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Causal soliton formation (e.g. oscillons, Q-balls) in the primordial Universe is expected to give rise to a universal gravitational wave (GW) background, at frequencies smaller than scales of nonlinearity. We show that modifications of the…

宇宙学与河外天体物理 · 物理学 2023-12-22 Kaloian D. Lozanov , Misao Sasaki , Volodymyr Takhistov

The reheating of the universe after hybrid inflation proceeds through the nucleation and subsequent collision of large concentrations of energy density in the form of bubble-like structures moving at relativistic speeds. This generates a…

高能物理 - 唯象学 · 物理学 2008-11-26 Juan Garcia-Bellido , Daniel G. Figueroa , Alfonso Sastre

The dynamics of a gravitational wave propagating through a cosmic gauge field are dramatically different than in vacuum. We show that a gravitational wave acquires an effective mass, is birefringent, and its normal modes are a linear…

广义相对论与量子宇宙学 · 物理学 2017-11-22 R. R. Caldwell , C. Devulder , N. A. Maksimova

Gravitational waves are expected to be radiated by supermassive black hole binaries formed during galaxy mergers. A stochastic superposition of gravitational waves from all such binary systems will modulate the arrival times of pulses from…

The combination of non-minimal couplings to gravity with the post-inflationary kinetic-dominated era typically appearing in quintessential inflation scenarios may lead to the spontaneous symmetry breaking of internal symmetries and its…

宇宙学与河外天体物理 · 物理学 2019-02-18 Dario Bettoni , Guillem Domènech , Javier Rubio

We investigate gravitational wave signals in a non-supersymmetric grand unified model where the group $SO(10)$ is broken in two steps to the Standard Model gauge group. We calculate the analytical form of the one-loop effective potential…

高能物理 - 唯象学 · 物理学 2026-03-31 Injun Jeong , Jörn Kersten , Stefano Scopel , Liliana Velasco-Sevilla

In the presence of an ultralight bosonic field, spinning black holes are unstable to superradiance. The rotational energy of the black hole is converted into a non-axisymmetric, oscillating boson cloud which dissipates through the emission…

广义相对论与量子宇宙学 · 物理学 2020-01-09 Nils Siemonsen , William E. East

We summarise the physics of first-order phase transitions in the early universe, and the possible ways in which they might come about. We then focus on gravitational waves, emphasising general qualitative features of stochastic backgrounds…

高能物理 - 唯象学 · 物理学 2026-02-17 Djuna Croon , David J. Weir

Gravitational waves, although generally associated with extremely microscopic effects, can displace by hundreds of kilometers the pulsar interstellar scintillation patterns that bathe the Earth. The combination of the pulsar and the…

天体物理学 · 物理学 2008-02-03 Redouane Fakir

Gravitational waves emitted by kinks on infinite strings are investigated using detailed estimations of the kink distribution on infinite strings. We find that gravitational waves from kinks can be detected by future pulsar timing…

宇宙学与河外天体物理 · 物理学 2014-11-20 Masahiro Kawasaki , Koichi Miyamoto , Kazunori Nakayama

In this paper we consider the Extra-solar Planetary Systems recently discovered in our Galaxy as potential sources of gravitational waves. We estimate the frequency and characteristic amplitude of the radiation they emit due to the orbital…

天体物理学 · 物理学 2009-10-31 Valeria Ferrari , Marco D'Andrea , Emanuele Berti

Recently Fuller & Shi proposed that the gravitational collapse of supermassive objects ($M \gtrsim 10^4M_\odot$) could be a cosmological source of $\gamma$-ray bursts (GRBs). The major advantage of their model is that supermassive object…

天体物理学 · 物理学 2009-11-06 J. C. N. de Araujo , O. D. Miranda , O. D. Aguiar

We consider the stochastic background of gravitational waves produced by a network of cosmic strings and assess their accessibility to current and planned gravitational wave detectors, as well as to big bang nucleosynthesis (BBN), cosmic…

天体物理学 · 物理学 2008-11-26 Xavier Siemens , Vuk Mandic , Jolien Creighton

The new millennium will see the upcoming of several ground-based interferometric gravitational wave antennas. Within the next decade a space-based antenna may also begin to observe the distant Universe. These gravitational wave detectors…

广义相对论与量子宇宙学 · 物理学 2009-10-31 B. S. Sathyaprakash

During supernova core collapse and bounce resonant active-to-active, as well as active-to-sterile, neutrino ($\nu$) oscillations can take place. Over this phase weak magnetism increases antineutrino mean free paths, and thus its luminosity.…

天体物理学 · 物理学 2011-05-24 Herman J. Mosquera Cuesta , Karen Fiuza

Over a hundred gravitational-wave signals have now been detected from the mergers of black holes and neutron stars, but other sources of gravitational waves have not yet been discovered. Some of the most violent explosive events in the…

高能天体物理现象 · 物理学 2025-01-24 Jade Powell , Paul D. Lasky

Gravitational-wave astronomy will soon become a new tool for observing the Universe. Detecting and interpreting gravitational waves will require deep theoretical insights into astronomical sources. The past three decades have seen…

广义相对论与量子宇宙学 · 物理学 2015-04-03 Alessandra Buonanno , B. S. Sathyaprakash

Gravitational-wave experiments with interferometers and with resonant masses can search for stochastic backgrounds of gravitational waves of cosmological origin. We review both experimental and theoretical aspects of the search for these…

广义相对论与量子宇宙学 · 物理学 2009-10-31 Michele Maggiore

There is a lot of current interest in sources of gravitational waves and active ongoing projects to detect such radiation, such as the LIGO project. These are long wavelength, low frequency gravitational waves. LISA would be sensitive to…

天体物理学 · 物理学 2011-09-27 C. Sivaram , Kenath Arun

Sources of high frequency gravitational waves are reviewed. Gravitational collapse, rotational instabilities and oscillations of the remnant compact objects are potentially important sources of gravitational waves. Significant and unique…

广义相对论与量子宇宙学 · 物理学 2010-11-19 Kostas D. Kokkotas