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相关论文: Dark Discrete Gauge Symmetries

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We review models of new physics in which dark matter arises as a composite bound state from a confining strongly-coupled non-Abelian gauge theory. We discuss several qualitatively distinct classes of composite candidates, including dark…

高能物理 - 唯象学 · 物理学 2016-08-24 Graham D. Kribs , Ethan T. Neil

We consider a simple class of models in which the relic density of dark matter is determined by the baryon asymmetry of the universe. In these models a $B - L$ asymmetry generated at high temperatures is transfered to the dark matter, which…

高能物理 - 唯象学 · 物理学 2009-07-09 David E. Kaplan , Markus A. Luty , Kathryn M. Zurek

In this paper we explore the possibility that the sterile neutrino and Dark Matter sectors in the Universe have a common origin. We study the consequences of this assumption in the simple case of coupling the dark sector to the Standard…

高能物理 - 唯象学 · 物理学 2017-03-03 Miguel Escudero , Nuria Rius , Verónica Sanz

Cosmologically long-lived, composite states arise as natural dark matter candidates in theories with a strongly interacting hidden sector at a scale of 10 - 100 TeV. Light axion-like states, with masses in the 1 MeV - 10 GeV range, are also…

高能物理 - 唯象学 · 物理学 2010-05-28 Jeremy Mardon , Yasunori Nomura , Jesse Thaler

We discuss the implications of a gauged Abelian hidden-sector communicating with the Standard Model (SM) fields via kinetic mixing with the SM hypercharge gauge field, or via the Higgs quartic interaction. We discuss signatures of the…

高能物理 - 唯象学 · 物理学 2015-05-14 Shrihari Gopalakrishna

We consider dark matter physics in a model for the dark sector with extra dark U(1)$_X$ gauge symmetry. The dark sector is composed of exotic fermions that are charged under both dark U(1)$_X$ and the standard model SU(3)$_C \times$U(1)$_Y$…

高能物理 - 唯象学 · 物理学 2016-12-14 P. Ko , Takaaki Nomura

The nature of dark matter is a problem with too many potential solutions. We investigate whether a consistent embedding into quantum gravity can decimate the number of solutions to the dark-matter problem. Concretely, we focus on a hidden…

高能物理 - 唯象学 · 物理学 2024-03-21 Gustavo P. de Brito , Astrid Eichhorn , Mads T. Frandsen , Martin Rosenlyst , Mattias E. Thing , Arthur F. Vieira

We introduce a novel dark matter scenario where the visible sector and the dark sector share a common asymmetry. The two sectors are connected through an unstable mediator with baryon number one, allowing the standard model baryon asymmetry…

高能物理 - 唯象学 · 物理学 2016-03-16 Nayara Fonseca , Lina Necib , Jesse Thaler

With the assistance of two extra groups, i.e., an extra hidden gauge group $SU(2)_D$ and a global $U(1)$ group, we propose a two component dark matter (DM) model. After the symmetry $SU(2)_D\times U(1)$ being broken, we obtain both the…

高能物理 - 唯象学 · 物理学 2015-03-05 Ligong Bian , Tianjun Li , Jing Shu , Xiao-Chuan Wang

We consider thermal production mechanisms of self-interacting dark matter in models with gauged $Z_3$ symmetry. A complex scalar dark matter is stabilized by the $Z_3$, that is the remnant of a local dark $U(1)_d$. Light dark matter with…

高能物理 - 唯象学 · 物理学 2017-02-01 Soo-Min Choi , Yoo-Jin Kang , Hyun Min Lee

A simple way of explaining dark matter without modifying known Standard Model physics is to require the existence of a hidden (dark) sector, which interacts with the visible one predominantly via gravity. We consider a hidden sector…

高能物理 - 唯象学 · 物理学 2020-03-04 R. Foot , S. Vagnozzi

Many models have recently been proposed in which dark matter (DM) couples to Standard Model fields via a GeV-scale dark sector. We consider scenarios of this type where the DM mass, at the electroweak/TeV scale, is generated by the VEV of a…

高能物理 - 唯象学 · 物理学 2010-06-11 David Krohn , Joshua T. Ruderman , Lian-Tao Wang

We show that a conformal-invariant dark sector, interacting conformally with the Standard Model (SM) fields through the Higgs portal, provides a viable framework where cold dark matter (CDM) and invisible Higgs decays can be addressed…

高能物理 - 唯象学 · 物理学 2014-01-27 Durmus A. Demir , Mariana Frank , Beste Korutlu

We consider a U(1)' gauge symmetry acting on three generations of right-handed neutrinos. The U(1)' symmetry is broken at the TeV scale and its remnant discrete symmetry makes one of the right-handed neutrinos stable. As a natural…

高能物理 - 唯象学 · 物理学 2014-01-29 Manfred Lindner , Daniel Schmidt , Atsushi Watanabe

Models of inelastic (or pseudo-Dirac) dark matter commonly introduce a gauge symmetry spontaneously broken by the introduction of a dark sector version of the Higgs mechanism. We find that this ubiquitous introduction of two extra fields, a…

高能物理 - 唯象学 · 物理学 2025-02-13 Giovani Dalla Valle Garcia

The vector boson dark matter particles which stem from some broken gauge symmetries usually requires some unbroken symmetries to keep themselves stable. In the previous literature, some simplest cases have been discussed, in which the…

高能物理 - 唯象学 · 物理学 2025-02-13 Chun-Xue Yuan , Zhao Zhang , Chengfeng Cai , Yi-Lei Tang , Hong-Hao Zhang

We study classically scale invariant models in which the Standard Model Higgs mass term is replaced in the Lagrangian by a Higgs portal coupling to a complex scalar field of a dark sector. We focus on models that are weakly coupled with the…

高能物理 - 唯象学 · 物理学 2015-06-22 Wolfgang Altmannshofer , William A. Bardeen , Martin Bauer , Marcela Carena , Joseph D. Lykken

We investigate the phenomenology of flavored dark matter (DM). DM stability is guaranteed by an accidental ${\mathcal Z}_3$ symmetry, a subgroup of the standard model (SM) flavor group that is not broken by the SM Yukawa interactions. We…

高能物理 - 唯象学 · 物理学 2016-01-27 Fady Bishara , Admir Greljo , Jernej F. Kamenik , Emmanuel Stamou , Jure Zupan

We revisit the possibility of a Dirac fermion dark matter candidate in the light of current $b \to s \ell^+ \ell^-$ anomalies by investigating a minimal extension of the Standard Model with a horizontal $\mathrm{U(1)}^{\prime}$ local…

高能物理 - 唯象学 · 物理学 2017-02-27 Alejandro Celis , Wan-Zhe Feng , Martin Vollmann

To properly solve the coincidence problem ($\Omega_\mathrm{DM} \simeq 5\Omega_\mathrm{VM}$) in a model of asymmetric dark matter, one cannot simply relate the number densities of visible and dark matter without also relating their particle…

高能物理 - 唯象学 · 物理学 2024-04-10 Alexander C. Ritter , Raymond R. Volkas