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相关论文: Gravitational Waves from Preheating in Gauss-Bonne…

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Inflation with Weyl scaling symmetry provides a viable scenario that can generate both the nearly scaling invariant primordial density fluctuation and a dark matter candidate. Here we point out that, in additional to the primordial…

宇宙学与河外天体物理 · 物理学 2024-10-11 Wei-Yu Hu , Qing-Yang Wang , Yan-Qing Ma , Yong Tang

I review two mechanisms by which gravitational waves can be generated at the end of inflation: preheating, and gravitons Hawking radiated during the decay of very small primordial black holes. These mechanisms are contrasted with the…

宇宙学与河外天体物理 · 物理学 2009-11-05 Richard Easther

We present a comprehensive analysis of the preheating dynamics and associated gravitational wave signatures in the Higgs--$R^2$ inflationary model. Using lattice simulations, we investigate the post-inflationary evolution of the system…

宇宙学与河外天体物理 · 物理学 2025-09-03 Jinsu Kim , Zihao Yang , Ying-li Zhang

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

Parametric resonance or preheating is a plausible mechanism for bringing about the transition between the inflationary phase and a hot, radiation dominated universe. This epoch results in the rapid production of heavy particles far from…

天体物理学 · 物理学 2008-11-26 Richard Easther , John T. Giblin , Eugene A. Lim

We study the preheating and the in-process production of gravitational waves (GWs) after inflation in which the inflaton is nonminimally coupled to the curvature in a self-interacting quartic potential with the method of lattice simulation.…

广义相对论与量子宇宙学 · 物理学 2018-05-02 Chengjie Fu , Puxun Wu , Hongwei Yu

In this paper, we investigate scalar-induced gravitational waves (GWs) generated in the post-inflationary universe to infer new limits on warm inflation. We specifically examine the evolution of primordial GWs by scalar perturbations…

宇宙学与河外天体物理 · 物理学 2025-03-26 Rocco D'Agostino , Matteo Califano

Assuming that inflation is succeeded by a phase of matter domination, which corresponds to a low temperature of reheating $T_r<10^9\rm{GeV}$, we evaluate the spectra of gravitational waves induced in the post-inflationary universe. We work…

宇宙学与河外天体物理 · 物理学 2015-06-15 Laila Alabidi , Kazunori Kohri , Misao Sasaki , Yuuiti Sendouda

Particle decays are always accompanied by the emission of graviton quanta of gravity through bremsstrahlung processes. However, the corresponding branching ratio is suppressed by the square of the ratio of particle's mass to the Planck…

高能物理 - 唯象学 · 物理学 2024-03-22 Weiyu Hu , Kazunori Nakayama , Volodymyr Takhistov , Yong Tang

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 gravitational wave production during kinetic preheating after inflation with a focus on scenarios that arise in $\alpha$-attractor models where a scalar dilaton-like inflaton is kinetically coupled to a second scalar field. We…

宇宙学与河外天体物理 · 物理学 2024-02-27 Peter Adshead , John T. Giblin , Avery Tishue

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

The gravitational wave equations form a parametric resonance system during oscillatory reheating after inflation, when cast in terms of the electric and magnetic parts of the Weyl tensor. This is in direct analogy with preheating. For…

高能物理 - 唯象学 · 物理学 2009-10-30 Bruce A. Bassett

In this work we shall calculate in detail the effect of an GW170817-compatible Einstein-Gauss-Bonnet theory on the energy spectrum of the primordial gravitational waves. The spectrum is affected by two characteristics, the overall…

广义相对论与量子宇宙学 · 物理学 2022-04-27 V. K. Oikonomou

We forecast high-frequency gravitational wave (GW) from preheating hosting gravitational dark matter (GDM) as the indirect probe of such GDM. We use proper lattice simulations to handle resonance, and to solve GW equation of motion with the…

高能物理 - 唯象学 · 物理学 2024-11-15 Ruopeng Zhang , Sibo Zheng

We study the evolution of Gravitational Waves (GWs) during and after inflation as well as the resulting observational consequences in a Lorentz-violating massive gravity theory with one scalar (inflaton) and two tensor degrees of freedom.…

广义相对论与量子宇宙学 · 物理学 2018-01-23 Sachiko Kuroyanagi , Chunshan Lin , Misao Sasaki , Shinji Tsujikawa

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…

广义相对论与量子宇宙学 · 物理学 2008-01-29 Juan Garcia-Bellido , Daniel G. Figueroa

The low energy effective action of quantum gravity may include the higher curvature terms such as the Gauss-Bonnet term. The inflaton dynamics may be affected by the Gauss-Bonnet term if there is an inflaton-Gauss-Bonnet coupling. We show…

宇宙学与河外天体物理 · 物理学 2024-01-15 Kamil Mudrunka , Kazunori Nakayama

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 investigate the generation of gravitational waves in power-law inflationary models. The energy spectrum of the gravitational waves is calculated using the method of continuous Bogoliubov coefficients. We show that, by looking at the…

天体物理学 · 物理学 2009-09-28 Paulo M. Sá , Alfredo B. Henriques