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相关论文: Red Shift from Gravitational Back Reaction

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In this lecture I address the issue of possible large distance modification of gravity and its observational consequences. Although, for the illustrative purposes we focus on a particular simple generally-covariant example, our conclusions…

高能物理 - 理论 · 物理学 2007-05-23 Gia Dvali

Newton's second law: "force = time-derivative of momentum", may also be defined for theories of gravitation endowing space-time with a curved metric. Thus, Einstein's assumption of a geodesic motion may be rewritten in that form, and it…

综合物理 · 物理学 2007-05-23 Mayeul Arminjon

The late-time cosmic acceleration may be due to infra-red modifications of General Relativity. In particular, we consider a maximal extension of the Hilbert-Einstein action and analyze several interesting features of the theory. Generally,…

广义相对论与量子宇宙学 · 物理学 2012-10-30 Tiberiu Harko , Francisco S. N. Lobo

A photon emitted near a compact object at an angle $\alpha$ with respect to the radial direction escapes to infinity at a different angle $\psi>\alpha$. This bending of light is caused by a strong gravitational field. We show that, in a…

天体物理学 · 物理学 2009-11-07 Andrei M. Beloborodov

At the present moment, there is an unresolved problem in the physics of cosmic rays. The problem concerns the origin of the ultrahigh energy cosmic rays. One of the possible mechanisms of the particle's birth with such energy is bound to…

广义相对论与量子宇宙学 · 物理学 2020-11-05 M. A. Misyura

A simple general relativity theory for objects moving in gravitational fields is developed based on studying the behavior of an atom in a gravitational field. The theory is applied to calculate the satellite time dilation, light deflection…

综合物理 · 物理学 2007-05-23 Yehea I. Ismail

A key observational prediction of Einstein's Equivalence Principle is that light undergoes redshift when it escapes from a gravitational field. Although astrophysics provides a wide variety of physical conditions in which this redshift…

星系天体物理 · 物理学 2022-04-20 Carlos M. Gutiérrez , Nataliya Ramos-Chernenko

The gravitational field of a particle of small mass $\mu$ moving through curved spacetime, with metric $g_{ab}$, is naturally and easily decomposed into two parts each of which satisfies the perturbed Einstein equations through $O(\mu)$.…

广义相对论与量子宇宙学 · 物理学 2009-09-01 Steven Detweiler

We give a short personally-biased review on the recent progress in our understanding of gravitational radiation reaction acting on a point particle orbiting a black hole. The main motivation of this study is to obtain sufficiently precise…

广义相对论与量子宇宙学 · 物理学 2009-11-11 Takahiro Tanaka

It has always been considered a serious error to treat the cosmological redshift as a Doppler velocity effect rather than the result of space expansion. It is demonstrated here that in practical terms this is not the case, and that the…

综合物理 · 物理学 2007-05-23 Alasdair Macleod

It is shown by the author that if gravitons are super-strong interacting particles and the low-temperature graviton background exists, the basic cosmological conjecture about the Dopplerian nature of redshifts may be false. In this case, a…

高能物理 - 理论 · 物理学 2007-05-23 Michael A. Ivanov

A relativistic transformation of the electrode potential has been derived to account for time dilation effects in electrode processes. This newly formulated Lorentz transformation is interpreted in terms of the generation of spin-2 boson…

综合物理 · 物理学 2026-03-27 Mirza Wasif Baig

Gravity is related to gravitational mass of the bodies. According to the weak form of Einstein's General Relativity equivalence principle, the gravitational and inertial masses are equivalent. However recent calculations (gr-qc/9910036)…

广义相对论与量子宇宙学 · 物理学 2014-11-17 Fran De Aquino

At gravitational interactions of bodies and particles there appears the defect of masses, i.e. the energy yields since the bodies (or particles) are attracted. It is shown that this changing of the effective mass of the body (or the…

天体物理学 · 物理学 2007-05-23 Kh. M. Beshtoev

Gravitational redshift is generally reported by most of the authors without considering the influence of the energy of the test particle using various spacetime geometries such as Schwarzschild, Reissner-Nordstrom, Kerr and Kerr-Newman…

综合物理 · 物理学 2017-10-06 Anuj Kumar Dubey , A. K. Sen , Bijoy Mazumdar

General relativistic deflection of light by mass, dipole, and quadrupole moments of gravitational field of a moving massive planet in the Solar system is derived in the approximation of the linearized Einstein equations. All terms of order…

广义相对论与量子宇宙学 · 物理学 2007-12-05 Sergei Kopeikin , Valeri Makarov

It is known that a relative translational motion between the deflector and the observer affects gravitational lensing. In this paper, a lens equation is obtained to describe such effects on actual lensing observables. Results can be easily…

天体物理学 · 物理学 2008-11-26 M. Sereno

Gravitational redshift is being generally calculated without considering the rotation of a body. Neglecting the rotation, the geometry of space time can be described by using the spherically symmetric Schwarzschild geometry. Rotation has…

广义相对论与量子宇宙学 · 物理学 2013-10-04 Anuj Kumar Dubey , Asoke Kumar Sen

Gravitational redshift is discussed in the context of quantum photons propagating in curved spacetime. A brief introduction to modelling realistic photons is first presented and the effect of gravity on the spectrum computed for photons…

When rotation is not taken into account, the measurement of the Gravitational Redshift can provide unique information about the compactness ($M/R$) of the star. Rotation alters the gravitational redshift rendering thereby a unique…

天体物理学 · 物理学 2011-06-10 Paul Nunez , Marek Nowakowski