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Alternative theories of gravity not only modify the polarization contents of the gravitational wave, but also affect the motions of the stars and the energy radiated away via the gravitational radiation. These aspects leave imprints in the…

广义相对论与量子宇宙学 · 物理学 2018-03-28 Shaoqi Hou , Yungui Gong

Gravitational lens models, some of which might act as if a concave lens, have been recently investigated by using a static and spherically symmetric modified spacetime metric that depends on the inverse distance to the $n$-th power…

广义相对论与量子宇宙学 · 物理学 2015-06-19 Koki Nakajima , Koji Izumi , Hideki Asada

A new iterative method for calculating the travel time of a photon as a function of the spatial positions of the emitter and the receiver in the field of a static, spherically symmetric body is presented. The components of the metric are…

广义相对论与量子宇宙学 · 物理学 2015-06-15 Bernard Linet , Pierre Teyssandier

The light trajectory in the gravitational field of one body at rest with monopole and quadrupole structure is determined in the second post-Newtonian (2PN) approximation. The terms in the geodesic equation for light rays are separated into…

广义相对论与量子宇宙学 · 物理学 2022-01-26 Sven Zschocke

We consider an alternative formula for time delay in gravitational lensing. Imposing a smoothness condition on the gravitationally deformed paths followed by the photons from the source to the observer, we show that our formula displays the…

宇宙学与河外天体物理 · 物理学 2018-07-04 Nicola Alchera , Marco Bonici , Roberta Cardinale , Alba Domi , Nicola Maggiore , Chiara Righi , Silvano Tosi

As an extension of a previous work in which perihelion advances are considered only and as an attempt to find more stringent constraints on its parameters, we investigate effects on astronomical observation and experiments conducted in the…

广义相对论与量子宇宙学 · 物理学 2013-12-17 Yi Xie , Xue-Mei Deng

The Sun's gravitational field deflects the apparent positions of close objects in accordance with the formulae of general relativity. Optical astrometry is used to test the prediction, but only with the stars close to the Sun and only…

广义相对论与量子宇宙学 · 物理学 2015-11-03 O. Titov , A. Girdiuk

Freire et al. (2009, MNRAS, 396, 1764) have put forward a technique for timing the double pulsar system PSR J0737-3039A/B (hereafter A and B, respectively). Their technique can be used to determine the sense of rotation of A relative to its…

太阳与恒星天体物理 · 物理学 2014-02-05 Zhu-Xing Liang , Yi Liang

Synergies between self-force theory and other approaches to the gravitational two-body problem have traditionally relied on calculations of gauge-invariant observables as functions of orbital frequencies. However, in self-force theory one…

广义相对论与量子宇宙学 · 物理学 2026-02-26 David Trestini , Zachary Nasipak , Adam Pound

General Relativity (GR) is shown to be a complete theory with respect to the isochrony of the pendulum. This guarantees that time can be measured with a mechanical clock within the theory itself as a matter of principle. The proper and…

广义相对论与量子宇宙学 · 物理学 2022-05-06 Miguel A. Martin-Delgado

By using the Gauss-Bonnet theorem, the bending angle of light in a static, spherically symmetric and asymptotically flat spacetime has been recently discussed, especially by taking account of the finite distance from a lens object to a…

广义相对论与量子宇宙学 · 物理学 2017-11-29 Toshiaki Ono , Asahi Ishihara , Hideki Asada

Time-domain (TD) Bayesian inference is important in ringdown analysis for gravitational wave (GW) astronomy. The validity of this method has been well studied by Isi and Farr [1]. Using GW190521 as an example, we study the TD method in…

广义相对论与量子宇宙学 · 物理学 2024-09-04 Hai-Tian Wang , Lijing Shao

A simplified formula for light-deflection in the quadrupole field of moving massive bodies has been obtained in [1,2,3], which will be applied for Gaia data reduction. So far, in Gaia data reduction it has been assumed that the positions of…

广义相对论与量子宇宙学 · 物理学 2011-05-17 Sven Zschocke

In this paper we first calculate the post-Newtonian gravitoelectric secular rate of the mean anomaly of a test particle freely orbiting a spherically symmetric central mass. Then, we propose a novel approach to suitably combine the…

广义相对论与量子宇宙学 · 物理学 2011-05-23 Lorenzo Iorio

The Sagnac effect is a time or phase shift observed between two beams of light traveling in opposite directions in a rotating interferometer. We show that the standard description of this effect within the framework of general relativity…

广义相对论与量子宇宙学 · 物理学 2012-06-12 Paolo Maraner , Jean-Pierre Zendri

New techniques to evaluate the clock effect using light are described. These are based on the flatness of the cylindrical surface containing the world lines of the rays constrained to move on circular trajectories about a spinning mass. The…

广义相对论与量子宇宙学 · 物理学 2009-10-31 A. Tartaglia

The general relativistic gravitomagnetic clock effect consists in the fact that two massive test bodies orbiting a central spinning mass in its equatorial plane along two identical circular trajectories, but in opposite directions, take…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Lorenzo Iorio

General relativity predicts that two counter-orbiting clocks around a spinning mass differ in the time required to complete the same orbit. The difference in these two values for the orbital period is generally referred to as the…

广义相对论与量子宇宙学 · 物理学 2024-03-26 Kaye Jiale Li , Kinwah Wu , Ziri Younsi , Joana Teixeira , Dinesh Singh

Using a cylindrical soliton solution to the four-dimensional vacuum Einstein equation, we study non-linear effects of gravitational waves such as Faraday rotation and time shift phenomenon. In the previous work, we analyzed the…

广义相对论与量子宇宙学 · 物理学 2015-06-24 Shinya Tomizawa , Takashi Mishima

Classical soft photon and soft graviton theorems determine long wavelength electromagnetic and gravitational waveforms for a general classical scattering process in terms of the electric charges and asymptotic momenta of the ingoing and…

高能物理 - 理论 · 物理学 2020-12-30 Biswajit Sahoo