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Related papers: Study of dark matter in the extended BLMSSM

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As the LHC continues to search for new weakly interacting particles, it is important to remember that the search is strongly motivated by the existence of dark matter. In view of a possible positive signal, it is essential to ask whether…

High Energy Physics - Phenomenology · Physics 2015-03-17 Giorgio Busoni , Andrea De Simone , Thomas Jacques , Enrico Morgante , Antonio Riotto

We investigate the constraints on the Inert Doublet Model (IDM), a minimal extension of the Standard Model of Particle Physics featuring a scalar dark matter candidate, using data from recent and future gamma-ray observatories. The…

High Energy Physics - Phenomenology · Physics 2026-03-19 Lucca Radicce Justino , Clarissa Siqueira , Aion Viana

The astronomical dark matter is an essential component of the Universe and yet its nature is still unresolved. It could be made of neutral and massive elementary particles which are their own antimatter partners. These dark matter species…

High Energy Astrophysical Phenomena · Physics 2015-06-19 Pierre Salati

We explore dark matter in the Finely Tuned Minimal Supersymmetric Standard model recently proposed by Arkani-Hamed and Dimopoulos. Relative to the MSSM, there are fewer particles at freeze-out, so the calculation of the relic abundance…

High Energy Physics - Phenomenology · Physics 2008-11-26 Aaron Pierce

In an extension of MSSM with two triplets and a singlet, called the TNMSSM, there are seven neutralinos which can enrich the study of cold dark matter if one expects that the weakly interacting massive particle (WIMP) is responsible for the…

High Energy Physics - Phenomenology · Physics 2024-11-28 Zhong-Jun Yang , Jin-Lei Yang , Shu-Min Zhao , Xing-Gang Wu , Tai-Fu Feng

Motivated by the hypothesis that dark matter self-interactions provide a solution to the small-scale structure formation problems, we investigate the possibilities that the relic density of a self-interacting dark matter candidate can…

High Energy Physics - Phenomenology · Physics 2016-11-16 Xiaoyong Chu , Camilo Garcia-Cely , Thomas Hambye

A conservative upper bound on the total dark matter (DM) annihilation rate can be obtained by constraining the appearance rate of the annihilation products which are hardest to detect. The production of neutrinos, via the process $\chi \chi…

High Energy Physics - Phenomenology · Physics 2008-12-22 Nicole F. Bell , James B. Dent , Thomas D. Jacques , Thomas J. Weiler

Thermal freeze-out is a prominent example of dark matter (DM) production mechanism in the early Universe that can yield the correct relic density of stable weakly interacting massive particles (WIMPs). At the other end of the mass scale,…

High Energy Physics - Phenomenology · Physics 2020-08-05 Sebastian Trojanowski , Philippe Brax , Carsten van de Bruck

PAMELA and ATIC recently reported excesses in e+ e- cosmic rays. Since the interpretation in terms of DM annihilations was found to be not easily compatible with constraints from photon observations, we consider the DM decay hypothesis and…

High Energy Physics - Phenomenology · Physics 2009-05-26 Enrico Nardi , Francesco Sannino , Alessandro Strumia

At the tail of its velocity distribution, cold dark matter (DM) can annihilate at finite temperature to states heavier than itself. We explore the possibility that DM freezeout is dictated by these "forbidden annihilations" at the…

High Energy Physics - Phenomenology · Physics 2017-02-15 Antonio Delgado , Adam Martin , Nirmal Raj

We present a comprehensive study of secluded dark matter (DM) $\chi$, where the relic abundance is set by annihilations into lighter dark mediators $\phi$ that couple only feebly to the Standard Model (SM). In contrast to canonical WIMPs,…

High Energy Physics - Phenomenology · Physics 2025-10-29 Mattia Di Mauro , Yanhan Wang

We show that the thermal relic abundance of dark matter can be affected by a new type of reaction: semi-annihilation. Semi-annihilation takes the schematic form X_i X_j -> X_k phi, where X_i are stable dark matter particles and phi is an…

High Energy Physics - Phenomenology · Physics 2015-03-13 Francesco D'Eramo , Jesse Thaler

In this work we study the annihilation of fermionic dark matter, considering it as a neutral particle with non-vanishing magnetic ($M$) and electric ($D$) dipole moments. Effective cross section of the process $\chi \overline{\chi}…

High Energy Physics - Phenomenology · Physics 2023-04-14 C. Arellano-Celiz , A. Avilez-López , J. E. Barradas-Guevara , A. Carrillo-Monteverde , J. L. Díaz-Cruz , O. Félix-Beltrán

In this work, we consider an extension of the Standard Model (SM) with an inert Higgs doublet and a real scalar singlet, in order to address problems around the origin of dark matter (DM). In this model, the lightest among the CP-odd and…

High Energy Physics - Phenomenology · Physics 2022-11-17 Mohammed Omer Khojali , Ammar Abdalgabar , Amine Ahriche , Alan S. Cornell

Recent anomalies in cosmic rays could be due to dark matter annihilation in our galaxy. In order to get the required large cross-section to explain the data while still obtaining the right relic density, we rely on a non standard thermal…

High Energy Physics - Phenomenology · Physics 2009-09-02 Bhaskar Dutta , Louis Leblond , Kuver Sinha

We consider an extension of the Standard Model of particle physics with an additional $SU(2)$ gauge sector along with an additional scalar bidoublet and a non-linear sigma field. The neutral components of the bidoublet serve as dark matter…

High Energy Physics - Phenomenology · Physics 2024-02-01 Baradhwaj Coleppa , Kousik Loho , Agnivo Sarkar

We present a dark sector model based on gauging the $L_\mu - L_\tau$ symmetry that addresses anomalies in $b \rightarrow s \mu^+ \mu^-$ decays and that features a particle dark matter candidate. The dark matter particle candidate is a…

High Energy Physics - Phenomenology · Physics 2017-03-14 Wolfgang Altmannshofer , Stefania Gori , Stefano Profumo , Farinaldo S. Queiroz

Recent breakthroughs in cosmology reveal that a quarter of the Universe is composed of dark matter, but the microscopic identity of dark matter remains a deep mystery. I review recent progress in resolving this puzzle, focusing on two…

Astrophysics · Physics 2009-11-13 Jonathan L. Feng

Recent cosmological measurements favour additional relativistic energy density beyond the one provided by the three active neutrinos and photons of the Standard Model (SM). This is often referred to as "dark radiation", suggesting the need…

High Energy Physics - Phenomenology · Physics 2015-06-12 M. C. Gonzalez-Garcia , V. Niro , Jordi Salvado

Unveiling the nature of cosmic dark matter (DM) is an urgent issue in cosmology. Here we make use of a strategy based on the search for the imprints left on the cosmic microwave background temperature and polarization spectra by the energy…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-11 Carmelo Evoli , Stefania Pandolfi , Andrea Ferrara
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