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We show that astrophysical gravitational waves can undergo an anomalous modulation when propagating through cosmic gauge field dark energy. A sufficiently strong effect, dependent on the gauge field energy density, would appear as a…

广义相对论与量子宇宙学 · 物理学 2019-12-17 R. R. Caldwell , C. Devulder

After a preliminary discussion of the relevance of the field nature of gravitation interaction, both for the fundamental interaction of particles and the topology of space time, a method is proposed to produce and detect a dynamical…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Bruno Ferretti

It is introduced a hypothesis that the gravitational potential in the universe changes linearly with the time. This enables to explain the Hubble red shift and the anomalous acceleration of Pioneer 10 and 11.

广义相对论与量子宇宙学 · 物理学 2007-05-23 Kostadin Trencevski

Gravitational waves transport very detailed information on the structure and evolution of astrophysical sources. For instance a binary system in the early stages of its evolution emits a wavetrain at specific frequencies that depend on the…

天体物理学 · 物理学 2017-08-23 Valeria Ferrari

Analyzing two simple experimental situations we show that from Newton's law of gravitation and Special Relativity it follows that the motion of particle in an external gravitational field can be described in terms of effective spatial…

广义相对论与量子宇宙学 · 物理学 2008-11-26 W. D. Flanders , G. S. Japaridze

The dynamics of pseudo-classical spinning particles in spacetime of gravitational plane waves of general polarization and harmonic profile is studied. The resulting equations of motion are solved exactly and the results are compared with…

广义相对论与量子宇宙学 · 物理学 2015-06-25 Morteza Mohseni

Extragalactic proper motions can reveal a variety of cosmological and local phenomena over a range of angular scales. These include observer-induced proper motions, such as the secular aberration drift caused by the solar acceleration about…

宇宙学与河外天体物理 · 物理学 2018-10-16 Jeremy Darling , Alexandra Truebenbach , Jennie Paine

Astrometric observations can, in principle, be used to detect gravitational waves. In this paper we give a practical overview of the gravitational wave effects which can be expected specifically in small-field astrometric data. Particular…

广义相对论与量子宇宙学 · 物理学 2026-01-12 Robin Geyer , Sven Zschocke , Michael Soffel , Sergei Klioner , Lennart Lindegren , Uwe Lammers

Quantum field theory, which is generally used to describe the origin of large-scale gravitational perturbations during cosmic inflation, has been shown to omit an important physical effect in curved space-time, the nonlocal entanglement…

广义相对论与量子宇宙学 · 物理学 2022-04-01 Craig Hogan

Gravitational waves propagating through a stationary gauge field transform into gauge field waves and back again. When multiple families of flavor-space locked gauge fields are present, the gravitational and gauge field waves exhibit novel…

广义相对论与量子宇宙学 · 物理学 2017-06-05 R. R. Caldwell , C. Devulder , N. A. Maksimova

Continuous wave gravitational radiation from isolated rotating neutron stars is discussed. The general waveform and orders of magnitude for the amplitude are presented for various known pulsars. The specific case of gravitational radiation…

天体物理学 · 物理学 2007-05-23 E. Gourgoulhon , S. Bonazzola

All anomalous velocity increases until now observed during the Earth flybys of the spacecrafts Galileo, NEAR, Rosetta, Cassini and Messenger have been correctly calculated by computer simulation using an asymmetric field term in addition to…

综合物理 · 物理学 2007-11-27 Hans-Juergen Busack

We investigate a generic source of stochastic gravitational wave background due to the parametric resonance of oscillating scalar fields in the early Universe. By systematically analyzing benchmark models through lattice simulations and…

高能物理 - 唯象学 · 物理学 2024-07-19 Yanou Cui , Pankaj Saha , Evangelos I. Sfakianakis

In this paper we discuss some general aspects of the gravitational wave background arising from post-inflationary short-lasting cosmological events such as phase transitions. We concentrate on the physics which determines the shape and the…

宇宙学与河外天体物理 · 物理学 2014-11-18 Chiara Caprini , Ruth Durrer , Thomas Konstandin , Geraldine Servant

We treat quantum creation of gravitons by small scale factor oscillations around the average of an expanding universe. Such oscillations can arise in standard general relativity due to oscillations of a homogeneous, minimally coupled scalar…

广义相对论与量子宇宙学 · 物理学 2016-10-26 Enrico D. Schiappacasse , L. H. Ford

In this chapter, we explore how gravitational interactions drive turbulent flows inside planetary cores and provide an interesting alternative to convection to explain dynamo action and magnetic fields around terrestrial bodies. In the…

地球物理 · 物理学 2019-07-04 Thomas Le Reun , Michael Le Bars

It is shown that F(R)-modified gravitational theories lead to curvature oscillations in astrophysical systems with rising energy density. The frequency and the amplitude of such oscillations could be very high and would lead to noticeable…

广义相对论与量子宇宙学 · 物理学 2015-06-12 E. V. Arbuzova , A. D. Dolgov , L. Reverberi

Below scales of about 100/h Mpc our universe displays a complex inhomogeneous structure dominated by voids, with clusters of galaxies in sheets and filaments. The coincidence that cosmic expansion appears to start accelerating at the epoch…

宇宙学与河外天体物理 · 物理学 2011-02-11 David L. Wiltshire

We study gravitational curvature effects in circular and radial geodesics in static, spherically symmetric space-times, using Fermi normal coordinates. We first set up these coordinates in the general case, and then use this to study…

广义相对论与量子宇宙学 · 物理学 2015-06-19 Anshuman Dey , Abhisek Samanta , Tapobrata Sarkar

Gravitational merging (or clustering) of cosmic objects is regarded as a possible source of the extra-acceleration of the universe at large scale. The merging/clustering of cosmic objects introduces a correction term in the equation of…

宇宙学与河外天体物理 · 物理学 2019-05-29 Mehrdad Khanpour , Ebrahim Yusofi , Bahman Khanpour