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相关论文: Probing Leptophobic Dark Sectors via Gravitational…

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We propose to search for a new type of gravitational wave signature relevant for particle physics models with symmetries broken at vastly different energy scales. The spectrum contains a characteristic double-peak structure consisting of a…

高能物理 - 唯象学 · 物理学 2023-09-26 Bartosz Fornal , Kassandra Garcia , Erika Pierre

We describe a unique gravitational wave signature for a class of models with a vast hierarchy between the symmetry breaking scales. The unusual shape of the signal is a result of the overlapping contributions to the stochastic gravitational…

高能物理 - 唯象学 · 物理学 2021-01-04 Bartosz Fornal , Barmak Shams Es Haghi

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 demonstrate that novel types of gravitational wave signatures arise in theories with new gauge symmetries broken at high energy scales. For concreteness, we focus on models with gauged baryon number and lepton number, in which neutrino…

高能物理 - 唯象学 · 物理学 2023-11-09 Jessica Bosch , Zoraida Delgado , Bartosz Fornal , Alejandra Leon

The quest for a common origin of neutrino mass and baryogenesis is one of the longstanding goals in particle physics. A minimal gauge extension of the Standard Model by $U(1)_{\rm B-L}$ symmetry provides a unique scenario to explain the…

高能物理 - 唯象学 · 物理学 2026-03-18 Anirban Biswas , Sougata Ganguly

We study the possibility of testing a dark matter (DM) scenario embedded in a global lepton number symmetry $U(1)_L$ via gravitational waves (GW) and cosmic microwave background (CMB) observations. The spontaneous breaking of $U(1)_L$…

高能物理 - 唯象学 · 物理学 2024-10-14 Debasish Borah , Nayan Das , Rishav Roshan

We discuss gravitational waves in an electroweakly interacting vector dark matter model. In the model, the electroweak gauge symmetry is extended to SU(2)$_0 \times$ SU(2)$_1 \times$SU(2)$_2 \times$ U(1)$_Y$ and spontaneously broken into…

高能物理 - 唯象学 · 物理学 2024-06-14 Tomohiro Abe , Katsuya Hashino

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

New gauge symmetries often appear in theories beyond the Standard Model. Here we study a model where lepton number is promoted to a gauge symmetry. Anomaly cancellation requires the introduction of additional leptons, the lightest of which…

高能物理 - 唯象学 · 物理学 2019-02-28 Eric Madge , Pedro Schwaller

We investigate the prospects for probing asymmetric dark matter models through their gravitational wave signatures. We concentrate on a theory extending the Standard Model gauge symmetry by a non-Abelian group, under which leptons form…

高能物理 - 唯象学 · 物理学 2023-01-03 Bartosz Fornal , Erika Pierre

We construct a classically scale invariant version of the Zee-Babu model governed by an $U(1)_{B-L}$ gauge symmetry wherein three right handed neutrinos with identical gauge charges are present. A $\mathbb{Z}_2$ symmetry is additionally…

高能物理 - 唯象学 · 物理学 2025-12-30 Indra Kumar Banerjee , Nabarun Chakrabarty , Ujjal Kumar Dey

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

The baryon asymmetry, together with a dark matter asymmetry, may be produced during a first order phase transition in a generative sector. We study the possibility of a gravitational wave signal in a model realising such a scenario. We…

高能物理 - 唯象学 · 物理学 2017-05-18 Iason Baldes

We discuss the phenomenology of a light U(1) gauge boson, $\gamma_B$, that couples only to baryon number. We assume that the new U(1) gauge symmetry is spontaneously broken and that the $\gamma_B$ mass is smaller than $m_Z$. Nevertheless,…

高能物理 - 唯象学 · 物理学 2009-09-29 Christopher D. Carone , Hitoshi Murayama

We study gravitational waves (GWs) with frequencies in the $\mu$Hz range, which arise from phase transitions related to dark confinement in the context of dark versions of Quantum Chromodynamics. Based on several compelling motivations, we…

高能物理 - 唯象学 · 物理学 2024-05-28 Martin Rosenlyst

We explore the gravitational wave probes of a two-component dark matter framework, consisting of an $SU(2)_L$ triplet scalar and a Standard Model singlet fermion. The triplet scalar dark matter typically remains underabundant in the region…

高能物理 - 唯象学 · 物理学 2025-05-16 Pankaj Borah , Pradipta Ghosh , Abhijit Kumar Saha

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

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

Many extensions of the Standard Model include a new $U(1)$ gauge group that is broken spontaneously at a scale much above TeV. If a $U(1)$-breaking phase transition occurs at nucleation temperature of $O(100)$-$O(1000)$~TeV, it can generate…

高能物理 - 唯象学 · 物理学 2020-04-22 Naoyuki Haba , Toshifumi Yamada

Motivated by some of the recent swampland conjectures, we study a model of dark energy, in which a quintessence axion slowly rolls in a steep potential due to its interactions with a U(1) or an SU(2) gauge field. The gauge fields produced…

宇宙学与河外天体物理 · 物理学 2020-11-13 Alexandros Papageorgiou
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