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相关论文: Ergodic Considerations in the Gravitational Potent…

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In a previous paper, using ergodic theory, Lo [1] derived a simple definite integral that provided an estimate of the view periods of ground stations to satellites. This assumes the satellites are in circular orbits with non-repeating…

地球与行星天体物理 · 物理学 2020-10-14 Andrew J. Graven , Martin W. Lo

Selection effects, such as interstellar extinction and varying survey depth, complicate efforts to determine the gravitational potential - and thus the distribution of baryonic and dark matter - throughout the Milky Way galaxy using stellar…

星系天体物理 · 物理学 2025-12-03 Taavet Kalda , Gregory Green

We present a novel method for constraining the length of the Galactic bar using 6D phase space information to directly integrate orbits. We define a pseudo-length for the Galactic bar, named $R_{Freq}$, based on the maximal extent of…

Recently, ergodic control has been suggested as a means to guide mobile sensors for information gathering tasks. In ergodic control, a mobile sensor follows a trajectory that is ergodic with respect to some information density distribution.…

系统与控制 · 计算机科学 2018-08-22 Louis Dressel , Mykel J. Kochenderfer

One of the major goals of the field of Milky Way dynamics is to recover the gravitational potential field. Mapping the potential would allow us to determine the spatial distribution of matter - both baryonic and dark - throughout the…

星系天体物理 · 物理学 2023-01-11 Gregory M. Green , Yuan-Sen Ting , Harshil Kamdar

One of the major goals of the field of Milky Way dynamics is to recover the gravitational potential field. Mapping the potential would allow us to determine the spatial distribution of matter - both baryonic and dark - throughout the…

星系天体物理 · 物理学 2020-11-11 Gregory M. Green , Yuan-Sen Ting

Quantifying long-term statistical properties of satellite trajectories typically entails time-consuming trajectory propagation. We present a fast, ergodic\cite{Arnold} method of analytically estimating these for $J_2-$perturbed elliptical…

地球与行星天体物理 · 物理学 2021-02-09 Andrew J. Graven , Alan H. Barr , Martin W. Lo

We develop two general methods to infer the gravitational potential of a system using steady-state tracers, i.e., tracers with a time-independent phase-space distribution. Combined with the phase-space continuity equation, the time…

星系天体物理 · 物理学 2016-01-13 Jiaxin Han , Wenting Wang , Shaun Cole , Carlos S. Frenk

In the framework of statistical mechanics the properties of macroscopic systems are deduced starting from the laws of their microscopic dynamics. One of the key assumptions in this procedure is the ergodic property, namely the equivalence…

统计力学 · 物理学 2024-01-09 Marco Baldovin , Raffaele Marino , Angelo Vulpiani

We present a method to calculate gravitational potential gradients within regions containing few tens of thousands stars with known phase space coordinates. The central idea of the method is to calculate orbital arcs for each star within a…

星系天体物理 · 物理学 2018-10-10 Rain Kipper , Elmo Tempel , Peeter Tenjes

The information contained in galactic rotation curves is examined under a minimal set of assumptions. If emission occurs from stable circular geodesic orbits of a static spherically symmetric field, with information propagated to us along…

广义相对论与量子宇宙学 · 物理学 2009-11-10 Kayll Lake

Ergodic Optimization is the process of finding invariant probability measures that maximize the integral of a given function. It has been conjectured that "most" functions are optimized by measures supported on a periodic orbit, and it has…

动力系统 · 数学 2015-03-17 Anthony Quas , Jason Siefken

We present a method to constrain the potential of the non-axisymmetric components of the Galaxy using the kinematics of stars in the solar neighborhood. The basic premise is that dynamical substructures in phase-space (i.e. due to the bar…

星系天体物理 · 物理学 2015-05-30 Giacomo Monari , Teresa Antoja , Amina Helmi

To evaluate a potential usually one analyzes trajectories of test particles. For the Galactic Center case astronomers use bright stars or photons, so there are two basic observational techniques to investigate a gravitational potential,…

广义相对论与量子宇宙学 · 物理学 2019-01-25 Alexander Zakharov

Advancement in astronomical observations and technical instrumentation implies taking into account the general relativistic effects due the gravitational fields encountered by the light while propagating from the star to the observer.…

星系天体物理 · 物理学 2013-05-22 Mariateresa Crosta

In this paper we prove the following result, useful and often needed in the study of the ergodic properties of hard ball systems: In any such system, for any phase point x with a non-singular forward trajectory and infinitely many connected…

动力系统 · 数学 2007-05-23 Nandor Simanyi

We present a new method for inferring the gravitational potential of the Galactic disk, using the time-varying structure of a phase-space spiral in the $(z,w)$-plane (where $z$ and $w$ represent vertical position and vertical velocity). Our…

星系天体物理 · 物理学 2021-11-30 Axel Widmark , Chervin F. P. Laporte , Pablo F. de Salas

In search and surveillance applications in robotics, it is intuitive to spatially distribute robot trajectories with respect to the probability of locating targets in the domain. Ergodic coverage is one such approach to trajectory planning…

机器人学 · 计算机科学 2017-07-25 Elif Ayvali , Hadi Salman , Howie Choset

In this paper we establish the ergodicity of Langevin dynamics for simple two-particle system involving a Lennard-Jones type potential. To the best of our knowledge, this is the first such result for a system operating under this type of…

We study the ergodic properties of a two-dimensional self-gravitating system using molecular dynamics simulations. We apply three different tests for ergodicity: a direct method comparing the time average of a particle momentum and position…

统计力学 · 物理学 2016-01-20 C. H. Silvestre , T. M. Rocha Filho
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