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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 study the gravitational waves (GWs) spectrum produced during the electroweak phase transition in a scale-invariant extension of the Standard Model (SM), enlarged by a dark $ U(1)_{D} $ gauge symmetry. This symmetry incorporates a vector…

高能物理 - 唯象学 · 物理学 2020-03-10 Ahmad Mohamadnejad

In this work we shall study the impact of a second order electroweak phase transition occurring at $\sim 150\,$GeV on the energy spectrum of the stochastic gravitational background. Specifically, we assume that the non-minimally coupled…

高能物理 - 唯象学 · 物理学 2025-10-21 V. K. Oikonomou

Cosmological phase transitions can be a source of Stochastic Gravitational Wave (SGW) background. Apart from the dynamics of the phase transition, the characteristic frequency and the fractional energy density $\Omega_{\rm gw}$ of the SGW…

高能物理 - 唯象学 · 物理学 2017-03-16 Sampurn Anand , Ujjal Kumar Dey , Subhendra Mohanty

We study a scenario where the Standard Model is extended by a SU(2) gauge group in the dark sector. The three associated dark gauge bosons are stabilised via a custodial symmetry triggered by an additional dark SU(2) scalar doublet, thus…

高能物理 - 唯象学 · 物理学 2025-12-03 Nico Benincasa , Luigi Delle Rose , Luca Panizzi , Maimoona Razzaq , Savio Urzetta

A first order electroweak phase transition probes physics beyond the Standard Model on multiple frontiers and therefore is of immense interest for theoretical exploration. We conduct a model-independent study of the effects of relevant…

高能物理 - 唯象学 · 物理学 2024-08-20 Upalaparna Banerjee , Sabyasachi Chakraborty , Suraj Prakash , Shakeel Ur Rahaman

We study the gravitational radiation produced by the collisions of bubble walls or thin fluid shells in cosmological phase transitions. Using the so-called envelope approximation, we obtain analytically the asymptotic behavior of the…

宇宙学与河外天体物理 · 物理学 2022-01-05 Ariel Megevand , Agustin Membiela

The recent detection of a gravitational wave background in the nano-Hertz frequency range by Pulsar Timing Array (PTA) collaborations, including NANOGrav, EPTA, and PPTA, has opened a new avenue for exploring fundamental physics in the…

宇宙学与河外天体物理 · 物理学 2026-02-17 Jinzheng Li , Pran Nath

The gravitational waves (GW) background generated in a double inflationary model, with two scalar fields mutually interacting through gravity only, and its relative contribution $T/S$ to large-angle temperature fluctuations of the relic…

天体物理学 · 物理学 2009-10-28 David Polarski , Alexei A. Starobinsky

We investigate the impact of a semi-decoupled dark sector with a temperature hierarchy relative to the Standard Model plasma on the electroweak phase transition and its associated gravitational wave signal. Working within a minimal…

高能物理 - 唯象学 · 物理学 2026-02-25 Arnab Chaudhuri

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 search for a first-order phase transition gravitational wave signal in 45 pulsars from the NANOGrav 12.5 year dataset. We find that the data can be modeled in terms of a strong first order phase transition taking place at temperatures…

Supercooled phase transitions, as predicted, e.g., in near-conformal and confining extensions of the Standard Model (SM), are established sources of strong stochastic gravitational wave backgrounds (SGWBs). In this work, we investigate…

高能物理 - 唯象学 · 物理学 2025-12-24 Satyabrata Datta , Rome Samanta

In this work, we present a self-consistent prediction for the gravitational wave signal arising from confinement-induced phase transitions in hidden non-Abelian SU(N) gauge theories with F light flavors. To do this, we impose perturbativity…

高能物理 - 唯象学 · 物理学 2025-12-01 Rachel Houtz , Martha Ulloa , Mia West

We consider the impact of thermal inflation -- a short, secondary period of inflation that can arise in supersymmetric scenarios -- on the stochastic gravitational wave background. We show that while the primordial inflationary…

天体物理学 · 物理学 2009-06-23 Richard Easther , John T. Giblin , Eugene A. Lim , Wan-Il Park , Ewan D. Stewart

We introduce an approximation to calculate the gravitational radiation produced by the collision of true-vacuum bubbles that is simple enough to allow the simulation of a phase transition by the collision of hundreds of bubbles. This…

天体物理学 · 物理学 2008-11-26 Arthur Kosowsky , Michael S. Turner

It has recently been suggested that collapse of neutron stars induced by a phase transition to quark matter can be a considerable source of gravitational waves with kHz frequencies. We demonstrate that if about one percent of all neutron…

天体物理学 · 物理学 2009-11-11 Guenter Sigl

We consider the effect of classical phase fluctuations on the quasiparticle spectra of underdoped high-$T_c$ cuprate superconductors in the pseudogap regime above $T_c$. We show that photoemission and tunneling spectroscopy data are well…

超导电性 · 物理学 2007-05-23 M. Franz , A. J. Millis

A rather minimal possibility is that dark matter consists of the gauge bosons of a spontaneously broken symmetry. Here we explore the possibility of detecting the gravitational waves produced by the phase transition associated with such…

高能物理 - 唯象学 · 物理学 2019-05-30 Iason Baldes , Camilo Garcia-Cely

This review article is based on a seminar presented at the Higgs pairs workshop 2025. Stochastic gravitational wave backgrounds can serve as probe of the diverse phenomenology encountered in beyond-Standard-Model scenarios featuring phase…

宇宙学与河外天体物理 · 物理学 2026-02-04 Chiara Caprini