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Related papers: Dark Matter Candidate from Conformality

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We consider the minimal model in which dark matter is stabilized by a non-Abelian discrete symmetry. The symmetry group is taken to be D_3, which is the smallest non-Abelian finite group. The minimal model contains (nontrivial) singlet and…

High Energy Physics - Phenomenology · Physics 2015-03-19 Adisorn Adulpravitchai , Brian Batell , Josef Pradler

The lack of evidence for low energy supersymmetry at the LHC implies a supersymmetry scale in excess a TeV. While this is consistent (and even helpful) with a Higgs boson mass at $\approx$ 125 GeV, simple supersymmetric models with scalar…

High Energy Physics - Phenomenology · Physics 2016-04-26 Keith A. Olive

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…

High Energy Physics - Phenomenology · Physics 2019-02-28 Eric Madge , Pedro Schwaller

The LEP experiment at CERN provided accurate measurements of the $Z$ neutral gauge boson properties. Although all measurements agree well with the SM predictions, the forward backward asymmetry of the bottom-quark remains almost 3$\sigma$…

High Energy Physics - Phenomenology · Physics 2018-03-19 Da Liu , Jia Liu , Carlos E. M. Wagner , Xiao-Ping Wang

Hints of direct dark matter detection coming from the DAMA, CoGeNT experiments point toward light dark matter with isospin-violating and possibly inelastic couplings. However an array of astrophysical constraints are rapidly closing the…

High Energy Physics - Phenomenology · Physics 2015-05-30 James M. Cline , Andrew R. Frey

We re-investigate the question whether a light higgsino-like neutralino is a viable Dark Matter candidate. To this end we compute the dominant one-loop corrections to the masses of the higgsino-like states in the minimal Supersymmetric…

High Energy Physics - Phenomenology · Physics 2014-11-17 M. Drees , M M. Nojiri , D. P. Roy , Y. Yamada

Scenarios for secluded WIMP dark matter models have been extensively studied in simplified versions. This paper shows a complete UV realization of a secluded WIMP dark matter model with an extra Abelian gauge symmetry that includes…

High Energy Physics - Phenomenology · Physics 2025-05-09 Kimy Agudelo , Diego Restrepo , Andrés Rivera , David Suarez

A dark sector resembling the standard model, where the abundance of matter is explained by baryon and lepton asymmetries, and stable constituents bind to form atoms, is a theoretically appealing possibility. We show that a minimal model…

High Energy Physics - Phenomenology · Physics 2015-12-23 Jeremie Choquette , James M. Cline

In the context of the relationship between physics of cosmological dark matter and symmetry of elementary particles a wide list of dark matter candidates is possible. New symmetries provide stability of different new particles and their…

High Energy Physics - Phenomenology · Physics 2017-04-26 M. Yu. Khlopov

Dark matter constitutes about $23\%$ of the total energy density of the universe but its properties are still little known besides that it should be composed by cold and weakly interacting particles. Many beyond standard model theories can…

High Energy Physics - Phenomenology · Physics 2017-05-18 Qiaoli Yang

We study a natural implementation of Asymmetric Dark Matter in Twin Higgs models. The mirroring of the Standard Model strong sector suggests that a twin baryon with mass around 5 GeV is a natural Dark Matter candidate once a twin baryon…

High Energy Physics - Phenomenology · Physics 2015-11-11 Marco Farina

We show that a metastable dark matter candidate arises naturally from the conformal transformation between the Einstein metric, where gravitons are normalised states, and the Jordan metric dictating the coupling between gravity and matter.…

High Energy Physics - Phenomenology · Physics 2021-06-23 Philippe Brax , Kunio Kaneta , Yann Mambrini , Mathias Pierre

I address the question of whether supersymmetry provides a viable candidate for the dark matter in the Universe. I review the properties of the lightest neutralino as a candidate for solving the dark matter problem. I discuss the…

High Energy Physics - Phenomenology · Physics 2007-05-23 Leszek Roszkowski

The extension of the Standard model (SM) with three heavy right handed neutrinos, a complex scalar and the gauged $U(1)_{\rm B-L}$ symmetry (the minimal $B-L$ model) is considered the most compelling minimal one: the presence and the…

High Energy Physics - Phenomenology · Physics 2021-01-19 Gongjun Choi , Tsutomu T. Yanagida , Norimi Yokozaki

Axion-like particles (ALPs) arise from well-motivated extensions to the Standard Model and could account for dark matter. ALP dark matter would manifest as a field oscillating at an (as of yet) unknown frequency. The frequency depends…

One of the major challenges of modern physics is to decipher the nature of dark matter. Astrophysical observations provide ample evidence for the existence of an invisible and dominant mass component in the observable universe, from the…

Cosmology and Nongalactic Astrophysics · Physics 2015-09-04 Laura Baudis

A lepto-baryonic left-right symmetric theory is considered along with pointing out stable dark matter candidates whose stability is ensured automatically where leptons and baryons are defined as local gauge symmetries. These theories are…

High Energy Physics - Phenomenology · Physics 2016-05-11 Sudhanwa Patra

The dark matter puzzle is one of the most important open problems in modern physics. The ultra-light axion is a well-motivated dark matter candidate, conceived to resolve the strong-CP problem of quantum chromodynamics. Numerous precision…

High Energy Physics - Phenomenology · Physics 2023-07-24 Alexander O. Sushkov

In the early Universe, any particle carrying a conserved quantum number and in chemical equilibrium with the thermal bath will unavoidably inherit a particle-antiparticle asymmetry. A new particle of this type, if stable, would represent a…

High Energy Physics - Phenomenology · Physics 2015-07-08 Sofiane M. Boucenna , Martin B. Krauss , Enrico Nardi
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