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Direct detection experiments, which are designed to detect the scattering of dark matter off nuclei in detectors, are a critical component in the search for the Universe's missing matter. The count rate in these experiments should…

宇宙学与河外天体物理 · 物理学 2017-01-04 Katherine Freese , Mariangela Lisanti , Christopher Savage

Self-interacting dark matter offers an interesting alternative to collisionless dark matter because of its ability to preserve the large-scale success of the cold dark matter model, while seemingly solving its challenges on small scales. We…

宇宙学与河外天体物理 · 物理学 2015-06-12 Mark Vogelsberger , Jesus Zavala

A convincing identification of dark matter (DM) particles can probably be achieved only through a combined analysis of different detections strategies, which provides an effective way of removing degeneracies in the parameter space of DM…

高能天体物理现象 · 物理学 2014-11-21 Pasquale D. Serpico , Gianfranco Bertone

The measurement of an annual modulation in the event rate of direct dark matter detection experiments is a powerful tool for dark matter discovery. Indeed, several experiments have already claimed such a discovery in the past decade. While…

宇宙学与河外天体物理 · 物理学 2020-05-05 Francis Froborg , Alan R Duffy

Due to Earth's revolution around the Sun, the expected scattering rate in direct dark matter searches is annually modulated. This modulation is expected to differ between experiments when given as a function of recoil energy $E_\text{R}$,…

高能物理 - 唯象学 · 物理学 2015-06-24 Eugenio Del Nobile , Graciela B. Gelmini , Samuel J. Witte

Plasma dark matter, which arises in dissipative dark matter models, can give rise to large annual modulation signals from keV electron recoils. Previous work has argued that the DAMA annual modulation signal could have an explanation within…

高能物理 - 唯象学 · 物理学 2018-09-13 R. Foot

Earth's rotation about the Sun produces an annual modulation in the expected scattering rate at direct dark matter detection experiments. The annual modulation as a function of the recoil energy $E_\text{R}$ imparted by the dark matter…

高能物理 - 唯象学 · 物理学 2016-02-17 Eugenio Del Nobile , Graciela B. Gelmini , Samuel J. Witte

In 2020 the XENON1T experiment observed an excess of events with an electron recoil energy $E_R$ in the range of $2\,$--$\,3\,$keV. Such an excess can arise from a variety of sources such as solar axions or a neutrino magnetic moment, but…

高能物理 - 唯象学 · 物理学 2022-07-19 Amin Aboubrahim , Lutz Althueser , Michael Klasen , Pran Nath , Christian Weinheimer

The long-standing model-independent annual modulation effect measured by the DAMA Collaboration, which fulfills all the requirements of a dark matter annual modulation signature, and the new result by the CoGeNT experiment that shows a…

高能物理 - 唯象学 · 物理学 2012-01-04 P. Belli , R. Bernabei , A. Bottino , F. Cappella , R. Cerulli , N. Fornengo , S. Scopel

Various issues related to the direct detection of supersymmetric dark matter are reviewed. Such are: 1) Construction of supersymmetric models with a number of parameters, which are constrained from the data at low energies as well as…

高能物理 - 唯象学 · 物理学 2008-11-26 J. D. Vergados

One of the next frontiers in dark-matter direct-detection experiments is to explore the MeV to GeV mass regime. Such light dark matter does not carry enough kinetic energy to produce an observable nuclear recoil, but it can scatter off…

高能物理 - 唯象学 · 物理学 2017-09-11 Samuel K. Lee , Mariangela Lisanti , Siddharth Mishra-Sharma , Benjamin R. Safdi

We discuss the positive indications of a possible dark matter signal in direct detection experiments in terms of a mechanism of interaction between the dark matter particle and the nuclei occurring via the exchange of a light mediator,…

高能物理 - 唯象学 · 物理学 2013-05-29 N. Fornengo , P. Panci , M. Regis

The differential event rate for direct detection of dark matter, both the time averaged and the modulated one due to the motion of the Earth, are discussed. The calculations focus on relatively light cold dark matter candidates (WIMP) and…

高能物理 - 唯象学 · 物理学 2015-05-30 J. D. Vergados

The sensitivity to dark matter signals at neutrino experiments is fundamentally challenged by the neutrino rates, as they leave similar signatures in their detectors. As a way to improve the signal sensitivity, we investigate a dark matter…

高能物理 - 唯象学 · 物理学 2024-11-28 Bhaskar Dutta , Doojin Kim , Shu Liao , Jong-Chul Park , Seodong Shin , Louis E. Strigari , Adrian Thompson

The CoGeNT collaboration has recently made available new data collected over a period of 15 months. In addition to more accurately measuring the spectrum of nuclear recoil candidate events they have announced evidence for an annual…

高能物理 - 唯象学 · 物理学 2011-08-25 R. Foot

We investigate the diurnal modulation of the event rate for dark matter scattering on solid targets arising from the directionally dependent defect creation threshold energy. In particular, we quantify how this effect would help in…

Dark matter in spiral galaxies like the Milky Way may take the form of a dark plasma. Hidden sector dark matter charged under an unbroken $U(1)'$ gauge interaction provides a simple and well defined particle physics model realising this…

星系天体物理 · 物理学 2016-01-27 Jackson D. Clarke , Robert Foot

The CoGeNT collaboration has recently presented the results of their first 15 months of data, including the measurement of the spectrum of nuclear recoil candidate events, and the time variation of those events. These results appear…

高能物理 - 唯象学 · 物理学 2013-05-29 Dan Hooper , Chris Kelso

We study the possibility that dark radiation, sourced through the decay of dark matter in the late Universe, carries electromagnetic interactions. The relativistic flux of particles induces recoil signals in direct detection and neutrino…

高能物理 - 唯象学 · 物理学 2021-06-30 Jui-Lin Kuo , Maxim Pospelov , Josef Pradler

Models of nuclear dark matter propose that the dark sector contains large composite states consisting of dark nucleons in analogy to Standard Model nuclei. We examine the direct detection phenomenology of a particular class of nuclear dark…

高能物理 - 唯象学 · 物理学 2017-11-01 A. Butcher , R. Kirk , J. Monroe , S. M. West
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