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Gravitational waves potentially represent our only direct probe of the universe when it was less than one second old. In particular, first-order phase transitions in the early universe can generate a stochastic background of gravitational…

天体物理学 · 物理学 2008-11-26 Tina Kahniashvili , Arthur Kosowsky , Grigol Gogoberidze , Yurii Maravin

We review the production of gravitational waves by an electroweak first order phase transition. The resulting signal is a good candidate for detection at next-generation gravitational wave detectors, such as LISA. Detection of such a source…

高能物理 - 唯象学 · 物理学 2023-07-28 David J. Weir

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

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

A stochastic background of gravitational waves can be generated during a cosmological first order phase transition, at least by two distinct mechanisms: collisions of true vacuum bubbles and turbulence in the cosmic fluid. I compare these…

广义相对论与量子宇宙学 · 物理学 2009-11-10 Alberto Nicolis

It is currently believed that the Standard Model is an effective low energy theory which in principle may contain higher dimensional non-renormalizable operators. These operators may modify the standard model Higgs potential in many ways,…

宇宙学与河外天体物理 · 物理学 2010-12-01 Eric Greenwood , Pascal M. Vaudrevange

The next generation of gravitational wave detectors holds out the prospect of detecting a stochastic gravitational background generated in the very early universe. In this article, we review the various cosmological processes which can lead…

天体物理学 · 物理学 2010-04-06 R. A. Battye , E. P. S. Shellard

We investigate the properties of a stochastic gravitational wave background produced by a first-order electroweak phase transition in the regime of extreme supercooling. We study a scenario whereby the percolation temperature that signifies…

高能物理 - 唯象学 · 物理学 2017-11-09 Archil Kobakhidze , Cyril Lagger , Adrian Manning , Jason Yue

First order phase transitions in the early Universe generate gravitational waves, which may be observable in future space-based gravitational wave observatiories, e.g. the European eLISA satellite constellation. The gravitational waves…

高能物理 - 格点 · 物理学 2015-11-17 Mark Hindmarsh , Stephan Huber , Kari Rummukainen , David Weir

After the discovery of the Higgs boson, understanding the nature of electroweak symmetry breaking and the associated electroweak phase transition has become the most pressing question in particle physics. Answering this question is a…

高能物理 - 唯象学 · 物理学 2017-05-16 Peisi Huang , Andrew J. Long , Lian-Tao Wang

We discuss spectra of gravitational waves which are originated by the strongly first order phase transition at the electroweak symmetry breaking, which is required for a successful scenario of electroweak baryogenesis. Such spectra are…

高能物理 - 唯象学 · 物理学 2015-12-16 Mitsuru Kakizaki , Shinya Kanemura , Toshinori Matsui

In this paper we consider an extension of the Standard Model(SM) with additional gauge singlets which exhibits a strong first order phase transition. Due to this first order phase transition in the early universe gravitational waves are…

高能物理 - 唯象学 · 物理学 2018-12-05 Mina Saeedhoseini , Ali Tofighi

We investigate the potential stochastic gravitational waves from first-order electroweak phase transitions in a model with pseudo-Nambu-Goldstone dark matter and two Higgs doublets. The dark matter candidate can naturally evade direct…

高能物理 - 唯象学 · 物理学 2023-01-11 Zhao Zhang , Chengfeng Cai , Xue-Min Jiang , Yi-Lei Tang , Zhao-Huan Yu , Hong-Hao Zhang

During a strongly first-order phase transition gravitational waves are produced by bubble collisions and turbulent plasma motion. We analyze the relevant characteristics of the electroweak phase transition in the nMSSM to determine the…

高能物理 - 唯象学 · 物理学 2008-11-26 Stephan J. Huber , Thomas Konstandin

We calculate the spectrum of gravitational waves originated from strongly first order electroweak phase transition in the extended Higgs model with a real singlet field. In order to calculate the bubble nucleation rate, we perform a…

高能物理 - 唯象学 · 物理学 2017-01-04 Katsuya Hashino , Mitsuru Kakizaki , Shinya Kanemura , Pyungwon Ko , Toshinori Matsui

We consider a standard model extension equipped with a dark sector where the $U(1)_X^{}$ Abelian gauge symmetry is spontaneously broken by the dark Higgs mechanism. In this framework, we investigate patterns of the electroweak phase…

高能物理 - 唯象学 · 物理学 2018-07-02 Katsuya Hashino , Mitsuru Kakizaki , Shinya Kanemura , Pyungwon Ko , Toshinori Matsui

We forecast the prospective of detection for a stochastic gravitational wave background sourced by cosmological first-order phase transitions. We focus on first-order phase transitions with negligible plasma effects, and consider the…

宇宙学与河外天体物理 · 物理学 2018-10-30 Daniel G. Figueroa , Eugenio Megias , Germano Nardini , Mauro Pieroni , Mariano Quiros , Angelo Ricciardone , Gianmassimo Tasinato

In many particle physics models, domain wall can form during the phase transition process after discrete symmetry breaking. We study the scenario within a complex singlet extended Standard Model framework, where a strongly first order phase…

高能物理 - 唯象学 · 物理学 2020-05-20 Ruiyu Zhou , Jing Yang , Ligong Bian

We investigate the production of a stochastic background of gravitational waves in the electroweak phase transition. We consider extensions of the Standard Model which can give very strongly first-order phase transitions, such that the…

宇宙学与河外天体物理 · 物理学 2016-05-25 Leonardo Leitao , Ariel Megevand

Theories of dynamical electroweak symmetry breaking predict a strong first order cosmological phase transition: we compute the resulting signals, primordial black holes and gravitational waves. These theories employ one SM-neutral scalar,…

高能物理 - 唯象学 · 物理学 2025-03-06 Martín Arteaga , Anish Ghoshal , Alessandro Strumia
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