right), where Wn(0)W_{n}^{(0)} is the nn-th cumulant for the environmental state ρE(0)\rho_{E}^{(0)}, and Wn(1)W_{n}^{(1)} depends on both environmental contributions ρE(0)\rho_{E}^{(0)} and ρE(1)\rho_{E}^{(1)}. For example, for n=2n=2

W2(1)(t1,t2)={B(t1),B(t2)}ρE(1)B(t1)ρE(1)B(t2)ρE(0)B(t1)ρE(0)B(t2)ρE(1).W_{2}^{(1)}(t_{1},t_{2})=\left\langle\left\{B(t_{1}),B(t_{2})\right\}\rho_{E}^{(1)}\right\rangle-\left\langle B(t_{1})\rho_{E}^{(1)}\right\rangle\left\langle B(t_{2})\rho_{E}^{(0)}\right\rangle-\left\langle B(t_{1})\rho_{E}^{(0)}\right\rangle\left\langle B(t_{2})\rho_{E}^{(1)}\right\rangle\,.

Since we consider that ρE(0)\rho_{E}^{(0)} has time reversal symmetry in the qubit-probe control, the main contributions to ΔWn\Delta W_{n} will be linear in ϵ\epsilon and due to the term

ΔWn(1)(t1,,tn)=Wn(1)(t1,,tn)(±1)nWn(1)(Tst1,,Tstn).\Delta W_{n}^{(1)}(t_{1},\dots,t_{n})=W_{n}^{(1)}(t_{1},\dots,t_{n})-\left(\pm 1\right)^{n}W_{n}^{(1)}(T_{s}-t_{1},\dots,T_{s}-t_{n})\,.

The measured SENSIT contrast is thus

Δ𝒥=ϵnin(n)!0Tsdt10Tsdtnf(t1)f(tn)ΔWn(1)(t1,,tn)+𝒪(ϵ2),\Delta\mathcal{J}=-\epsilon\sum_{n}\frac{i^{n}}{\left(n\right)!}\int_{0}^{T_{s}}\mathrm{d}t_{1}\dots\int_{0}^{T_{s}}\mathrm{d}t_{n}\,f(t_{1})\dots f(t_{n})\,\Delta W_{n}^{(1)}(t_{1},\dots,t_{n})\,+\mathcal{O}\left(\epsilon^{2}\right),

manifesting that when the environment is near to a state that satisfies the conditions for time-reversal symmetry in the qubit-probe control, the SENSIT contrast is proportional to the parameter ϵ\epsilon that quantifies the distance to the stationary environmental state.

Appendix F SENSIT Contrast of a Quenched Ornstein-Uhlenbeck Process

We consider the paradigmatic example of a quenched OU process for the noise operator fluctuations, with a self-correlation time τ\tau and the standard deviation σ0\sigma_{0} at equilibrium, i.e. at long times. This stochastic process is Gaussian with zero mean, thus all cumulants with n2n\neq 2 are null Wn=0W_{n}=0. The quench is generated by an out-of-equilibrium initial condition, corresponding to a Gaussian distribution with a standard deviation different from the one at equilibrium σσ0\sigma\neq\sigma_{0}. The self-correlation function of the quenched process is

W2(t1,t2)\displaystyle W_{2}\left(t_{1},t_{2}\right) =\displaystyle= W2Eq(t1,t2)+W2Q(t1,t2),\displaystyle W_{2}^{\text{Eq}}\left(t_{1},t_{2}\right)+W_{2}^{\text{Q}}\left(t_{1},t_{2}\right)\,,

where

W2Eq(t1,t2)\displaystyle W_{2}^{\text{Eq}}\left(t_{1},t_{2}\right) =\displaystyle= σ0e|t1t2|τ\displaystyle\sigma_{0}\mathrm{e}^{-\frac{\left|t_{1}-t_{2}\right|}{\tau}\,}

and

W2Q(t1,t2)\displaystyle W_{2}^{\text{Q}}\left(t_{1},t_{2}\right) =\displaystyle= (σσ0)et1+t2τ\displaystyle\left(\sigma-\sigma_{0}\right)\mathrm{e}^{-\frac{t_{1}+t_{2}}{\tau}}\,

are the equilibrium and quench contributions to the correlation function [18]. The SENSIT contrast measured from a qubit-probe coupled to this noise process is ReΔ𝒥=0Tsdt1f(t1)0Tsdt2f(t2)[W2Q(t1,t2)W2Q(Tst1,Tst2)]\text{Re}\Delta\mathcal{J}=-\int_{0}^{T_{s}}\mathrm{d}t_{1}f(t_{1})\int_{0}^{T_{s}}\mathrm{d}t_{2}f(t_{2})\left[W_{2}^{\text{Q}}\left(t_{1},t_{2}\right)-W_{2}^{\text{Q}}\left(T_{s}-t_{1},T_{s}-t_{2}\right)\right]. Since W2Eq(t1,t2)=W2Eq(Tst1,Tst2)W_{2}^{\text{Eq}}\left(t_{1},t_{2}\right)=W_{2}^{\text{Eq}}\left(T_{s}-t_{1},T_{s}-t_{2}\right), the equilibrium correlation function does not contribute to the SENSIT contrast. After replacing the cumulants, the SENSIT contrast can be written as ReΔ𝒥=(σσ0)Σ[f]\text{Re}\Delta\mathcal{J}=\left(\sigma-\sigma_{0}\right)\Sigma\left[f\right], with

Σ[f]=12[(0Tsdtf(t)etτ)2(0Tsdtf(t)eTstτ)2].\Sigma\left[f\right]=-\frac{1}{2}\left[\left(\int_{0}^{T_{s}}\mathrm{d}tf(t)\,\mathrm{e}^{-\frac{t}{\tau}}\right)^{2}-\left(\int_{0}^{T_{s}}\mathrm{d}tf(t)\mathrm{e}^{-\frac{T_{s}-t}{\tau}}\right)^{2}\right]\,.

Note that the SENSIT contrast is proportional to (σσ0)\left(\sigma-\sigma_{0}\right), i.e. a variance distance defining how far from equilibrium the initial state of the environment is, weighted by the term Σ[f]\Sigma\left[f\right] that measures the ability of the chosen control modulation function ff to detect the time-reversal symmetry breaking. This thus sets a paradigmatic example about how the SENSIT contrast is proportional to (σσ0)\left(\sigma-\sigma_{0}\right) quantifying the distance from the initial state of the environment to its stationary state at equilibrium.

Appendix G Solid-state NMR Quantum Simulations

G.1 Experimental setup and system

The quantum simulations were performed with solid-state NMR experiments on a Bruker Avance III HD 9.4T WB spectrometer with a H1{}^{1}\text{H} resonance frequency of 400.15400.15 MHz and a C13{}^{13}\text{C} resonance frequency of 100.61100.61 MHz. We used the nuclear spins of a polycrystalline adamantane C10H16C_{10}H_{16} sample to set up the qubit-probe and its environment. Most hydrogen nuclei (98.93%) in the sample are protons, with a spin 1/2\nicefrac{{1}}{{2}}, while only approximately 1.07%1.07\% of the carbons are C13{}^{13}C, with spin 1/21/2, the remaining carbons has no magnetic moment. The low concentration of 13C allows to neglect the interaction between them as the interaction with the hydrogens is dominant. We therefore consider the sample as an ensemble of C13{}^{13}C qubit-probes that interact with the protons near them, considered as the environment.

The experiments are carried out at a high magnetic field, as the Zeeman energy is 105\gtrsim 10^{5} times stronger that the spin-spin interactions. Thus only the secular part of the internuclear dipolar Hamiltonian contributes to the dynamics [52]. Therefore the full Hamiltonian of the system is

H=HS+HE+HSE,H=H_{S}+H_{E}+H_{SE}\,, (A.15)

where the qubit-probe (carbon) considered as our system SS, the environment (protons) and the system-environment interaction Hamiltonians are

HS\displaystyle H_{S} =γCB0Sz𝕀E+control,\displaystyle=\gamma_{C}B_{0}S_{z}\otimes\mathbb{I}_{E}+\text{control}\,,
HE\displaystyle H_{E} =γHB0𝕀SIz+ijdijH(2IziIzjIxiIxjIyiIyj)+control,\displaystyle=\gamma_{H}B_{0}\mathbb{I}_{S}\otimes I_{z}+\sum_{i\neq j}d_{ij}^{H}\left(2I_{z}^{i}I_{z}^{j}-I_{x}^{i}I_{x}^{j}-I_{y}^{i}I_{y}^{j}\right)+\text{control}\,,
HSE\displaystyle H_{SE} =SzidiIzi=SzB,\displaystyle=S_{z}\sum_{i}d_{i}I_{z}^{i}=S_{z}B\,,
respectively.

Here, the sums run over the environmental spins (the protons), γC\gamma_{C} and γH\gamma_{H} are the gyromagnetic ratios of the C13{}^{13}C and proton, respectively, B0B_{0} is the static field applied in the zz-direction, the spin operators 𝐒\mathbf{S} is the qubit-probe (C13{}^{13}C spin) and 𝐈i\mathbf{I}^{i} are the environmental spins with 𝐈=i𝐈i\mathbf{I}=\sum_{i}\mathbf{I}^{i} the total spin moment of the environment, dijHd_{ij}^{H} are the dipolar couplings between the environmental spins ii and jj, did_{i} is the dipolar coupling between the qubit-probe and the ii-th spin of the environment. The noise operator is B=idiIziB=\sum_{i}d_{i}I_{z}^{i} that represents the field that the qubit-probe experiences due to the environment.

In the interaction picture with respect to the Zeeman interactions, the Hamiltonians become [52]

HS\displaystyle H_{S} =control,\displaystyle=\text{control}\,,
HE\displaystyle H_{E} =ijdijH(2IziIzjIxiIxjIyiIyj)+control.\displaystyle=\sum_{i\neq j}d_{ij}^{H}\left(2I_{z}^{i}I_{z}^{j}-I_{x}^{i}I_{x}^{j}-I_{y}^{i}I_{y}^{j}\right)+\text{control}\,.
HSE\displaystyle H_{SE} =SzidiIzi=SzB.\displaystyle=S_{z}\sum_{i}d_{i}I_{z}^{i}=S_{z}B\,.

We utilize control over the environment solely to create the nonstationary initial state. Subsequently, during the quantum simulations of the SENSIT protocol, only the qubit-probe is controlled. For our experiments, we applied on-resonance π\pi-pulses with the qubit-probe. In the interaction picture with respect to this control, i.e. the toggling frame [53], the Hamiltonian is

HS\displaystyle H_{S} =0,\displaystyle=0\,,
HE\displaystyle H_{E} =ijdijH(2IziIzjIxiIxjIyiIyj),\displaystyle=\sum_{i\neq j}d_{ij}^{H}\left(2I_{z}^{i}I_{z}^{j}-I_{x}^{i}I_{x}^{j}-I_{y}^{i}I_{y}^{j}\right),
HSE\displaystyle H_{SE} =f(t)SzidiIzi=f(t)SzB,\displaystyle=f(t)S_{z}\sum_{i}d_{i}I_{z}^{i}=f(t)S_{z}B\,,

where the function f(t)f(t), switches its signs whenever a π\pi-pulse is applied [4].

These Hamiltonians have time-reversal symmetry. To write this explicitly, we use the representation Iαi=12σαiI_{\alpha}^{i}=\frac{1}{2}\sigma_{\alpha}^{i}, Sz=12σαSS_{z}=\frac{1}{2}\sigma_{\alpha}^{S}, where σαi\sigma_{\alpha}^{i} are Pauli matrices that act on the space of the ii-th environment spin and σαS\sigma_{\alpha}^{S} are Pauli matrices that act on the qubit space. The time reversal operator is

T=σySiσyiK,T=\sigma_{y}^{S}\prod_{i}\sigma_{y}^{\text{i}}K\,, (A.17)

where KK is the complex conjugation operator [38]. Since the system is at high temperature, the contribution of noncommutation terms to the SENSIT contrast will be negligible, thus any measured SENSIT contrast is due to asymmetry generated by the environment initial state. In particular, if the state commutes with the environmental Hamiltonian and has time-reversal symmetry, then the system will have time-reversal symmetry in the control functions.

To finally obtain a Hamiltonian with the form of Eq. (1) in the main text, we switch to an interaction picture with respect to the environmental Hamiltonian

H(t)=HSE(t)=f(t)SzB(t),H(t)=H_{SE}(t)=f(t)S_{z}B(t),

where B(t)=eiHEtBeiHEtB(t)=\mathrm{e}^{iH_{E}t}B\mathrm{e}^{-iH_{E}t} is the time-dependent noise operator. This is the experimental implementation of Eq. (1) of the main text in our quantum simulations.

G.2 Out-of-equilibrium environmental-state preparation

Refer to caption
Figure 4: Pulse sequence used for the SENSIT experiments. The different blocks represents different conceptual steps. First, cross polarization is used to initialize the system and increase the signal-to-noise ratio. Then, the 1010ms delay time ensures that all qubit-environment correlations and environmental initial state are erased due to T2T_{2} relaxation before further control. This is then followed by a (π/2)y\left(\nicefrac{{\pi}}{{2}}\right)_{y} pulse, to put the qubit-probe state in-plane. Then L0L_{0} cycles of the MREV-8 sequence are implemented to correlate the qubit-probe and the environment and a (π/2)y\left(\nicefrac{{\pi}}{{2}}\right)_{-y} pulse returns the qubit-probe state to the zz direction. The preparation time TpT_{p} is the total duration of the L0L_{0} MREV-8 cycles. After that, the MREV-8 sequence is used again to mimic a projective measurement on the qubit-probe and turn the correlated state into a state where the qubit and environment are uncorrelated, but with the environment out of equilibrium. To ensure the completeness of the projective measurement, we attain a stationary state by varying L1L_{1}. Specifically, we set L1=42L_{1}=42 because for larger values, the qubit-probe state remained unchanged despite alterations in L1L_{1}. The environment then is scrambled by letting it evolve freely during an environmental scrambling time TET_{E}. The qubit-probe state is then put in plane with a (π/2)y\left(\nicefrac{{\pi}}{{2}}\right)_{y} pulse, and the SDR sequence is applied during the sensing time TsT_{s} to sense the environment via the readout of the qubit-probe state. During this readout, the environment is decoupled for improving the signal-to-noise ratio using continuous wave decoupling. To obtain the SENSIT contrast the experiment is repeated exchanging the SDR sequence by the TSDR sequence.

In this section we describe the pulse sequence used in the experiments described in Fig. 4. For the quantum simulations, we first need to prepare an out-of-equilibrium environment state of the form

ρ0=SxρE,\rho_{0}=S_{x}\otimes\rho_{E}\,,

with [ρE,HE]0\left[\rho_{E},H_{E}\right]\neq 0. Before this preparation, the initial state of the full system is in a Boltzmann thermal equilibrium state. Since the experiments were conducted at room temperature, and the Zeeman energy is 15000\lesssim 15000 times lower than the thermal energy, the state is described in the high temperature limit [52]. Therefore, the initial state is ρ1tr[𝕀](𝕀βH)\rho\simeq\frac{1}{\text{tr}[\mathbb{I}]}\left(\mathbb{I}-\beta H\right). As the Zeeman coupling to the external magnetic field is dominant over the dipolar coupling between nuclei, the state is further simplified ρ1tr[𝕀][𝕀βγCB0Sz𝕀EβγHB0𝕀SIz]\rho\simeq\frac{1}{\text{tr}[\mathbb{I}]}\left[\mathbb{I}-\beta\gamma_{C}B_{0}S_{z}\otimes\mathbb{I}_{E}-\beta\gamma_{H}B_{0}\mathbb{I}_{S}\otimes I_{z}\right]. The initial step in the experiments involves performing cross-polarization between the environment (the protons) and the qubit (the carbons) just to increase the nuclear polarization of the carbons, and thus improve the signal-to-noise ratio of the qubit-probe signal by a factor of γH/γC3.97\nicefrac{{\gamma_{H}}}{{\gamma_{C}}}\simeq 3.97. Then to remove any possible correlation between the carbons and protons, we store the qubit (carbon) magnetization in the zz direction and wait 1010ms (time longer than T2T_{2} of both spin species) to scramble out any proton signal and carbon-proton correlations. This process is shown in the Qubit-Sensor Initialization block of Fig. 4. The π2\frac{\pi}{2} pulse durations we used for the protons and carbons were 3.4μ3.4\mus and 5.5μ5.5\mus, respectively. The duration of the carbon π\pi pulses was 11μ11\mus. After this we apply a (π/2)y\left(\nicefrac{{\pi}}{{2}}\right)_{y}-pulse on the qubit-probe around the y-axis, to obtain the state of the qubit-environment systemρ1tr[𝕀][𝕀βγHB0Sx𝕀E]\rho\simeq\frac{1}{\text{tr}[\mathbb{I}]}\left[\mathbb{I}-\beta\gamma_{H}B_{0}S_{x}\otimes\mathbb{I}_{E}\right].We can thus write the state of our system just before the preparation time period as ρ=(12+p~Sx)𝕀Etr[𝕀E]\rho=\left(\frac{1}{2}+\tilde{p}S_{x}\right)\otimes\frac{\mathbb{I}_{E}}{\text{tr}\left[\mathbb{I}_{E}\right]}, a separable state where the environment is at infinite temperature and the qubit-probe is polarized in the xx direction. Here the polarization of the qubit is p~=βγHB0\tilde{p}=\beta\gamma_{H}B_{0}. Hereafter, we drop the term 12𝕀Etr[𝕀E]\frac{1}{2}\otimes\frac{\mathbb{I}_{E}}{\text{tr}\left[\mathbb{I}_{E}\right]}, since it does not contribute to the qubit-probe signal, and we get

ρ=p~Sx𝕀Etr[𝕀E],\rho=\tilde{p}S_{x}\otimes\frac{\mathbb{I}_{E}}{\text{tr}\left[\mathbb{I}_{E}\right]}\,, (A.18)

The environmental state 𝕀Etr[𝕀E]\frac{\mathbb{I}_{E}}{\text{tr}\left[\mathbb{I}_{E}\right]} is proportional to the identity and thus it is invariant under the time reversal operation of Eq. (A.17), and it also commutes with the environmental Hamiltonian. Since the experiments are carried out at high temperature (See SI G.1), if the environmental state ρE\rho_{E} is stationary and invariant under time reversal, then the conditions outlined in SI C are satisfied, indicating that the system possesses time-reversal symmetry in the qubit-probe control functions. We therefore predict to observe a null SENSIT contrast when the environment is in this state.

Then to turn this state into an out-of-equilibrium state, we perform the following preparation step. We apply the MREV-8 pulse sequence [54] during the preparation time TpT_{p} on the environmental spins to decouple them, i.e. cancel out the dipole-dipole interaction between them thus making null the environmental Hamiltonian. We used a MREV cycle time of 54,4μ54,4\mus. This is shown in Fig. 4, in the block labeled Sensor-Environment Correlation HSEH_{SE}. The effective full system Hamiltonian HH in the rotating frame of both the qubit-probe and the environmental spins (i.e., in the interaction picture with respect to the Zeeman Hamiltonians) is solely the interaction Hamiltonian HSEH_{SE}, with the field BB fixed in time as the evolution stemming from the environmental Hamiltonian is refocused by the MREV sequence

HSE=SzidiIzi=SzB.H_{SE}=S_{z}\sum_{i}d_{i}I_{z}^{i}=S_{z}B\,.

During this step the qubit dephases due to interaction with the environment. The full qubit-environment state becomes ρ(Tp)=p~eiSzBTp(12+p~Sx)𝕀Etr[𝕀E]eiSzBTp\rho(T_{p})=\tilde{p}\mathrm{e}^{-iS_{z}BT_{p}}\left(\frac{1}{2}+\tilde{p}S_{x}\right)\otimes\frac{\mathbb{I}_{E}}{\text{tr}\left[\mathbb{I}_{E}\right]}\mathrm{e}^{iS_{z}BT_{p}}, or equivalently

ρ(Tp)=p~(Sxcos(BTp)tr[𝕀E]+Sysin(BTp)tr[𝕀E]).\rho(T_{p})=\tilde{p}\left(S_{x}\otimes\frac{\cos\left(BT_{p}\right)}{\text{tr}\left[\mathbb{I}_{E}\right]}+S_{y}\otimes\frac{\sin\left(BT_{p}\right)}{\text{tr}\left[\mathbb{I}_{E}\right]}\right)\,. (A.19)

As this state is not separable, we have created quantum correlations between the environmental spins and the qubit-probe. This is simply a free induction decay due to the constant but random field BB felt by the qubit-probe.

We then proceeded to erase the qubit-environment correlations mimicking a quantum non-demolition (QND) measurement on the qubit-probe, while maintaining the non-equilibrium status of the environmental state to attain a state like the one described in Eq. (A.1). To do this, we apply a (π/2)y\left(\nicefrac{{\pi}}{{2}}\right)_{-y}-pulse around the y-y direction, and get the state

p~[Szcos(BTp)tr[𝕀E]+Sysin(BTp)tr[𝕀E]].\tilde{p}\left[S_{z}\otimes\frac{\cos\left(BT_{p}\right)}{\text{tr}\left[\mathbb{I}_{E}\right]}+S_{y}\otimes\frac{\sin\left(BT_{p}\right)}{\text{tr}\left[\mathbb{I}_{E}\right]}\right]\,.

The first term satisfies [Szcos(BTp)tr[𝕀E],HSE]=0\left[S_{z}\otimes\frac{\cos\left(BT_{p}\right)}{\text{tr}\left[\mathbb{I}_{E}\right]},H_{SE}\right]=0 and thus does not evolve, but the second one does evolve, and it will be dephased –vanished– due to the interaction with the environmental field BB. We thus apply the MREV-8 sequence for a sufficient duration to dephase the second term, effectively simulating a quantum non-demolition (QND) measurement on the qubit-probe state, where the state is projected onto the subspace proportional to SzS_{z}. This is shown in the Quantum Non-Demolition Measurements block in Fig. 4. As long as we do not refocus this dephasing with a time-reversion, the qubit-probe signal we measure only comes from the state p~Szcos(BTp)tr[𝕀E]\tilde{p}S_{z}\otimes\frac{\cos\left(BT_{p}\right)}{\text{tr}\left[\mathbb{I}_{E}\right]}.

For the experiments described in Fig. 3 of the main text, this is the step where environmental scrambling is introduced. During the scrambling time TET_{E} a waiting period is introduced without applying the MREV-8 sequence, as shown in Fig. 4 within the Environmental Scrambling block, so the environment Hamiltonian produces the information scrambling on the environmental state. The created state is thus p~SzeiHETEcos(BTp)tr[𝕀E]eiHETE\tilde{p}S_{z}\otimes\mathrm{e}^{-iH_{E}T_{E}}\frac{\cos\left(BT_{p}\right)}{\text{tr}\left[\mathbb{I}_{E}\right]}\mathrm{e}^{iH_{E}T_{E}}. This scrambling step is skipped for the experiments of Fig. 2.

Finally we apply a last (π/2)y\left(\nicefrac{{\pi}}{{2}}\right)_{y}-pulse (Fig. 4, Sensor Initialization), and obtain when the scrambling time is included on the sequence

ρ0=p~SxeiHETEcos(BTp)tr[𝕀E]eiHETE.\rho_{0}=\tilde{p}S_{x}\otimes\mathrm{e}^{-iH_{E}T_{E}}\frac{\cos\left(BT_{p}\right)}{\text{tr}\left[\mathbb{I}_{E}\right]}\mathrm{e}^{iH_{E}T_{E}}\,.

This state is again separable, but it does not commute with the environment Hamiltonian, as [B,HE]0\left[B,H_{E}\right]\neq 0, and thus it is now in an out-of-equilibrium state that produces non-stationary noise fluctuations on the qubit-probe. Thus, we rewrite this as

ρ0=pSxρE,\rho_{0}=pS_{x}\otimes\rho_{E}\,,

where p=p~tr[cos(BTp)]tr[𝕀E]p=\tilde{p}\frac{\text{tr}\left[\cos\left(BT_{p}\right)\right]}{\text{tr}\left[\mathbb{I}_{E}\right]} is the initial qubit-probe polarization for the sensing process, and ρE=eiHETEcos(BTp)tr[cos(BTp)]eiHETE\rho_{E}=\mathrm{e}^{-iH_{E}T_{E}}\frac{\cos\left(BT_{p}\right)}{\text{tr}\left[\cos\left(BT_{p}\right)\right]}\mathrm{e}^{iH_{E}T_{E}} is the out-of-equilibrium environmental density matrix. In experiments of Fig. 2, without including the scrambling time, the environmental state is ρE=cos(BTp)tr[cos(BTp)]\rho_{E}=\frac{\cos\left(BT_{p}\right)}{\text{tr}\left[\cos\left(BT_{p}\right)\right]}. Again, since [B,HE]0\left[B,H_{E}\right]\neq 0 this state is nonstationary. This shows how the initial out-of-equilibrium state is prepared in our experiments.

The last step of the pulse sequence measures the SENSIT contrast. In our experiments, we applied the selective dynamical recoupling (SDR) sequence [40, 41], which is based on a dynamical decoupling sequences that is asymmetric under time-reversal, thus satisfying the requirements for obtaining nonzero SENSIT contrasts. Figure 4 shows the SDR implementation of the sequence in the SDR sequence block. We used 1212 pulses and a total sensing time of Ts=750μsT_{s}=750\mu\text{s} for the experiments of Fig. 2 and 3. To measure the SENSIT contrast we also applied the the time reversed version of SDR, the TSDR sequence, by reversing the order in which the pulses and delays are applied. The SDR sequence interpolates continuously a Hahn echo sequence of duration TsT_{s} with a CPMG sequence consisting of NN equidistant π\pi pulses between t=0t=0 and t=Tst=T_{s}. It consists of N1N-1 equidistant π\pi pulses between t=0t=0 and t=xTst=xT_{s} and a last π\pi pulse at x+12Ts\frac{x+1}{2}T_{s}. The dimensionless parameter xx of the sequence interpolates the sequence between the Hahn echo at x=0x=0 and the CPMG sequence of NN pulses at x=N1Nx=\frac{N-1}{N}. It can be interpreted as concatenating N1N-1 spin echoes of duration xN1Ts\frac{x}{N-1}T_{s}, and a last single spin echo of duration (1x)Ts(1-x)T_{s}. For the time-reversed version TSDR , one first applies the single spin echo of duration (1x)Ts(1-x)T_{s}, and then concatenates the N1N-1 spin echoes of duration xN1Ts\frac{x}{N-1}T_{s}. The two different sequences are shown side by side in Fig. 2 of the main text. Finally, the signal of the qubit-probe after the SDR and TSDR sequences is measured under CW decoupling being applied to the protons to increase the signal-to-noise ratio (Fig. 4, Qubit-Sensor Readout).

The SENSIT contrast vanishes for Tp=0T_{p}=0 as the system is in the state described in Eq. (A.18). As the preparation time TpT_{p} increases, the state is driven further away from equilibrium, leading to a growth in the nonstationary contributions to the cumulants. Therefore, a growth of the SENSIT contrast is expected with increasing TpT_{p} , as shown in Fig. 2c of the main text. If the scrambling time TET_{E} is included, we anticipate a decrease in the SENSIT contrast with increasing TET_{E}. This is because the local information about the nonstationary state becomes increasingly scrambled in nonlocal degrees of freedom that are not accessible from the sensor qubit. This phenomenon is shown in Fig. 3 of the main text.

G.3 Quantifying the number KK of correlated spins in the Environment due to initial state preparation

Refer to caption
Figure 5: Pulse sequence used to measure the number KK of environmental spins correlated to the qubit-sensor. First, cross polarization is used to initialize the system and increase the signal-to-noise ratio. Then, the 1010ms delay time ensures that all qubit-environment correlations and environmental initial state are erased due to T2T_{2} relaxation before further control. This is followed by a (π/2)y\left(\nicefrac{{\pi}}{{2}}\right)_{y} pulse, putting the qubit-probe state in plane. Then L0L_{0} cycles of the MREV-8 sequence are implemented to correlate the qubit-probe and the environment, as done when measuring the SENSIT contrast. After this, a (ϕ)x\left(\phi\right)_{x} pulse is applied on the environment to encode the formed correlations [46]. Then an time-reversal echo is created by means of a (π)y\left(\pi\right)_{-y} pulse on the qubit-probe followed by L0L_{0} cycles of the MREV-8 sequence to produce an effective backwards evolution. Finally the qubit-probe state is read out, while it is decoupled from the environment with continuous wave irradiation for improving the signal-to-noise ratio.

As we use the qubit-probe as a resource to create the out-of-equilibrium state in the environment, by driven correlations between the qubit and environmental spins, we measure the number of correlated environmental spins as a measure of the out-of-equilibrium degree. We use the method developed in [55] to measure the multiple-quantum coherence (MQC) spectrum of the density matrix state. Based on this approach the second moment of the MQC spectrum gives an out-of-time-order commutator KK that quantifies the number of correlated spins where the information was scrambled from a local probe [13, 43, 56, 46] . Given that the nonstationary state post-preparation arises from correlations established between the qubit-sensor and the environment, the out-of-time-order commutator KK serves as an indicator of the system’s distance from equilibrium.

To measure the number of correlated spins KK we begin with the same initialization as for the experiments to measure the SENSIT contrast: A cross polarization followed by a dephasing of correlations (see Fig. 5, Qubit-Sensor Initialization). We then correlate the qubit and the environment in the same way as done when measuring the SENSIT contrast: we apply a (π/2)y\left(\nicefrac{{\pi}}{{2}}\right)_{y} pulse to put the qubit-probe state in plane, then apply L0L_{0} cycles of the MREV-8 pulse sequence to create a state where the qubit-probe and environment are correlated (see Fig. 5, Sensor-Environment Correlation HSEH_{SE}). This creates the correlated state described in Eq. (A.19). We then apply a rotation pulse eiϕIx\mathrm{e}^{i\phi I_{x}} on the environment spins by an angle ϕ\phi around the xx direction. To then create a time-reversal echo, we apply a π\pi-pulse on the qubit-probe to effectively change the sign of the system-environment Hamiltonian that creates the correlations, and apply again the MREV-8 sequence during a time TpT_{p} (see Fig. 5, Sensor-Environment Backwards Propagation HSE-H_{SE}). This last step effectively creates a backward evolution to refocus the initial state. After that, a time reversal echo is created whose amplitude depends on ϕ\phi to allow encoding the number of correlated spins KK [13, 43, 56, 46]. Finally, the amplitude of the echo is measured, as shown in Fig. 5, Qubit-Sensor Readout.

The total evolution operator of this time reversal quantum evolution is thus Uecho=eiSzBTpeiϕIxeiSzBTpU_{\text{echo}}=\mathrm{e}^{iS_{z}BT_{p}}\mathrm{e}^{i\phi I_{x}}\mathrm{e}^{-iS_{z}BT_{p}}. The density matrix of Eq. (A.19) can be written as ρ(Tp)=MρM\rho(T_{p})=\sum_{M}\rho_{M}, where ρM\rho_{M} are the multiple.quantum coherence blocks of order MM, defined by the property eiϕIxρMeiϕIx=eiϕMρM\mathrm{e}^{i\phi I_{x}}\rho_{M}\mathrm{e}^{-i\phi I_{x}}=\mathrm{e}^{i\phi M}\rho_{M}. The effect of rotating the environmental spins around the xx axis thus adds a different phase to each coherence component ρM\rho_{M} of the density matrix, i.e. eiϕIxρ(Tp)eiϕIx=MeiϕMρM\mathrm{e}^{i\phi I_{x}}\rho(T_{p})\mathrm{e}^{-i\phi I_{x}}=\sum_{M}\mathrm{e}^{i\phi M}\rho_{M}. The measured echo is therefore

ρ0Uechoρ0Uecho=ρ(Tp)eiϕIxρ(Tp)eiϕIx=MeiϕMρMρM.\left\langle\rho_{0}U_{\text{echo}}\rho_{0}U_{\text{echo}}^{\dagger}\right\rangle=\left\langle\rho(T_{p})\mathrm{e}^{i\phi I_{x}}\rho(T_{p})\mathrm{e}^{-i\phi I_{x}}\right\rangle=\sum_{M}\mathrm{e}^{i\phi M}\left\langle\rho_{M}^{\dagger}\rho_{M}\right\rangle\,.

The dependence of this measured echo with respect to ϕ\phi encodes the MQC spectrum ρMρM\left\langle\rho_{M}^{\dagger}\rho_{M}\right\rangle, as they are multiplied by eiϕM\mathrm{e}^{i\phi M}. The Fourier transform of the echo signal with respect to the phase ϕ\phi is the MQC spectrum ρMρM\left\langle\rho_{M}^{\dagger}\rho_{M}\right\rangle. The effective number of correlated spins KK is determined from the width of the MQC spectrum, i.e. its second moment K=MM2ρMρM2MρMρM2=[ρ,Ix][ρ,Ix]K=\frac{\sum_{M}M^{2}\left\langle\rho_{M}^{\dagger}\rho_{M}\right\rangle^{2}}{\sum_{M}\left\langle\rho_{M}^{\dagger}\rho_{M}\right\rangle^{2}}=\left\langle\left[\rho,I_{x}\right]^{\dagger}\left[\rho,I_{x}\right]\right\rangle, where MρMρM=trρ2\sum_{M}\left\langle\rho_{M}^{\dagger}\rho_{M}\right\rangle=\text{tr}\rho^{2} is constant [13, 43, 56, 46]. The second moment KK quantifies the norm of the commutator between the localized initial state before the preparation time with the evolved density matrix after the preparation time [43, 56]. This thus determine a measure of distance to equilibrium based on the number of correlated spins. Notice that this state does not commute with the equilibrium state, thus relaxes to equilibrium during the scrambling time.

References

  • [1] [Awschalom, Hanson, Wrachtrup, and Zhou]D. D. Awschalom, R. Hanson, J. Wrachtrup,  and B. B. Zhou, Nat. Photonics 12, 516 (2018).
  • Acín et al. [2018] A. Acín, I. Bloch, H. Buhrman, T. Calarco, C. Eichler, J. Eisert, D. Esteve, N. Gisin, S. J. Glaser, F. Jelezko, S. Kuhr, M. Lewenstein, M. F. Riedel, P. O. Schmidt, R. Thew, A. Wallraff, I. Walmsley,  and F. K. Wilhelm, New J. Phys. 20, 080201 (2018).
  • Pelucchi et al. [2022] E. Pelucchi, G. Fagas, I. Aharonovich, D. Englund, E. Figueroa, Q. Gong, H. Hannes, J. Liu, C.-Y. Lu, N. Matsuda, J.-W. Pan, F. Schreck, F. Sciarrino, C. Silberhorn, J. Wang,  and K. D. Jöns, Nat. Rev. Phys. 4, 194 (2022).
  • Suter and Álvarez [2016] D. Suter and G. A. Álvarez, Rev. Mod. Phys. 88, 041001 (2016).
  • Degen et al. [2017] C. L. Degen, F. Reinhard,  and P. Cappellaro, Rev. Mod. Phys. 89, 035002 (2017).
  • Aslam et al. [2023] N. Aslam, H. Zhou, E. K. Urbach, M. J. Turner, R. L. Walsworth, M. D. Lukin,  and H. Park, Nat. Rev. Phys. 5, 157 (2023).
  • Zwick and Álvarez [2023] A. Zwick and G. A. Álvarez, Journal of Magnetic Resonance Open 16-17, 100113 (2023).
  • Barry et al. [2016] J. F. Barry, M. J. Turner, J. M. Schloss, D. R. Glenn, Y. Song, M. D. Lukin, H. Park,  and R. L. Walsworth, PNAS 113, 14133 (2016).
  • Nie et al. [2021] L. Nie, A. C. Nusantara, V. G. Damle, R. Sharmin, E. P. P. Evans, S. R. Hemelaar, K. J. van der Laan, R. Li, F. P. Perona Martinez, T. Vedelaar, M. Chipaux,  and R. Schirhagl, Sci. Adv. 7 (2021).
  • Lovchinsky et al. [2016] I. Lovchinsky, A. O. Sushkov, E. Urbach, N. P. de Leon, S. Choi, K. De Greve, R. Evans, R. Gertner, E. Bersin, C. Muller, L. McGuinness, F. Jelezko, R. L. Walsworth, H. Park,  and M. D. Lukin, Science 351, 836 (2016).
  • Schlipf et al. [2017] L. Schlipf, T. Oeckinghaus, K. Xu, D. B. R. Dasari, A. Zappe, F. F. de Oliveira, B. Kern, M. Azarkh, M. Drescher, M. Ternes, K. Kern, J. Wrachtrup,  and A. Finkler, Science Advances 3, e1701116 (2017).
  • Neumann et al. [2013] P. Neumann, I. Jakobi, F. Dolde, C. Burk, R. Reuter, G. Waldherr, J. Honert, T. Wolf, A. Brunner, J. H. Shim, D. Suter, H. Sumiya, J. Isoya,  and J. Wrachtrup, Nano Lett. 13, 2738 (2013).
  • Álvarez et al. [2015] G. A. Álvarez, D. Suter,  and R. Kaiser, Science 349, 846 (2015).
  • Buča et al. [2019] B. Buča, J. Tindall,  and D. Jaksch, Nat. Commun. 10, 1730 (2019).
  • Lewis-Swan et al. [2019] R. J. Lewis-Swan, A. Safavi-Naini, A. M. Kaufman,  and A. M. Rey, Nat. Rev. Phys. 1, 627 (2019).
  • Landsman et al. [2019] K. A. Landsman, C. Figgatt, T. Schuster, N. M. Linke, B. Yoshida, N. Y. Yao,  and C. Monroe, Nature 567, 61 (2019).
  • Chalermpusitarak et al. [2021] T. Chalermpusitarak, B. Tonekaboni, Y. Wang, L. M. Norris, L. Viola,  and G. A. Paz-Silva, PRX Quantum 2, 030315 (2021).
  • Kuffer et al. [2022] M. Kuffer, A. Zwick,  and G. A. Álvarez, PRX Quantum 3, 020321 (2022).
  • Kotler et al. [2013] S. Kotler, N. Akerman, Y. Glickman,  and R. Ozeri, Phys. Rev. Lett. 110, 110503 (2013).
  • Norris et al. [2016] L. M. Norris, G. A. Paz-Silva,  and L. Viola, Phys. Rev. Lett. 116, 150503 (2016).
  • Sung et al. [2019] Y. Sung, F. Beaudoin, L. M. Norris, F. Yan, D. K. Kim, J. Y. Qiu, U. von Lüpke, J. L. Yoder, T. P. Orlando, S. Gustavsson, L. Viola,  and W. D. Oliver, Nat. Commun. 10, 3715 (2019).
  • Wang et al. [2019] P. Wang, C. Chen, X. Peng, J. Wrachtrup,  and R.-B. Liu, Phys. Rev. Lett. 123, 050603 (2019).
  • Wang and Clerk [2020] Y.-X. Wang and A. A. Clerk, Phys. Rev. Res. 2, 033196 (2020).
  • Wang and Clerk [2021] Y.-X. Wang and A. A. Clerk, Nat. Commun. 12, 6528 (2021).
  • Jerger et al. [2023] P. C. Jerger, Y.-X. Wang, M. Onizhuk, B. S. Soloway, M. T. Solomon, C. Egerstrom, F. J. Heremans, G. Galli, A. A. Clerk,  and D. D. Awschalom, PRX Quantum 4, 040315 (2023).
  • Álvarez and Suter [2011] G. A. Álvarez and D. Suter, Phys. Rev. Lett. 107, 230501 (2011).
  • Bylander et al. [2011] J. Bylander, S. Gustavsson, F. Yan, F. Yoshihara, K. Harrabi, G. Fitch, D. G. Cory, Y. Nakamura, J. Tsai,  and W. D. Oliver, Nat. Phys. 7, 565 (2011).
  • Romach et al. [2015] Y. Romach, C. Müller, T. Unden, L. J. Rogers, T. Isoda, K. M. Itoh, M. Markham, A. Stacey, J. Meijer, S. Pezzagna, B. Naydenov, L. P. McGuinness, N. Bar-Gill,  and F. Jelezko, Phys. Rev. Lett. 114, 017601 (2015).
  • Schmid-Lorch et al. [2015] D. Schmid-Lorch, T. Häberle, F. Reinhard, A. Zappe, M. Slota, L. Bogani, A. Finkler,  and J. Wrachtrup, Nano. Lett. 15, 4942 (2015).
  • Ma et al. [2014] W.-L. Ma, G. Wolfowicz, N. Zhao, S.-S. Li, J. J. L. Morton,  and R.-B. Liu, Nat. Commun. 5, 4822 (2014).
  • Connors et al. [2022] E. J. Connors, J. Nelson, L. F. Edge,  and J. M. Nichol, Nat. Commun. 13, 940 (2022).
  • Muhonen et al. [2014] J. T. Muhonen, J. P. Dehollain, A. Laucht, F. E. Hudson, R. Kalra, T. Sekiguchi, K. M. Itoh, D. N. Jamieson, J. C. McCallum, A. S. Dzurak,  and A. Morello, Nat. Nanotechnol. 9, 986 (2014).
  • Frey et al. [2017] V. M. Frey, S. Mavadia, L. M. Norris, W. de Ferranti, D. Lucarelli, L. Viola,  and M. J. Biercuk, Nat. Commun. 8, 2189 (2017).
  • Viola et al. [1999] L. Viola, E. Knill,  and S. Lloyd, Phys. Rev. Lett. 82, 2417 (1999).
  • Sagi et al. [2010] Y. Sagi, I. Almog,  and N. Davidson, Phys. Rev. Lett. 105, 053201 (2010).
  • Malinowski et al. [2017] F. K. Malinowski, F. Martins, Ł. Cywiński, M. S. Rudner, P. D. Nissen, S. Fallahi, G. C. Gardner, M. J. Manfra, C. M. Marcus,  and F. Kuemmeth, Phys. Rev. Lett. 118, 177702 (2017).
  • Lange et al. [2010] G. d. Lange, Z. H. Wang, D. Ristè, V. V. Dobrovitski,  and R. Hanson, Science 330, 60 (2010).
  • Bernevig and Hughes [2013] B. A. Bernevig and T. L. Hughes, Topological Insulators and Topological Superconductors (Princeton University Press, 2013).
  • Nakajima et al. [2019] T. Nakajima, A. Noiri, J. Yoneda, M. R. Delbecq, P. Stano, T. Otsuka, K. Takeda, S. Amaha, G. Allison, K. Kawasaki, A. Ludwig, A. D. Wieck, D. Loss,  and S. Tarucha, Nat. Nanotechnol. 14, 555 (2019).
  • Smith et al. [2012] P. E. S. Smith, G. Bensky, G. A. Álvarez, G. Kurizki,  and L. Frydman, PNAS 109, 5958 (2012).
  • Álvarez et al. [2013] G. A. Álvarez, N. Shemesh,  and L. Frydman, Phys. Rev. Lett. 111, 080404 (2013).
  • Xu and Swingle [2024] S. Xu and B. Swingle, PRX Quantum 5, 010201 (2024).
  • Domínguez et al. [2021] F. D. Domínguez, M. C. Rodríguez, R. Kaiser, D. Suter,  and G. A. Álvarez, Phys. Rev. A 104, 012402 (2021).
  • Li et al. [2017] J. Li, R. Fan, H. Wang, B. Ye, B. Zeng, H. Zhai, X. Peng,  and J. Du, Phys. Rev. X 7, 031011 (2017).
  • Gärttner et al. [2018] M. Gärttner, P. Hauke,  and A. M. Rey, Phys. Rev. Lett. 120, 040402 (2018).
  • Niknam et al. [2020] M. Niknam, L. F. Santos,  and D. G. Cory, Phys. Rev. Res. 2, 013200 (2020).
  • Li et al. [2024] S. Li, L. Lu, S. Bhattacharyya, C. Pearce, K. Li, E. T. Nienhuis, G. Doumy, R. D. Schaller, S. Moeller, M.-F. Lin, G. Dakovski, D. J. Hoffman, D. Garratt, K. A. Larsen, J. D. Koralek, C. Y. Hampton, D. Cesar, J. Duris, Z. Zhang, N. Sudar, J. P. Cryan, A. Marinelli, X. Li, L. Inhester, R. Santra,  and L. Young, Science 383, 1118 (2024).
  • Greilich et al. [2024] A. Greilich, N. E. Kopteva, A. N. Kamenskii, P. S. Sokolov, V. L. Korenev,  and M. Bayer, Nat. Phys. , 1 (2024).
  • Sridhar et al. [2024] S. K. Sridhar, S. Ghosh, D. Srinivasan, A. R. Miller,  and A. Dutt, Nat. Phys. , 1 (2024).
  • Shimasaki et al. [2024] T. Shimasaki, M. Prichard, H. E. Kondakci, J. E. Pagett, Y. Bai, P. Dotti, A. Cao, A. R. Dardia, T.-C. Lu, T. Grover,  and D. M. Weld, Nat. Phys. 20, 409 (2024).
  • van Kampen [1992] N. G. van Kampen, Stochastic Processes in Physics and Chemistry (Elsevier Science Publishers, Amsterdam, 1992).
  • Slichter [1996] C. Slichter, Principles of Magnetic Resonance (Springer Berlin Heidelberg, Berlin, Heidelberg, 1996).
  • Abragam [1983] A. Abragam, Principles of Nuclear Magnetism, International Series of Monographs on Physics (Oxford University Press, Oxford, New York, 1983).
  • Rhim et al. [1973] W. K. Rhim, D. D. Elleman,  and R. W. Vaughan, J. Chem. Phys. 58, 1772 (1973).
  • Baum et al. [1985] J. Baum, M. Munowitz, A. N. Garroway,  and A. Pines, J. Chem. Phys. 83, 2015 (1985).
  • Domínguez and Álvarez [2021] F. D. Domínguez and G. A. Álvarez, Phys. Rev. A 104, 062406 (2021).