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In the vicinity of merging neutron strar binaries or supernova remnants, gravitational waves can interact with the prevailing strong magnetic fields. The resulting partial conversion of gravitational waves into electromagnetic (radio) waves…

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

After their generation, cosmological backgrounds of gravitational waves propagate nearly freely but for the expansion of the Universe and the anisotropic stress of free-streaming particles. Primordial signals -- both that from inflation and…

宇宙学与河外天体物理 · 物理学 2025-08-20 Marilena Loverde , Zachary J. Weiner

Gravitational waves are considered as metric perturbations about a curved background metric, rather than the flat Minkowski metric since several situations of physical interest can be discussed by this generalization. In this case, when the…

广义相对论与量子宇宙学 · 物理学 2008-12-21 Donato Bini , Salvatore Capozziello , Giampiero Esposito

Previous work has developed the theory of linearized gravitational wave (GW) interactions with matter using the Bondi-Sachs formalism, but with the perturbations restricted to be quadrupolar, i.e., the angular dependence is spherical…

广义相对论与量子宇宙学 · 物理学 2026-05-26 Ulrich K. Beckering Vinckers , Nigel T. Bishop

Cosmological gravitational wave backgrounds (CGWBs) are the conglomeration of unresolved gravitational wave signals from early Universe sources, which make them a promising tool for cosmologists. Because gravitons decouple from the cosmic…

广义相对论与量子宇宙学 · 物理学 2023-12-27 Tatsuya Daniel , Marcell Howard , Morgane König

The interaction, in the long--wavelength approximation, of normal and superconducting electromagnetic circuits with gravitational waves is investigated. We show that such interaction takes place by modifying the physical parameters R, L, C…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Pierluigi Fortini , Enrico Montanari , Antonello Ortolan , Gerhard Schaefer

We discuss the gravitational wave background generated by primordial density perturbations evolving during the radiation era. At second-order in a perturbative expansion, density fluctuations produce gravitational waves. We calculate the…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Kishore N. Ananda , Chris Clarkson , David Wands

It is shown here that a cloud of charged particles could in principle absorb energy from gravitational waves (GWs) incident upon it, resulting in wave attenuation. This could in turn have implications for the interpretation of future data…

广义相对论与量子宇宙学 · 物理学 2015-02-04 Thulsi Wickramasinghe , Will Rhodes , Mitchell Revalski

Gravitational waves are propagating undulations in the spacetime fabric, which interact very weakly with their environment. In cosmology, gravitational-wave distortions are produced by most of the inflationary scenarios and their…

广义相对论与量子宇宙学 · 物理学 2016-03-30 Despoina Pazouli , Christos G. Tsagas

We lay a theoretical foundation in the observation of gravitational waves (GWs) by electromagnetic waves (EMWs) performing a full electromagnetic analysis without any optical approximation. For that, the perturbation of plane EMWs is…

广义相对论与量子宇宙学 · 物理学 2022-11-22 Chan Park

We consider the collisions of plane gravitational and electromagnetic waves with distinct wavefronts and of arbitrary polarizations in a Minkowski background. We first present a new, completely geometric formulation of the characteristic…

广义相对论与量子宇宙学 · 物理学 2008-11-26 G. A. Alekseev , J. B. Griffiths

We study the interaction between gravitational waves and a quantum two-level system consisting of a spin 1/2 particle using the formalism of the proper detector frame. This approach highlights the effects of gravitational waves on both the…

广义相对论与量子宇宙学 · 物理学 2025-02-28 Matteo Luca Ruggiero

Gravitational wave observations have significantly broadened our capacity to explore fundamental physics beyond the Standard Model, providing crucial insights into dark matter that are inaccessible through conventional methods. Here, we…

宇宙学与河外天体物理 · 物理学 2025-10-21 Jeong Han Kim , Xing-Yu Yang

Gravitational waves (GW) are expected to interact with dark energy and dark matter, affecting their propagation on cosmological scales. In order to model this interaction, we derive a gauge invariant effective equation and action valid for…

宇宙学与河外天体物理 · 物理学 2024-03-29 Antonio Enea Romano

Even though one could already constrain different models in cosmology and Beyond Standard Model physics using CMB data, these models remained unconstrained at shorter wavelength scales, and knowledge of new physics at higher energy scales…

宇宙学与河外天体物理 · 物理学 2025-01-22 Rafael R. Lino dos Santos , Linda M. van Manen

Previous work has shown that the interaction between gravitational waves (GWs) and a shell of viscous matter leads to damping of the GWs and heating of the matter, and that these effects may be astrophysically significant. This result was…

广义相对论与量子宇宙学 · 物理学 2025-07-24 Nigel T. Bishop

The behaviour of a "test" electromagnetic field in the background of an exact gravitational plane wave is investigated in the framework of Einstein's general relativity. We have expressed the general solution to the de Rham equations as a…

广义相对论与量子宇宙学 · 物理学 2009-10-31 Enrico Montanari , Mirco Calura

We discuss the conversion mechanism from scalar field to gravitational waves in magnetic background in $f(R)$ gravity minimal coupled to the Maxwell electrodynamics. Applying the conversion in early universe with primordial magnetic field…

广义相对论与量子宇宙学 · 物理学 2025-12-01 Salvatore Capozziello , Qingyu Gan

We study the interaction of a gravitational wave (GW) with a plasma that is strongly magnetized. The GW is considered a small disturbance, and the plasma is modeled by the general relativistic analogue of the induction equation of ideal MHD…

天体物理学 · 物理学 2008-11-26 H. Isliker , L. Vlahos

We study the generation of gravitational radiation by sources moving in the de Sitter background. Exploiting the maximal symmetry and the conformal flatness of de Sitter space-time we prove that the derivation of this gravitational…

天体物理学 · 物理学 2009-10-31 H. J. de Vega , J. Ramirez , N. Sanchez