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Particle sedimentation in the vicinity of a fixed horizontal vortex with time-dependent intensity can be chaotic, provided gravity is sufficient to displace the particle cloud while the vortex is off or weak. This "stretch, sediment and…

流体动力学 · 物理学 2010-03-23 J. R. Angilella

We study the motion of a charged particle in a tokamak magnetic field and discuss its chaotic nature. Contrary to most of recent studies, we do not make any assumption on any constant of the motion and solve numerically the cyclotron…

混沌动力学 · 物理学 2014-12-05 Benjamin Cambon , Xavier Leoncini , Michel Vittot , Rémi Dumont , Xavier Garbet

$f(R)$ theories of gravity are one of the most popular alternative explanations for dark energy and therefore studying the possible astrophysical implications of these theories is an important task. In the present paper we make a…

广义相对论与量子宇宙学 · 物理学 2015-06-23 Stoytcho S. Yazadjiev , Daniela D. Doneva , Kostas D. Kokkotas

The motion of massive test particles in dark matter is studied. It is shown that if the energy density of the dark matter making up a galactic halo has a large $r$ behavior of $1/r^2$, then contrary to intuition the motion of these test…

高能物理 - 唯象学 · 物理学 2008-02-03 Achilles D. Speliotopoulos

As a first step towards a comprehensive investigation of stellar motions within globular clusters, we present here the results of a study of stellar orbits in a mildly triaxial globular cluster that follows a circular orbit inside a galaxy.…

天体物理学 · 物理学 2009-10-31 D. D. Carpintero , J. C. Muzzio , F. C. Wachlin

The gravitational potentials of realistic galaxy models are in general non-integrable, in the sense that they admit orbits that do not have three independent isolating integrals of motion and are therefore chaotic. However, if chaotic…

星系天体物理 · 物理学 2021-09-29 R. Pascale , C. Nipoti , L. Ciotti

The bulk viscosity in quark matter is sufficiently high to reduce the effective pressure below the corresponding vapor pressure during density perturbations in neutron stars and strange stars. This leads to mechanical instability where the…

太阳与恒星天体物理 · 物理学 2009-09-30 Jes Madsen

The observational data from some black hole candidates suggest the importance of electromagnetic fields in the vicinity of a black hole. Highly magnetized disk accretion may play an importance rule, and large scale magnetic field may be…

天体物理学 · 物理学 2011-02-11 Masaaki Takahashi , Hiroko Koyama

The dynamical status of isolated quantum systems, partly due to the linearity of the Schrodinger equation is unclear: Conventional measures fail to detect chaos in such systems. However, when quantum systems are subjected to observation --…

量子物理 · 物理学 2009-11-10 Salman Habib , Kurt Jacobs , Kosuke Shizume

Coherent motion of cold atoms in a standing-wave field is interpreted as a propagation in two optical potentials. It is shown that the wave-packet dynamics can be either regular or chaotic with transitions between these potentials after…

量子物理 · 物理学 2012-01-06 S. V. Prants

We investigate dynamics of a jet collimated by magneto-torsional oscillations. The problem is reduced to an ordinary differential equation containing a singularity and depending on a parameter. We find a parameter range for which this…

宇宙学与河外天体物理 · 物理学 2011-07-21 G. S. Bisnovatyi-Kogan , A. I. Neishtadt , Z. F. Seidov , O. Yu. Tsupko , Yu. M. Krivosheyev

We investigate the evolution of the relative angle between the stellar rotation axis and the circumstellar disc axis of a star that forms in a stellar cluster from the collapse of a turbulent molecular cloud. This is an inherently chaotic…

太阳与恒星天体物理 · 物理学 2015-05-14 M. R. Bate , G. Lodato , J. E. Pringle

We investigate the orbits of compact binary systems during the final inspiral period before coalescence by integrating numerically the second-order post-Newtonian equations of motion. We include spin-orbit and spin-spin coupling terms,…

广义相对论与量子宇宙学 · 物理学 2009-11-07 Jeremy D. Schnittman , Frederic A. Rasio

We consider test particle motion in a gravitational field generated by a homogeneous circular ring placed in $n$-dimensional Euclidean space. We observe that there exist no stable stationary orbits in $n=6, 7, \ldots, 10$ but exist in $n=3,…

广义相对论与量子宇宙学 · 物理学 2020-08-18 Takahisa Igata

We study the chaotic dynamics of spinless extended bodies in a wide class of spherically symmetric spacetimes, which encompasses black-hole scenarios in many modified theories of gravity. We show that a spherically symmetric pulsating ball…

广义相对论与量子宇宙学 · 物理学 2024-10-01 Fernanda de F. Rodrigues , Ricardo A. Mosna , Ronaldo S. S. Vieira

We study the geodesic motion of test particles in the space-time of non-compact boson stars. These objects are made of a self-interacting scalar field and -- depending on the scalar field's mass -- can be as dense as neutron stars or even…

广义相对论与量子宇宙学 · 物理学 2013-08-21 Valeria Diemer , Keno Eilers , Betti Hartmann , Isabell Schaffer , Catalin Toma

We study the motion of test particles around a center of attraction represented by a monopole (with and without spheroidal deformation) surrounded by a ring, given as a superposition of Morgan & Morgan discs. We deal with two kinds of…

地球与行星天体物理 · 物理学 2012-09-24 Javier Ramos-Caro , Juan F. Pedraza , Patricio S. Letelier

The Rayleigh criterion is used to study the stability of circular orbits of particles moving around static black holes surrounded by different axially symmetric structures with reflection symmetry, like disks, rings and halos. We consider…

广义相对论与量子宇宙学 · 物理学 2009-11-10 Patricio. S. Letelier

A set of theoretical mass-radius relations for rigidly rotating neutron stars with exotic cores, obtained in various theories of dense matter, is reviewed. Two basic observational constraints are used: the largest measured rotation…

高能天体物理现象 · 物理学 2016-04-20 P. Haensel , M. Bejger , M. Fortin , J. L. Zdunik

We extend recent investigations on the integrability of oblique orbits of test particles under the gravitational field corresponding to the superposition of an infinitesimally thin disk and a monopole to the more realistic case, for…

广义相对论与量子宇宙学 · 物理学 2009-10-31 Alberto Saa