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Dark sectors lying beyond the Standard Model and containing sub-GeV particles which are bilinearly coupled to nucleons would induce quantum forces of the Casimir-Polder type in ordinary matter. Such new forces can be tested by a variety of…

高能物理 - 唯象学 · 物理学 2018-06-27 Philippe Brax , Sylvain Fichet , Guillaume Pignol

Dark matter (DM) particles with mass in the sub-GeV range are an attractive alternative to heavier weakly-interacting massive particles, but direct detection of such light particles is challenging. If however DM-nucleus scattering leads to…

高能物理 - 唯象学 · 物理学 2018-09-12 Matthew J. Dolan , Felix Kahlhoefer , Christopher McCabe

All attempts to directly detect particle dark matter (DM) scattering on nuclei suffer from the partial or total loss of sensitivity for DM masses in the GeV range or below. We derive novel constraints from the inevitable existence of a…

高能物理 - 唯象学 · 物理学 2019-05-08 Torsten Bringmann , Maxim Pospelov

Traditional direct searches for dark matter, looking for nuclear recoils in deep underground detectors, are challenged by an almost complete loss of sensitivity for light dark matter particles. Consequently, there is a significant effort in…

We point out that power measurements of single quasiparticle devices open a new avenue to detect dark matter (DM). The threshold of these devices is set by the Cooper pair binding energy, and is therefore so low that they can detect DM as…

高能物理 - 唯象学 · 物理学 2024-03-26 Anirban Das , Noah Kurinsky , Rebecca K. Leane

Due to the low nuclear recoils, sub-GeV dark matter (DM) is usually beyond the sensitivity of the conventional DM direct detection experiments. The boosted and Migdal scattering mechanisms have been proposed as two new complementary avenues…

高能物理 - 唯象学 · 物理学 2023-02-28 Victor V. Flambaum , Liangliang Su , Lei Wu , Bin Zhu

We study the direct detection prospects for a representative set of simplified models of sub-GeV dark matter (DM), accounting for existing terrestrial, astrophysical and cosmological constraints. We focus on dark matter lighter than an MeV,…

高能物理 - 唯象学 · 物理学 2018-01-03 Simon Knapen , Tongyan Lin , Kathryn M. Zurek

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

Detection of sub-GeV dark matter (DM) particles in direct detection experiments is inherently difficult, as their low kinetic energies in the galactic halo are insufficient to produce observable recoils of the heavy nuclei in the detectors.…

高能物理 - 唯象学 · 物理学 2025-10-17 Richard Diurba , Helena Kolešová

Light Dark Matter (DM), defined here as having a mass between 1 MeV and about 1 GeV, is an interesting possibility both theoretically and phenomenologically, at one of the frontiers of current progress in the field of DM searches. Its…

高能物理 - 唯象学 · 物理学 2022-07-06 Marco Cirelli , Nicolao Fornengo , Bradley J. Kavanagh , Elena Pinetti

We use Super-K data to place new strong limits on interactions of sub-GeV Dark Matter (DM) with nuclei, that rely on the DM flux inevitably induced by cosmic-ray upscatterings. We derive analogous sensitivities at Hyper-K and DUNE and…

高能物理 - 唯象学 · 物理学 2021-03-24 Yohei Ema , Filippo Sala , Ryosuke Sato

We investigate the effect of new physics interacting with both Dark Matter (DM) and neutrinos at DM direct detection experiments. Working within a simplified model formalism, we consider vector and scalar mediators to determine the…

In the past few years, many mesoscale systems have been proposed as possible detectors of sub-GeV dark matter particles. In this work, we point out the feasibility of probing dark matter-nucleon scattering cross section using…

高能物理 - 唯象学 · 物理学 2023-11-15 Anirban Das , Noah Kurinsky , Rebecca K. Leane

The direct detection of sub-GeV dark matter interacting with nucleons is hampered by the low recoil energies induced by scatterings in the detectors. This experimental difficulty is avoided in the scenario of boosted dark matter where a…

高能物理 - 唯象学 · 物理学 2022-01-07 Roberta Calabrese , Marco Chianese , Damiano F. G. Fiorillo , Ninetta Saviano

We study the probing prospects of cosmic ray boosted dark matter (DM) in the framework of simplified electron-philic dark photon model. Focusing on the dark matter and dark photon masses around keV $\sim $ MeV scale, we consider the bounds…

高能物理 - 唯象学 · 物理学 2023-02-13 Jinmian Li , Junle Pei , Cong Zhang

We propose the nucleon consumption induced by dark matter (DM) as a new scenario to overcome the energy threshold of direct detection. It can be realized with proton ($\chi + p \rightarrow \chi + \ell^+$) or neutron ($\chi + n \rightarrow…

高能物理 - 唯象学 · 物理学 2024-12-20 Shao-Feng Ge , Xiao-Dong Ma

Sub-GeV Dark Matter particles upscattered by cosmic rays gain enough kinetic energy to pass the thresholds of large volume detectors on Earth. We then use public Super-Kamiokande and MiniBooNE data to derive a novel limit on the scattering…

高能物理 - 唯象学 · 物理学 2019-05-15 Yohei Ema , Filippo Sala , Ryosuke Sato

We study the effect of a long-range DM-nuclei interaction occurring via the exchange of a light mediator. We consider the main direct detection experiments: DAMA, CoGeNT, CRESST, CDMS and XENON100. We find that a long-range force is a…

高能物理 - 唯象学 · 物理学 2012-06-12 Paolo Panci

Scattering of sub-GeV dark matter (DM) particles with hydrogen atoms is studied in this paper. The interactions of DM with electrons and nucleons are both included and formulated in a general framework based on nonrelativistic effective…

高能物理 - 唯象学 · 物理学 2015-12-09 Jiunn-Wei Chen , Hsin-Chang Chi , C. -P. Liu , Chih-Liang Wu , Chih-Pan Wu

Dark Matter (DM) comprising particles in the mass range of a few MeV to GeV is waiting to be explored, given the many theoretical models accommodating cosmological abundance. We hereby propose an experiment with the LHC proton beam of 7 TeV…

高能物理 - 实验 · 物理学 2016-09-04 Ashok Kumar , Archana Sharma
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