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Related papers: F\'eeton dark matter above the $e^-e^+$ threshold

200 papers

We present a unified theory of inflation, neutrino mass, baryogenesis and dark matter where global lepton number symmetry and its breaking play a crucial role. The basic idea is to use a lepton number carrying complex scalar field as the…

High Energy Physics - Phenomenology · Physics 2022-03-14 Rabindra N. Mohapatra , Nobuchika Okada

Gauge coupling unification and the success of TeV-scale weakly interacting dark matter are usually taken as evidence of low energy supersymmetry (SUSY). However, if we assume that the tuning of the higgs can be explained in some unnatural…

High Energy Physics - Phenomenology · Physics 2009-11-11 Rakhi Mahbubani , Leonardo Senatore

A new fifth force between particles carrying $B-L$ charges is well-motivated by the intriguing $U(1)_{B-L}$ extension of the standard model. The gauge boson mediator, F\'eeton, also serves as a dark matter candidate. In this letter, we…

High Energy Physics - Phenomenology · Physics 2025-02-04 Yu Cheng , Jie Sheng , Tsutomu T. Yanagida

Extensions of the Standard Model (SM) gauge group with a new $U(1)_X$ predict an additional gauge boson. Through kinetic mixing with the SM photons featured by a coupling $\epsilon$, the ensuing so-called dark photons $\gamma'$, which…

High Energy Physics - Phenomenology · Physics 2020-02-05 Monica D'Onofrio , Oliver Fischer , Zeren Simon Wang

A new dark matter candidate is proposed that arises as the lightest baryon from a confining $SU(N)$ gauge theory which equilibrates with the Standard Model only through electroweak interactions. Surprisingly, this candidate can be as light…

High Energy Physics - Phenomenology · Physics 2025-09-22 George T. Fleming , Graham D. Kribs , Ethan T. Neil , David Schaich , Pavlos M. Vranas

We propose a simple extension of the minimal supersymmetric standard model by introducing a gauge singlet in addition to right-handed neutrinos. The model resolves the strong CP problem by Pecci-Quinn symmetry, explains the origin of…

High Energy Physics - Phenomenology · Physics 2010-08-02 Wan-Il Park

Weak scale supersymmetry has a generic problem of fine-tuning in reproducing the correct scale for electroweak symmetry breaking. The problem is particularly severe in the minimal supersymmetric extension of the standard model (MSSM). We…

High Energy Physics - Phenomenology · Physics 2009-09-29 Ryuichiro Kitano , Yasunori Nomura

Two moderate extensions of the minimal supersymmetric standard model are considered. The first one includes a U(1)_{B-L} gauge group, while the second is based on a left-right symmetric gauge group. In these models, hybrid inflation is…

High Energy Physics - Phenomenology · Physics 2008-11-26 G. Lazarides

The lack of information before Big Bang Neucleosynthesis (BBN) allow us to assume the presence of a new species $\phi$ whose energy density redshifts as $a^{-(4+n)}$ where $n>0$ and $a$ is the scale factor. This non-standard cosmological…

High Energy Physics - Phenomenology · Physics 2023-02-27 Sougata Ganguly , Sourov Roy , Ananya Tapadar

To explain the dark matter and the baryon asymmetry of the Universe, the parameters of the $\nu$MSM (an extension of the Minimal Standard Model by three singlet neutrinos with masses smaller than the electroweak scale) must be fine-tuned:…

High Energy Physics - Phenomenology · Physics 2008-11-26 Mikhail Shaposhnikov

Dark matter consisting of a Bose--Einstein condensate (BEC) of ultra-light particles is predicted to have a soliton shape that shifts with the dark matter mass fraction in galaxies containing a centrally localized point mass (or black…

Astrophysics of Galaxies · Physics 2026-01-21 Dor Ben-Amotz

We propose a new physics model which has a cold dark matter candidate and can explain the $b \to s \mu^+\mu^-$ anomaly at the same time. Our model includes a scalar quark $\widetilde{q}$ and a scalar lepton $\widetilde{\ell}$ which are…

High Energy Physics - Phenomenology · Physics 2018-11-12 Seungwon Baek , Chaehyun Yu

We show how to enlarge the $\nu$MSM (the minimal extension of the standard model by three right-handed neutrinos) to incorporate inflation and provide a common source for electroweak symmetry breaking and for right-handed neutrino masses.…

High Energy Physics - Phenomenology · Physics 2011-05-05 Mikhail Shaposhnikov , Igor Tkachev

We investigate dark matter (DM) phenomenology and cosmic inflation within a unified framework based on a dark $U(1)_D$ gauge extension of the Standard Model (SM). The associated dark gauge boson, namely the dark photon, serves as a viable…

High Energy Physics - Phenomenology · Physics 2026-04-16 Sarif Khan , Jinsu Kim , Pyungwon Ko

It has recently been pointed out that the 511 keV emission line detected by INTEGRAL/SPI from the bulge of our galaxy could be explained by annihilations of light dark matter particles into $e^+ e^-$. We present the possibility that dark…

High Energy Physics - Phenomenology · Physics 2007-05-23 H. N. long , N. Q. Lan , D. V. Soa , L. N. Thuc

We study the possibility to directly detect the boosted dark matter generated from the scatterings with high energetic cosmic particles such as protons and electrons. As a concrete example, we consider the sub-GeV dark matter mediated by a…

High Energy Physics - Phenomenology · Physics 2020-11-18 Wonsub Cho , Ki-Young Choi , Seong Moon Yoo

We investigate the possibility of having a vector boson dark matter in a $U(1)_X$ extended two-Higgs-doublet model (2HDM) setup. The gauge boson gains mass when a SM singlet complex scalar, which is charged under the dark $U(1)_X$ symmetry,…

High Energy Physics - Phenomenology · Physics 2026-01-09 Nandini Das , Juhi Dutta , Dilip Kumar Ghosh , Santosh Kumar Rai

We consider experimental constraints in the MeV region in order to determine the parameter space for the $U(1)_X$ extension of the Standard Model, presented in the first part of our work. In particular, we focus on the model UV-completed by…

High Energy Physics - Phenomenology · Physics 2020-01-08 F. C. Correia , Svjetlana Fajfer

Conventional scenarios of purely gravitationally produced dark matter with masses below the Hubble parameter at the end of inflation are in tension with Cosmic Microwave Background (CMB) constraints on the isocurvature power spectrum. We…

High Energy Physics - Phenomenology · Physics 2024-02-15 Marcos A. G. Garcia , Mathias Pierre , Sarunas Verner
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