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Atomic superheterodyne receiver Sensitivity estimation based on homodyne readout

Shanchi Wu, Chen Gong, Rui Ni Shanchi Wu, Chen Gong are with University of Science and Technology of China, Email address: [email protected], [email protected] Ni is with Huawei Technology, Email address: [email protected].
Abstract

The electric field measurement sensitivity based on the Rydberg atomic vapor cell has great theoretical advantages over traditional dipole antennas. We combine the Rydberg atomic heterodyne receiver and the Mach-Zehnder interferometer (MZI) with high phase detection sensitivity to evaluate the system reception sensitivity based on the transmitted laser phase shift. We conduct a theoretical investigation into the impacts of local microwave electric field frequency detuning, and laser frequency detuning on enhancing the sensitivity of heterodyne Rydberg atomic receiver based on MZI. To optimize the output signal’s amplitude given the input microwave signal, we derive the steady-state solutions of the atomic density matrix. Numerical results show that laser frequency detuning and local microwave electric field frequency detuning can improve the system detection sensitivity, which can help the system achieve extra sensitivity gain. It also shows that the phase-based readout scheme of heterodyne Rydberg atomic receiver based on MZI can achieve better sensitivity than the intensity-based readout scheme of heterodyne Rydberg atomic receiver.

Index Terms:
Rydberg atom, phase, homodyne readout, frequency detuning, sensitivity optimization.

I Introduction

Rydberg atoms show extremely strong microwave transition electric dipole moments, which are sensitive to external electromagnetic fields. At room temperature, electromagnetic fields can be measured with high sensitivity and precision using atomic quantum coherence effects. Due to their small size, high sensitivity, and wide operating frequency band, Rydberg atomic electric field sensors offer great potential for the detection of radio frequency signals.

Utilizing EIT (electromagnetically induced transparency) spectroscopy, a Rydberg atomic sensor with sensitivity 30 uV\cdotcm-1Hz-1/2 and minimum detectable electric field intensity of 88 uV/cm has been demonstrated [1]. Rydberg atomic sensors’ sensitivity can be raised to 22 uV\cdotcm-1Hz-1/2 using balanced homodyne detection and frequency modulation methods based on optical interferometers [2, 3]. Combining the Rydberg atomic sensor with the traditional superheterodyne approach results in a significant increase in sensitivity. Such method introduces a local microwave signal and the phase and frequency measurement of microwaves can be realized by the Rydberg atomic sensor, improving the sensitivity of microwave electric field detection to 5555 nV\cdotcm-1Hz-1/2 [4]. The setting of laser parameters also affects the electric field detection sensitivity of the Rydberg atomic sensor. Numerical simulations and experimental results show that the sensitivity of the Rydberg atomic sensor is related to the amplitude intensity of the two lasers and microwave electric. The microwave electric detection sensitivity can be improved to 12.512.5 nV\cdotcm-1Hz-1/2 by detuning the coupling laser frequency, which is the highest sensitivity achieved in experiments so far [5]. For applications in communication systems, improving the detection sensitivity and predicting the Rydberg atomic sensor performance under different parameter settings through theoretical analysis and numerical simulation are significant.

Rydberg atomic sensors’ detection sensitivity is fundamentally constrained by quantum noise, which is orders of magnitude less prevalent than thermal noise. The coherence time of the atoms can be decreased in real systems by a variety of variables, which lowers the system’s sensitivity to detection. The main relaxation mechanisms that affect Rydberg atomic sensor’s sensitivity include collision broadening, transition time broadening [6], power broadening [7] and laser linewidth [8, 9]. Atomic collisions with cavity walls as well as atomic collisions with one another cause the collision broadening effect. The collision broadening effect can be efficiently decreased by low atomic density. The atoms’ mobility causes the transition time broadening effect, which depends on the temperature, atomic mass, and laser beam size. The power broadening originates from the instability of laser power, which can be squeezed by the power stabilization module in experiment. The laser linewidth is an inherent property of lasers, and narrow linewidth laser can improve the performance of Rydberg atomic sensors. Finding technical methods to eliminate or reduce the influence of these factors is crucial for future applications in communication system.

Recent progress in experiments show that reducing the laser linewidth and power fluctuation are feasible improvement methods. Experimental techniques with ultrastable cavities can achieve extremely narrow linewidth laser beam and high power stabilization, which can increase the system sensitivity to the level higher than 100100 nV\cdotcm-1Hz-1/2. The optical readout noise is the dominant factor limiting the detection sensitivity [4, 5]. Except for apparatus performance improvement, new detection and readout techniques are the options left. In the perspective of readout techniques, the experiment based on optical interferometer provides ideas for reducing readout noise. Methods that combine circulating cavity with compressed state light have the potential to further reduce the readout noise limit of the system. Existing experimental schemes adopt different detection techniques depending on the atomic response regime, such as AT splitting effect of atomic resonance [1], AC Stark effect under off-resonant [10], and the heterodyne readout technique with tuning capability [11]. A continuously tunable electric field measurement based on the far off-resonant AC stark effect in a Rydberg atomic vapor cell shows comparable detection sensitivity with a resonant microwave-dressed Rydberg heterodyne receiver using the same system [12]. Additional research about electric field detuning can make smooth transitions among these operating regimes, especially for modulated signals. The frequency modulation spectroscopy [3], lower noise photodetector, and the setting of operating state in the experiment are all sensitivity optimization methods worth trying.

In previous work, the intensity-based readout scheme has been widely studied [4, 5], and the most sensitive Rydberg atomic heterodyne receiver receives the intensity signal of the transmitted laser through a photodetector[5]. Although phase-based homodyne readout scheme also has been demonstrated[2, 13, 14], the relationship between the transmitted laser phase shift and electric field strength remains to be studied. Considering that atomic media changes the phase of transmitted laser, and optical interferometer is highly sensitive to the phase shift, we construct the phase-based Rydberg atomic heterodyne receiver embedded in Mach-Zehnder interferometer. This scheme is expected to further improve the performance of atomic-based electric field sensing sensitivity. In this work, we further characterize the effects of local microwave, probing laser and coupling laser frequency detuning on the sensitivity of Rydberg atomic superheterodyne receiver based on homodyne readout.

The reminder of this paper is organized as follows. In Section II, we introduce the system structure of proposed scheme, and outline the basic detection principles based on homodyne readout. In Section III, we optimize the frequency parameters based on atomic four-level model. We theoretically investigate the detection response to the local microwave, coupling laser and probing laser frequency detuning. In Section IV, we numerically characterize the system sensitivity variation. In Section V, we evaluate the electric field detection sensitivity based on different noise baselines. Finally in Section VI, we conclude this work.

II System Model

II-A System Structure

A schematic diagram of the Rydberg atomic superheterodyne receiver based on homodyne readout is shown in Fig. 1. It can be seen that compared with the Rydberg atomic heterodyne receiver based on intensity readout, the Rydberg atomic heterodyne receiver based on homodyne readout studied in this paper uses the MZI in the transmitted laser readout. The probing laser and coupling laser are locked on the desired wavelength and simultaneously excite the atoms in the atomic vapor cell. When the microwave signal radiates cross the atomic vapor cell, the atomic vapor cell changes the phase of transmitted probing laser, which is superimposed with the reference light through a beam splitter. Finally, the photodetector receives the mixed light for subsequent signal processing. The system response is sensitive to the direction of polarization. It has been demonstrated that the microwave electric field polarization can also be obtained by atomic system[15]. In this work, we assume that the lasers and microwave signal have the same polarization.

Refer to caption
Figure 1: The diagram of the atomic heterodyne detection system based on homodyne readout.

In order to obtain a narrower laser linewidth and lower power fluctuations, the actual system is more complex. Fig. 2 shows the proposed system setup. The 852nm laser uses a frequency stabilization scheme based on atomic absorption spectroscopy, while the 509nm laser uses a frequency stabilization scheme based on EIT effect of atomic absorption spectra. The two lasers pass through the power stabilization module and then enter the detection atomic vapor cell to excite the atoms to the Rydberg state. Under the radiation of electric field, the atomic vapor cell changes the phase of the transmitted laser, which is received by the photodetector through a MZI. The frequency stabilization scheme can be replaced by other higher performance schemes, such as ultra-low expansion cavity scheme.

Refer to caption
Figure 2: Overview of the system setup. We have used the following notations: (1) ISO: isolator, (2) HWP: half wave plate, (3) PBS: polarized beam splitter, (4) AOM: The acousto-optic modulators which shift the frequencies of the probing and coupling lights to atomic resonances, (5) PSM: power stabilization module, (6) PD: photodetector, (7) DM: dichroic mirror, (8) RM: reflective mirror, (9) LFSM: laser frequency stabilization module, (10) MZI: Mach-Zehnder interferometer.

II-B Theoretical Model

The diagram for a typical atomic four-level structure is shown in Fig. 3. The probing laser and coupling laser are tuned with detuning Δp\Delta_{p} and Δc\Delta_{c}, respectively; and the local microwave electric field is tuned with detuning ΔL\Delta_{L}. Assume that the frequency and phase difference between local microwave electric field and signal microwave electric field is δs\delta_{s} and ϕs\phi_{s}, respectively. The corresponding Hamiltonian in the rotating frame is given by

H=2(0Ωp00Ωp2ΔpΩc00Ωc2(Δp+Δc)ΩL+ΩseiS(t)00ΩL+ΩseiS(t)2(Δp+Δc+ΔL)),H=\frac{{\hbar}}{2}\left(\begin{matrix}0&\Omega_{p}&0&0\\ \Omega_{p}&2\Delta_{p}&\Omega_{c}&0\\ 0&\Omega_{c}&2\left(\Delta_{p}+\Delta_{c}\right)&\Omega_{L}+\Omega_{s}e^{-iS\left(t\right)}\\ 0&0&\Omega_{L}+\Omega_{s}e^{iS\left(t\right)}&2\left(\Delta_{p}+\Delta_{c}+\Delta_{L}\right)\\ \end{matrix}\right), (1)

where Ωp\Omega_{p} and Ωc\Omega_{c} are the corresponding Rabi frequencies for transitions |1|2\left.|1\right>\rightarrow\left.|2\right> and |2|3\left.|2\right>\rightarrow\left.|3\right>, respectively. The local microwave electric field and signal microwave electric field couple with Rydberg transition between state |3\left.|3\right> and state |4\left.|4\right>, with Rabi frequencies ΩL\Omega_{L} and Ωs\Omega_{s}, respectively. Let Ω=|ΩL+ΩseiS(t)|\Omega=|\Omega_{L}+\Omega_{s}e^{-iS\left(t\right)}|, where S(t)=2πδst+ϕsS\left(t\right)=2\pi\delta_{s}t+\phi_{s} is the cumulative phase difference of the signal microwave relative to the local microwave.

Refer to caption
Figure 3: The diagram of four-level configuration.

Due to the relaxation effect caused by the spontaneous radiation, collision of atoms and transit relaxation effect, as well as the atoms repopulation, the complete Liouville equation for the rotating-frame density matrix of the system can be written as [16]

iddtρ=[H,ρ]i12(Γρ+ρΓ)+iΛ,i{\hbar}\frac{d}{dt}\rho=\left[H,\ \rho\right]-i{\hbar}\frac{1}{2}\left(\Gamma\rho+\rho\Gamma\right)+i{\hbar}\Lambda, (2)

where ρ\rho is the density matrix. Relaxation matrix Γ\Gamma, which represents the relaxation rate of each state, is given by

Γ=(γ0000γ+γ20000γ+γ3+γc0000γ+γ4),\Gamma=\left(\begin{matrix}\gamma&0&0&0\\ 0&\gamma+\gamma_{2}&0&0\\ 0&0&\gamma+\gamma_{3}+\gamma_{c}&0\\ 0&0&0&\gamma+\gamma_{4}\\ \end{matrix}\right), (3)

where γ2\gamma_{2}, γ3\gamma_{3} and γ4\gamma_{4} represent the spontaneous decay rates of atoms on the three high levels; γc\gamma_{c} and γ\gamma are the relaxation rates of the atoms collision and transit effect, respectively. We assume that each level undergoes the same relaxation rate γ\gamma due to the exit of atoms from the laser beam.

In addition, the atoms that spontaneously decay from the upper states also repopulate the lower sates. In this work, we only consider the decay paths shown in Fig. 3. Repopulation matrix Λ\Lambda is given by

Λ=(γ+γ2ρ22+γ4ρ440000γ3ρ330000000000).\Lambda=\left(\begin{matrix}\gamma+\gamma_{2}\rho_{22}+\gamma_{4}\rho_{44}&0&0&0\\ 0&\gamma_{3}\rho_{33}&0&0\\ 0&0&0&0\\ 0&0&0&0\\ \end{matrix}\right). (4)

The dynamics equation of the atomic system can be expressed as

ddtρ=i[H,ρ]+L,\frac{d}{dt}\rho=-\frac{i}{{\hbar}}\left[H,\rho\right]+L, (5)

where L=12(Γρ+ρΓ)+ΛL=-\frac{1}{2}\left(\Gamma\rho+\rho\Gamma\right)+\Lambda represents the Lindbladian operator that defines the relaxation progress in the system, which matrix form is given by

L=(γ+γ2ρ22+γ4ρ44γ2+2γ2ρ12γ3+γc+2γ2ρ13γ4+2γ2ρ14γ2+2γ2ρ21(γ3+γc+γ)ρ33(γ2+γ)ρ22(γ23+γc+2γ2)ρ23(γ24+2γ2)ρ24γ3+γc+2γ2ρ31(γ23+γc+2γ2)ρ32(γ3+γc+γ)ρ33(γ34+γc+2γ2)ρ34γ4+2γ2ρ41(γ24+2γ2)ρ42(γ34+γc+2γ2)ρ43(γ4+γ)ρ44).L=\left(\begin{matrix}\gamma+\gamma_{2}\rho_{22}+\gamma_{4}\rho_{44}&-\frac{\gamma_{2}+2\gamma}{2}\rho_{12}&-\frac{\gamma_{3}+\gamma_{c}+2\gamma}{2}\rho_{13}&-\frac{\gamma_{4}+2\gamma}{2}\rho_{14}\\ -\frac{\gamma_{2}+2\gamma}{2}\rho_{21}&\left(\gamma_{3}+\gamma_{c}+\gamma\right)\rho_{33}-\left(\gamma_{2}+\gamma\right)\rho_{22}&-\left(\frac{\gamma_{23}+\gamma_{c}+2\gamma}{2}\right)\rho_{23}&-\left(\frac{\gamma_{24}+2\gamma}{2}\right)\rho_{24}\\ -\frac{\gamma_{3}+\gamma_{c}+2\gamma}{2}\rho_{31}&-\left(\frac{\gamma_{23}+\gamma_{c}+2\gamma}{2}\right)\rho_{32}&-\left(\gamma_{3}+\gamma_{c}+\gamma\right)\rho_{33}&-\left(\frac{\gamma_{34}+\gamma_{c}+2\gamma}{2}\right)\rho_{34}\\ -\frac{\gamma_{4}+2\gamma}{2}\rho_{41}&-\left(\frac{\gamma_{24}+2\gamma}{2}\right)\rho_{42}&-\left(\frac{\gamma_{34}+\gamma_{c}+2\gamma}{2}\right)\rho_{43}&-\left(\gamma_{4}+\gamma\right)\rho_{44}\\ \end{matrix}\right). (6)

II-C Principle

We begin with analytical derivations based on cold atoms. Within the adiabatic approximation, the probe laser transmission associated with the instantaneous steady state is written in terms of the imaginary component of the susceptibility as P(t)=PiekpL(χ)P\left(t\right)=P_{i}e^{-k_{p}L\Im\left(\chi\right)}. Here, PiP_{i} is the incident light power, LL is the length of atomic vapor cell and kp=2π/λpk_{p}=2\pi/\lambda_{p} is the probing laser wavevector [4]. The linear susceptibility can be given by

χ=2N0μ212ε0Ωpρ21,\chi=-\frac{2N_{0}\mu_{21}^{2}}{{\hbar}\varepsilon_{0}\Omega_{p}}\rho_{21}, (7)

where N0N_{0} is the total density of atoms, μ21\mu_{21} is the dipole moment of transition |1|2|1\rangle\rightarrow|2\rangle and ϵ0\epsilon_{0} is the permittivity in vacuum, and ρ21\rho_{21} is the density matrix element that describes the atomic coherence between the ground and first excited state and is found by solving Eq. 5 in steady state.

The presence of the atomic ensemble causes absorption and phase shifts on the probe light that depend on the density matrix via the differential equations [17]

dΩpdz=kpN0μ2122ε0(ρ21),\frac{d\Omega_{p}}{dz}=\frac{k_{p}N_{0}\mu_{21}^{2}}{2{\hbar}\varepsilon_{0}}\Im\left(\rho_{21}\right), (8)

and

dϕdz=kpN0μ2122ε0Ωp(z)(ρ21).\frac{d\phi}{dz}=\frac{k_{p}N_{0}\mu_{21}^{2}}{2{\hbar}\varepsilon_{0}\Omega_{p}\left(z\right)}\Re\left(\rho_{21}\right). (9)

We analyze the thin optical depth case and ignore the space dependency of Ωp\Omega_{p}. This yields the phase difference through the atomic vapor cell,

Δϕ=kpL(χ)/4.\Delta\phi=k_{p}L\Re\left(\chi\right)/4. (10)

Then, the output electric field through the atomic medium is given by

Eout=EiekpL(χ)/2eiΔϕ.E_{out}=E_{i}\cdot e^{-k_{p}L\Im\left(\chi\right)/2}\cdot e^{i\Delta\phi}. (11)

In the framework of MZI, the electric field of signal arm (through the atomic vapor cell) and reference arm received by the photodetector are given by

ESIG\displaystyle E_{\text{SIG}} =E1eikn0LSIGekpL(χ)/2eiΔϕ,\displaystyle=E_{1}\cdot e^{ikn_{0}L_{\text{SIG}}}\cdot e^{-k_{p}L\Im\left(\chi\right)/2}\cdot e^{i\Delta\phi}, (12)
EREF\displaystyle E_{\text{REF}} =E2eikn0LREF,\displaystyle=E_{2}\cdot e^{ikn_{0}L_{\text{REF}}},

where E1E_{1} and LSIGL_{\text{SIG}} are the incident electric field and optical path length of signal arm, and E2E_{2} and LREFL_{\text{REF}} are the incident electric field and optical path length of reference arm; n0n_{0} is the refractive index. The differential signal of the balanced homodyne detectors (not shown in Fig. 2) is given by [14]

ΔId2|EREF||ESIG|ekpL(χ)/2cos(ϕREF+Δϕ).\Delta I_{d}\propto 2|E_{\text{REF}}||E_{\text{SIG}}|e^{-k_{p}L\Im\left(\chi\right)/2}\cos\left(\phi_{\text{REF}}+\Delta\phi\right). (13)

According to the signal of photodetector, the small phase shift Δϕ\Delta{\phi} can be inferred. The strength of signal electric field can be extracted based on Eq. (10) and the relationship between (χ)\Re({\chi}) and Ωs\Omega_{s}, which is investigated in this work. Based on the steady-state solution of the system Liouville equation, we derive the expression of the linear susceptibility and phase shift, and then find the optimal values.

III Parameters Optimization

III-A Methodology

In experimental systems, in order to reduce the interaction and collision rate between atoms, the atomic density and laser power are usually limited, although increasing the laser power can theoretically increase the signal-to-noise ratio of the output signal and improve the sensitivity. Therefore, in the current experimental setups, the detection laser power is usually at a weak level, and the coupled laser power is also limited. For Rydberg atom sensors using EIT readout, the optimal Rabi frequencies for transitions |1|2|1\rangle\rightarrow|2\rangle and |2|3|2\rangle\rightarrow|3\rangle depend on the decay rate of each state and relaxation rate caused by atom collision [17]. We analyze the influence of laser frequencies and local microwave electric field frequency detuning on the system sensitivity.

We set a detuning parameter Δ\Delta (which can be Δp\Delta_{p}, Δc\Delta_{c}, or ΔL\Delta_{L}). Assuming γ3=γ4=γc=γ=0\gamma_{3}=\gamma_{4}=\gamma_{c}=\gamma=0, the steady-state solution ρ21(Δ)\rho_{21}\left(\Delta\right) can be obtained based on Eq. (5). Assuming ΩsΩL\Omega_{s}\ll\Omega_{L}, the output optical power has the formalism as follows,

P(t)P¯0+κΩscos(2πδst+ϕs),P\left(t\right)\approx\bar{P}_{0}+\kappa\Omega_{s}\cos\left(2\pi\delta_{s}t+\phi_{s}\right), (14)

where κ\kappa is a conversion coefficient [4]. Similarly, the corresponding linear susceptibility real component of the atomic medium can be written as

(χ(t,Δ))χ0(Δ)+χ1(Δ)Ωscos(2πδst+ϕs),\Re\left(\chi\left(t,\ \Delta\right)\right)\approx\chi_{0}\left(\Delta\right)+\chi_{1}\left(\Delta\right)\Omega_{s}\cos\left(2\pi\delta_{s}t+\phi_{s}\right), (15)

which has a time-invariant part χ0(Δ)\chi_{0}\left(\Delta\right) and the coefficient of time variant part χ1(Δ)\chi_{1}\left(\Delta\right). The first part contributes a constant phase shift, and the second part represents a phase variation that depends on the electric field strength.

The probing laser transmission phase shift is associated with the real component of the susceptibility as

Δϕ=kpL(χ)/4=kpLχ0(Δ)+kpLχ1(Δ)Ωscos(2πδs+ϕs).\displaystyle\Delta\phi=k_{p}L\Re(\chi)/4=k_{p}L\chi_{0}(\Delta)+k_{p}L\chi_{1}(\Delta)\Omega_{s}\cos(2\pi\delta_{s}+\phi_{s}). (16)

Fig. 4 shows the transmitted laser phase shift evolution over time with different signal electric field strengths.

Refer to caption
Figure 4: Transmitted laser phase shift Δϕ\Delta\phi evolution over time.

Since the amplitude of microwave signal is linearly dependent on its corresponding Rabi frequency Ωs\Omega_{s}, we can optimize coefficient χ1(Δ)\chi_{1}\left(\Delta\right) in Eq. (16) to maximize the system sensitivity. It should be noted that the case of weak signal corresponds to small variation of probing laser transmission power. We analyze phase shift individually and do not consider laser power variation with time.

III-B Local Microwave Detuning

Assuming that Δc=Δp=γ3=γ4=0\Delta_{c}=\Delta_{p}=\gamma_{3}=\gamma_{4}=0, the steady-state solution ρ21(ΔL)\rho_{21}(\Delta_{L}) can be obtained according to Eq. (5) as follows,

ρ21(ΔL)=iγ2ΩpΩ42ΔLΩpΩ2Ωc2γ22Ω4+4ΔL2(Ωc2+Ωp2)2+2Ω2Ωp2(Ωc2+Ωp2+Ω2).\rho_{21}(\Delta_{L})=-\frac{i\gamma_{2}\Omega_{p}\Omega^{4}-2\Delta_{L}\Omega_{p}\Omega^{2}\Omega_{c}^{2}}{\gamma_{2}^{2}\Omega^{4}+4\Delta_{L}^{2}\left(\Omega_{c}^{2}+\Omega_{p}^{2}\right)^{2}+2\Omega^{2}\Omega_{p}^{2}\left(\Omega_{c}^{2}+\Omega_{p}^{2}+\Omega^{2}\right)}.\\ (17)

The real component is given by

(ρ21(ΔL))=2ΔLΩpΩ2Ωc2γ22Ω4+4ΔL2(Ωc2+Ωp2)2+2Ω2Ωp2(Ωc2+Ωp2+Ω2).\Re\left(\rho_{21}\left(\Delta_{L}\right)\right)=\frac{2\Delta_{L}\Omega_{p}\Omega^{2}\Omega_{c}^{2}}{\gamma_{2}^{2}\Omega^{4}+4\Delta_{L}^{2}\left(\Omega_{c}^{2}+\Omega_{p}^{2}\right)^{2}+2\Omega^{2}\Omega_{p}^{2}\left(\Omega_{c}^{2}+\Omega_{p}^{2}+\Omega^{2}\right)}. (18)

In the weak signal regime, ΩsΩL\Omega_{s}\ll\Omega_{L}, the first order approximation of Ωs/ΩL\Omega_{s}/\Omega_{L} is given by,

(ρ21(ΔL))CLDC+CLACΩscos(S(t))(γ22ΩL4+4ΔL2(Ωc2+Ωp2)2+2ΩL2Ωp2(Ωc2+Ωp2+ΩL2))2,\Re\left(\rho_{21}\left(\Delta_{L}\right)\right)\approx\frac{C_{L-DC}+C_{L-AC}\Omega_{s}\cos\left(S\left(t\right)\right)}{\left(\gamma_{2}^{2}\Omega_{L}^{4}+4\Delta_{L}^{2}\left(\Omega_{c}^{2}+\Omega_{p}^{2}\right)^{2}+2\Omega_{L}^{2}\Omega_{p}^{2}\left(\Omega_{c}^{2}+\Omega_{p}^{2}+\Omega_{L}^{2}\right)\right)^{2}}, (19)

where CLDCC_{L-DC} and CLACC_{L-AC} are as follows,

CLDC=2ΔLΩpΩc2ΩL2(γ22ΩL4+4ΔL2(Ωp2+Ωc2)2+2ΩL2Ωp2(Ωp2+Ωc2+ΩL2)),C_{L-DC}=2\Delta_{L}\Omega_{p}\Omega_{c}^{2}\Omega_{L}^{2}\left(\gamma_{2}^{2}\Omega_{L}^{4}+4\Delta_{L}^{2}\left(\Omega_{p}^{2}+\Omega_{c}^{2}\right)^{2}+2\Omega_{L}^{2}\Omega_{p}^{2}\left(\Omega_{p}^{2}+\Omega_{c}^{2}+\Omega_{L}^{2}\right)\right), (20)

and

CLAC=4ΔLΩc2ΩpΩL(4ΔL2(Ωp2+Ωc2)2ΩL4(γ22+2Ωp2)).C_{L-AC}=4\Delta_{L}\Omega_{c}^{2}\Omega_{p}\Omega_{L}\left(4\Delta_{L}^{2}\left(\Omega_{p}^{2}+\Omega_{c}^{2}\right)^{2}-\Omega_{L}^{4}\left(\gamma_{2}^{2}+2\Omega_{p}^{2}\right)\right). (21)

The corresponding linear susceptibility of the atomic system can be written as

(χ(t,ΔL))=χ0(ΔL)+χ1(ΔL)ΩscosS(t),\Re\left(\chi\left(t,\ \Delta_{L}\right)\right)=\chi_{0}\left(\Delta_{L}\right)+\chi_{1}\left(\Delta_{L}\right)\Omega_{s}\cos S\left(t\right), (22)

which has a time-invariant part,

χ0(ΔL)=2N0μ122ε0CLDC[γ22ΩL4+4ΔL2(Ωc2+Ωp2)2+2ΩL2Ωp2(Ωp2+Ωc2+ΩL2)]2,\chi_{0}\left(\Delta_{L}\right)=\frac{2N_{0}\mu_{12}^{2}}{{\hbar}\varepsilon_{0}}\frac{C_{L-DC}}{[\gamma_{2}^{2}\Omega_{L}^{4}+4\Delta_{L}^{2}\left(\Omega_{c}^{2}+\Omega_{p}^{2}\right)^{2}+2\Omega_{L}^{2}\Omega_{p}^{2}\left(\Omega_{p}^{2}+\Omega_{c}^{2}+\Omega_{L}^{2}\right)]^{2}}, (23)

and a time variant part coefficient,

χ1(ΔL)=2N0μ122ε0CLAC[γ22ΩL4+4ΔL2(Ωc2+Ωp2)2+2ΩL2Ωp2(Ωc2+Ωp2+ΩL2)]2.\chi_{1}\left(\Delta_{L}\right)=\frac{2N_{0}\mu_{12}^{2}}{{\hbar}\varepsilon_{0}}\frac{C_{L-AC}}{\left[\gamma_{2}^{2}\Omega_{L}^{4}+4\Delta_{L}^{2}\left(\Omega_{c}^{2}+\Omega_{p}^{2}\right)^{2}+2\Omega_{L}^{2}\Omega_{p}^{2}\left(\Omega_{c}^{2}+\Omega_{p}^{2}+\Omega_{L}^{2}\right)\right]^{2}}. (24)

(P1): Sensitivity Maximization in General Case via Local Microwave Detuning

ΔL=argmax ΔL|χ1(ΔL)|.\Delta_{L}^{*}=\underset{\Delta_{L}}{\text{argmax }}|\chi_{1}(\Delta_{L})|. (25)

III-C Probing Laser Frequency Detuning

Assuming that Δc=ΔL=γ3=γ4=γc=γ=0\Delta_{c}=\Delta_{L}=\gamma_{3}=\gamma_{4}=\gamma_{c}=\gamma=0, the steady-state solution ρ21(Δp)\rho_{21}(\Delta_{p}) can be obtained according to Eq. (5) as follows,

ρ21(Δp)\displaystyle\rho_{21}(\Delta_{p}) =Ωp(4Δp2Ω2)(iγ2(4Δp2Ω2)+2Δp(4Δp2Ωc2Ω2))CP(Ω),\displaystyle=\frac{\Omega_{p}\left(4\Delta_{p}^{2}-\Omega^{2}\right)\left(i\gamma_{2}\left(4\Delta_{p}^{2}-\Omega^{2}\right)+2\Delta_{p}\left(4\Delta_{p}^{2}-\Omega_{c}^{2}-\Omega^{2}\right)\right)}{C_{P}(\Omega)}, (26)
CP(Ω)\displaystyle C_{P}(\Omega) =64Δp6+γ22(Ω24Δp2)2+4Δp2((Ω2+Ωc2)2+2Ωp2(Ωp2+Ωc22Ω2))\displaystyle=64\Delta_{p}^{6}+\gamma_{2}^{2}\left(\Omega^{2}-4\Delta_{p}^{2}\right)^{2}+4\Delta_{p}^{2}\left(\left(\Omega^{2}+\Omega_{c}^{2}\right)^{2}+2\Omega_{p}^{2}\left(\Omega_{p}^{2}+\Omega_{c}^{2}-2\Omega^{2}\right)\right)
32Δp4(Ω2+Ωc2Ωp2)+2Ωp2Ω2(Ωp2+Ωc2+Ω2).\displaystyle-32\Delta_{p}^{4}\left(\Omega^{2}+\Omega_{c}^{2}-\Omega_{p}^{2}\right)+2\Omega_{p}^{2}\Omega^{2}\left(\Omega_{p}^{2}+\Omega_{c}^{2}+\Omega^{2}\right).

The real component is given by

(ρ21(Δp))=2ΔpΩp(4Δp2Ω2)(4Δp2Ω2Ωc2)CP(Ω).\Re\left(\rho_{21}\left(\Delta_{p}\right)\right)=\frac{2\Delta_{p}\Omega_{p}\left(4\Delta_{p}^{2}-\Omega^{2}\right)\left(4\Delta_{p}^{2}-\Omega^{2}-\Omega_{c}^{2}\right)}{C_{P}\left(\Omega\right)}. (27)

In weak signal regime, ΩsΩL\Omega_{s}\ll\Omega_{L}, the first order approximation of Ωs/ΩL\Omega_{s}/\Omega_{L} is given by,

(ρ21(Δp))CPDC+CPACΩscos(S(t))CP(ΩL)2,\Re\left(\rho_{21}\left(\Delta_{p}\right)\right)\approx-\frac{C_{P-DC}+C_{P-AC}\Omega_{s}\cos\left(S\left(t\right)\right)}{C_{P}\left(\Omega_{L}\right)^{2}}, (28)

where CPDCC_{P-DC} and CPACC_{P-AC} are as follows,

CPDC=2ΔpΩp(4Δp2ΩL2)(4Δp2Ωc2ΩL2)CP(ΩL),C_{P-DC}=2\Delta_{p}\Omega_{p}\left(4\Delta_{p}^{2}-\Omega_{L}^{2}\right)\left(4\Delta_{p}^{2}-\Omega_{c}^{2}-\Omega_{L}^{2}\right)C_{P}\left(\Omega_{L}\right), (29)

and

CPAC\displaystyle C_{P-AC} =4ΔpΩpΩL(64Δp6Ωc2γ22(4Δp2ΩL2)2Ωc2+2ΩL4Ωp432Δp4(Ωc4+3Ωp4+Ωc2(ΩL2+4Ωp2)))\displaystyle=4\Delta_{p}\Omega_{p}\Omega_{L}\left(64\Delta_{p}^{6}\Omega_{c}^{2}-\gamma_{2}^{2}\left(4\Delta_{p}^{2}-\Omega_{L}^{2}\right)^{2}\Omega_{c}^{2}+2\Omega_{L}^{4}\Omega_{p}^{4}-32\Delta_{p}^{4}\left(\Omega_{c}^{4}+3\Omega_{p}^{4}+\Omega_{c}^{2}\left(\Omega_{L}^{2}+4\Omega_{p}^{2}\right)\right)\right)- (30)
16Δp3ΩpΩL(Ωc6+4ΩL2Ωp4+2Ωc4(ΩL2+2Ωp2)+Ωc2(ΩL4+8ΩL2Ωp2+4Ωp4)).\displaystyle 16\Delta_{p}^{3}\Omega_{p}\Omega_{L}\left(\Omega_{c}^{6}+4\Omega_{L}^{2}\Omega_{p}^{4}+2\Omega_{c}^{4}\left(\Omega_{L}^{2}+2\Omega_{p}^{2}\right)+\Omega_{c}^{2}\left(\Omega_{L}^{4}+8\Omega_{L}^{2}\Omega_{p}^{2}+4\Omega_{p}^{4}\right)\right).

The corresponding real component of linear susceptibility of the atomic system can be written as

(χ(t,Δp))=χ0(Δp)+χ1(Δp)ΩscosS(t),\Re\left(\chi\left(t,\ \Delta_{p}\right)\right)=\chi_{0}\left(\Delta_{p}\right)+\chi_{1}\left(\Delta_{p}\right)\Omega_{s}\cos S\left(t\right), (31)

which has a time-invariant part,

χ0(Δp)=2N0μ122ε0CPDCCP(ΩL)2,\chi_{0}\left(\Delta_{p}\right)=\frac{2N_{0}\mu_{12}^{2}}{{\hbar}\varepsilon_{0}}\frac{C_{P-DC}}{C_{P}(\Omega_{L})^{2}}, (32)

and a time variant part coefficient,

χ1(Δp)=2N0μ122ε0CPACCP(ΩL)2.\chi_{1}\left(\Delta_{p}\right)=\frac{2N_{0}\mu_{12}^{2}}{{\hbar}\varepsilon_{0}}\frac{C_{P-AC}}{C_{P}(\Omega_{L})^{2}}. (33)

(P2): Sensitivity Maximization in General Case via Probing Laser Frequency Detuning

Δp=argmax Δp|χ1(Δp)|.\Delta_{p}^{*}=\underset{\Delta_{p}}{\text{argmax }}|\chi_{1}(\Delta_{p})|. (34)

III-D Coupling Laser Frequency Detuning

Assuming that Δp=ΔL=γ3=γ4=γc=γ=0\Delta_{p}=\Delta_{L}=\gamma_{3}=\gamma_{4}=\gamma_{c}=\gamma=0, the steady-state solution ρ21(Δc)\rho_{21}(\Delta_{c}) can be obtained according to Eq. (5) as follows,

ρ21(Δc)\displaystyle\rho_{21}(\Delta_{c}) =iγ2Ωp(4Δc2Ω2)22ΩpΩc2Δc(4Δc2Ω2)CC(Ω),\displaystyle=\frac{i\gamma_{2}\Omega_{p}\left(4\Delta_{c}^{2}-\Omega^{2}\right)^{2}-2\Omega_{p}\Omega_{c}^{2}\Delta_{c}\left(4\Delta_{c}^{2}-\Omega^{2}\right)}{C_{C}(\Omega)}, (35)
CC(Ω)\displaystyle C_{C}(\Omega) =32Δc4Ωp2+γ22(Ω24Δc2)2+2Ωp2Ω2(Ωp2+Ωc2+Ω2)\displaystyle=32\Delta_{c}^{4}\Omega_{p}^{2}+\gamma_{2}^{2}\left(\Omega^{2}-4\Delta_{c}^{2}\right)^{2}+2\Omega_{p}^{2}\Omega^{2}\left(\Omega_{p}^{2}+\Omega_{c}^{2}+\Omega^{2}\right)
+4Δc2((Ωp2+Ωc2)2+Ωp2(Ωp24Ω2)).\displaystyle+4\Delta_{c}^{2}\left(\left(\Omega_{p}^{2}+\Omega_{c}^{2}\right)^{2}+\Omega_{p}^{2}\left(\Omega_{p}^{2}-4\Omega^{2}\right)\right).

The real component is given by

(ρ21(Δc))=2ΔcΩpΩc2(4Δc2Ω2)CC(Ω).\Re\left(\rho_{21}\left(\Delta_{c}\right)\right)=-\frac{2\Delta_{c}\Omega_{p}\Omega_{c}^{2}\left(4\Delta_{c}^{2}-\Omega^{2}\right)}{C_{C}\left(\Omega\right)}. (36)

In weak signal regime, ΩsΩL\Omega_{s}\ll\Omega_{L}, the first order approximation of Ωs/ΩL\Omega_{s}/\Omega_{L} is given by,

(ρ21(Δc))=CCDC+CCACΩscos(S(t))CC(ΩL)2,\Re\left(\rho_{21}\left(\Delta_{c}\right)\right)=-\frac{C_{C-DC}+C_{C-AC}\Omega_{s}\cos\left(S\left(t\right)\right)}{C_{C}\left(\Omega_{L}\right)^{2}}, (37)

where CCDCC_{C-DC} and CCACC_{C-AC} are as follows,

CCDC=2ΔcΩpΩc2(4Δc2ΩL2)CC(ΩL),C_{C-DC}=2\Delta_{c}\Omega_{p}\Omega_{c}^{2}\left(4\Delta_{c}^{2}-\Omega_{L}^{2}\right)C_{C}\left(\Omega_{L}\right), (38)

and

CCAC=4ΔcΩpΩc2ΩL(γ22(4Δc2+ΩL2)2+32Δc4Ωp2+2ΩL4Ωp24Δc2(Ωc4+4Ωc2Ωp2+4Ωp2(ΩL2+Ωp2))).C_{C-AC}=4\Delta_{c}\Omega_{p}\Omega_{c}^{2}\Omega_{L}\left(\gamma_{2}^{2}\left(-4\Delta_{c}^{2}+\Omega_{L}^{2}\right)^{2}+32\Delta_{c}^{4}\Omega_{p}^{2}+2\Omega_{L}^{4}\Omega_{p}^{2}-4\Delta_{c}^{2}\left(\Omega_{c}^{4}+4\Omega_{c}^{2}\Omega_{p}^{2}+4\Omega_{p}^{2}\left(\Omega_{L}^{2}+\Omega_{p}^{2}\right)\right)\right). (39)

The corresponding real component of linear susceptibility χ(t,Δc)\chi\left(t,\Delta_{c}\right) of the atomic system can be written as

(χ(t,Δc))=χ0(Δc)+χ1(Δc)ΩscosS(t),\Im\left(\chi\left(t,\Delta_{c}\right)\right)=\chi_{0}(\Delta_{c})+\chi_{1}(\Delta_{c})\Omega_{s}\cos S(t), (40)

which has a time-invariant part,

χ0(Δc)=2N0μ122ε0CCDCCC(ΩL)2,\chi_{0}\left(\Delta_{c}\right)=\frac{2N_{0}\mu_{12}^{2}}{{\hbar}\varepsilon_{0}}\frac{C_{C-DC}}{C_{C}(\Omega_{L})^{2}}, (41)

and a time variant part coefficient,

χ1(Δc)=2N0μ122ε0CCACCC(ΩL)2.\chi_{1}\left(\Delta_{c}\right)=\frac{2N_{0}\mu_{12}^{2}}{{\hbar}\varepsilon_{0}}\frac{C_{C-AC}}{C_{C}(\Omega_{L})^{2}}. (42)

(P3): Sensitivity Maximization in General Case via Coupling Laser Detuning

Δc=argmax Δc|χ1(Δc)|.\Delta_{c}^{*}=\underset{{\Delta_{c}}}{\text{argmax }}|\chi_{1}(\Delta_{c})|. (43)

We numerically characterize the frequency detuning effect on the weak signal response in Section IV.

IV Numerical Results

We adopt some parameters from the experimental setups in [4]. Cs atoms were filled in a vapour cell at room temperature. The cell contained ground-state atoms at a total density of N0=4.89×1010N_{0}=4.89\times 10^{10} cm-3. For Rydberg atom EIT, the residence time in the Rydberg state is small. Under typical conditions, the population in Rydberg states is 0.0001~{}0.0001. Only a small distribution of atomic velocity classes in the vapor cell are selected by the EIT lasers, roughly 1/100~{}1/100 for the scheme shown in Fig. 3 [18]. The effective atoms density for atomic vapor is approximated as N0,eff4.89×108N_{0,\text{eff}}\approx 4.89\times 10^{8} cm-3. The four-level configuration in Fig. 3 using four states in a Cs atom: |16S1/2,F=4|1\rangle\rightarrow 6S_{1/2},F=4; |26P3/2,F=5|2\rangle\rightarrow 6P_{3/2},F=5; |347D5/2|3\rangle\rightarrow 47D_{5/2}; and |448P3/2|4\rangle\rightarrow 48P_{3/2}. States |2|2\rangle, |3|3\rangle, and |4|4\rangle have the inverse lifetimes γ2=2π×5.2\gamma_{2}=2\pi\times 5.2 MHz, γ3=2π×3.9\gamma_{3}=2\pi\times 3.9 kHz, and γ4=2π×1.7\gamma_{4}=2\pi\times 1.7 kHz. In this section, we ignore the atoms collision effect, γc=0\gamma_{c}=0, the effective Rabi frequencies for the transitions |1|2|1\rangle\rightarrow|2\rangle and |2|3|2\rangle\rightarrow|3\rangle are Ωp=2π×5.7\Omega_{p}=2\pi\times 5.7 MHz, Ωc=2π×0.97\Omega_{c}=2\pi\times 0.97 MHz, respectively. The frequency intervals between the hyperfine states 6P3/26P_{3/2} are 151.2151.2 MHz (F=2F=3F=2\rightarrow F=3), 201.2201.2 MHz (F=3F=4F=3\rightarrow F=4), and 251.1251.1 MHz (F=4F=5F=4\rightarrow F=5) [19]. In the case of resonance, the system is locked to a specific hyperfine state. We consider a detuning range from 50-50 MHz to 5050 MHz for laser frequency and another range from 100-100 MHz to 100100 MHz for electric field frequency in numerical results.

Local microwave frequency detuning case: The relationship between ΔL\Delta_{L} and conversion coefficient |χ1ΔLΩs||\chi_{1}{\Delta_{L}}\Omega_{s}| is shown in Fig. 5. The maximum values of |χ1ΔLΩs||\chi_{1}{\Delta_{L}}\Omega_{s}| at ΩL/2π=2\Omega_{L}/2\pi=2 MHz, 4 MHz, 6 MHz are 4.125×1094.125\times 10^{-9}, 3.217×1093.217\times 10^{-9}, 2.491×1092.491\times 10^{-9}, respectively. It can be found that weaker local microwave electric field strength corresponds to larger conversion coefficient maximum. At the same time, the detuning value at the maximum point will also become smaller.

Refer to caption
Figure 5: Conversion coefficient |χ1(ΔL)Ωs||\chi_{1}(\Delta_{L})\Omega_{s}| with respect to local microwave detuning ΔL\Delta_{L} in the general case, Ωs=2π×105\Omega_{s}=2\pi\times 10^{5} Hz (P1).

Probing laser frequency detuning case: The relationship between Δp\Delta_{p} and conversion coefficient |χ1ΔpΩs||\chi_{1}{\Delta_{p}}\Omega_{s}| is shown in Fig. 6. The maximum values of |χ1ΔpΩs||\chi_{1}{\Delta_{p}}\Omega_{s}| at ΩL/2π=2\Omega_{L}/2\pi=2 MHz, 4 MHz, 6 MHz are 7.309×1087.309\times 10^{-8}, 1.144×1071.144\times 10^{-7}, 1.430×1071.430\times 10^{-7}, respectively. In contrast to local microwave frequency detuning case, stronger local microwave electric field strength corresponds to larger conversion coefficient maximum in this case. Besides, we can obtain bigger conversion coefficient by setting optimal probing laser frequency.

Refer to caption
Figure 6: Conversion coefficient |χ1(Δp)Ωs||\chi_{1}(\Delta_{p})\Omega_{s}| with respect to probing laser detuning Δp\Delta_{p} in the general case, Ωs=2π×105\Omega_{s}=2\pi\times 10^{5} Hz (P2).

Coupling laser frequency detuning case: The relationship between Δc\Delta_{c} and conversion coefficient |χ1ΔcΩs||\chi_{1}{\Delta_{c}}\Omega_{s}| is shown in Fig. 7. The maximum values of |χ1ΔpΩs||\chi_{1}{\Delta_{p}}\Omega_{s}| at ΩL/2π=2\Omega_{L}/2\pi=2 MHz, 4 MHz, 6 MHz are 1.112×1091.112\times 10^{-9}, 2.743×1092.743\times 10^{-9}, 5.737×1075.737\times 10^{-7}, respectively. This case has similar gain than local microwave frequency detuning case.

Refer to caption
Figure 7: Conversion coefficient |χ1(Δc)Ωs||\chi_{1}(\Delta_{c})\Omega_{s}| with respect to coupling laser detuning Δc\Delta_{c} in the general case, Ωs=2π×105\Omega_{s}=2\pi\times 10^{5} Hz (P3).

V Sensitivity Estimation

V-A Calculation

The power sensitivity of a conventional receiver is usually expressed by the minimum power received by the antenna connector to guarantee certain throughput or BER (bit-error-rate) requirements. Assuming that the length of the atomic vapor cell is LL, the probing laser beam diameter is dd, the effective signal acquisition area AeffA_{\text{eff}} equals to L times d. The equivalent signal power sensitivity is given by

Pmin =|S|Aeff=12ε0cEmin 2Aeff,P_{\min\text{\,\,}}=\left<|\vec{S}|\right>\cdot A_{\text{eff}}=\frac{1}{2}\varepsilon_{0}cE_{\min\text{\,\,}}^{2}\cdot A_{\text{eff}}, (44)

where ε0\varepsilon_{0} and cc are the dielectric constant and speed of light in vacuum, EminE_{min} is the minimum detectable electric field strength, and S\vec{S} is the Poynting vector of electromagnetic field.

V-B Atomic shot noise limit sensitivity

Theoretically, the minimum detectable electric field strength corresponding to the shot noise limit is given by [18]

Emin=hμETN,E_{\min}=\frac{h}{\mu_{\text{E}}T\sqrt{N}}, (45)

where TT is the integration time, NN is the atom involved in the measurement in TT time, and hh and μE\mu_{E} represent Planck constant and transition dipole momentum coupled electric field, respectively. Considering the limit of the actual EIT (electromagnetic induced transparency) process on time TT (TT cannot be longer than the T2T_{2} time of the EIT process), a more useful form can be obtained. The measurement that occurs within TT^{{}^{\prime}} can be understood as N=NatT/T2N=N_{at}T^{{}^{\prime}}/T_{2}, where NatN_{at} is the number of atoms involved in the measurement. The minimum detectable electric field strength of the EIT process can be expressed as

Emin=hμENatTT2.E_{\min}=\frac{h}{\mu_{\text{E}}\sqrt{N_{\text{at}}T^{{}^{\prime}}T_{2}}}. (46)

Taking T=1T^{{}^{\prime}}=1 s, we can get the time-normalized electric field detection sensitivity as

EminHz=hμENatT2.\frac{E_{\min}}{\sqrt{\text{Hz}}}=\frac{h}{\mu_{\text{E}}\sqrt{N_{\text{at}}T_{2}}}. (47)

The Rydberg atomic heterodyne receiver has achieved great improvement in sensitivity, the system electric field measurement sensitivity obtained in the experiment reached 5555 nV\cdotcm-1Hz-1/2 [4]. Using the power sensitivity calculation method in Eq. (44), the power sensitivity of the system is approximately -144.7 dBm\cdotHz-1 based on the data provided in the literature. Based on the Rydberg atomic heterodyne receiver, the optimal electric field measurement sensitivity obtained by combining coupled laser frequency detuning is about 12.512.5 nV\cdotcm-1Hz-1/2 [5], which corresponds to a power sensitivity about 157.5-157.5 dBm\cdotHz-1 (assuming that the vapor cell size and laser beam diameter parameters are consistent with the parameters in the work of Jing et al. [4]). The detection sensitivity of the Rydberg atomic heterodyne receiver is mainly limited by the thermal noise of electronic devices, and the technical noise caused by atomic transition broadening and laser linewidth. The atomic transition broadening can be reduced by amplifying the probing laser and coupling laser beam waist. Replacing balanced detection with homodyne or heterodyne detection can reduce photodetector noise. Using a more stable laser source can eliminate laser frequency noise. These factors can be combined to allow the system to approximate the quantum projection noise limit of atomic sensors, about 700700 pV\cdotcm-1Hz-1/2 [4]. The power detection sensitivity corresponding to the quantum projection noise limit is about 182.6-182.6 dBm\cdotHz-1.

V-C Photon shot noise limit

As described in Section V.A, intensity-based readout methods have achieved great improvement in sensitivity, but are still far from the theoretical limit. In this paper, the performance of the zero-difference readout method is evaluated, and the relationship between the phase conversion coefficient and frequency detuning under different local oscillator electric field strengths is obtained. Referring to the results of the phase noise, the corresponding minimum detectable electric field strength can be given to calculate the power sensitivity.

We model an ideal measurement by assuming a photon-shot-noise limited homodyne measurement of the acquired phase ϕ\phi on the transmitted probe light, where ϕ\phi is calculated by Eq. (16). The noise density phiNphi_{N} in measuring this quantity for a coherent state is defined as

ϕN=2μ21dΩpkphε0,\phi_{N}=\frac{2\mu_{21}}{d\Omega_{p}}\sqrt{\frac{k_{p}}{h\varepsilon_{0}}}, (48)

where detection efficiency assumed to be unity in this work.

The SNR (signal-to-noise ratio) density is given by

ΔϕϕN=kpLdΩpΩs8μ21hε0kpχ1(Δ).\frac{\Delta\phi}{\phi_{N}}=\frac{k_{p}Ld\Omega_{p}\Omega_{s}}{8\mu_{21}}\sqrt{\frac{h\varepsilon_{0}}{k_{p}}}\chi_{1}\left(\Delta\right). (49)

Assume that readout requirement is 0 dB, the minimum detectable electric field is given by

EminHz=4μ21πLdμEΩpχ1(Δ)hkpε0.\frac{E_{\min}}{\sqrt{\text{Hz}}}=\frac{4\mu_{21}}{\pi Ld\mu_{E}\Omega_{p}\chi_{1}\left(\Delta\right)}\sqrt{\frac{h}{k_{p}\varepsilon_{0}}}. (50)

Numerical results in Fig. 5, Fig. 6, and Fig. 7 show that the largest conversion coefficient is obtained in the probing laser frequency detuning case with ΩL=2π×6\Omega_{L}=2\pi\times 6 MHz, χ1(Δp)=1.430×107\chi_{1}(\Delta_{p})=1.430\times 10^{-7}. According to Eq. (50), the electric field detection sensitivity is 0.1850.185 nV\cdotcm-1Hz-1/2, and the corresponding power detection sensitivity is 194.1-194.1 dBm\cdotHz-1. The phase-based readout method improves the sensitivity with 36.636.6 dB gain. It is important to note that we consider the sensitivity improvement of three frequency components detuning independently for three arbitrarily selected local oscillator electric field strengths. The results obtained are not theoretically optimal sensitivity of the proposed method in this work.

VI Conclusion

Based on the atomic superheterodyne receiver and Mach-Zehnder interferometer, we evaluate the detection sensitivity of phase-based readout method. We have derived the steady-state solutions of the density matrix of the Rydberg atomic system operating with frequency detuning. Given the input microwave signal, we have established an optimization problem of the linear susceptibility of atomic medium to maximize the amplitude of the output phase signal. We have numerically analyzed the effects of electric field, probing laser, and coupling laser frequency detuning on the optimization target. Numerical results show that the detection sensitivity can be improved by setting appropriate frequency detuning, especially for probing laser. The photon shot noise limit sensitivity of the phase-based readout method has 36.6 dB gain compared with that of experimental result of the intensity-based readout method.

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