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International Conference on Signal Propagation and Computer Technology (ICSPCT)

Estimation of Variance and Skewness of non-Gaussian zero mean white noise from measurements of the atomic transition probabilities

Kapil Prajapati, Harish Parthasarthy

Published Jul 1, 2014• 0 citations
Publisher

Abstract

Estimation of noise parameters is always an important and tedious task when the system under consideration is of the order of atomic level. The majority of estimation algorithms available in the literature assume that the additive noise has a Gaussian distribution. Though it is good model for thermal noise, but in the real world, noise experienced is due to a variety of man-made sources, which deviates from the Gaussian way and is non-Gaussian in nature. Though there are other methods to estimate the parameters of a random non-Gaussian process, for e.g. - Maximum Likelihood Estimator (MLE). In order to construct the MLE of σ2and γ based on quantum measurement would involve constructing the joint pdf of the samples of complex wave function at discrete times. This would be a highly nonlinear function of σ2and γ. The optimization would involve computationally heavy search algorithms. Moments matching is simpler though sub optimal and hence, we have chosen this. In this paper, we proposed a new method to estimate the parameters of non-Gaussian random process based on the higher order statistics (spectra) analysis and quantum measurement which involve the measurement of atomic transition probabilities. Simulated results and comparison between the theoretical values of Variance (finite) and Skewness (non-zero triple moment) have been presented here.

DOI
10.1109/icspct.2014.6884940

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Estimation of noise parameters is always an important and tedious task when the system under consideration is of the order of atomic level. The majority of estimation algorithms available in the literature assume that the additive noise has a Gaussian distribution. Though it is good model for thermal noise, but in the real world, noise experienced is due to a variety of man-made sources, which deviates from the Gaussian way and is non-Gaussian in nature. Though there are other methods to estimate the parameters of a random non-Gaussian process, for e.g. - Maximum Likelihood Estimator (MLE). In order to construct the MLE of σ2and γ based on quantum measurement would involve constructing the joint pdf of the samples of complex wave function at discrete times. This would be a highly nonlinear function of σ2and γ. The optimization would involve computationally heavy search algorithms. Moments matching is simpler though sub optimal and hence, we have chosen this. In this paper, we proposed a new method to estimate the parameters of non-Gaussian random process based on the higher order statistics (spectra) analysis and quantum measurement which involve the measurement of atomic transition probabilities. Simulated results and comparison between the theoretical values of Variance (finite) and Skewness (non-zero triple moment) have been presented here.
Many quantum algorithms contain an important subroutine---the quantum amplitude estimation. As the name implies, this is essentially the parameter estimation problem and thus can be handled via the established statistical estimation theory. However, this problem has an intrinsic difficulty that the system, i.e., the real quantum computing device, inevitably introduces unknown noise; the probability distribution model then has to incorporate many nuisance noise parameters, resulting that the construction of an optimal estimator becomes inefficient and difficult. For this problem we apply the theory of nuisance parameters (more specifically, the parameter orthogonalization method) to precisely compute the maximum likelihood estimator for only the target amplitude parameter by removing the other nuisance noise parameters. That is, we can estimate the amplitude parameter without estimating the noise parameters. We validate the parameter orthogonalization method in a numerical simulation and study the performance of the estimator in the experiment using a real superconducting quantum device.
We present a new quantum algorithm for estimating the mean of a real-valued random variable obtained as the output of a quantum computation. Our estimator achieves a nearly-optimal quadratic speedup over the number of classical i.i.d. samples needed to estimate the mean of a heavy-tailed distribution with a sub-Gaussian error rate. This result subsumes (up to logarithmic factors) earlier works on the mean estimation problem that were not optimal for heavy-tailed distributions [Brassard et al., 2002; Brassard et al., 2011], or that require prior information on the variance [Heinrich, 2002; Montanaro, 2015; Hamoudi and Magniez, 2019]. As an application, we obtain new quantum algorithms for the (ε,δ)-approximation problem with an optimal dependence on the coefficient of variation of the input random variable.
We present a new quantum algorithm for estimating the mean of a real-valued random variable obtained as the output of a quantum computation. Our estimator achieves a nearly-optimal quadratic speedup over the number of classical i.i.d. samples needed to estimate the mean of a heavy-tailed distribution with a sub-Gaussian error rate. This result subsumes (up to logarithmic factors) earlier works on the mean estimation problem that were not optimal for heavy-tailed distributions [BHMT02,BDGT11], or that require prior information on the variance [Hein02,Mon15,HM19]. As an application, we obtain new quantum algorithms for the (ϵ,δ)(\epsilon,\delta)(ϵ,δ)-approximation problem with an optimal dependence on the coefficient of variation of the input random variable.
Error mitigation in a noisy quantum device requires a very good estimate of the noise channel. The accuracy of probabilistic error cancellation is often limited by the high sample complexity of channel tomography. In principle, optimal sample complexity is attained by maximum likelihood estimation (MLE), but MLE is computationally challenging. We show that MLE can be made computationally tractable in certain cases of interest. For the common case of a 1D-local sparse Pauli-Lindblad channel, the likelihood function reduces to an efficiently-evaluable Bayesian network. We show that the resulting computation leads to substantially improved tomography. In addition, we demonstrate by simulation that this can lead to meaningful improvements to the overhead of error mitigation. We also discuss possible extensions of our algorithm to more general settings, such as non-1D circuits and non-Pauli errors.
The James-Stein estimator is a biased estimator -- for a finite number of samples its expected value is not the true mean. The maximum-likelihood estimator (MLE), is unbiased and asymptotically optimal. Yet, when estimating the mean of 333 or more normally-distributed random variables, the James-Stein estimator has a smaller total (expected) error than the MLE. We introduce the James-Stein estimator to the field of quantum metrology, from both the frequentist and Bayesian perspectives. We characterise the effect of quantum phenomena on the James-Stein estimator through the lens of quantum Gaussian sensing, the task of estimating the mean of an unknown multivariate quantum Gaussian state. We find that noiseless entanglement or coherence improves performance of the James-Stein estimator, but diminishes its advantage over the MLE. In the presence of noise, the James-Stein advantage is restored. Quantum effects can also boost the James-Stein advantage. We demonstrate this by investigating multivariate postselective metrology (generalised weak-value amplification), a strategy that uses quantum effects to measure parameters with imperfect detectors. Simply by post-processing measured data differently, our techniques reduce errors in quantum experiments.
Direct measurement of quantum non-Gaussianity requires some variant of a discrete photon-resolving detection, which is feasible only for low mean photon numbers. For a large mean photon number, intensity detection by linear photodiodes provides a continuous signal; therefore, the Fock probabilities of the unknown input state are not directly available. On the other hand, intensity moments can be measured directly, and photon-number moments can be estimated. Therefore, we derive and analyze a quantum non-Gaussianity witness based solely on the photon-number mean and variance (or alternatively, the second-order correlation g ( 2 ) ) of an unknown state. Due to the simplicity of the used photon-number moments, the measurement results are easy to correct for losses and additive noise. We provide examples of simple amplification-based measurement schemes where our witness can be applied directly, thereby opening pathways to proof-of-principle tests and applications.