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相关论文: Direct Detection with Dark Mediators

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We explore the singlet scalar dark matter (DM) from direct detections and high energy neutrino signals generated by the solar DM annihilation. Two singlet scalar DM models are discussed, one is the real singlet scalar DM model as the simple…

高能物理 - 唯象学 · 物理学 2015-05-27 Wan-Lei Guo , Yue-Liang Wu

Assuming for Weakly Interacting Massive Particles (WIMPs) a Maxwellian velocity distribution in the Galaxy we explore in a systematic way the relative sensitivity of an extensive set of existing and projected Dark Matter (DM) direct…

高能物理 - 唯象学 · 物理学 2019-03-01 Sunghyun Kang , Stefano Scopel , Gaurav Tomar , Jong-Hyun Yoon

Light dark matter (DM) in the GeV ballpark faces weaker constraint from direct detection experiments. If such DM also has sufficient self-interactions due to a light mediator, it can alleviate the small-scale problems of the cold dark…

高能物理 - 唯象学 · 物理学 2023-10-23 Debasish Borah , Satyabrata Mahapatra , Narendra Sahu

We investigate whether nearby white dwarfs (WDs) can constrain dark matter (DM) interactions with ordinary matter. As experimental sensitivity improves, driven by the Gaia mission, the sample volume of nearby WDs has been increasing over…

高能物理 - 唯象学 · 物理学 2025-10-28 Pooja Bhattacharjee , Sandra Robles , Stephan A. Meighen-Berger , Francesca Calore

We recap the main features of Minimal Dark Matter (MDM) and assess its status in the light of the recent experimental data. The theory selects an electroweak 5-plet with hypercharge Y=0 as a fully successful DM candidate, automatically…

高能物理 - 唯象学 · 物理学 2014-11-18 Marco Cirelli , Alessandro Strumia

Dark matter and neutrinos provide the two most compelling pieces of evidence for new physics beyond the Standard Model of Particle Physics but they are often treated as two different sectors. In this paper, we consider how neutrino…

高能物理 - 唯象学 · 物理学 2018-05-28 Andres Olivares-Del Campo , Sergio Palomares-Ruiz , Silvia Pascoli

We introduce a Minimal Simplified Dark Matter (MSDM) framework to quantitatively characterise dark matter (DM) searches at the LHC. We study two MSDM models where the DM is a Dirac fermion which interacts with a vector and axial-vector…

高能物理 - 唯象学 · 物理学 2015-01-19 Oliver Buchmueller , Matthew J. Dolan , Sarah A. Malik , Christopher McCabe

Paleo-detectors are a recently proposed method for the direct detection of Dark Matter (DM). In such detectors, one would search for the persistent damage features left by DM--nucleus interactions in ancient minerals. Initial sensitivity…

Direct detection dark matter experiments, lead by the CDMS collaboration, have placed increasingly stronger constraints on the cross sections for elastic scattering of WIMPs on nucleons. These results impact the prospects for the indirect…

高能物理 - 唯象学 · 物理学 2016-09-06 Francis Halzen , Dan Hooper

In this study, we propose an investigation into dark photon dark matter (DPDM) within the infrared frequency band, utilizing highly sensitive infrared light detectors commonly integrated into space telescopes, such as the James Webb Space…

高能物理 - 唯象学 · 物理学 2026-02-11 Haipeng An , Shuailiang Ge , Jia Liu , Zhiyao Lu

In the cosmological paradigm, cold dark matter (DM) dominates the mass content of the Universe and is present at every scale. Candidates for DM include many extensions of the Standard Model with weakly interacting massive particles (WIMPs)…

高能天体物理现象 · 物理学 2017-08-25 Benjamin Zitzer , VERITAS Collaboration

We propose a dark matter direct-detection strategy using charged particle decays at accelerator-based experiments. If ultralight $(m_\phi \ll \text{eV})$ dark matter has a misalignment abundance, its local field oscillates in time at a…

高能物理 - 唯象学 · 物理学 2025-05-23 Innes Bigaran , Patrick J. Fox , Yann Gouttenoire , Roni Harnik , Gordan Krnjaic , Tony Menzo , Jure Zupan

Direct searches for Dark Matter (DM) are continuously improving, probing down to lower and lower DM-nucleon interaction cross sections. For strongly-interacting massive particle (SIMP) Dark Matter, however, the accessible cross section is…

高能物理 - 唯象学 · 物理学 2018-07-03 Bradley J. Kavanagh

In this work, we make a detailed discussion on the phenomenology of the scotogenic Dirac model, which could accommodate the Dirac neutrino mass and dark matter. We have studied the LFV processes in this model, which are mediated by the…

高能物理 - 唯象学 · 物理学 2020-12-11 Shu-Yuan Guo , Zhi-Long Han

Indirect searches for dark matter (DM) have conventionally been applied to the products of DM annihilation or decay. If DM couples to light force carriers, however, it can be captured into bound states via dissipation of energy that may…

高能物理 - 唯象学 · 物理学 2020-11-11 Iason Baldes , Francesca Calore , Kalliopi Petraki , Vincent Poireau , Nicholas L. Rodd

We study the possibility of identifying dark matter properties from direct (XENON100) and indirect (GLAST) detection experiments. In the same way, we examine the perspectives given by the next generation of colliders (ILC). All this…

高能物理 - 唯象学 · 物理学 2008-05-16 Nicolas Bernal

This White Paper is an input to the ongoing discussion about the extension and refinement of simplified Dark Matter (DM) models. Based on two concrete examples, we show how existing simplified DM models (SDMM) can be extended to provide a…

Among the different strategies aiming to detect WIMP dark matter (DM), a neutrino signal coming from the Sun would be a smoking gun. This possibility relies on the DM capture by the Sun driven by the local DM distribution assumptions: the…

星系天体物理 · 物理学 2019-12-18 A. Nuñez-Castiñeyra , E. Nezri , V. Bertin

Directional detection of Dark Matter allows for unambiguous direct detection of WIMPs as well as discrimination between various Dark Matter models in our galaxy. The DMTPC detector is a low-pressure TPC with optical readout designed for…

The next generation of dark matter (DM) direct detection experiments and neutrino telescopes will probe large swaths of dark matter parameter space. In order to interpret the signals in these experiments, it is necessary to have good models…

高能天体物理现象 · 物理学 2009-07-30 Annika H. G. Peter
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