Broadband spectroscopy of quantum noise
Abstract
Characterizing noise is key to the optimal control of the quantum system it affects. Using a single-qubit probe and appropriate sequences of and non- pulses, we show how one can characterize the noise a quantum bath generates across a wide range of frequencies – including frequencies below the limit set by the probe’s time. To do so we leverage an exact expression for the dynamics of the probe in the presence of non- pulses, and a general inequality between the symmetric (classical) and anti-symmetric (quantum) components of the noise spectrum generated by a Gaussian bath. Simulation demonstrates the effectiveness of our method.
I Introduction
Characterizing noise is key not only to the implementation of high fidelity operations in quantum devices, but to enable detailed understanding of the physical processes inducing such noise [1, 2]. Protocols capable of providing such information infer it from the measured response of a quantum system to probing control (which need not be unitary) in the presence of the noise one desires to characterize. Depending on the purpose and control capabilities, different protocols can be used, mostly under the term quantum noise spectroscopy (QNS). For example, relatively costly frequency comb-based [3] or Slepian control [4] protocols can in principle sample frequency-domain representations of the noise correlations in high detail, while [5] reconstructs a large frequency regime of the spectrum. Efficient frame-based protocols [6, 7] extract only the relevant information necessary to control the system given fixed control constraints/capabilities. Others can provide information not on noise correlations, but rather a description of the process tensor describing the open system dynamics [8].
Generally speaking, such protocols are perturbative in nature, in the sense that they rely on the perturbative expansion of the time-dependent behaviour of expectation values, typically as a function of the leading-order bath correlation functions111Process tensor methods are in general not perturbative, but their complexity grows exponentially with the number of interventions – roughly speaking the “complexity of the control”. Tractable process tensor approaches rely on perturbative-like approximations based on other criteria which we will not consider here.. This results in either increasingly more complex and costly implementations, or less accurate/reliable reconstructions. Indeed, under certain conditions, protocols that provide a qualitative – rather than quantitative – description of classical and quantum noise have been recently proposed [9, 10, 11]. That is, they are essentially applicable to systems where the noise-inducing environment is weakly coupled to the system of interest. While this can be a reasonable assumption for systems where the weak coupling is a necessity and has been in a sense hard-coded in its physical description and design, e.g. for quantum computing purposes, it may not be for a general system where a strong system-bath coupling regime is of interest, e.g., for sensing if the environment is the object of interest or in the road to designing a low noise physical system.
A notable exception to this is when the physical model of interest admits an exact solution in the presence of the probing control. In such cases, no weak coupling assumption is necessary, allowing one, in principle, to study the problem in typically inaccessible regimes, e.g., in the long-time regime. This, in turn, implies the ability to study the noise in great detail. Particularly relevant to this paper, this allows one to analyze the effect of very low frequency noise [12], which is inherently difficult for methods relying on perturbative expansions and thus on “total evolution time”-bounded experiments. This is of interest beyond the full characterization scenario, for example opening the possibility to wide-range bath thermometry, which would not be possible otherwise.
In practice, however, few exactly solvable models are known. Prominent among these is the case of dephasing Gaussian noise in the presence of instantaneous -pulse control [13, 15, 14] – described in detail in Eq. (1). The drawback of this model is that some components of the noise do not contribute to the -pulse-modulated dynamics and are thus invisible to the system qubit. Indeed, one can show that only the symmetric component of the bath correlations, i.e., the classical component (dubbed in this paper), contribute, while the antisymmetric, i.e., the quantum component (dubbed ), disappear from the equations. In other words, in the above scenario the quantum nature of the bath is invisible. And yet, it not only would contribute when more general control is applied, but also contains highly coveted information about the physical source of such noise. It is worth highlighting in view of recent results that the above is true for the common type of coupling we will use here – see Ref. [15] for more exotic coupling types whose dynamics reveals the presence of the antisymmetric component of the bath correlations – and under the assumption that the bath state at initialization (time zero) is independent of the system state, i.e., an initialization procedure can prepare for a set of but fixed When the latter is not the case [10], the resulting effective model can be mapped to one of the exotic couplings mentioned, and thus depends on the quantum component of the noise.
In this paper, we show how one can leverage non- pulses to extract information about the quantum component of the noise while using non-perturbative equations for the dynamics. In addition to the existing capabilities granted by -pulse-only control, the new paradigm allows us to study both classical and quantum components in the elusive strong coupling, long evolution time regime. Further, we propose a systematic method to selectively reconstruct any frequency range of interest of the noise spectra based on the observed single-qubit reduced dynamics. Moreover, we establish a novel inequality bounding the strength of the quantum spectrum by the classical counterpart, which for the first time clarifies the relationship between the two spectra.
The structure of this paper is as follows. Sec. II summarizes the basic model, motivation and results of this paper. Sec. III derives and analyzes the exact solution for the reduced qubit dynamics in the time domain. Sec. IV moves to the frequency domain and presents a systematic method reconstructing the and spectra, together with a novel inequality characterizing their quantitative relationship. Sec. V provides simulation results to validate our spectra reconstruction algorithm. Conclusions are presented in Sec. VI.
II Key elements and results
Let us start by summarizing some of the key elements and results in this paper, while leaving the derivations to the later sections.
We consider a controlled single qubit probe dephasingly coupled to an uncontrollable bath . In the interaction picture associated with the bath Hamiltonian , the joint system-bath dynamics is governed by a Hamiltonian of the form
(1) |
where is a bath operator and is the control Hamiltonian.
The and the initial state of the bath are assumed to lead to noise that is zero-mean, Gaussian and stationary. That is, noise which is entirely described by the second-order cumulant, i.e., , where the expectation includes both the classical ensemble average and the quantum expectation . A paradigmatic example of this noise is the one generated by a bosonic bath, where is linear in the creation and annihilation operators and is a thermal state with inverse temperature .
We will further assume that the control Hamiltonian is capable of implementing instantaneous rotations around a given axis – here for concreteness. We will assume a minimum time of between pulses and control time resolution , i.e., if the position of the -th pulse is denoted by , then and for integers . Since , we must have . Since the action of -pulses preserves the dephasing character of the Hamiltonian, it will be useful to divide the control Hamiltonian into a part that solely executes -pulses and the complement, i.e. In this way, introducing the propagator , the interaction picture Hamiltonian with respect to (i.e., the “toggling frame”) yields
(2) |
where is the so-called “switching function” taking values . The non- pulses play a dual purpose in our protocol. First, as is common in Ramsey-type experiments, as a way to prepare the initial state. Second, and more importantly for this paper, to break the dephasing symmetry in the toggling-frame Hamiltonian.
Under these conditions, one can show (see Sec. III for details) that the exact dynamics of the qubit at time depends on the integrals
where we have used the short-hand notation , with , to denote the classical (+) and quantum (-) components of the cumulants describing the noise statistics. We will refer to their Fourier transform as the and spectra. Additionally, here the are user-defined switching functions taking values in that satisfy what we dub the incompatibility condition, namely
(3) |
II.1 Consequences of dephasing-preserving control
Since a key ingredient of our scheme is breaking the dephasing preserving symmetry, it is worth understanding some of the constraints that arise due to such strong symmetry:
(i) The qubit is insensitive to the component of the noise.- In the dephasing-preserving scenario one finds that and so that and
i.e., only the classical component of the bath contributes to the dynamics. This can be overcome in at least two ways: using multiple qubits or using non dephasing-preserving control. The former implies a considerable increase in physical resources and control complexity, e.g., entangled probes or entangling operations, but has the distinct advantage of admitting exact equations [15], while the latter can no longer be studied via exact equations and thus is limited to short-time/weak-coupling [16] or steady state [9] regimes.
This limitation in turn implies the inability to extract the information encoded in the spectra or in the relationship between the and spectra, such as the temperature of the thermal bath in the bosonic bath case.
(ii) The noise frequency which can be sampled is effectively lower bounded.- Even if one is only interested in the spectrum, the dephasing-preserving scenario leads to sampling limitations. To see this, let us expand the (stationary) correlation function in Fourier series so that
(4) |
for some small frequency resolution . Extracting the “low frequency” information implies the need to learn for . Even more, assume the values of for and the function value of from up to some are known. The problem is then to generate a system of (linear) equations out of Eq. (4) from which the unknown can be reliably estimated.
Analysing the relative difference between the “coefficients” associated to and i.e., the corresponding cosines, one finds that for small
This shows that differentiating between two subsequent s becomes harder the smaller and are, unless can be made large, say
On the other hand, the contribution of to the dynamics is contained in an integral like , for some small , mixed with the full history of the probe . Indeed, measuring the expectation value of at a time given an initial state (the eigenstate of corresponding to ) leads to
i.e., the signal associated to is obscured by the decay from the history of the dynamics and its contribution is thus harder to discriminate experimentally the larger – the smaller the target frequency range – is.
Additionally, the inability to accurately and broadbandly sample also implies the inability to extract reliable information about physical parameters which lie within certain ranges. For example, characterizing low bath temperatures (high regime) in the bosonic example we alluded to earlier becomes impractical.
II.2 Beyond dephasing-preserving control
Overcoming these limitations will be the main contribution of this work, and we will do so by exploiting the ability to generate effective switching functions with zero values in set domains.
One way to do so, is to use incoherent mechanisms. This was done for the purely classical bath scenario in [17, 18, 19], by interleaving blocks of preparation, noisy evolution and measurement, with idle periods. Importantly, in this idle periods the qubit effectively does not interact with the bath or rather the effect of the noise on the qubit during those idle periods is deleted in the preparation of the following block. In this way, these protocols eventually allow one to sample the low frequency region of the (classical) noise spectrum.
In the quantum bath scenario, however, the situation is different. While a preparation would indeed delete the effect of the bath on the probe qubit, the opposite is not true. The presence of the qubit influences the bath, and the final expectation values will reflect this.
To overcome this limitation we propose to use instead coherent control and a detailed analysis of the system evolution in the presence of the quantum bath. That is, we exploit instead of sequential measurements. WE observe that when control is not dephasing-preserving need not vanish, and take values in This allows one to build combinations of expectation values of operators which are only sensitive to part of the history, in the sense that they only depend on integrals of the form
for useful (but not quite arbitrary) values of and In other words, even in the quantum bath scenario, our protocol allows combinations of expectation values which yield quantities that mimic the ’idle’ behaviour in the protocols mentioned earlier. Section III focuses on deriving this result and on showing how these integrals can be isolated by appropriate combinations of observables, control sequences, and initial states. Importantly, we shall show how to do so exactly, i.e., without invoking any approximation, allowing us to characterize the effect of both and baths in a quantitatively accurate way, in contrast with recent results [11].
With this ability in hand, we achieve broadband characterization of the noise (both and components), i.e., even in the long-time & strong-coupling regime. In particular, we demonstrate how this ability allows us to characterize the very low frequency range of both the and spectra of a general stationary Gaussian bath – below the one set by the time of the probe.
III Time-domain derivation
III.1 Reduced qubit dynamics
While moving away from the dephasing-preserving scenario is desirable from the point of view of allowing the qubit to be sensitive to more features of the bath, a considerable complication is added to the analysis: the ability to write exact analytical expressions for the response of the qubit to control and the noise is lost (or at the very least severely compromised). This leads to the need for perturbative approaches, which in turn restrict the ability to extract information which is encoded in the long-time behaviour of the qubit, e.g., low frequency features of the noise. In terms of going beyond -pulses, for example, Ref. [20] proposed a protocol non-trivially employing non- pulses to reconstruct a spectrum with a simplified structure, which leverages many approximations in the deduction, but does not develop a systematic general solution. To overcome these sort of complications, we derive an exact solution for the reduced qubit dynamics subject to general non- pulses, laying a foundation for resolving both the and spectra. While the scaling of the complexity of the solution – which may be of independent interest222The expression derived here can be related to the process tensor approach [21] . This is an avenue that we will explore in a latter work. – is exponential in the number of non- pulses being considered and is thus impractical in many scenarios of interest, only a few non- pulses are necessary to achieve the results in this work.
Let us start by denoting . Let the non- pulse control implement angle pulse at , where and are the preparation and measurement times, respectively. They generate unitaries which can be generically written as with the constraint . Concretely, the coefficients are related to the rotation angle via for the unitary control we consider here333Notice that the decomposition can be made also if the operations/interventions are not unitary, e.g., measurements or projectors, albeit with a different constraints for the .. Dividing the full-time propagator into time intervals defined by the non- pulse timings, one obtains
(5) |
with and . The summation in Eq. (5) ranges over all the combinations of , and for the last line we define
In our protocols, it will be sufficient to work with up to four non- pulses ( in the above equations).
Any information we extract from the system comes in the form of system measurements. The expectation value of a system-only operator is given by , where . Furthermore, the system operator can be calculated, by considering with and introducing the shorthand notation where , as
(6) | |||
from which we see that the quantity of interest contains the information about how the noise interacts which the unitaries associated to each
The crucial observation is that each of the can be written in terms of an effective dephasing Hamiltonian. Thus, given the Gaussian bath scenario we are considering, one can write an exact expression for each of them using the cumulant expansion technique [22, 23, 15, 16]. In more detail, can be written in a time-ordered exponential form
(7) | ||||
In the first equality, we have used the effective Hamiltonian
with the piece-wise function
(8) |
which results from using the configuration vector to modulate the original switching function . In turn, to reach the second equality of (7) we exploit the Gaussian character of the noise so that the cumulant expansion truncates exactly at order two. The two contributing cumulants (see Appendix A),
(9) |
and
(10) | ||||
can be compactly written in terms of the effective switching functions
(11) |
Since it will be enough for our purpose to use as observables or we can set and thus drop the superscript in , and below. Notice that because the non-vanishing cumulant is proportional to , the qubit’s reduced dynamics is in essence a linear combination of the functions
(12) |
with the specific linear coefficients depending on and the control. Note that is purely imaginary, and we write it as above to emphasize the imaginary character of the exponential associated to it. In the same vein, is a real quantity. The above implies that noise generates decoherence, while noise is in charge of generating a phase in our expectation values. Notice that the periodic character of the complex exponential will complicate the task of inferring information about the component of the noise. We will call this the multi-value problem and show it can be overcome via a proper analysis in Section IV.4.2.
These equations encode the key ingredient of our result: the use of non- control in principle enables us to access functions which depend on integrals (i) containing effective switching functions with zeros, i.e., as if the coupling could be effectively and exactly switched off during in a portion of the evolution, and, (ii) in the case of the contribution, containing two different switching functions, allowing us to exploit their constructive/destructive interference effects for noise characterization.
Before proceeding to show how the can be isolated, and how useful doing this is, it will be convenient to explore the structure of the integrals involved.
III.2 Properties of the effective switching functions and consequences
Let us first note that from the definition of one has
and
We dub this the incompatibility condition, as it implies that at any time while That is, it cannot be that both effective switching functions vanish or are non-zero simultaneously.
This suggests that to keep track of the effect of non- pulses it is enough to track the vanishing/non-vanishing character of in each interval. This follows from the observation that we can propose the representation
where is a purely -pulse generated switching function, which suggests that multiple configurations can lead to the same This multiplicity follows from the fact that while pulses define , they can also implement a transformation with i.e., they can change the sign but not the vanishing/non-vanishing character of in a given time interval. Concretely, a pair of pulses at and would enforce and . Clearly, this can also be interpreted as a change in , but thinking of it as a transformation of is useful for our purposes. Considering , for example, one can achieve a partial inversion of the ’s by applying extra pulses at so that while . More over a full inversion, implementing and , can be executed by applying pulses at . Similar arguments follow for any .
The usefulness of this “gauge-free” representation becomes apparent when one considers the effect of switching functions on integration domains and, in turn, of the One can rewrite a given integral in terms of the by making the association with
Note we have dropped the superscript to avoid cumbersome notation, since in what follows we will specialize to .
Furthermore, let us note that is invariant under a full inversion, namely On the other hand, the time-ordered character of implies that
Notice that the above also implies that the integrals of the form do not contribute to the probe dynamics, and are thus in principle not learnable. This does not imply, however, that does not contribute to the dynamics. In fact, is in principle learnable for any
Finally, as with the dynamical integrals, the representation where
allows us to make explicit the different ways in which and noise influence the dynamics. Namely, noise induces decay via , while noise induces a phase via
For exposition purposes, we will often represent the former as where the makes explicit the symmetry with respect to the diagonal , and the latter by where now the makes explicit the time ordering in the relevant integral and the matrix form facilitates keeping track of the generated equivalence between different vector pairs of . We will say that is a function of the integral
Our task will be to infer the value of for all those configurations such that and i.e., where only one of the matrix entries is non-vanishing (for , two entries are non-zero, one of which is hidden among the dots).
III.3 Extractable information
To achieve this, one must first determine which among (or linear combinations of them) can be extracted via linear combinations of expectation values. Let us first recall one is interested in expectation values of after applying a set of pulses of angles at times We denote the explicit pulse dependence by From Eq. (6), one sees that each of these expectation values can be written as a sum of terms – each containing a specific linear combination of ’s – with coefficients of the form for This is a linear system which can be solved by cycling over an appropriate set of angles for any , e.g., for there are 81 configurations resulting from cycling , which yields the aforementioned linear combinations of interest444Note that this is a raw recipe but later we will be interested in minimizing the number of experiments, i.e., the number of configuration sets , needed to extract a given expectation value.. Building a linear system using for and one finds that the 81 linear combinations reduce to 18 quantities that can now be accessed. Namely,
involving both and spectra, and those in the set for involving only the noise contribution. Also note that
are always zero and thus do not need to be learned.
III.4 Inferrable information
Inferring the values of the various integrals requires combining the accessible quantities in a non-linear way, by exploiting the fact that
and
With this in hand, one can for example start by combining and to achieve
This provides the knowledge of and which can in turn be leveraged in to infer Further, since one has that
and and are known, one can then also infer
Then, using and one finds that
which not only makes superfluous, but gives us access to the integrals and consequently to . The final step is to realize that
which completes the picture. That is, one can infer the value (up to a multiple of in the quantum case) of integrals of the form
where and .
III.4.1 The multivalue problem
An important caveat in the above argument is that, as highlighted, the and spectra appear in two different ways. Importantly, the latter appears within a periodic function. This is specially significant in our scenario as we want to be able to study the strong coupling regime. Thus, it need not be that the relevant integrals have values within the first period of or functions. In other words, one can only estimate modulo . If the noise is weak such that one can assume this is not a problem. In the general strong coupling regime this represents a considerable obstacle to the accurate characterization of the component of the noise. For now, we shall assume that the problem can be solved, and will indeed provide a solution later on when all the necessary tools have been deployed.
III.5 The power of control and stationarity considerations
Stationarity has a considerable effect in what sort of integrals can be learned. To explore it let us first note that
holds for any , provided that This implies that can be reduced to an integral like
(13) |
for provided suitable -pulse configurations have been chosen. Given fixed , however, it would seem that the value of – thought of as a function of – cannot be directly accessed. This apparent limitation can be overcome by combining information from different experimental configurations.
To see this, let us consider the situation where each and is zero or greater than . Then, one can access the value of using the scheme in Fig. 1, where the pulses form a Hahn Echo filter while other pulse sequences are also allowed. Notice that depending on the / spectra, one must be aware of the incompatibility condition. One starts then by implementing an experiment granting access to with and , which corresponds to the green shaded region of the integral. Additionally, non- pulses at and give us access to , the orange region. Then importantly, one can perform a carefully-designed experiment to indirectly infer the value of , the red region, with two such examples provided in Fig. 1. Finally, adding up the integral values of the three colored regions, one obtains the value of as desired.
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Reaching the control limit.- Control constraints naturally impose a limit to what information can be learnt. In the presence of a minimum switching time the above argument shows one can access information about for with the difference between any two pulse timings being or not smaller than In particular, one is able to infer the value of for . Notice that this can be done in a history-independent way by applying our basic three-interval setup using The argument can obviously be extended to any grid size larger than , provided it is an integer multiple of
Control can take us further, if one is willing to pay the cost. The previous set up required a small number of experiments to infer or any appropriate for that matter. Using experiments scaling with however, one can infer values of limited by the time solution

Starting form the previous result, consider now the integrals
with and the subscript denoting the scenario where (Thus ), corresponding to the blue and red squares in Fig. 2. By subtracting them, one can infer the value of an “angle” strip (the green enclosed region). One can then build another such “angle” strip (the orange region) with and , so that the difference between the “angles” is the yellow square for i.e., the average of over a integration domain. Taking this to the extreme, one can in principle infer integrals of the form for any positive integer . We stress that the lower bound on comes from the minimum switching time, as it also implies a minimum measurement time Notice, that if the lower bound on the measurement time is not present, then there is no lower bound on above.
Since any integral can be reconstructed by an appropriate linear combination of this represents the most detailed information that can be inferred using the declared control constraints. While access to such detailed information can undoubtedly be very useful, its acquisition may not be practical. This is specially true if in addition to counting raw resources, e.g,. number of necessary experimental configurations, one also considers extra experimental limitations, such as measurement and finite-sampling errors. Thus, here we will use this full-access reconstruction as a benchmark to our more cost-effective, but less detailed, reconstruction protocols, and will leave its detailed analysis for future work.
III.6 Overcoming limitations
The result in the previous section allows us to overcome the limitations associated to dephasing-preserving control (assuming for now the multivalue problem is solved).
(i) The component of the noise can be sampled, in a manner that is weakly dependent on the component. Consider, for example, the ability to access
via a linear combination of expectation values. Notice that the contribution of the noise is restricted to the domain and thus the component does not depend on the history of the contribution before . This is important, as one can now make and in principle arbitrarily large, while maintaining fixed, i.e., maintaining the “damping” of the signal due to the noise contribution restricted.
This can be taken farther by assuming that control for is such that While this limit is not physically achievable, in principle a sufficiently powerful error suppression mechanism like dynamical decoupling can make the integral small. A similar argument has been considered in [11]. We highlight, however, that the validity of this simplification depends on being well matched to the mechanism being used, e.g., DD requires that the noise is mostly low frequency to be effective. Without a prior knowledge of or relevant assumptions in place, this is an oversimplification which will eventually reduce us to seek qualitatively correct [11] – rather than quantitatively accurate – estimations of We will not make such approximations in this paper to maintain generality and access to the full information provided by the probe’s dynamics.
(ii) There is in principle no lower bound to the frequency that can be sampled. Combining our ability to infer the different integrals, one has now the ability to infer the value of as (13), which allows us to obtain knowledge of for , without significant concerns for the history of dynamics, as was the case in the dephasing-preserving control scenario. This is a direct consequence of the weak dependence of the accessible quantities, i.e., one can access simple quantities involving the / component with only a weak dependence on the / component. We stress that weak does not mean non-existent, and the codependence will impact – if in a relatively minor and controllable way – our ability to accurately extract noise correlation information, as we will see in the next section.
III.7 Specific measurement equations
The deduction in Sec. III.4 demonstrates the existence of a systematic method to infer the knowledge of the integral values from the observed expectation values. However, the specific initial states and observables are not listed and the equations therein might not always be the most efficient, if considering to minimize the number of experimental configuration sets needed. Hence, here we list alternative full equations showing how to extract information efficiently. In this subsection, and are nonexistent and pulses are only applied at , denote , is simplified as where , and we take unless otherwise specified. We also employ stationarity to reduce the number of integral values of interest. For example, having access to suffices to infer the values of and .
(i) The elements in can be accessed from
(14) |
Also, using stationarity, the value of equals to the result of an experiment of
(15) |
which will be used later for other purposes.
(ii) To access , intervals suffice and we have
(16) |
In practice, one can first consume a small number of state copies to roughly estimate which one of in (16) is larger, and then only employ the corresponding equation. Through (14), one knows the value of , and finally can infer .
(iii) To access such that the low-frequency information of -component can be extracted, we first denote
(17) | ||||
(18) |
Then after collecting the values of , we can deduce from
(19) |
(iv) To access , we notice that
(20) |
(21) |
Note that Eq. (15) gives the value of , which after input to Eq. (21) leads to .
Close to the end of Sec. III.1, we have pointed out that noise introduces a phase to the observable expectation value and induces no decoherence, in sharp contrast with noise. Despite this, to estimate the low-frequency information of noise, it is still necessary to generate zero-value filter functions to avoid decoherence resulting from noise, considering that noise always accompanies the appearance of noise (while the contrary is not true), as exemplified by in Eq. (20). The advantage of Eqs. (22) and (23) is that, when is forced to be large in order to probe the long-time correlation of noise, the RHSs do not decohere, so long as is not overlarge.
IV Frequency-domain analysis
The previous sections equipped us with access to the fundamental integral values of the correlation functions in the time domain. As is common in signal processing, here we move to the frequency domain to complete our analysis. We expect to gain two things from this: (i) further insight on the noise structure, and (ii) a way to achieve such insight at a reduced cost, i.e., without requiring information about the bath correlations in every integration domain.
IV.1 From time to frequency
The key quantity in the frequency domain analysis of stationary noise processes is the power spectrum which follows from the Fourier transform of the cumulant, i.e.,
(24) | |||||
In the same way one can write the symmetric and anti-symmetric versions of the correlation function, i.e., and the / power spectra are given by
where we note that the spectrum is symmetric about and non-negative, while the spectrum is antisymmetric and can be negative. In this language, noticing that can be built to have a completely different -pulse generated structure in the intervals and and choosing one can rewrite
(27) |
where and are the filter functions associated to the intervals and , respectively. Eq. (27) is the cornerstone of this paper, as it opens multiple avenues for improving existing frequency-domain QNS protocols and overcoming some of their most notable limitations.
Concretely, we will showcase a method using the full Fourier machinery and outputting a fine-grained sample of the spectra, with a resolution determined by the experimental limitations.
IV.2 Fourier-based reconstruction
This algorithm stems from the observation that when (i) and (ii) combining results from when the sequences in intervals and are exchanged, then Eq. (27) leads to the quantities
(32) |
The key is to recognize – specially given the symmetry/anti-symmetry of – that for any given ,
(33) |
i.e., one can experimentally access the (inverse) Fourier transform of modulated by the real/imaginary part of . From this point of view, a natural way to do spectroscopy is as follows: (i) choose certain filter functions ; (ii) for a series of different values, perform experiments and reconstruct the values of , and perform an even/odd extension to according to the symmetry/antisymmetry of ; (iii) perform, e.g., Discrete Fourier Transform (DFT) or Discrete-Time Fourier Transform (DTFT) on the collected values of and invert by the real/imaginary part of to reconstruct the spectrum curve in certain frequency range; (iv) repeat (i)-(iii) for different to reconstruct the spectrum in different frequency ranges.
The details on how the above can be done and what are the limits of the approach depend heavily on the experimental constraints.
First, note that can only be sampled at multiples of This implies that the Fourier transform can provide reliable information up to a frequency On the other hand, since in theory is not upper bounded (in the limit of purely dephasing noise as we consider here) one can in principle sample the spectrum with very high frequency resolution. We notice that in practice, when there is also non-dephasing noise, will be limited. Moreover, any new time-trace, i.e., value of , implies a new experimental setup and thus adds to the overall cost of the characterization.
Second, one notices that the reconstruction of is “windowed” in a frequency domain by and control constraints influence what sort of filter window can be generated. An obvious implication of the above is that can only be inferred in the region where is non-zero. To formalize this, we define the main frequency support (MFS) of the chosen filters as the region where
and
with and the factors being some convenient values, e.g., Thus, to infer the value of in a subregion of interest , one would like to generate a filter whose MFS is One can then infer the full by sweeping over the whole relevant frequency range. A second implication, is that one would like the filter to be sufficiently smooth in the region of interest, so as to facilitate the Fourier transform step, i.e., one does not want that the filter adds more frequency components to The ideal scenario is then where is a square window function of variable centre and width.
We will use DD sequences [25, 24, 26, 27, 23] composed of -pulse sequences (free evolution is the case where no -pulses are applied) to generate and , since the filter function structure of such sequences is well understood and are thus practical if one is interested in setting their MFS in a controllable frequency range. Notice that – in the absence of knowledge about the noise – a sufficiently powerful DD sequence can in principle mitigate the effect of the noise, i.e., ensuring that is not close to zero, thus allowing us to extract information from observables. For example, one can use -CPMG sequences made in the and intervals, implemented in a length- interval by applying pulses at plus a pulse at the final time if is even. The key property is that by changing , one can move the MFS of the filter function as desired, with only a minimal loss in power in the MFS (see Fig. 3). Although it should be noted that the minimum switching time implies that not every sequence can be used in the windows of length . For example, for only free-evolution can be considered in the window. Moreover, note that the minimum switching time imposes an upper bound to the frequency that can be uniquely sampled, namely Thus, to bypass this issue and avoid aliasing in our estimation, we will assume that the spectra under consideration have a frequency cut-off

As information about the noise is gained, the choice of filter can be adapted to maximize the information gain in a given frequency band. Moreover, note that DD sequences provide a systematic way to produce filters with varying MFSs, that can eventually be glued together as needed. This can be taken further, however. Indeed, one can build filters with optimal spectral concentration in a window of interest using -pulse sequences, as was shown in [28], which shares the key property of Slepian functions, i.e., being concentrated in both frequency and time.
Technical details of performing this Fourier transform method are presented in Appendix C.
IV.3 Full-access reconstruction
One can take the above further. Recall, we have in principle access to the values of the integrals , for . Provided that is sufficiently small and that is sufficiently smooth so that it can be taken approximately constant in the small integration domain, one can then assume that this implies access to the piecewise constant , for . With this, one can then use classical processing to build
for a suitable so that provides information about a feature of interest. For example, choosing and having data for sufficiently large values of , would yield i.e., the value of the spectrum at The freedom in and the seemingly unlimited ability to exploit is nothing but a reflection of the great level of detail control can provide.
This level of detail in the time domain, however, comes at a cost. Inferring the value of requires nonlinear combinations of expectation values resulting from a number of control setups (choice of observable, control sequence, , and ) that scales with Hence, while one gets more detail, the error in the estimation of each integral also grows. We present it here for completeness since it may be of use if the interest is to access a particularly fine feature in the bath correlation functions, but leaving for future work going over the practicalities. As for the specific algorithm used to reconstruct the spectrum curve from values of or more generally from observable expectation values, there are certainly multiple choices that can be developed. For example, Bayesian estimation algorithms [29] are particularly helpful when the measurement shot number is not large and a prior structure of the spectrum function is given. In Sec. V, we focus on simulating our Fourier-based method that requires no prior knowledge on the structure of the spectrum.
IV.4 Overcoming the multivalue problem
An additional benefit of the frequency domain, is that it provides the means to overcome the multivalue problem. Concretely, it allows one to establish a bound relating the spectrum and its counterpart, which can then be leveraged for noise estimation purposes.
IV.4.1 Relationship between and spectra
A superficial deduction would suggest that the and components of the noise statistics are only loosely related. Two observations support this. First, there are scenarios where the spectrum can be any physically-allowed function while the -noise is zero. This is the case, for example, when the noise is classical, i.e., when with a -stochastic process and an arbitrary non-zero time-independent bath operator. Second, if one considers an environment consisting of a single qubit such that then the relations and indicate that it is possible for the -correlation function at while the -correlation at , i.e., the opposite behaviour as in the first observation. Thus, establishing a clear relationship in the time domain does not seem straightforward.
In the frequency domain, however, one can prove the following result.
Theorem 1
Let the bath operator and bath state acting on a Hilbert space describe a wide-sense stationary noise process. Let any operator on then be represented by If at least one of the following is satisfied,
(34) | |||
for arbitrary and resolution of identity on , and provided exist, then
(35) |
for all .
Two useful corollaries follow from Eq. (35). Namely, we further have
(36) |
for all , and
(37) |
for arbitrary .
Further, it follows that given arbitrary real antisymmetric and symmetric such that holds for all , then, assuming that exist, there exist , and capable of generating a wide-sense stationary process with such spectra .
While full details of the proof are provided in the Appendix D, we highlight that the conditions in Eq. (34) require that the bath correlation functions decay sufficiently fast, so that one can employ the Fubini-Tonelli theorem in a key step of the proof. Moreover, Theorem 1 means a sufficient and necessary condition for QNS results to be physical is Eq. (35) under mild assumptions, which establishes a point-wise hierarchy relating the and spectra. Thus, after performing QNS and obtaining estimates for , one needs to check Eq. (35) to ensure that it holds for all and that one has physically consistent estimation.
The existence of Eq. (35) is not without any hint in history. For example, in thermal equilibrium, the fluctuation-dissipation theorem shows [30, 31]. Using Fermi’s golden rule, Ref. [32, 9] establish a relationship at zero tilt: where is the steady-state population. These relationships are clearly consistent with Eq. (35), and so are the experimentally reconstructed spectra in Ref. [11].
As should be expected, the two corollaries are weaker statements than Eq. (35). For example, Eq. (36) is insufficient for Eq. (35). To see this imagine two independent bath operators , with . Let with , and with . Then one can verify that . However, and . Hence, when , we have , invalidating Eq. (35). On the other hand, Eq. (37) is even weaker, which can be seen by taking one of to be zero. Nevertheless, this inequality might still be useful in practical experiments, as its 2D time integral form often appears explicitly in the expression of , and is thus useful as a cross check for inconsistencies in the measurement data.
In addition to providing a consistency-check mechanism for QNS results, Theorem 1 is fundamental to overcoming the multi-value problem, as we now demonstrate.
IV.4.2 A solution to the multivalue problem
Let us start by summarizing the problem. The component of the spectrum influences the dynamics of a quantum system via integrals which are in turn the arguments of periodic functions. This implies that – simplifying considerations absent – the value of any such integral can only be inferred up to a factor of This clearly limits our ability to estimate the component of the noise in the strong coupling limit, when the values of typical integrals may exceed As detailed in Sec. III.4.1, the problem reduces to estimating , given and , and fixed To uniquely determine , one can apply the following strategy.
First, let us recall that the estimation of the -spectrum can be done independently of the -spectrum, in the sense that one can isolate regardless of the multivalue problem. Thus, one can assume an accurate estimate of is available, which we denote It follows then that
One can then define a safe zone in which the multi-value problem is non-existent. That is, a range of values for where, for fixed , knowledge of and provides a unique estimate of The trivial solution is when but can also include domains in which the range of is in a known iteration of the interval, the fundamental domain of the function.
The trivial safe zone can be found as follows. Given knowledge of one can numerically search for an interval such that when . For a general this can happen for “small” i.e., when , with the effective cut-off frequency of or “large” i.e., when oscillates (as a function of ) much faster than , but can be in an intermediate regime given a specific . However, while in the above scenarios one can safely estimate by using when , in practice one requires knowledge of for a wide – ideally infinite – range of values in order to be able to perform a Fourier transform and obtain an estimate for (33). Thus, one would like a mechanism in which the trivial safe zone can be systematically extended.
To do so, imagine now one has identified one of these values, say , in the trivial safe zone. Then, one samples in increments of some until the estimate approaches say at Take Fig. 4 for example, where and thus . At this point, assuming the sampling step-size is sufficiently small to ensure that has been “continuously” sampled as a function of one can assess the range of when leaving the original safe zone by monitoring the experimentally inferred value of . If it must be that i.e., one realizes that . In contrast, if it must be that , i.e., one has that . In both cases, one knows how to correctly determine , and thus has expanded the original safe zone from to . One can then continue the sampling of , and decide at the next point where if the value of has moved to the next iteration of the fundamental domain by assessing the negative/positive character of . In this way, one can systematically extend the safe zone and keep track of in which iteration of the fundamental domain is for a sampled As such, when is in the -th iteration of the fundamental domain provides a unique estimate, as desired.

IV.5 Limits and comparisons with other methods
Let us now discuss what are the limits of our method. Since we use Fourier analysis by sampling via Eq. (33), Nyquist-Shannon sampling theorem implies that our method can resolve a frequency range up to (Hz) where is the minimum pulse separation time implemented. We highlight that this is true even in the situation were a minimal time for the first pulse, say exists. Notice that this apparent obstacle can be overcome by using stationarity to move to a proper in the language of Sec. III.4.
On the other hand, the lower frequency limit of our method is , which can be easily seen from a discrete Fourier transform point of view on Eq. (33). Interestingly, in the strictly dephasing scenario we consider here, despite the existence of a time, i.e., the time for which for a given pulse sequence , our method in principle allows an unrestricted reconstruction of the spectrum. This can be seen from noting that the combinations of and quantities (see Sec. III.4) give us direct access to and these signals are only ever suppressed by , i.e., the exponents only involve integrals over a domain of size rather than . In practice, when the noise is not purely dephasing, is effectively bounded by the energy relaxation time , which sets the lower frequency limit as about . In contrast, the situation with the spectrum is more delicate, since quantities containing are suppressed by which contain integrals explicitly depending on and can be suppressed by the exponential factor for large Thus, it would seem that in the component case is effectively bounded. Notice, however, that stationarity implies that and the latter can be recovered via and thus, as exemplified in Sec. III.7, it implies that estimation of the component is also not -limited.
We are now in a position to make concrete comparisons with the existing methods in literature. First, standard spectroscopy experiments with -pulse control sequences – e.g., Hahn echo and CPMG sequences – reveal the -spectrum curve roughly above [36, 35, 33, 34]. There are various methods aiming at overcoming this limit, [38, 39, 37]. A notable one is to periodically repeat Ramsey experiment (allowed to be decorated with DD sequences) and single-shot measurement on the probe qubit, perform Fourier transform on the binary time series record and average the reconstructed spectrum curves obtained from different time series [40]. The upper cutoff frequency is where is the consecutive measurement time difference. The lower cutoff frequency is the reciprocal of the total acquisition time which can exceed . Hence their method can enter a lower frequency region of the -spectrum even in systems with a short . On the flip side, since is often significantly larger than [40, 34], this implies that the high frequency cut-off of this method is considerably smaller. For example, there is a frequency gap of about four orders of magnitude between this Ramsey measurement-based method and the CPMG method (the Comb method with a single frequency comb) in [34]. We note that the repeated Ramsey measurement method in [40] was further analyzed in [41] to obtain Eq. (26) therein, the same as Eq. (27)’s -spectrum part in our paper. Regretfully, [41] did not develop a systematic approach based on this formula to reconstruct arbitrary unknown -spectrum, but only developed the formulas for several specific spectra types. Furthermore, a common feature in the above existing works is that the role and effect of -noise is absent.
IV.5.1 Comparison with existing techniques in NMR employing non- pulses
The application of non- pulses in NMR has a long history and significant success in aiding to resolve material structure. For example, Stimulated Echo (STE) [42] has the same pulse sequence as our low-frequency protocol (e.g., Eqs. (17) and (18)), with three 90 degree pulses (including the state preparation pulse that is omitted in this paper) followed by a projective measurement, generating the same sandwich structure of a middle interval ( in our language), where the switching function takes zero value and the spin captures no phase [43], surrounded by two phase-capturing intervals ( and ). As a result, STE and the developed other techniques such as HYSCORE [44] have wide applications in volume-selective spectroscopy, diffusion spectroscopy, MRI, etc. In contrast, here we extend the system model from the semi-classical one to a full quantum-mechanical version (1) and reestablish the technique, reminiscent of the formulation of DD in quantum information on the basis of existing pulse techniques in NMR. Therefore, the wide-range classical and quantum-mechanical spectra of the bath sensed by a single qubit can now both be reconstructed after subtracting the influence of each other, and the system dynamics can be more accurately characterized and predicted when richer control settings (beyond the dephasing-preserving scenario) are considered.
V Simulation
We demonstrate our protocol with detailed numerical simulations, where we explore - among other things - the effect of the error induced by a limited number of measurements. Concretely, we simulate the measurement outcomes resulting from a bath with spectra decorated with some “bumps” as
(38) |
and The parameters are tuned such that Eq. (35) is satisfied and the -spectrum resembles the curve in the experimental result in Ref. [33]. Specifically they are , , , (), , , , , , (), , . , , , , , , , , , , . Furthermore, we add a constant value to in the region to simulate the white noise floor in [33]. Finally, in the region , we multiply with to add some fluctuation features to the curve. We set the high frequency cutoff of the spectra as .

We start by employing our Fourier Transform Method (with the first and third intervals sharing the same -pulse sequences for simplicity, i.e., ) to reconstruct the -spectrum (divided by ). The results are shown in Fig. 5. Subplots (a)-(f) explore the effect of a finite number of time traces (values of ) in the different frequency regions associated to the sequences used and their corresponding MFS, but assume an infinite number of shots per measurement. The more resource intensive implementation (green) requires 530 different experimental setups (combinations of DD sequences and ) and the spectrum estimation shows excellent agreement with the simulated noise. While cutting the number of setups in principle leads to a loss in performance (orange), cutting them by a factor of three did not have a significant impact in our simulations. On the other hand, subplots (g)-(l) explore the effect of a finite number of shots per measurement, i.e., the finite sampling error. The effect of finite measurements is more appreciable (in terms of the absolute value of the error) in the very low frequency range ( kHz), in the limit of applicability of the of our protocol given the constraints. This can be improved in principle by optimizing the scenario.

Once the -spectrum is estimated, we reconstruct the -spectrum. As seen from Fig. 6, our method can also faithfully estimate it. The settings in both Fig. 5 and 6 satisfy the requirements (43) and (44). The behaviour and performance for the -spectrum is similar to the -spectrum in most aspects, with some exceptions. Mainly in the very low frequency range (around ), we reach the limit of applicability of our protocol as in the -spectrum estimation. In contrast to the -estimation, however, is often a discontinuous point for a type -spectrum while DTFT, which is adopted by our simulation, must output a continuous function on frequency. Further note that in the highest frequency range, the orange curve in (f) fails to capture the oscillations. This is mainly because the added fluctuation in our model being highly concentrated in the frequency domain and easily missed by the modulation term generated from merely time traces therein. The estimation error is generally larger in (l) than in other subplots, due to weaker spectrum strength and thus higher relative sensitivity to noise and errors in measurement.
VI Conclusions
Employing a single-qubit probe system, we introduced a quantum noise spectroscopy protocol capable of faithfully reconstructing both the low-frequency and the non-classical aspect of a dephasing Gaussian bath spectra. Our protocol relies on a systematic investigation and employment of non- pulses on the qubit probe, which allows to generate zero-valued effective switching functions concentrating the long-time information of the bath correlation function, and endows us with an exact system evolution equation revealing the effect of non-classical bath. We exploit these equations to propose our exact noise characterization protocol and demonstrate its effectiveness through detailed simulations.
Moreover, under mild assumptions, we proved a sufficient and necessary characterization on the relationship between classical and non-classical spectra from the same bath, which helps to solve the multi-value problem to determine the non-classical noise, and also can be necessary and useful in curbing QNS results to be physical.
As a step towards a QNS protocol completely characterizing a general decoherence process from an arbitrary bath, our results reveal the crucial role of non- pulses in performing a broadband QNS task, and systematically extend the current single-qubit QNS working regime to the scenario where the non-classical nature of the bath needs to be considered or investigated. We expect this work to be a useful tool to fill in the low-frequency estimation gaps in current QNS results and to investigate the quantum nature of practical baths. It would also be valuable to extend our protocol to more general scenarios, such as baths with non-Gaussian features or scenarios including noise from the control signals.
Acknowledgements
Work at Griffith was supported (partially) by the Australian Government through the Australian Research Council’s Discovery Projects funding scheme (Project No. DP210102291) and via AUSMURI Grant No. AUSMURI000002. Yuanlong Wang was also supported by the National Natural Science Foundation of China (No. 12288201).
Appendix A Calculation of the cumulants of
Appendix B Procedures to efficiently exploit Eq. (19)
When exploiting Eq. (19) to estimate , a necessary condition for the estimation result to be reliable is that should not be too close to zero (otherwise the calculated function value from Eq. (19) may deviate significantly from the true value). If one directly tests the value of based on Eq. (19), it is neither efficient nor accurate, because there are altogether six expectation values of observables under different system configurations to be measured. Here we introduce an approach to efficiently test the value of under any effective switching function chosen/to test, denoted as .
We start from the expression of as
(39) |
(i) We note that based on Eq. (14), the value of can be obtained from an experiment of . After a pair of candidate , possibly with a traditional switching function (-pulse sequence) to be tested encoded inside the first interval, and are proposed based on certain reconstruction algorithm, e.g., the one in Sec. IV.2, one can experimentally evaluate the value of , with modulating the first interval . If the obtained expectation value decoheres, and are not appropriate settings for the specific noise environment.

(ii) The remaining undetermined quantity in Eq. (39) is the square of
(40) |
which should not be close to zero. One way to control the magnitude of the component is to choose to be a DD sequence (the second interval is absent in the RHS of Eq. (19), so we have the freedom to determine its -pulse sequence), such that is not close to zero. As for the third interval, if it shares the same -pulse sequence with the first interval, we then know by stationarity that , which is already determined. Otherwise if employs a different -pulse sequence or interval length, then we notice that the two terms in Eq. (40) are the red solid and dashed blocks in Fig. 7, which can be moved to the green blocks using stationarity. Hence, by performing an experiment of Eq. (20) matching the green configurations in Fig. 7 and employing and sequences in the first and second intervals respectively, one can immediately obtain the value of Eq. (40) and confirm the applicability of , and .
Now after measuring only two expectation values of observables (possibly each repeated for several rounds to determine a proper setting), we can determine the magnitude of Eq. (39) to ensure it is large enough.
Appendix C How to determine the sampling setting
Assuming that the different values (which we call time traces, similar to the usage in [45]) are equidistant such that . Under the assumption of infinite measurement shots for each observable, given certain , one is sampling the function with period , obtaining the values of , to reconstruct the Fourier transform of in the frequency region. Utilizing the symmetry/antisymmetry of , one can extend to . Here we analyze how the values of and affect the reconstruction accuracy, by reviewing the procedures of proving the Nyquist–Shannon sampling theorem in, e.g., [46].
One can view the sampling results as the product of the target function with an impulse-train function . Its Fourier series expansion is , where . By the convolution () theorem, the Fourier transform of the practical data is
(41) | |||
When ideally there are infinite time traces (), . Hence, (41) becomes
(42) |
which repeats shifting the original filtered spectrum by a distance of multiple , adds all the images together and divides them by . If there is a high frequency cutoff for , then guarantees that the shifted images do not overlap/alias and a perfect recover of the original spectrum is allowed in principle, which is the famous sampling theorem. Differently, here we are only interested in the MFS and allow frequency aliasing to happen outside MFS. Therefore, we only require , i.e.,
(43) |
The filter function is typically equipped with high frequency lobes, causing spectral leakage [4]. An ideal thus does not really exist, and in practice one can take to be the first positive root of or a sufficiently large value. Moreover, there are potential tricks worth developing. For example, (i) special values can be chosen such that clean regions (where is basically zero and without non-negligible lobes) of the filter function cover the MFS, or (ii) different groups of values can be employed such that the position of the lobes differ from groups to groups and the reconstruction results in the unaffected subregions of MFS can be pieced together. We do not delve into these technical details in this paper and only point out the potentials.
Assuming that is already properly chosen such that the frequency aliasing problem is solved, we illustrate the effect of a finite . If is not large enough, will not be close enough to , distorting the ideal result of (42). Hence, by depicting the plot of the Dirichlet kernel versus the ideal in the regime , one can roughly estimate whether certain value is large enough. A natural intuitive requirement is that the first positive root of should be significantly small compared with , which reads
(44) |
Hence, there is a trade-off between and : for a given filter function , the smaller is the sampling period , the larger is the needed sampling time trace number . Although increasing the sampling frequency mitigates the frequency aliasing problem, the price is that more resources (time traces) are needed.
A special scenario breaking Eq. (44) is when , i.e., a free evolution filter function is employed whose MFS covers , especially for 1/f spectra. Related to this, an important observation is that the larger is , the better does the reconstructed spectrum capture the peaks or steep slopes on the spectral curve. Imagine that is small enough such that the filtered spectrum is mainly supported in such that the aliasing error can be neglected. Assuming that the filtered spectrum has a finite-term Fourier series expansion in this region as
(45) |
Then (41) becomes
(46) | ||||
When , Eq. (46) and can be correctly reconstructed in theory. Otherwise when , (46) contains no information about the high-order Fourier terms constituting the peaks on the spectrum curve. Hence, when the time trace sequence is not long enough, the peaks or steep slopes in the spectrum curve usually might not be fully captured.
Denote the aliasing error, in the sense of
(47) |
from (42). Assuming that the aliasing error and finite-time-trace error are neglected by the spectrum reconstruction algorithm (DTFT here) while they still exist in the actual physics process, we now analyze the net error, including the sampling error , e.g., from finite sampling (i.e., finite statistics when measuring each observable). The spectrum estimation error can be bounded as
(48) | ||||
where on the RHS of the last equality the first term is the spectrum estimation error from finite time traces, the second term is the aliasing error and the third term can be bounded as
(49) | ||||
representing the estimation error from the inaccuracy of each recorded time trace. Eqs. (48) and (49) give an error upper bound separating different error sources. Moreover, (49) can be linked with finite sampling through error propagation formula, bounding the error contribution from there and assisting in determining proper measurement shot numbers. It is also possible to mitigate the aliasing error using (47) based on the existing estimation results. We do not elaborate on these potential developments in this paper.
Appendix D Proof of Theorem 1
Proof. To prove Eq. (35), firstly we will show that it suffices to assume is pure. Define
where . Clearly are two real linear functionals defined over the space of all the quantum states on . Since mixed states are convex combinations of pure states, to prove Eq. (35), it suffices to prove that hold for any pure , given arbitrary . We thus assume .
Next, take a resolution of identity such that (but we allow ). For any , denote where and are classical wide-sense stationary stochastic processes. We then know
(50) |
Since one of Eq. (34) holds, using Fubini–Tonelli theorem, we can swap the double integrals in Eq. (50) to reach
Denote the classical spectrum of and to be and , respectively. Let the cross spectrum of be , which can be complex. A key ingredient is the cross-spectrum inequality in classical signal processing (see e.g., Eq. (5.89b) of [47]) as
(51) |
We thus know
Similarly, one can prove , which completes the proof of Eq. (35).
As for the scenario where are given as illustrated, we take to be the common position-momentum space (in instead of ) with a resolution of identity . As before, from we take such that . Let , , and be four independent white noise processes indexed by , all with zero means and unit variances. We then define
which have correlation functions
(52) |
and
(53) |
Therefore, both and are zero-mean wide-sense stationary processes. We take the bath operator such that . Using Eq. (50), we know
and together with Eqs. (52) and (53) we know
which completes the proof.
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