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Journal of Experimental and Theoretical Physics

Dynamics of dispersive photon-number QND measurements in a micromaser

A. V. Kozlovskiĭ

Published Apr 1, 2007• 0 citations
Publisher

Abstract

A numerical analysis of dispersive quantum nondemolition measurement of the photon number of a microwave cavity field is presented. Simulations show that a key property of the dispersive atom-field interaction used in Ramsey interferometry is the extremely high sensitivity of the dynamics of atomic and field states to basic parameters of the system. When a monokinetic atomic beam is sent through a microwave cavity, a qualitative change in the field state can be caused by an uncontrollably small deviation of parameters (such as atom path length through the cavity, atom velocity, cavity mode frequency detuning, or atom-field coupling constants). The resulting cavity field can be either in a Fock state or in a super-Poissonian state (characterized by a large photon-number variance). When the atoms have a random velocity spread, the field is squeezed to a Fock state for arbitrary values of the system’s parameters. However, this makes detection of Ramsey fringes impossible, because the probability of detecting an atom in the upper or lower electronic state becomes a random quantity almost uniformly distributed over the interval between zero and unity, irrespective of the cavity photon number.

DOI
10.1134/s1063776107040012

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A numerical analysis of dispersive quantum nondemolition measurement of the photon number of a microwave cavity field is presented. Simulations show that a key property of the dispersive atom-field interaction used in Ramsey interferometry is the extremely high sensitivity of the dynamics of atomic and field states to basic parameters of the system. When a monokinetic atomic beam is sent through a microwave cavity, a qualitative change in the field state can be caused by an uncontrollably small deviation of parameters (such as atom path length through the cavity, atom velocity, cavity mode frequency detuning, or atom-field coupling constants). The resulting cavity field can be either in a Fock state or in a super-Poissonian state (characterized by a large photon-number variance). When the atoms have a random velocity spread, the field is squeezed to a Fock state for arbitrary values of the system’s parameters. However, this makes detection of Ramsey fringes impossible, because the probability of detecting an atom in the upper or lower electronic state becomes a random quantity almost uniformly distributed over the interval between zero and unity, irrespective of the cavity photon number.
Dispersive quantum nondemolition measurement of the number of photons is analyzed in the micromaser scheme. It has been shown that the stationary Fock state of the field in a cavity that is considered as the result of quantum nondemolition measurement is realized only in a particular case for strictly determined parameters of the system, and small variation in one of the parameters of the system results in a qualitative change in the field state. In the general case, the field state is characterized by large fluctuations of the number of photons and the mean number of photons, which are very sensitive to the parameters of the system. It has been shown that the detection of the Ramsey interference pattern is possible only when the sequence of atoms passing through the cavity is highly monokinetic.
A quantum-nondemolition method to measure the number of photons stored in a high-Q cavity, introduced by Brune et al. [Phys. Rev. Lett. 65, 976 (1990)], is described in detail. It is based on the detection of the dispersive phase shift produced by the field on the wave function of nonresonant atoms crossing the cavity. This shift can be measured by atomic interferometry, using the Ramsey separated-oscillatory-field method. The information acquired by detecting a sequence of atoms modifies the field step by step, until it eventually collapses into a Fock state. At the same time, the field phase undergoes a diffusive process as a result of the back action of the measurement on the photon-number conjugate variable. Once a Fock state has been generated, its evolution under weak perturbation can be continuously monitored, revealing quantum jumps between various photon numbers. When applied to an initial coherent field, the intermediate steps of the measuring sequence produce quantum superpositions of classical fields, known as ``Schr\"odinger cat states.'' Ways to prepare and detect these states in a cavity subjected to a weak relaxation process are discussed. The effects analyzed in this article could realistically be observed by using circular Rydberg atoms and very high-Q superconducting microwave cavities. The possibility of photon ``manipulation'' through nonresonant atom-field interactions opens a domain in cavity QED studies.
In the last decades the interest in studying interactions of Rydberg atoms or ensembles thereof with electromagnetic fields at optical and microwave frequencies has steadily increased. The physics Nobel prize of 2012, for instance, has been partially awarded to cavity quantum electrodynamics (QED) experiments with single Rydberg atoms that allow for quantum nondemolition measurements of the photon number in a superconducting microwave cavity. These experiments detect the dispersive shift of the atomic transition frequency that results from the interaction with the photons to measure the photon number nondestructively. In this thesis, we employ the reversed effect, the dispersive shift of the resonance frequency of the TE301 mode of a rectangular microwave cavity induced an ensemble of helium Rydberg atoms, to perform nondestructive measurements of the atom number. In a first experiment, we measure the dispersive interaction between a few thousand atoms in the 36s singlet state and a copper cavity with a quality factor of about Q = 5 · 10^3. We detect the dispersive shift by continuously measuring the changes in cavity transmission with a weak coherent probe tone that injects a few hundred photons into the cavity. We model the observed time dependence of the dispersive shift, which results from the interplay between the time-dependent collective interaction strength and atom-cavity detuning. Controlling the parameters of the atom cloud, we then directly measure the dependence of the dispersive shift on the atom-cavity detuning and on the number of Rydberg atoms. The results are in good agreement with the Tavis-Cummings Hamiltonian in the dispersive regime, and indicate collective coupling strengths of gN/2pi = 1 MHz, which correspond to more than N = 3 · 10^3 Rydberg atoms. This nondestructive detection of Rydberg atoms achieves a relative precision of 4.5% and an accuracy of 20 %, which are both limited by the inhomogeneity of the atom-cavity detuning over the size of the atom cloud. In a second experiment, we reduce the inhomogeneity by decreasing the size of the atomic cloud and employing the triplet Rydberg transition at n = 42, which is less sensitive to dc electric fields. The precision of the atom number detection is further enhanced by increasing the cavity quality factor to Q = 10^5 with a superconducting niobium cavity. The combined improvements result in the nondestructive detection of a few hundred Rydberg atoms with an accuracy of 3% and a precision of 1 %, which is an order of magnitude improvement over the previous experiment. Motivated by these results obtained from averaging over about 4 × 10^4 repetitions of the experiment, we consider the nondestructive detection of the atom number in single-shot measurements with a high number of photons in the cavity. By studying the dispersive shift and the probability to excite the 42p states as functions of the photon number, we find a critical photon number ncrit = 4.4×10^4 close to the estimated value and verify that the excitation probability remains below 2.2% for all photon numbers. For optimal precision, we then use a photon number close to the critical value and perform single-shot measurements of the atom number that show a linear correlation between the results of the nondestructive detection method using the dispersive shift and the destructive detection with a microchannel plate. We achieve a single-shot uncertainty of delta N = 65 in the nondestructive atom number detection, which is close to the width of a Poissonian distribution square-root(N) = 25 for the highest atom numbers N = 600. We estimate that the precision in the single-shot measurements can be further enhanced to delta N = 5 (delta N/N = 1 %) by using quantum-limited amplifiers and increasing the single-shot integration time with Stark deceleration of the Rydberg atoms. Such precise nondestructive single-shot measurements of the number of Rydberg atoms are relevant for the quantitative evaluation of scattering cross-sections in experiments with Rydberg atoms and molecules. Moreover, the demonstrated collective coupling strengths open up the prospect for hybrid cavity QED with Rydberg atoms and superconducting quantum bits in rectangular waveguide cavities.
We propose a quantum nondemolition measurement of the photon-number distribution for a two-mode cavity field. In the scheme two sequences of two-level atoms interact dispersively with the respective cavity modes and resonantly with two classical fields, and then are detected continually. The field finally reduces to a two-mode Fock state. The probability of collapsing to a given Fock state is determined by the initial photon-number distribution. The scheme can be easily generalized to a field with N modes.