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If dark matter (DM) acquires mass during a first order phase transition, there will be a filtering-out effect when DM enters the expanding bubble. In this paper we study the filtering-out effect for a pseudo-scalar DM, whose mass may…

高能物理 - 唯象学 · 物理学 2021-06-30 Wei Chao , Xiu-Fei Li , Lei Wang

First-order phase transitions (FOPT) are ubiquitous in beyond the Standard Model physics and leave distinctive echoes in the history of early universe. We consider a FOPT serving the well-motivated role of dark matter mass generation and…

高能物理 - 唯象学 · 物理学 2026-02-13 Miha Nemevšek , Yue Zhang

We explore the emissions of the Gravitational Waves (GWs) from a strong first-order ekectroweak phase transition. To this end, a dark matter model has been investigated in Feebly Interacting Massive Particle (FIMP) scenario, where the dark…

高能物理 - 唯象学 · 物理学 2020-03-24 Madhurima Pandey , Avik Paul

In this paper we present a novel mechanism for producing the observed Dark Matter(DM) relic abundance during the First Order Phase Transition (FOPT) in the early universe. We show that the bubble expansion with ultra-relativistic velocities…

高能物理 - 唯象学 · 物理学 2021-01-15 Aleksandr Azatov , Miguel Vanvlasselaer , Wen Yin

We explore the production of gravitational waves (GW) resulting from a first-order phase transition (FOPT) in a non-minimally coupled `Dark Higgs Inflation' model. Utilizing a dark sector scalar field as the inflaton, we demonstrate how…

高能物理 - 唯象学 · 物理学 2025-04-21 Jörn Kersten , Seong Chan Park , Yeji Park , Juhoon Son , Liliana Velasco-Sevilla

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

We conducted three-dimensional lattice simulations to study the density perturbation and gravitational waves (GWs) during first-order phase transition (FOPT). We find that for phase transition strength $\alpha > 1$, the forward motion of…

高能物理 - 唯象学 · 物理学 2026-04-13 Jintao Zou , Zhiqing Zhu , Zizhuo Zhao , Ligong Bian

We describe a new mechanism of dark matter production in the early Universe, based on the dynamics of a first order phase transition. We assume that dark matter particles acquire mass during the phase transition, making it energetically…

高能物理 - 唯象学 · 物理学 2020-10-14 Michael J. Baker , Joachim Kopp , Andrew J. Long

Although searches for dark matter have lasted for decades, no convincing signal has been found without ambiguity in underground detections, cosmic ray observations, and collider experiments. We show by example that gravitational wave (GW)…

高能物理 - 唯象学 · 物理学 2022-07-26 Bo-Qiang Lu , Cheng-Wei Chiang , Da Huang

In this work, we show that a large class of models with a composite dark sector undergo a strong first order phase transition in the early universe, which could lead to a detectable gravitational wave signal. We summarise the basic…

高能物理 - 唯象学 · 物理学 2015-11-04 Pedro Schwaller

Gravitational waves (GWs) were recently detected for the first time. This revolutionary discovery opens a new way of learning about particle physics through GWs from first-order phase transitions (FOPTs) in the early Universe. FOPTs could…

高能物理 - 唯象学 · 物理学 2024-01-23 Peter Athron , Csaba Balázs , Andrew Fowlie , Lachlan Morris , Lei Wu

We study the feebly interacting massive particle dark matter whose production processes are significantly affected by the phase evolution and the complicated thermal corrections to the vector boson. We calculate the freeze-in processes to…

高能物理 - 唯象学 · 物理学 2022-09-14 Ligong Bian , Yi-Lei Tang , Ruiyu Zhou

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 study the possibility of generating dark matter (DM) purely from ultra-light primordial black hole (PBH) evaporation with the latter being produced from a first order phase transition (FOPT) in the early Universe. If such ultra-light PBH…

高能物理 - 唯象学 · 物理学 2024-07-23 Debasish Borah , Suruj Jyoti Das , Indrajit Saha

Strongly supercooled first order phase transitions (FOPTs) can produce primordial black hole (PBH) dark matter (DM) along with observable gravitational waves (GWs) from bubble collisions. Such FOPTs may also produce coherent magnetic fields…

高能物理 - 唯象学 · 物理学 2025-03-24 Shyam Balaji , Malcolm Fairbairn , Maria Olalla Olea-Romacho

We study the production of primordial gravitational waves (GWs) from first-order phase transitions (FOPTs) in extensions of the Standard Model based on Flavour Deconstruction (FD). The link fields inherent to FD generically form a rich…

高能物理 - 唯象学 · 物理学 2025-09-17 Noemi Fabri , Gino Isidori , Davide Racco

Gravitational waves signatures from dynamical scalar field configurations provide a compelling observational window on the early universe. Here we identify intriguing connections between dark matter and scalars fields that emit…

高能物理 - 唯象学 · 物理学 2021-07-13 Amit Bhoonah , Joseph Bramante , Simran Nerval , Ningqiang Song

We propose a framework to account for neutrino masses at the two-loop level. This mechanism introduces new scalars and Majorana fermions to the Standard Model. It is assumed the existence of a global $\mathrm{U(1)\times \mathcal{Z}_2}$…

We study the production, spectrum and detectability of gravitational waves in models of the early Universe where first order phase transitions occur during inflation. We consider all relevant sources. The self-consistency of the scenario…

宇宙学与河外天体物理 · 物理学 2011-02-16 Diego Chialva

The nature of dark matter remains one of the greatest unsolved mysteries in elementary particle physics. It might well be that the dark matter particle belongs to a dark sector completely secluded or extremely weakly coupled to the visible…

高能物理 - 唯象学 · 物理学 2024-10-28 Nelleke Bunji , Bartosz Fornal , Kassandra Garcia
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