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We suggest the new feature of primordial gravitational waves sourced by the axion-gauge couplings, whose forms are motivated by the dimensional reduction of the form field in the string theory. In our inflationary model, as an inflaton we…

宇宙学与河外天体物理 · 物理学 2017-07-05 Ippei Obata

The detection of Primordial Gravitational Waves (PGWs) is one of the most important goals of modern cosmology since PGWs can both provide substantial evidence for primordial inflation and shed light on its physical nature. Small scale…

宇宙学与河外天体物理 · 物理学 2021-02-17 William Giarè , Alessandro Melchiorri

In this work we analyse in detail the possibility of using small and intermediate-scale gravitational wave anisotropies to constrain the inflationary particle content. First, we develop a phenomenological approach focusing on anisotropies…

宇宙学与河外天体物理 · 物理学 2022-03-09 Ema Dimastrogiovanni , Matteo Fasiello , Ameek Malhotra , P. Daniel Meerburg , Giorgio Orlando

We explore a novel process in the early Universe in which thermalized photons are converted into gravitons in the presence of strong primordial magnetic fields. It is found that the frequency of generated gravitational waves (GWs) is…

宇宙学与河外天体物理 · 物理学 2020-11-19 Tomohiro Fujita , Kohei Kamada , Yuichiro Nakai

We extend the reach of the ``cosmological collider'' for massive gauge boson production during inflation from the CMB scales to the interferometer scales. Considering a Chern-Simons coupling between the gauge bosons and the pseudoscalar…

高能物理 - 唯象学 · 物理学 2023-02-10 Xuce Niu , Moinul Hossain Rahat , Karthik Srinivasan , Wei Xue

Primordial gravitational waves generated during inflation lead to the B-mode polarization in the cosmic microwave background and a stochastic gravitational wave background in the Universe. We will explore the current constraint on the tilt…

宇宙学与河外天体物理 · 物理学 2025-03-28 Jun Li , Zu-Cheng Chen , Qing-Guo Huang

We consider the possibility that the massive graviton is a viable candidate of dark matter in the context of bimetric gravity. We first derive the energy-momentum tensor of the massive graviton and show that it indeed behaves as that of…

高能物理 - 理论 · 物理学 2016-07-19 Katsuki Aoki , Shinji Mukohyama

The primordial spectrum of fluctuations may present a large peak as a result of enhancing features during inflation. This may include, but is not limited to, bumps in the inflaton's potential, phases of ultra-slow-roll or turns in…

宇宙学与河外天体物理 · 物理学 2022-09-30 Shyam Balaji , Guillem Domenech , Joseph Silk

Supersolid inflation is a class of inflationary theories that simultaneously breaks time and space reparameterization invariance during inflation, with distinctive features for the dynamics of cosmological fluctuations. We investigate…

宇宙学与河外天体物理 · 物理学 2017-07-19 Angelo Ricciardone , Gianmassimo Tasinato

Gravitational waves (GWs) from gravitational three-body decay (graviton Bremsstrahlung process) can leave an indelible signal at ultrahigh frequencies. We focus on a scenario where superheavy particles are produced gravitationally at a…

宇宙学与河外天体物理 · 物理学 2024-08-21 Ryoto Inui , Yusuke Mikura , Shuichiro Yokoyama

We propose that there may be a substantial stochastic gravitational wave background from particle origin, mainly from the gravitational three-body decay of the inflaton. The emitted gravitons could constitute a sizable contribution to dark…

高能物理 - 唯象学 · 物理学 2024-10-30 Kazunori Nakayama , Yong Tang

The detection of primordial gravitational waves would offer a direct evidence of inflation and valuable insights into the dynamics of the early universe. During post-inflation reheating period, when the inflaton coherently oscillates at the…

高能物理 - 唯象学 · 物理学 2026-03-06 Diganta Das , Mihika Sanghi , Sourav

Inflation generates gravitational waves, which may be observable in the low multipoles of the cosmic microwave background (cmb) anisotropy but only if the inflaton field variation is at least of order the Planck scale. Such a large…

高能物理 - 唯象学 · 物理学 2009-10-28 David H. Lyth

We study the stochastic background of gravitational waves which accompany the sudden freeze-out of dark matter triggered by a cosmological first order phase transition that endows dark matter with mass. We consider models that produce the…

高能物理 - 唯象学 · 物理学 2021-02-03 Danny Marfatia , Po-Yan Tseng

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 discuss the detectability of gravitational waves with a time dependent mass contribution, by means of the stochastic gravitational wave observations. Such a mass term typically arises in the cosmological solutions of massive gravity…

高能物理 - 理论 · 物理学 2012-12-13 A. Emir Gumrukcuoglu , Sachiko Kuroyanagi , Chunshan Lin , Shinji Mukohyama , Norihiro Tanahashi

We study the formation of primordial black holes and the generation of gravitational waves in a class of cosmological models that are direct supersymmetric analogs of the observationally favored nonminimally coupled Higgs inflation model.…

宇宙学与河外天体物理 · 物理学 2023-03-01 Shinsuke Kawai , Jinsu Kim

A generic consequence of supersymmetry is formation of a scalar condensate along the flat directions of the potential at the end of cosmological inflation. This condensate is usually unstable, and it can fragment into non-topological…

天体物理学 · 物理学 2008-12-18 Alexander Kusenko , Anupam Mazumdar

We study the tilt of the primordial gravitational waves spectrum. A hint of blue tilt is shown from analyzing the BICEP2 and POLARBEAR data. Motivated by this, we explore the possibilities of blue tensor spectra from the very early universe…

宇宙学与河外天体物理 · 物理学 2015-06-19 Yi Wang , Wei Xue

The production of a stochastic background of gravitational waves is a fundamental prediction of any cosmological inflationary model. The features of such a signal encode unique information about the physics of the Early Universe and beyond,…

宇宙学与河外天体物理 · 物理学 2016-09-05 Maria Chiara Guzzetti , Nicola Bartolo , Michele Liguori , Sabino Matarrese