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This paper presents an estimate for the spectral properties of the stochastic background of gravitational waves emitted by a population of hot, young, rapidly rotating neutron stars throughout the Universe undergoing $f$-mode instabilities,…

宇宙学与河外天体物理 · 物理学 2016-02-03 Marco Surace , Kostas D. Kokkotas , Pantelis Pnigouras

Stellar core collapse events are expected to produce gravitational waves via several mechanisms, most of which are not yet fully understood due to the current limitations in the numerical simulations of these events. In this paper, we begin…

宇宙学与河外天体物理 · 物理学 2017-04-05 Kyle Crocker , Tanner Prestegard , Vuk Mandic , Tania Regimbau , Keith Olive , Elisabeth Vangioni

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

We present the first end-to-end nonperturbative analysis of the gravitational wave power spectrum from a thermal first-order electroweak phase transition (EWPT), using the framework of dimensionally reduced effective field theory and…

高能物理 - 唯象学 · 物理学 2019-12-18 Oliver Gould , Jonathan Kozaczuk , Lauri Niemi , Michael J. Ramsey-Musolf , Tuomas V. I. Tenkanen , David J. Weir

Gravitational waves offer an unprecedented opportunity to look into the violent high-energy processes happening during the reheating phase of our Universe. We consider a Hubble-induced phase transition scenario as a source of a…

广义相对论与量子宇宙学 · 物理学 2025-10-21 Dario Bettoni , Giorgio Laverda , Asier Lopez-Eiguren , Javier Rubio

Flavourful extensions of the Standard Model aimed at explaining its fermionic mass structure typically rely on symmetries, broken at high-energy scales far beyond the reach of foreseeable direct collider searches. We illustrate, using a…

高能物理 - 唯象学 · 物理学 2025-12-03 Anna Chrysostomou , Alan S. Cornell , Luc Darmé , Aldo Deandrea , Thibault Demartini

Stochastic backgrounds of gravitational waves (GWs) from the pre-BBN era offer a unique opportunity to probe the universe beyond what has already been achieved with the Cosmic Microwave Background (CMB). If the source is short in duration,…

高能物理 - 唯象学 · 物理学 2023-06-13 Joshua Berger , Amit Bhoonah , Biswajit Padhi

We study stochastic gravitational wave production and baryon number generation at electroweak phase transition with the two Higgs doublet models. The produced stochastic gravitational wave during the strongly first-order phase transition…

高能物理 - 唯象学 · 物理学 2022-04-19 Ruiyu Zhou , Ligong Bian

Sphaleron electroweak phase transition (EWPT) is calculated in two phase transition stages, thereby showing that the twin (or double) bubble nucleation structure of the phase transition and gravitational wave is in the investigation area of…

高能物理 - 唯象学 · 物理学 2025-09-09 Vo Quoc Phong , Nguyen Xuan Vinh , Phan Hong Khiem

We consider a holographic study of coupling dependent gravitational waves produced by the cosmic first order QCD phase transition at finite baryochemical potential. In the dual description, the first-order QCD phase transition corresponds…

高能物理 - 理论 · 物理学 2020-06-09 M. Ahmadvand , K. Bitaghsir Fadafan , S. Rezapour

We study gravitational-wave production from bubble dynamics (bubble collisions and sound waves) during a cosmic first-order phase transition with an analytic approach. We first propose modeling the system with the thin-wall approximation…

高能物理 - 唯象学 · 物理学 2021-09-14 Ryusuke Jinno , Masahiro Takimoto

We show that quantum fluctuations of an expanding phase transition bubble give rise to gravitational wave (GW) emission, even when considering a single bubble, without bubble collisions or plasma effects. The ratio of GW energy to the total…

广义相对论与量子宇宙学 · 物理学 2024-04-03 Kfir Blum , Mehrdad Mirbabayi

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

We study the electroweak phase transition within a 5D warped model including a scalar potential with an exponential behavior, and strong back-reaction over the metric, in the infrared. By means of a novel treatment of the superpotential…

高能物理 - 唯象学 · 物理学 2018-10-17 Eugenio Megias , Germano Nardini , Mariano Quiros

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 type-II seesaw model is a possible candidate for simultaneously explaining non-vanishing neutrino masses and the observed baryon asymmetry of the Universe. In this work, we study in detail the pattern of phase transition and the…

高能物理 - 唯象学 · 物理学 2022-09-07 Ruiyu Zhou , Ligong Bian , Yong Du

Particle phase transitions in the early universe including electroweak and grand unification ones are well-studied subjects. We point out that there are new possible particle phase transitions around inflation. Those new inflationary…

宇宙学与河外天体物理 · 物理学 2019-02-27 Sichun Sun

We investigate the properties of gravitational waves generated by heating induced phase transitions in warm inflation. In this scenario, the heating phase of inflation followed by subsequent cosmological cooling can trigger two associated…

广义相对论与量子宇宙学 · 物理学 2025-10-28 Xiao-Bin Sui , Jing Liu , Rong-Gen Cai

We study gravitational waves from the first-order electroweak phase transition in the $SU(N_c)$ gauge theory with $N_f/N_c\gg 1$ ("large $N_f$ QCD") as a candidate for the walking technicolor, which is modeled by the $U(N_f)\times U(N_f)$…

高能物理 - 唯象学 · 物理学 2020-01-08 Kohtaroh Miura , Hiroshi Ohki , Saeko Otani , Koichi Yamawaki

We investigate the evolution of the electroweak phase transition, using a one-Higgs effective potential that can be regarded as an approximation for the Minimal Supersymmetric Standard Model. The phase transition occurs in a small interval…

高能物理 - 唯象学 · 物理学 2009-10-31 Ariel Megevand