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Dark matter in the form of particles from a hidden mirror sector has recently been proposed as an explanation for the DAMA annual modulation signal. Here one assumes that there exists a small mixing between photons and mirror photons. We…

天体物理学 · 物理学 2007-05-23 Saibal Mitra

The scattering of light dark matter off thermal electrons inside the Sun produces a "fast" sub-component of the dark matter flux that may be detectable in underground experiments. We update and extend previous work by analyzing the…

高能物理 - 唯象学 · 物理学 2023-09-27 Haipeng An , Haoming Nie , Maxim Pospelov , Josef Pradler , Adam Ritz

Particle dark matter could have a mass anywhere from that of ultralight candidates, $m_\chi\sim 10^{-21}\,$eV, to scales well above the GeV. Conventional laboratory searches are sensitive to a range of masses close to the weak scale, while…

高能物理 - 唯象学 · 物理学 2019-09-13 Rodrigo Alonso , Diego Blas , Peter Wolf

Dark photons can be the ultralight dark matter candidate, interacting with Standard Model particles via kinetic mixing. We propose to search for ultralight dark photon dark matter (DPDM) through the local absorption at different radio…

高能物理 - 唯象学 · 物理学 2023-05-12 Haipeng An , Shuailiang Ge , Wen-Qing Guo , Xiaoyuan Huang , Jia Liu , Zhiyao Lu

Atmospheric collisions can copiously produce dark sector particles in the invisible dark photon model, leading to detectable signals in underground neutrino detectors. We consider the dark photon model with the mass mixing mechanism and use…

高能物理 - 唯象学 · 物理学 2025-09-11 Mingxuan Du , Rundong Fang , Zuowei Liu , Wenxi Lu , Zicheng Ye

We investigate the direct detection phenomenology of a class of dark matter (DM) models in which DM does not directly interact with nuclei, {but rather} the products of its annihilation do. When these annihilation products are very light…

高能物理 - 唯象学 · 物理学 2015-06-17 John F. Cherry , Mads T. Frandsen , Ian M. Shoemaker

It has been proposed that an additional U(1) sector of hidden photons could account for the Dark Matter observed in the Universe. When passing through an interface of materials with different dielectric properties, hidden photons can give…

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…

高能物理 - 唯象学 · 物理学 2008-11-26 Aaron Pierce

The physics of the solar dark matter (DM) that are captured and thermalise through the DM-nucleon interaction has been extensively studied. In this work, we consider the leptophilic DM scenario where the DM particles interact exclusively…

高能物理 - 唯象学 · 物理学 2018-10-31 Zheng-Liang Liang , Yi-Lei Tang , Zi-Qing Yang

Dark matter that gets captured in the Sun may form positronium-like bound states if it self-interacts via light dark photons. In this case, dark matter can either annihilate to dark photons or recombine in bound states which subsequently…

高能物理 - 唯象学 · 物理学 2016-10-19 Chris Kouvaris , Kasper Langaeble , Niklas Grønlund Nielsen

The existence of Dark Matter (DM) is a well established fact since many decades, thanks to the observation of the effects of its gravitational interaction with the ordinary matter in the Universe. However, our knowledge of the Dark Matter…

高能物理 - 唯象学 · 物理学 2020-09-08 Alessandra Filippi , Marzio De Napoli

Light new particles with masses below 10 keV, often considered as a plausible extension of the Standard Model, will be emitted from the solar interior, and can be detected on the Earth with a variety of experimental tools. Here we analyze…

高能物理 - 唯象学 · 物理学 2013-08-21 Haipeng An , Maxim Pospelov , Josef Pradler

At a level too faint for astronomy, particle dark matter may interact with Standard Model states via the photon. We derive limits from direct detection experiments on photon-mediated nuclear interactions up to operator dimension-6, viz.,…

高能物理 - 唯象学 · 物理学 2025-09-30 Jason Kumar , Biprajit Mondal , Girish Muralidhara , Nirmal Raj

We examine the possibility that dark matter may be the manifestation of dark forces of a hidden sector, i.e. "Dark Force = Dark Matter." As an illustrative and minimal example we consider the hidden SU(2)_h x U(1)_h gauge group. The hidden…

高能物理 - 唯象学 · 物理学 2014-04-02 Hooman Davoudiasl , Ian M. Lewis

The 79-string IceCube search for dark matter in the Sun public data is used to test Secluded Dark Matter models. No significant excess over background is observed and constraints on the parameters of the models are derived. Moreover, the…

高能天体物理现象 · 物理学 2018-05-07 M. Ardid , I. Felis , A. Herrero , J. A. Martínez-Mora

In supersymmetric unified theories the dark matter particle can decay, just like the proton, through grand unified interactions with a lifetime of order of 10^{26} sec. Its decay products can be detected by several experiments -- including…

高能物理 - 唯象学 · 物理学 2009-09-24 Asimina Arvanitaki , Savas Dimopoulos , Sergei Dubovsky , Peter W. Graham , Roni Harnik , Surjeet Rajendran

We study novel scenarios where thermal dark matter (DM) can be efficiently captured in the Sun and annihilate into boosted dark matter. In models with semi-annihilating DM, where DM has a non-minimal stabilization symmetry, or in models…

高能物理 - 唯象学 · 物理学 2015-06-23 Joshua Berger , Yanou Cui , Yue Zhao

We review the prospects for discovering supersymmetric dark matter in a recently proposed set of post-LEP supersymmetric benchmark scenarios. We consider direct detection through spin-independent nuclear scattering, as well as indirect…

高能物理 - 唯象学 · 物理学 2009-09-11 John Ellis , Jonathan L. Feng , Andrew Ferstl , Konstantin T. Matchev , Keith A. Olive

Dark matter pervades the Solar System, free-streaming at the halo's local Galactic orbital velocity and density. As these objects pass through the Solar system, they perturb gravitationally, and thus very weakly, all nearby inertial masses.…

天体物理学 · 物理学 2007-05-23 A. W. Adams , J. S. Bloom

The detection of non-baryonic dark matter through its gamma-ray annihilation in the centre of our galaxy has been studied. The gamma fluxes according to different models have been simulated and compared to those expected to be observed with…