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Using the neutral gauginos of SU(2)L* U(1)Y and hybridization ideas below the GUT scale, we approach the Dark Matter particle within the Minimal Supersymmetric Standard Model. In the energy range MGUT-MZ where supergravity effects can be…

High Energy Physics - Phenomenology · Physics 2014-06-12 S-E. Ennadifi , E. H. Saidi

Recently, several astrophysical data or would-be signals has been observed in different dark-matter oriented experiments. In each case, one could fit the data at the price of specific nature of the coupling between the Standard Model (SM)…

High Energy Physics - Phenomenology · Physics 2015-05-28 Yann Mambrini , Bryan Zaldívar

The nature of the cosmic dark matter is unknown. The most compelling hypothesis is that dark matter consists of weakly interacting massive particles (WIMPs) in the 100 GeV mass range. Such particles would annihilate in the galactic halo,…

Astrophysics · Physics 2009-11-11 Edward A. Baltz , James E. Taylor , Lawrence L. Wai

We show that colliders can impose strong constraints on models of dark matter, in particular when the dark matter is light. We analyze models where the dark matter is a fermion or scalar interacting with quarks and/or gluons through an…

High Energy Physics - Phenomenology · Physics 2011-04-05 Jessica Goodman , Masahiro Ibe , Arvind Rajaraman , William Shepherd , Tim M. P. Tait , Hai-Bo Yu

It is well known that for the pure standard model triplet fermionic WIMP-type dark matter (DM), the relic density is satisfied around 2 TeV. For such a heavy mass particle, the production cross-section at 13 TeV run of LHC will be very…

High Energy Physics - Phenomenology · Physics 2018-04-24 Sandhya Choubey , Sarif Khan , Manimala Mitra , Subhadeep Mondal

The Weakly Interacting Massive Particles(WIMPs) have long been the favored CDM candidate in the standard $\Lambda$CDM model. However, owing to great improvement in the experimental sensitivity in the past decade, some parameter space of the…

Cosmology and Nongalactic Astrophysics · Physics 2023-11-15 Abineet Parichha , Shiv Sethi

The prospects for detecting a candidate supersymmetric dark matter particle at the LHC are reviewed, and compared with the prospects for direct and indirect searches for astrophysical dark matter, on the basis of a frequentist analysis of…

High Energy Physics - Phenomenology · Physics 2010-11-02 John Ellis

In the left-right twin Higgs (LRTH) model, the neutral $\hat{S}$ is a candidate for weakly interacting massive particle (WIMP) dark matter (DM). If its mass is lighter than half of the SM-like Higgs boson $h$, the new invisible decay $h \to…

High Energy Physics - Phenomenology · Physics 2015-03-23 Yao-Bei Liu , Zhen-Jun Xiao

This article gives an overview on the status of experimental searches for dark matter at the end of 2014. The main focus is on direct searches for weakly interacting massive particles (WIMPs) using underground-based low-background…

Cosmology and Nongalactic Astrophysics · Physics 2015-07-29 Marc Schumann

We consider the lightest supersymmetric particle (LSP), neutralino in minimal anomaly mediated supersymmetry breaking model (mAMSB) to be a possible candidate for weakly interacting massive particles (WIMP) or cold dark matter and…

High Energy Physics - Phenomenology · Physics 2013-06-28 Kamakshya Prasad Modak , Debasish Majumdar

The details of what constitutes the majority of the mass that makes up dark matter in the Universe remains one of the prime puzzles of cosmology and particle physics today - eighty years after the first observational indications. Today, it…

High Energy Astrophysical Phenomena · Physics 2015-12-16 Stefan Funk

Cold dark matter may be made of superweakly-interacting massive particles, superWIMPs, that naturally inherit the desired relic density from late decays of metastable WIMPs. Well-motivated examples are weak-scale gravitinos in supergravity…

High Energy Physics - Phenomenology · Physics 2008-11-26 Jonathan L. Feng , Arvind Rajaraman , Fumihiro Takayama

We consider a simplified model for Majorana fermion dark matter and explore constraints from direct, indirect and LHC collider searches. The dark matter is assumed to couple to the Standard Model through a vector mediator with axial-vector…

High Energy Physics - Phenomenology · Physics 2016-03-29 Jan Heisig , Michael Krämer , Mathieu Pellen , Christopher Wiebusch

We study the top quark portal dominated dark matter interactions, and its implications for the gamma ray line searches. In this picture, the dark matter interactions with photons and gluons are loop induced by the axial anomaly of the top…

High Energy Physics - Phenomenology · Physics 2015-06-12 Yue Zhang

We explore the relationship between astrophysical gamma-ray signals and LHC signatures for a class of phenomenologically successful secluded dark matter models, motivated by recent evidence for a ~130 GeV gamma-ray line. We consider in…

High Energy Physics - Phenomenology · Physics 2013-08-20 Joachim Kopp , Ethan T. Neil , Reinard Primulando , Jure Zupan

The recent WMAP data provide a rather restricted range of the Cold Dark Matter (CDM) density $ \Omega_{CDM} h^2 $ of unprecedented accuracy. We combine these new data along with data from BNL E821 experiment measuring $ {(g_{\mu}-2)}$, $…

High Energy Physics - Phenomenology · Physics 2008-11-26 A. B. Lahanas , D. V. Nanopoulos

A gluphilic scalar dark matter (GSDM) model has recently been proposed as an interesting vision for WIMP dark matter communicating dominantly with the Standard Model via gluons. We discuss the collider signature of a hard jet recoiling…

High Energy Physics - Phenomenology · Physics 2017-07-05 Rohini M. Godbole , Gaurav Mendiratta , Ambresh Shivaji , Tim M. P. Tait

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

The DArk Matter Particle Explorer (DAMPE) recently reported an excess of electrons/positrons above expected background fluxes even when a double power-law background spectrum is assumed. Several dark matter models that involve TeV-scale…

High Energy Astrophysical Phenomena · Physics 2019-05-03 Geoff Beck , Sergio Colafrancesco

The perturbative unitarity bound is studied in the monojet process at LHC. The production of the dark matter is described by the low-energy effective theory. The analysis of the dark matter signal is not validated, if the unitarity…

High Energy Physics - Phenomenology · Physics 2014-06-24 Motoi Endo , Yasuhiro Yamamoto