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The aim of this research work is to compare the reliability of several variational indicators of chaos on mappings. The Lyapunov Indicator (LI); the Mean Exponential Growth factor of Nearby Orbits (MEGNO); the Smaller Alignment Index…

混沌动力学 · 物理学 2011-08-11 N. P. Maffione , L. A. Darriba , P. M. Cincotta , C. M. Giordano

We investigate linear perturbations in the recently proposed cosmon-bolon model of coupled scalar field dark matter and quintessence. We provide an analytical mechanism to average over the quick oscillations appearing both in the background…

宇宙学与河外天体物理 · 物理学 2014-07-03 Joschka Beyer

Whether a dwarf spheroidal galaxy is in equilibrium or being tidally disrupted by the Milky Way is an important question for the study of its dark matter content and distribution. This question is investigated using 328 recent observations…

应用统计 · 统计学 2009-05-18 Bodhisattva Sen , Moulinath Banerjee , Michael Woodroofe , Mario Mateo , Matthew Walker

Synchronized chaos has previously been predicted and observed in a small number (3) of mutually coupled lasers. In this work, we demonstrate that this phenomenon can theoretically persist in significantly broader scenarios, extending to…

光学 · 物理学 2026-05-05 Zhanning Liu , Herbert G. Winful

We present the emission-line fluxes and kinematics of 48 representative elliptical and lenticular galaxies obtained with our custom-built integral-field spectrograph SAURON. Hb, [OIII], and [NI] emission lines were measured using a new…

We investigate chaos in mixed-phase-space Hamiltonian systems using time series of the finite- time Lyapunov exponents. The methodology we propose uses the number of Lyapunov exponents close to zero to define regimes of ordered…

混沌动力学 · 物理学 2015-06-16 R. M. da Silva , C. Manchein , M. W. Beims , E. G. Altmann

The microlensing signal in the light curves of gravitationally lensed quasars can shed light on the dark matter (DM) composition in their lensing galaxies. Here, we investigate a sample of six lensed quasars from the most recent and best…

星系天体物理 · 物理学 2023-04-05 Petra Awad , James H. H. Chan , Martin Millon , Frederic Courbin , Eric Paic

In recent years, the investigation of chaos has become a bridge connecting gravity theory and quantum field theory, especially within the framework of gauge-gravity duality. In this work, we study holographically the chaos in the matrix…

高能物理 - 理论 · 物理学 2025-10-07 Si-wen Li , Xun Chen

Until now, most memristor-based chaotic circuits proposed in the literature are based on mathematical models which assume ideal characteristics such as piece-wise linear or cubic non-linearities. The idea, illustrated here and originating…

混沌动力学 · 物理学 2015-09-02 L. V. Gambuzza , L. Fortuna , M. Frasca , E. Gale

Starting from the Hamiltonian representation of the dynamics in \cite{rosengren2015chaos,colombo2019long}, this work proposes an innovative procedure to design fully-analytical maneuvers for post-mission disposal of HEOs satellites,…

地球与行星天体物理 · 物理学 2024-01-29 Francesca Scala , Ioannis Gkolias , Camilla Colombo

A future measurement of Lense-Thirring (LT) precession using a binary radio pulsar is expected to yield the pulsar's moment of inertia ($I_{\rm p}$). However, most of the known pulsar-binary systems expected to provide this opportunity will…

高能天体物理现象 · 物理学 2025-12-02 Emmanuel Fonseca

Many nonlinear dynamical systems can be written as Lure systems, which are described by a linear time-invariant system interconnected with a diagonal static sector-bounded nonlinearity. Sufficient conditions are derived for the global…

系统与控制 · 计算机科学 2015-09-07 Kwang-Ki K. Kim , Richard D. Braatz

Halo coronal mass ejections (HCMEs) are responsible of the most severe geomagnetic storms. A prediction of their geoeffectiveness and travel time to Earth's vicinity is crucial to forecast space weather. Unfortunately coronagraphic…

天体物理学 · 物理学 2009-11-13 G. Michalek , N. Gopalswamy , S. Yashiro

The dynamical evolution of the Prometheus and Pandora pair of satellites is chaotic, with a short 3.3 years Lyapunov time. It is known that the anti-alignment of the apses line of Prometheus and Pandora, which occurs every 6.2 years, is a…

地球与行星天体物理 · 物理学 2022-02-16 A. R. Gomes-Júnior , T. Santana , O. C. Winter , R. Sfair

A simple model for the Milky Way halo is presented. It has a flat rotation curve in the inner regions, but the density falls off sharply beyond an outer edge. This truncated, flat rotation curve (TF) model possesses a rich family of simple…

天体物理学 · 物理学 2008-11-26 M. I. Wilkinson , N. W. Evans

The Luminous Convolution Model (LCM) is an empirical formula, based on a heuristic convolution of Relativistic transformations, which makes it possible to predict the observed rotation curves of a broad class of spiral galaxies from…

星系天体物理 · 物理学 2015-06-16 S. Cisneros , J. G. O'Brien , N. S. Oblath , J. A. Formaggio

We provide measurements of the absolute reflectivity of Jupiter and Saturn along their central meridians in filters covering a wide range of visible and near-infrared wavelengths (from 0.38 to 1.7 $\mu$m) that are not often presented in the…

地球与行星天体物理 · 物理学 2017-09-29 I. Mendikoa , A. Sánchez-Lavega , S. Pérez-Hoyos , R. Hueso , J. F. Rojas , J. López-Santiago

The amount of dark matter in the solar neighbourhood is a poorly constrained quantity which is nevertheless used to normalise the properties of the dark halo. While the current surveys towards the LMC, SMC and the Galactic bulge probe the…

天体物理学 · 物理学 2007-05-23 T. Dimeo , D. Valls-Gabaud , E. J. Kerins

Galactic transients, X-ray and gamma-ray binaries provide a proper environment for particle acceleration. This leads to the production of gamma rays with energies reaching the GeV-TeV regime. MAGIC has carried out deep observations of…

Due to the failure of the second reaction wheel, a new mission was conceived for the otherwise healthy Kepler space telescope. In the course of the K2 Mission, the telescope is staring at the plane of the Ecliptic, hence thousands of Solar…

地球与行星天体物理 · 物理学 2016-11-30 R. Szabó , A. Pál , K. Sárneczky , Gy. M. Szabó , L. Molnár , L. L. Kiss , O. Hanyecz , E. Plachy , Cs. Kiss