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Recent gamma-ray and radio observations provide stringent constraints for annihilating dark matter. The current $2\sigma$ lower limits of dark matter mass can be constrained to $\sim 100$ GeV for thermal relic annihilation cross section. In…

高能天体物理现象 · 物理学 2021-01-05 Man Ho Chan , Chak Man Lee

Direct detection experiments obtain 90% upper limits on the elastic scattering cross sections of dark matter with nucleons assuming point-like interactions and standard astrophysical and cosmological parameters. In this paper we provide a…

高能物理 - 唯象学 · 物理学 2021-05-27 Genevieve Belanger , Ali Mjallal , Alexander Pukhov

Dark matter (DM) charged under a dark U(1) force appears in many extensions of the Standard Model, and has been invoked to explain anomalies in cosmic-ray data, as well as a self-interacting DM candidate. In this paper, we perform a…

高能物理 - 唯象学 · 物理学 2017-05-23 Marco Cirelli , Paolo Panci , Kalliopi Petraki , Filippo Sala , Marco Taoso

We report first results from the Cryogenic Dark Matter Search (CDMS II) experiment running with its full complement of 30 cryogenic particle detectors at the Soudan Underground Laboratory. This report is based on the analysis of data…

天体物理学 · 物理学 2012-08-27 CDMS Collaboration

Recent results from the CoGeNT collaboration (as well as the annual modulation reported by DAMA/LIBRA) point toward dark matter with a light (5-10 GeV) mass and a relatively large elastic scattering cross section with nucleons (\sigma ~…

高能物理 - 唯象学 · 物理学 2011-08-09 Matthew R. Buckley , Dan Hooper , Tim M. P. Tait

Traditional direct detection experiments lack the sensitivity to probe the sub-GeV dark matter (DM), primarily due to the low energy of the expected nuclear recoils. In this work, we investigate cosmic-ray (CR) upscattering as a mechanism…

高能天体物理现象 · 物理学 2025-12-30 Yang Yu , Guan-Sen Wang , Bo Zhang , Tian-Peng Tang , Bing-Yu Su , Lei Feng

Dark matter particles with Planck-scale mass ($\simeq10^{19}\text{GeV}/c^2$) arise in well-motivated theories and could be produced by several cosmological mechanisms. Using a blind analysis of data collected over a 813 d live time with…

Given the recent progress in dark matter direction detection experiments, we examine a light bino-higgsino dark matter (DM) scenario ($M_1<100$ GeV and $\mu<300$ GeV) in natural supersymmetry with the electroweak fine tuning measure…

高能物理 - 唯象学 · 物理学 2018-01-17 Murat Abdughani , Lei Wu , Jin Min Yang

We suggest a minimal model for GeV-scale Majorana Dark Matter (DM) coupled to the standard model lepton sector via a charged scalar singlet. We show that there is an anti-correlation between the spin-independent DM-Nucleus scattering…

高能物理 - 唯象学 · 物理学 2021-04-21 Adil Jueid , Salah Nasri , Rachik Soualah

We propose that dark matter is dominantly comprised of atomic bound states. We build a simple model and map the parameter space that results in the early universe formation of hydrogen-like dark atoms. We find that atomic dark matter has…

高能物理 - 唯象学 · 物理学 2015-05-14 David E. Kaplan , Gordan Z. Krnjaic , Keith R. Rehermann , Christopher M. Wells

A search for evidence of particle dark matter (DM) and unparticle production at the LHC has been performed using events containing two charged leptons, consistent with the decay of a Z boson, and large missing transverse momentum. This…

高能物理 - 实验 · 物理学 2016-04-14 CMS Collaboration

We present constraints on decaying and annihilating dark matter (DM) in the 4 keV to 10 GeV mass range, using published results from the satellites HEAO-1, INTEGRAL, COMPTEL, EGRET, and the Fermi Gamma-ray Space Telescope. We derive…

高能物理 - 唯象学 · 物理学 2015-06-17 Rouven Essig , Eric Kuflik , Samuel D. McDermott , Tomer Volansky , Kathryn M. Zurek

Traditional dark matter models, eg. WIMPs, assume dark matter is weakly coupled to the standard model so that elastic scattering between dark matter and baryons can be described perturbatively by Born approximation. Most direct detection…

高能物理 - 唯象学 · 物理学 2021-12-03 Xingchen Xu , Glennys R. Farrar

The era of precision cosmology has revealed that about 85% of the matter in the universe is dark matter. Two well-motivated candidates are weakly interacting massive particles (WIMPs) and weakly interacting sub-eV particles (WISPs) (e.g.…

The mass of the dark matter particle is unknown, and may be as low as ~$10^{-22}$ eV. The lighter part of this range, below ~eV, is relatively unexplored both theoretically and experimentally but contains an array of natural dark matter…

高能物理 - 唯象学 · 物理学 2016-04-27 Peter W. Graham , David E. Kaplan , Jeremy Mardon , Surjeet Rajendran , William A. Terrano

Isospin-violating dark matter (IVDM), which couples differently with protons and neutrons, provides a promising mechanism to ameliorate the tension among recent direct detection experiments. Assuming DM is non-interacting bosonic asymmetric…

核理论 · 物理学 2015-03-26 Hao Zheng , Kai-Jia Sun , Lie-Wen Chen

Using low redshift data on astrophysical reionization, we report new Lyman-$\alpha$ limit on axion-like particle (ALP) as cold dark matter in ALP mass range of $m_{a}\sim 30-1000$ eV. Compared to the Leo T and soft-X ray bound, this limit…

高能物理 - 唯象学 · 物理学 2025-03-11 Zixuan Xu , Sibo Zheng

Recent observations by the CoGeNT collaboration (as well as long standing observations by DAMA/LIBRA) suggest the presence of a $\sim 5$-10 GeV dark matter particle with a somewhat large elastic scattering cross section with nucleons…

高能物理 - 唯象学 · 物理学 2011-10-13 Alexander V. Belikov , John F. Gunion , Dan Hooper , Tim M. P. Tait