29,223 research outputs found

    Apollo docking test device design study final report

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    Docking simulation system for confirming Apollo probe design and drogue docking mechanisms under simulated space condition

    Stochastic Heisenberg limit: Optimal estimation of a fluctuating phase

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    The ultimate limits to estimating a fluctuating phase imposed on an optical beam can be found using the recently derived continuous quantum Cramer-Rao bound. For Gaussian stationary statistics, and a phase spectrum scaling asymptotically as 1/omega^p with p>1, the minimum mean-square error in any (single-time) phase estimate scales as N^{-2(p-1)/(p+1)}, where N is the photon flux. This gives the usual Heisenberg limit for a constant phase (as the limit p--> infinity) and provides a stochastic Heisenberg limit for fluctuating phases. For p=2 (Brownian motion), this limit can be attained by phase tracking.Comment: 5+4 pages, to appear in Physical Review Letter

    On the size of approximately convex sets in normed spaces

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    Let X be a normed space. A subset A of X is approximately convex if d(ta+(1t)b,A)1d(ta+(1-t)b,A) \le 1 for all a,bAa,b \in A and t[0,1]t \in [0,1] where d(x,A)d(x,A) is the distance of xx to AA. Let \Co(A) be the convex hull and \diam(A) the diameter of AA. We prove that every nn-dimensional normed space contains approximately convex sets AA with \mathcal{H}(A,\Co(A))\ge \log_2n-1 and \diam(A) \le C\sqrt n(\ln n)^2, where H\mathcal{H} denotes the Hausdorff distance. These estimates are reasonably sharp. For every D>0D>0, we construct worst possible approximately convex sets in C[0,1]C[0,1] such that \mathcal{H}(A,\Co(A))=\diam(A)=D. Several results pertaining to the Hyers-Ulam stability theorem are also proved.Comment: 32 pages. See also http://www.math.sc.edu/~howard

    Extremal Approximately Convex Functions and Estimating the Size of Convex Hulls

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    A real valued function ff defined on a convex KK is anemconvex function iff it satisfies f((x+y)/2)(f(x)+f(y))/2+1. f((x+y)/2) \le (f(x)+f(y))/2 + 1. A thorough study of approximately convex functions is made. The principal results are a sharp universal upper bound for lower semi-continuous approximately convex functions that vanish on the vertices of a simplex and an explicit description of the unique largest bounded approximately convex function~EE vanishing on the vertices of a simplex. A set AA in a normed space is an approximately convex set iff for all a,bAa,b\in A the distance of the midpoint (a+b)/2(a+b)/2 to AA is 1\le 1. The bounds on approximately convex functions are used to show that in Rn\R^n with the Euclidean norm, for any approximately convex set AA, any point zz of the convex hull of AA is at a distance of at most [log2(n1)]+1+(n1)/2[log2(n1)][\log_2(n-1)]+1+(n-1)/2^{[\log_2(n-1)]} from AA. Examples are given to show this is the sharp bound. Bounds for general norms on RnR^n are also given.Comment: 39 pages. See also http://www.math.sc.edu/~howard

    Concepts of quantum non-Markovianity: a hierarchy

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    Markovian approximation is a widely-employed idea in descriptions of the dynamics of open quantum systems (OQSs). Although it is usually claimed to be a concept inspired by classical Markovianity, the term quantum Markovianity is used inconsistently and often unrigorously in the literature. In this report we compare the descriptions of classical stochastic processes and quantum stochastic processes (as arising in OQSs), and show that there are inherent differences that lead to the non-trivial problem of characterizing quantum non-Markovianity. Rather than proposing a single definition of quantum Markovianity, we study a host of Markov-related concepts in the quantum regime. Some of these concepts have long been used in quantum theory, such as quantum white noise, factorization approximation, divisibility, Lindblad master equation, etc.. Others are first proposed in this report, including those we call past-future independence, no (quantum) information backflow, and composability. All of these concepts are defined under a unified framework, which allows us to rigorously build hierarchy relations among them. With various examples, we argue that the current most often used definitions of quantum Markovianity in the literature do not fully capture the memoryless property of OQSs. In fact, quantum non-Markovianity is highly context-dependent. The results in this report, summarized as a hierarchy figure, bring clarity to the nature of quantum non-Markovianity.Comment: Clarifications and references added; discussion of the related classical hierarchy significantly improved. To appear in Physics Report

    The quantum Bell-Ziv-Zakai bounds and Heisenberg limits for waveform estimation

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    We propose quantum versions of the Bell-Ziv-Zakai lower bounds on the error in multiparameter estimation. As an application we consider measurement of a time-varying optical phase signal with stationary Gaussian prior statistics and a power law spectrum 1/ωp\sim 1/|\omega|^p, with p>1p>1. With no other assumptions, we show that the mean-square error has a lower bound scaling as 1/N2(p1)/(p+1)1/{\cal N}^{2(p-1)/(p+1)}, where N{\cal N} is the time-averaged mean photon flux. Moreover, we show that this accuracy is achievable by sampling and interpolation, for any p>1p>1. This bound is thus a rigorous generalization of the Heisenberg limit, for measurement of a single unknown optical phase, to a stochastically varying optical phase.Comment: 18 pages, 6 figures, comments welcom

    Optimal Heisenberg-style bounds for the average performance of arbitrary phase estimates

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    The ultimate bound to the accuracy of phase estimates is often assumed to be given by the Heisenberg limit. Recent work seemed to indicate that this bound can be violated, yielding measurements with much higher accuracy than was previously expected. The Heisenberg limit can be restored as a rigorous bound to the accuracy provided one considers the accuracy averaged over the possible values of the unknown phase, as we have recently shown [Phys. Rev. A 85, 041802(R) (2012)]. Here we present an expanded proof of this result together with a number of additional results, including the proof of a previously conjectured stronger bound in the asymptotic limit. Other measures of the accuracy are examined, as well as other restrictions on the generator of the phase shifts. We provide expanded numerical results for the minimum error and asymptotic expansions. The significance of the results claiming violation of the Heisenberg limit is assessed, followed by a detailed discussion of the limitations of the Cramer-Rao bound.Comment: 22 pages, 4 figure
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