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The equations of motion of $N$ gravitationally bound bodies are derived from the field equations of Projective Unified Field Theory. The Newtonian and the post-Newtonian approximations of the field equations and of the equations of motion…

广义相对论与量子宇宙学 · 物理学 2012-05-18 Alexander Gorbatsievich , Ernst Schmutzer

A point mass at the center of an ellipsoidal homogeneous fluid is used as a simple model to study the effect of rotation on the shape and external gravitational field of planets and stars. Maclaurin's analytical result for a homogenous body…

天体物理学 · 物理学 2014-05-07 Hanno Essen

The evidence for the accelerated expansion of the universe and the time-dependence of the fine-structure constant suggests the existence of at least one scalar field with a mass of order H_0. If such a field exists, then it is generally…

天体物理学 · 物理学 2009-11-10 Justin Khoury , Amanda Weltman

Post-Newtonian theory was instrumental in conducting the critical experimental tests of general relativity and in building the astronomical ephemerides of celestial bodies in the solar system with an unparalleled precision. The cornerstone…

广义相对论与量子宇宙学 · 物理学 2012-09-06 Sergei Kopeikin

We test numerically the recently proposed linear relationship between the scale-invariant period $T_{\rm s.i.} = T |E|^{3/2}$, and the topology of an orbit, on several hundred planar Newtonian periodic three-body orbits. Here $T$ is the…

经典物理 · 物理学 2018-12-31 V. Dmitrašinović , Ana Hudomal , Mitsuru Shibayama , Ayumu Sugita

The notions of centrifugal (centripetal) and Coriolis velocities and accelerations are introduced and considered in spaces with affine connections and metrics used as models of space or of space-time. It is shown that these types of…

广义相对论与量子宇宙学 · 物理学 2018-02-14 Sawa Manoff

Kepler's orbits with corrections due to Special Relativity are explored using the Lagrangian formalism. A very simple model includes only relativistic kinetic energy by defining a Lagrangian that is consistent with both the relativistic…

地球与行星天体物理 · 物理学 2016-04-21 Tyler J. Lemmon , Antonio R. Mondragon

In recent years it has been shown that the tidal coupling between extrasolar planets and their stars could be an important mechanism leading to orbital evolution. Both the tides the planet raises on the star and vice versa are important and…

太阳与恒星天体物理 · 物理学 2015-05-27 Kaloyan Penev , Dimitar Sasselov

The two dominant features in the distribution of orbital parameters for close-in exoplanets are the prevalence of circular orbits for very short periods, and the observation that planets on closer orbits tend to be heavier. The first…

地球与行星天体物理 · 物理学 2015-05-27 Frederic Pont , Nawal Husnoo , Tsevi Mazeh , Daniel Fabrycky

Context: Tidal and rotational deformation of fluid giant extra-solar planets may impact their transit light curves, making the $k_2$ Love number observable in the upcoming years. Studying the sensitivity of $k_2$ to mass concentration at…

地球与行星天体物理 · 物理学 2023-08-02 Anastasia Consorzi , Daniele Melini , Giorgio Spada

Most of the logical objections against the classical laws of motion, as they are usually presented in textbooks, centre on the fact that defining force in terms of mass and acceleration, the first two laws are mere assertions of concepts to…

综合物理 · 物理学 2007-05-23 R Assumpcao

Using a new approach, we have obtained a formula for calculating the rotation period and radius of planets. In the ordinary gravitomagnetism the gravitational spin ($S$) orbit ($L$) coupling, $\vec{L}\cdot\vec{S}\propto L^2$, while our…

综合物理 · 物理学 2013-11-07 A. I. Arbab , Saadia E. Salih , Sultan H. Hassan , Ahmed Agali , Husam Abubaker

A statistical thermodynamic approach of moving particles forming an elastic body is presented which leads to reveal molecular-mechanical properties of classical and nonextensive dynamical systems. We derive the Boltzmann-Gibbs (BG) entropy…

统计力学 · 物理学 2009-11-10 Enrique Canessa

The equations of the relativistic causal Newton gravity law for the planets of the solar system are studied in the approximation when the Sun rests at the coordinate origin and the planets do not interact between each other. The planet…

数学物理 · 物理学 2013-11-05 Yury M. Zinoviev

We derive a simple analytical expression for the two-body force in a sub-class of MOND-like theories and make testable predictions in the modification to the two-body orbital period, shape, and precession rate, and escape speed etc. We…

星系天体物理 · 物理学 2010-11-11 Hongsheng Zhao , Baojiu Li , Olivier Bienaymé

We summarize a recent work on the title subject, skipping the detailed calculations but introducing the basic points with enough detail. The theory considered is formulated in a preferred reference frame in a four-dimensional spacetime…

综合物理 · 物理学 2017-10-18 Mayeul Arminjon

The classical Laplace surface defines the location of circular particle orbits that do not undergo nodal precession around a planet with some obliquity. Close to the planet the surface coincides with the equator of the planet, while far…

地球与行星天体物理 · 物理学 2025-04-01 Stephen H. Lubow , Gordon I. Ogilvie

Both Stefan-Boltzmann law and the Casimir effect, in a universe described by the FRW metric with zero curvature, are calculated. These effects are described by Thermo Field Dynamics (TFD). The gravitational energy-momentum tensor is defined…

广义相对论与量子宇宙学 · 物理学 2022-04-20 A. F. Santos , S. C. Ulhoa , E. P. Spaniol , Faqir C. Khanna

In this paper we present a new approach to tidal theory. Assuming a Maxwell viscoelastic rheology, we compute the instantaneous deformation of celestial bodies using a differential equation for the gravity field coefficients. This method…

地球与行星天体物理 · 物理学 2014-11-19 Alexandre C. M. Correia , Gwenaël Boué , Jacques Laskar , Adrián Rodríguez

With the discovery during the past decade of a large number of extrasolar planets orbiting their parent stars at a distance lower than 0.1 astronomical unit (and the launch and the preparation of dedicated space missions such as CoRoT and…

天体物理学 · 物理学 2008-12-12 Stephane Mathis , Christophe Le Poncin-Lafitte