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相关论文: Split fermionic WIMPs evade direct detection

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Light fermionic/scalar dark matter (DM) (m_DM ~ 8 GeV) neutral under the standard model can be responsible for the CDMS and CoGeNT signals, and the Fermi-LAT gamma-ray excesses. In order to explain them in a relatively simple framework, we…

高能物理 - 唯象学 · 物理学 2015-06-17 Bumseok Kyae , Jong-Chul Park

As astronomical observations and their interpretation improve, the case for cold dark matter (CDM) becomes increasingly persuasive. A particularly appealing version of CDM is a weakly interacting massive particle (WIMP) with a mass near the…

高能物理 - 唯象学 · 物理学 2022-10-28 Bailey Tallman , Alexandra Boone , Adhithya Vijayakumar , Fiona Lopez , Samuel Apata , Jehu Martinez , Roland Allen

The 'WIMP miracle' for the relic abundance of thermal dark matter motivates weak scale dark matter with renormalizable couplings to standard model particles. We study minimal models with such couplings that explain dark matter as a thermal…

高能物理 - 唯象学 · 物理学 2014-01-22 Spencer Chang , Ralph Edezhath , Jeffrey Hutchinson , Markus Luty

The WIMP-nucleon scattering cross section in a simple dark matter model and its constraints from the latest direct detection experiment are treated here at the loop level. We consider a scenario with an emerging vector dark matter field…

高能物理 - 唯象学 · 物理学 2020-11-23 Juan Yepes

In this article, we focus on a new scalar $\phi$ mediated scalar/vectorial WIMPs (weakly interacting massive particles) with $\phi$'s mass slightly below the WIMP mass. To explain the Galactic center 1 - 3 GeV gamma-ray excess, here we…

高能物理 - 唯象学 · 物理学 2016-12-07 Lian-Bao Jia

A recently proposed dark matter WIMP has only second-order couplings to gauge bosons and itself. As a result, it has small annihilation, scattering, and creation cross-sections, and is consequently consistent with all current experiments…

The leptophilic weakly interacting massive particle (WIMP) is realized in a minimal renormalizable model scenario where scalar mediators with lepton number establish the WIMP interaction with the standard model (SM) leptons. We perform a…

高能物理 - 唯象学 · 物理学 2021-09-08 Shun-ichi Horigome , Taisuke Katayose , Shigeki Matsumoto , Ipsita Saha

Effective WIMP models are minimal extensions of the standard model that explain the relic density of dark matter by the ``WIMP miracle.'' In this paper we consider the phenomenology of effective WIMPs with trilinear couplings to leptons and…

高能物理 - 唯象学 · 物理学 2014-07-16 Spencer Chang , Ralph Edezhath , Jeffrey Hutchinson , Markus Luty

Weakly Interacting Massive Particles (WIMPs) are among the main candidates for the relic dark matter (DM). The idea of the direct DM detection relies on elastic spin-dependent (SD) and spin-independent (SI) interaction of WIMPs with target…

高能物理 - 唯象学 · 物理学 2009-10-20 V. A. Bednyakov , H. V. Klapdor-Kleingrothaus

There is evidence for a spectral line at $E_\gamma\approx 130$ GeV in the Fermi-LAT data that can be explained as dark mater particles annihilating into photons. We review a well known dark matter model that consists in a singlet Dirac…

高能物理 - 唯象学 · 物理学 2014-10-13 T. H. Franarin , C. A. Z. Vasconcellos , D. Hadjimichef

The search for weakly-interacting massive particle (WIMP) dark matter is multi-pronged. Ultimately, the WIMP-dark-matter picture will only be confirmed if different classes of experiments see consistent signals and infer the same WIMP…

宇宙学与河外天体物理 · 物理学 2013-10-29 Annika H. G. Peter , Vera Gluscevic , Anne M. Green , Bradley J. Kavanagh , Samuel K. Lee

Weakly interacting massive particles (WIMPs) can self-annihilate, thus providing us with a way to indirectly detect dark matter (DM). Dwarf spheroidal (dSph) galaxies are excellent places to search for annihilation signals because they are…

宇宙学与河外天体物理 · 物理学 2023-06-09 L. Gajović , F. Welzmüller , V. Heesen , F. de Gasperin , M. Vollmann , M. Brüggen , A. Basu , R. Beck , D. J. Schwarz , D. J. Bomans , A. Drabent

The singlet scalar model is a minimal extension of the Standard Model that can explain the dark matter. We point out that in this model the dark matter constraint can be satisfied not only in the already considered WIMP regime but also, for…

高能物理 - 唯象学 · 物理学 2011-09-08 Carlos E. Yaguna

We examine the possibility that the dark matter (DM) interpretation of the GeV scale Fermi gamma-ray excess at the Galactic Center can be realized in a specific framework - secluded singlet fermionic dark matter model with small mixing…

高能物理 - 唯象学 · 物理学 2016-06-29 Yeong Gyun Kim , Kang Young Lee , Chan Beom Park , Seodong Shin

We systematically explore the phenomenology of the recently proposed extended dark matter effective field theory (\eDMEFT), which allows for a consistent effective description of DM scenarios across different energy scales. The framework…

高能物理 - 唯象学 · 物理学 2020-12-02 Tommi Alanne , Giorgio Arcadi , Florian Goertz , Valentin Tenorth , Stefan Vogl

In this work, we study multicomponent dark sectors comprised of a fermionic and a scalar dark matter candidate. In the scalar sector, we mostly focus on the Inert Doublet Model while in the fermionic sector we study three different models.…

高能物理 - 唯象学 · 物理学 2020-12-18 Amalia Betancur , Guillermo Palacio , Andrés Rivera

We consider a simple extension of the Standard Model with a scalar top-philic Dark Matter (DM) $S$ coupling, apart from the Higgs portal, exclusively to the right-handed top quark $t_R$ and a colored vector-like top partner $T$ with a…

高能物理 - 唯象学 · 物理学 2016-11-23 Seungwon Baek , Pyungwon Ko , Peiwen Wu

We consider the doublet-triplet fermionic model in the scheme of the custodial limit when the dark matter (DM) candidate is pure doublet and lies at the electroweak scale. This scheme, despite being an appealing and promising DM model, is…

高能物理 - 唯象学 · 物理学 2018-11-12 Amalia Betancur , Óscar Zapata

We study a minimal model with an imposed $\mathbb{Z}_2$ symmetry incorporating two singlet fermions and a singlet scalar which communicate with the SM particles through a scalar-Higgs portal. We probe regions in the parameter space where…

高能物理 - 唯象学 · 物理学 2026-04-10 Karim Ghorbani

We promote the idea of multi-component Dark Matter (DM) to explain results from both direct and indirect detection experiments. In these models as contribution of each DM candidate to relic abundance is summed up to meet WMAP/Planck…

高能物理 - 唯象学 · 物理学 2015-06-18 Kamakshya Prasad Modak , Debasish Majumdar , Subhendu Rakshit