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相关论文: Freezing-In Gravitational Waves

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Because of physical processes ranging from microscopic particle collisions to macroscopic hydrodynamic fluctuations, any plasma in thermal equilibrium emits gravitational waves. For the largest wavelengths the emission rate is proportional…

高能物理 - 唯象学 · 物理学 2015-08-06 J. Ghiglieri , M. Laine

In a previous paper [1] we considered the possibility that (within the early-radiation epoch) there has been (also) a short period of a significant presence of cosmic strings. During this radiation-plus-strings stage the Universe…

高能物理 - 理论 · 物理学 2015-06-03 Kostas Kleidis , Apostolos Kuiroukidis , Demetrios B. Papadopoulos , Enric Verdaguer

We report on the first 3-dimensional numerical simulations of first-order phase transitions in the early universe to include the cosmic fluid as well as the scalar field order parameter. We calculate the gravitational wave (GW) spectrum…

高能物理 - 唯象学 · 物理学 2014-01-30 Mark Hindmarsh , Stephan J. Huber , Kari Rummukainen , David J. Weir

Dark gauge fields have been discussed as candidates for dark matter recently. If they existed, primordial dark magnetic fields during inflation would have existed. It is believed that primordial gravitational waves (PGWs) arise out of…

高能物理 - 理论 · 物理学 2023-06-09 Sugumi Kanno , Ann Mukuno , Jiro Soda , Kazushige Ueda

Gravitational waves (GWs) have a great potential to probe cosmology. We review early universe sources that can lead to cosmological backgrounds of GWs. We begin by presenting definitions of GWs in flat space-time and in a cosmological…

宇宙学与河外天体物理 · 物理学 2020-07-23 Chiara Caprini , Daniel G. Figueroa

We study the production, spectrum and detectability of gravitational waves in models of the early Universe where first order phase transitions occur during inflation. We consider all relevant sources. The self-consistency of the scenario…

宇宙学与河外天体物理 · 物理学 2011-02-16 Diego Chialva

We assume that the cosmological dark matter is composed of massive neutral scalar particles that decay into two massless particles. The decay produces a stochastic background of gravitational waves (GWs) via a 'memory effect' mechanism. We…

广义相对论与量子宇宙学 · 物理学 2020-02-14 Bruce Allen

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

Gravitational waves (GWs) originating from cosmological sources offer direct insights into the physics of the primordial Universe, the fundamental nature of gravity, and the cosmic expansion of the Universe. In this review paper, we present…

Anisotropies in the cosmic microwave background radiation due to gravity waves are investigated. An initial spectrum of gravity waves may have been induced during an epoch of inflation. We study the propagation of such a spectrum in a…

天体物理学 · 物理学 2008-02-03 Ruth Durrer , Tina Kahniashvili

The discovery of gravitational waves opens new opportunities to test BSM physics. In particular, the production of a stochastic background of primordial gravitational waves could provide a signature of the generation of the right-right…

高能物理 - 唯象学 · 物理学 2022-05-13 Pasquale Di Bari

First order phase transitions in the early universe can give rise to a stochastic background of gravitational waves. A hypothetical first order electroweak phase transition is particularly interesting in this respect, since the signal is in…

宇宙学与河外天体物理 · 物理学 2015-03-17 Chiara Caprini

Quantum fluctuations of the gravitational field in the early Universe, amplified by inflation, produce a primordial gravitational-wave background across a broad frequency band. We derive constraints on the spectrum of this gravitational…

Cosmological phase transitions in the primordial universe can produce anisotropic stochastic gravitational wave backgrounds (GWB), similar to the cosmic microwave background (CMB). For adiabatic perturbations, the fluctuations in GWB follow…

宇宙学与河外天体物理 · 物理学 2021-12-01 Soubhik Kumar , Raman Sundrum , Yuhsin Tsai

The recent finding of the gravitational wave (GW) signal by the NANOGrav collaboration in the nHZ frequency range has opened up the door for the existence of stochastic GWs. In the present work, we have argued that in a hot dense neutrino…

宇宙学与河外天体物理 · 物理学 2021-05-11 Arun Kumar Pandey

In warm inflation (WI), the persistent thermal bath that is sustained by dissipative interactions with the inflaton field produces a stochastic background of gravitational waves (GWs). In this paper we study the production and evolution of…

高能物理 - 唯象学 · 物理学 2025-09-30 Gabriele Montefalcone , Barmak Shams Es Haghi , Tao Xu , Katherine Freese

We study the induced primordial gravitational waves (GW) coming from the effect of scalar perturbation on the tensor perturbation at the second order of cosmological perturbation theory. We use the evolution of the standard model degrees of…

高能物理 - 唯象学 · 物理学 2020-02-19 Fazlollah Hajkarim , Jürgen Schaffner-Bielich

We investigate the primordial gravitational waves (PGWs) in the general scenario where the inflation is preceded by a pre-inflationary stage with the effective equation of state $w$. Comparing with the results in the usual inflationary…

宇宙学与河外天体物理 · 物理学 2017-01-31 Kai Wang , Larissa Santos , Jun-Qing Xia , Wen Zhao

We study primordial gravitational waves (GWs) generated from first-order phase transitions (PTs) during cosmic reheating. Using a minimal particle physics model, and a general parametrization of the inflaton energy density and the evolution…

宇宙学与河外天体物理 · 物理学 2025-06-04 Amitayus Banik , Nicolás Bernal , Fazlollah Hajkarim

We propose a novel scenario of Dark Matter production naturally connected with generation of gravitational waves. Dark Matter is modelled as a real scalar, which interacts with the hot primordial plasma through a portal coupling to another…

高能物理 - 唯象学 · 物理学 2022-04-06 S. Ramazanov , E. Babichev , D. Gorbunov , A. Vikman