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Gravitational perturbations of neutron stars and black holes are well known sources of gravitational radiation. If the compact object is immersed in or endowed with a magnetic field, the gravitational perturbations would couple to…

高能天体物理现象 · 物理学 2015-06-15 Hajime Sotani , Kostas D. Kokkotas , Pablo Laguna , Carlos F. Sopuerta

The evolution of globular cluster systems in some galaxies can be cause of merging of globulars in the very central regions. This high stellar density favours the growth of a central nucleus via swallowing of surrounding stars. The infall…

天体物理学 · 物理学 2016-08-30 Roberto Capuzzo-Dolcetta , Paolo Miocchi

We review sources of high-frequency gravitational waves, summarizing our current understanding of emission mechanisms, expected amplitudes and event rates. The most promising sources are gravitational collapse (formation of black holes or…

广义相对论与量子宇宙学 · 物理学 2017-08-23 Kostas D. Kokkotas , Nikolaos Stergioulas

These lectures aim at providing an introduction to the properties of gravitational waves and in particular to those gravitational waves that are expected as a consequence of perturbations of black holes and neutron stars. Imprinted in the…

广义相对论与量子宇宙学 · 物理学 2009-04-16 Luciano Rezzolla

Neutron stars are excellent emitters of gravitational waves. Squeezing matter beyond nuclear densities invites exotic physical processes, many of which violently transfer large amounts of mass at relativistic velocities, disrupting…

高能天体物理现象 · 物理学 2015-11-20 Paul D. Lasky

Gravitational waves astronomy allows us to study objects and events invisible in electromagnetic waves. It is crucial to validate the theories and models of the most mysterious and extreme matter in the Universe: the neutron stars. In…

高能天体物理现象 · 物理学 2019-11-06 Magdalena Sieniawska , Michał Bejger

Non radial oscillations of neutron stars are associated with the emission of gravitational waves. The characteristic frequencies of these oscillations can be computed using the theory of stellar perturbations, and they are shown to carry…

广义相对论与量子宇宙学 · 物理学 2011-05-10 Valeria Ferrari

The coalescence of black hole-neutron star binaries is expected to be a principal source of gravitational waves for the next generation of detectors, Advanced LIGO and Advanced Virgo. Ideally, these and other gravitational wave sources…

高能天体物理现象 · 物理学 2015-05-27 Sean T. McWilliams , Janna Levin

Gravitational waves are tiny disturbances in space-time and are a fundamental, although not yet directly confirmed, prediction of General Relativity. Rapidly rotating neutron stars are one of the possible sources of gravitational radiation…

天体物理学 · 物理学 2008-12-03 Aaron Worley , Plamen G. Krastev , Bao-An Li

Wave propagation of field disturbances is ubiquitous. The electromagnetic and gravitational are cousin theories in which the corresponding waves play a relevant role to understand several related physical. It has been established that small…

广义相对论与量子宇宙学 · 物理学 2017-11-22 W. Barreto , H. P. de Oliveira , E. L. Rodrigues

Multimessenger observations may hold the key to learn about the most energetic sources in the universe. The recent construction of large scale observatories opened new possibilities in testing non thermal cosmic processes with alternative…

高能天体物理现象 · 物理学 2019-06-05 Dafne Guetta

The extragalactic background of gravitational waves produced by tri-axial rotating neutron stars was calculated, under the assumption that the properties of the underlying pulsar population are the same of those of the galactic population,…

天体物理学 · 物理学 2009-11-06 T. Regimbau , J. A. de Freitas Pacheco

We present the derivation and the solutions to the coupled electromagnetic and gravitational perturbations with sources in a charged black hole background. We work in the so called ghost gauge and consider as source of the perturbations the…

广义相对论与量子宇宙学 · 物理学 2017-06-21 Claudia Moreno , Juan Carlos Degollado , Dario Nunez

We provide details and present additional results on the numerical study of the gravitational-wave emission from the collapse of neutron stars to rotating black holes in three dimensions. More specifically, we concentrate on the advantages…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Luca Baiotti , Ian Hawke , Luciano Rezzolla

It is presented a brief review on gravitational waves (GWs). It is shown how the wave equation is obtained from Einstein's equations and how many and how are the polarization modes of these waves. It is discussed the reasons why GWs sources…

高能天体物理现象 · 物理学 2013-05-14 J. C. N. de Araujo

Gravitational Wave Astronomy is becoming a reality as Earth-based interferometric gravitational-wave detectors reach the design sensitivities and move towards advanced configurations that may lead to gravitational-wave detections in the…

天体物理学 · 物理学 2008-08-05 Carlos F. Sopuerta

We discuss different ways that neutron stars can generate gravitational waves, describe recent improvements in modelling the relevant scenarios in the context of improving detector sensitivity, and show how observations are beginning to…

太阳与恒星天体物理 · 物理学 2011-01-28 N. Andersson , V. Ferrari , D. I. Jones , K. D. Kokkotas , B. Krishnan , J. Read , L. Rezzolla , B. Zink

Gravitational waves are perturbations in the spacetime that propagate at the speed of light. The study of such phenomenon is interesting because many cosmological processes and astrophysical objects, such as binary systems, are potential…

宇宙学与河外天体物理 · 物理学 2015-04-27 E. F. D. Evangelista , J. C. N. de Araujo

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

Neutron stars are one of the most mysterious wonders in the Universe. Their extreme densities hint at new and exotic physics at work within. Gravitational waves could be the key to unlocking their secrets. In particular, a first detection…

广义相对论与量子宇宙学 · 物理学 2024-01-09 Neil Lu , Susan M. Scott , Karl Wette
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