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The process of reheating the universe after hybrid inflation is extremely violent. It proceeds through the nucleation and subsequent collision of large concentrations of energy density in bubble-like structures, which generate a significant…

天体物理学 · 物理学 2008-11-26 Juan Garcia-Bellido , Daniel G. Figueroa

In this work we highlight an important perspective for the complete understanding of the stochastic gravitational background structure. The stochastic gravitational wave background is perhaps the most important current and future tool…

广义相对论与量子宇宙学 · 物理学 2024-07-02 S. D. Odintsov , V. K. Oikonomou

Several mechanisms exist for generating a stochastic background of gravitational waves in the period following inflation. These mechanisms are generally classical in nature, with the gravitational waves being produced from inhomogeneities…

天体物理学 · 物理学 2008-11-26 Larry R. Price , Xavier Siemens

The stochastic gravitational wave (GW) background provides a fascinating window to the physics of the very early universe. Beyond the nearly scale-invariant primordial GW spectrum produced during inflation, a spectrum with a much richer…

宇宙学与河外天体物理 · 物理学 2018-04-04 Stefan Antusch , Francesco Cefala , Stefano Orani

Preheating and other particle production phenomena in the early Universe can give rise to high- energy out-of-equilibrium fermions with an anisotropic stress. We develop a formalism to calculate the spectrum of gravitational waves due to…

宇宙学与河外天体物理 · 物理学 2015-06-04 Kari Enqvist , Daniel G. Figueroa , Tuukka Meriniemi

Oscillations in the frequency profile of the scalar-induced contribution to the stochastic gravitational wave background are a characteristic signal for small-scale features during inflation. We investigate how this oscillatory frequency…

宇宙学与河外天体物理 · 物理学 2022-05-25 Lukas T. Witkowski , Guillem Domènech , Jacopo Fumagalli , Sébastien Renaux-Petel

A stochastic background of gravitational waves can be created by the superposition of a large number of independent sources. The physical processes occurring at the earliest moments of the universe certainly created a stochastic background…

广义相对论与量子宇宙学 · 物理学 2018-11-22 Nelson Christensen

We consider the space-condensate inflation model to study the primordial gravitational waves generated in the early Universe. We calculate the energy spectrum of gravitational waves induced by the space-condensate inflation model for full…

广义相对论与量子宇宙学 · 物理学 2016-04-27 Seoktae Koh , Bum-Hoon Lee , Gansukh Tumurtushaa

The spectrum of thermal gravitational waves is obtained by including the high frequency thermal gravitons created from extra-dimensional effect and is a new feature of the spectrum. The amplitude and spectral energy density of gravitational…

广义相对论与量子宇宙学 · 物理学 2013-06-21 Basem Ghayour , P K Suresh

We undertake a careful analysis of stochastic gravitational wave production from cosmological phase transitions in an expanding universe, studying both a standard radiation as well as a matter dominated history. We analyze in detail the…

高能物理 - 唯象学 · 物理学 2021-01-07 Huai-Ke Guo , Kuver Sinha , Daniel Vagie , Graham White

The direct detection of gravitational waves has provided new opportunities for studying the universe, but also new challenges, such as the detection and characterization of stochastic gravitational-wave backgrounds at different…

宇宙学与河外天体物理 · 物理学 2019-04-17 Ciarán Conneely , Andrew H. Jaffe , Chiara M. F. Mingarelli

We discuss the quantum mechanical description of a gravitational wave interacting with a cavity electromagnetic field. Quantum fluctuations of the gravitational vacuum induce squeezing in the optical field. Moreover, this squeezing…

量子物理 · 物理学 2020-06-19 Thiago Guerreiro

The low frequency part of the gravitational wave spectrum generated by local physics, such as a phase transition or parametric resonance, is largely fixed by causality, offering a clean window into the early Universe. In this work, this low…

高能物理 - 唯象学 · 物理学 2021-03-17 Anson Hook , Gustavo Marques-Tavares , Davide Racco

Physical scenarios, leading to highly energetic stochastic gravitational waves backgrounds (for frequencies ranging from the $\mu$Hz up to the GHz) are examined. In some cases the typical amplitude of the logarithmic energy spectrum can be…

高能物理 - 唯象学 · 物理学 2016-11-03 Massimo Giovannini

A stochastic background of gravitational waves is expected to arise from a superposition of a large number of unresolved gravitational-wave sources of astrophysical and cosmological origin. It is expected to carry unique signatures from the…

宇宙学与河外天体物理 · 物理学 2012-08-27 The LIGO Scientific Collaboration , the Virgo Collaboration

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 are a unique probe of the early Universe, as the Universe is transparent to gravitational radiation right back to the end of inflation. In this article, we summarise detection prospects and the wide scope of primordial…

高能物理 - 唯象学 · 物理学 2024-09-09 Rishav Roshan , Graham White

We identify a characteristic pattern in the scalar-induced stochastic gravitational wave background from particle production during inflation. If particle production is sufficiently efficient, the scalar power spectrum exhibits…

宇宙学与河外天体物理 · 物理学 2021-09-24 Jacopo Fumagalli , Sébastien Renaux-Petel , Lukas T. Witkowski

We carry out a theoretical investigation on the collective dynamics of an ensemble of correlated atoms, subject to both vacuum fluctuations of spacetime and stochastic gravitational waves. A general approach is taken with the derivation of…

广义相对论与量子宇宙学 · 物理学 2018-03-20 Diego A. Quinones , Teodora Oniga , Benjamin T. H. Varcoe , Charles H. -T. Wang

Future space-based interferometers offer an unprecedented opportunity to detect signals from the stochastic gravitational wave background originating from a first-order phase transition at the electroweak scale. The phase transition is…

广义相对论与量子宇宙学 · 物理学 2024-09-04 Lorenzo Giombi , Jani Dahl , Mark Hindmarsh
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