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相关论文: Gravitational Techniwaves

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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

Several phenomenologically viable walking technicolor models have been proposed recently. I demonstrate that these models can have first order electroweak phase transitions, which are sufficiently strong for electroweak baryogenesis. Strong…

高能物理 - 唯象学 · 物理学 2015-05-20 Matti Jarvinen

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 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

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 study the generation of gravitational waves in the electroweak phase transition. We consider a few extensions of the Standard Model, namely, the addition of scalar singlets, the minimal supersymmetric extension, and the addition of TeV…

宇宙学与河外天体物理 · 物理学 2012-10-19 Leonardo Leitao , Ariel Megevand , Alejandro D. Sanchez

Thermal corrections in classically conformal models typically induce a strong first-order electroweak phase transition, thereby resulting in a stochastic gravitational wave background that could be detectable at gravitational wave…

高能物理 - 唯象学 · 物理学 2017-08-02 Luca Marzola , Antonio Racioppi , Ville Vaskonen

Multi-peaked spectra of the primordial gravitational waves are considered as a phenomenologically relevant source of information about the dynamics of sequential phase transitions in the early Universe. In particular, such signatures trace…

高能物理 - 唯象学 · 物理学 2020-04-29 António P. Morais , Roman Pasechnik

We explore the possibility of detecting gravitational waves generated by first order phase transitions in multiple dark sectors. Nnaturalness is taken as a sample model that features multiple additional sectors, many of which undergo phase…

高能物理 - 唯象学 · 物理学 2020-05-25 Paul Archer-Smith , Dylan Linthorne , Daniel Stolarski

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

We discuss possibilities to observe stochastic gravitational wave backgrounds produced by the electroweak phase transition in the early universe. Once the first-order phase transition occurs, which is still predicted in a lot of theories…

高能物理 - 唯象学 · 物理学 2014-06-06 Yohei Kikuta , Kazunori Kohri , Eunseong So

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

A chiral-symmetric technicolor model successfully reconciles the tension between electroweak precision tests and traditional technicolor models. Focusing on its simplest realization preserving the conventional Higgs mechanism, we study its…

高能物理 - 唯象学 · 物理学 2022-06-01 Hao Yang , Felipe F. Freitas , Antonino Marciano , António P. Morais , Roman Pasechnik , João Viana

First order phase transitions are well-motivated and extensively studied sources of gravitational waves (GWs) from the early Universe. The vacuum energy released during such transitions is assumed to be transferred primarily either to the…

广义相对论与量子宇宙学 · 物理学 2026-02-06 Ryusuke Jinno , Bibhushan Shakya , Jorinde van de Vis

We perform a three dimensional lattice simulation of the electroweak symmetry breaking process through a two-step phase transition, where one of the two steps is a first order phase transition. Our results show that: 1) when the electroweak…

高能物理 - 唯象学 · 物理学 2022-04-12 Zizhuo Zhao , Yuefeng Di , Ligong Bian , Rong-Gen Cai

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

This study undertakes a reconsideration of the potential for a first-order electroweak phase transition, focusing on the next-to-minimal two Higgs doublet model (N2HDM). Our exploration spans diverse parameter spaces associated with the…

高能物理 - 唯象学 · 物理学 2024-04-17 Arnab Chaudhuri , Kazunori Kohri

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

I discuss the generation of a stochastic background of gravitational waves during a first order phase transition. I present simple general arguments which explain the main features of the gravitational wave spectrum like the $k^3$ power law…

宇宙学与河外天体物理 · 物理学 2010-06-02 Ruth Durrer
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