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Quasinormal mode (QNM) gravitational radiation from black holes is expected to be observed in a few years. A perturbative formula is derived for the shifts in both the real and the imaginary part of the QNM frequencies away from those of an…

广义相对论与量子宇宙学 · 物理学 2009-10-31 P. T. Leung , Y. T. Liu , W. -M. Suen , C. Y. Tam , K. Young

In this paper we briefly present our works on the relic gravitational waves (RGW) and the CMB polarization in the accelerating universe. The spectrum of RGW has been obtained, showing the influence of the dark energy. Compared with those…

天体物理学 · 物理学 2009-11-13 Y. Zhang , W. Zhao , T. Y. Xia , X. Z. Er , H. X. Miao

The influence of a possible low gravity scale, concretely through the presence of extra dimensions or additional species, on radiation properties of micro black holes is investigated. In particular, the suppression of evaporation through…

高能物理 - 理论 · 物理学 2025-07-02 Manuel Ettengruber , Florian Kuhnel

Gravitational waves can teach us not only about sources and the environment where they were generated, but also about the gravitational interaction itself. Here we study the features of gravitational radiation produced during the scattering…

广义相对论与量子宇宙学 · 物理学 2018-02-28 Seth Hopper , Vitor Cardoso

After a review of a traditional analysis, it is shown a variation of a more recent treatment on the spectrum of relic gravitational waves (GWs). Then, a connection between the two different treatments will be analysed. Such a connection…

广义相对论与量子宇宙学 · 物理学 2010-04-30 Christian Corda

A classical black hole is characterized by a horizon that absorbs radiation of all frequencies incident on it. Perturbation of these black holes is well-understood via exponentially damped sinusoids known as quasi-normal modes. Any…

广义相对论与量子宇宙学 · 物理学 2022-03-09 Kabir Chakravarti , Rajes Ghosh , Sudipta Sarkar

The energy density of relic gravitational waves (GWs) emitted by primordial black holes (PBHs) is calculated. We estimate the intensity of GWs produced at quantum and classical scattering of PBHs, the classical graviton emission from the…

宇宙学与河外天体物理 · 物理学 2011-07-19 Alexander D. Dolgov , Damian Ejlli

We study the superradiant scattering of gravitational waves by a nearly extremal black hole (dimensionless spin $a=0.99$) by numerically solving the full Einstein field equations, thus including backreaction effects. This allows us to study…

广义相对论与量子宇宙学 · 物理学 2014-03-26 William E. East , Fethi M. Ramazanoğlu , Frans Pretorius

We investigate the dependence of the gravitational wave spectrum from quintessential inflation on the reheating process. We consider two extreme reheating processes. One is the gravitational reheating by particle creation in the expanding…

广义相对论与量子宇宙学 · 物理学 2009-10-09 Hiroyuki Tashiro , Takeshi Chiba , Misao Sasaki

Modelling of gravitational waves from binary black hole inspiral has played an important role in the recent observations of such signals. The late-stage ringdown phase of the gravitational waveform is often associated with the null particle…

广义相对论与量子宇宙学 · 物理学 2017-05-03 Gaurav Khanna , Richard H. Price

Gravitons radiated from light, evaporating black holes contribute to the stochastic background of gravitational waves. The spectrum of such emission depends on both the mass and the spin of the black holes, as well as on the redshifting…

广义相对论与量子宇宙学 · 物理学 2023-05-10 Aurora Ireland , Stefano Profumo , Jordan Scharnhorst

Observations have recently indicated that the Universe at the present stage is in an accelerating expansion, a process that has great implications. We evaluate the spectrum of relic gravitational waves in the current accelerating Universe…

天体物理学 · 物理学 2007-05-23 Yang Zhang , Yefei Yuan , Wen Zhao , Ying-Tian Chen

We investigate the impact of the post-inflationary thermal histories on the cosmic graviton spectrum caused by the inflationary variation of their refractive index. Depending on the frequency band, the spectral energy distribution can be…

广义相对论与量子宇宙学 · 物理学 2018-11-21 Massimo Giovannini

We show that gravitational-wave astronomy has the potential to inform us on quantum aspects of black holes. Based on Bekenstein's quantization, we find that black hole area discretization could impart observable imprints to the…

广义相对论与量子宇宙学 · 物理学 2021-02-09 Ivan Agullo , Vitor Cardoso , Adrian del Rio , Michele Maggiore , Jorge Pullin

We discuss the conditions under which plane electromagnetic and gravitational waves can be amplified by a rotating black hole due to superradiant scattering. We show, in particular, that amplification can occur for low-frequency waves with…

广义相对论与量子宇宙学 · 物理学 2017-03-22 Joao G. Rosa

Ultracompact objects with photonspheres are known to mimic many observational features of black holes. It has been suggested that anomalous tidal heating or the presence of resonances in gravitational wave signals would be a clear imprint…

广义相对论与量子宇宙学 · 物理学 2022-05-25 Vitor Cardoso , Francisco Duque

We investigate the propagation of gravitational waves on a black hole background within the low energy effective field theory of gravity, where effects from heavy fields are captured by higher dimensional curvature operators. Depending on…

高能物理 - 理论 · 物理学 2020-08-05 Claudia de Rham , Jérémie Francfort , Jun Zhang

The recent detections of gravitational waves from binary systems of black holes are in remarkable agreement with the predictions of General Relativity. In this pedagogical mini-review, I will go through the physics of the different phases…

广义相对论与量子宇宙学 · 物理学 2021-11-24 Enrico Barausse

In order to describe inflation in general relativity, scalar fields must inevitably be used, with all the setbacks of that description. On the other hand, $f(R)$ gravity and other modified gravity theories seem to provide a unified…

广义相对论与量子宇宙学 · 物理学 2022-06-03 S. D. Odintsov , V. K. Oikonomou

The prediction that black holes radiate due to quantum effects is often considered one of the most secure in quantum field theory in curved space-time. Yet this prediction rests on two dubious assumptions: that ordinary physics may be…

广义相对论与量子宇宙学 · 物理学 2009-11-10 Adam D. Helfer