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相关论文: DirectDM: a tool for dark matter direct detection

200 篇论文

In this work we study the constraints on the dark matter interaction with the standard model particles, from the observations of dark matter relic density, the direct detection experiments of CDMS and XENON, and the indirect detection of…

高能物理 - 唯象学 · 物理学 2011-10-07 Jia-Ming Zheng , Zhao-Huan Yu , Jun-Wen Shao , Xiao-Jun Bi , Zhibing Li , Hong-Hao Zhang

We present comparisons of direct dark matter (DM) detection data for light WIMPs with exothermic scattering with nuclei (exoDM), both assuming the Standard Halo Model (SHM) and in a halo model - independent manner. Exothermic interactions…

高能物理 - 唯象学 · 物理学 2015-06-19 Graciela B. Gelmini , Andreea Georgescu , Ji-Haeng Huh

We study the case of multi-component dark matter, in particular how direct detection signals are modified in the presence of several stable weakly-interacting-massive particles. Assuming a positive signal in a future direct detection…

高能物理 - 唯象学 · 物理学 2017-11-29 Juan Herrero-Garcia , Andre Scaffidi , Martin White , Anthony G. Williams

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

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

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…

We study the global dynamics of the universe within the framework of the Interacting Dark Matter (IDM) scenario. Assuming that the dark matter obeys the collisional Boltzmann equation, we can derive analytical solutions of the global…

天体物理学 · 物理学 2015-05-13 S. Basilakos , M. Plionis

Massive vector particles are minimal dark matter candidates that motivate a wide range of laboratory searches, primarily exploiting a postulated kinetic mixing with the photon. However, depending on the high energy field content, the…

高能物理 - 唯象学 · 物理学 2023-08-16 Gordan Krnjaic , Tanner Trickle

A non-relativistic effective field theory (NREFT) offers a bottom-up framework to classify Dark Matter (DM)-nucleon interactions relevant for scattering at direct detection experiments by organizing the interactions in powers of the…

高能物理 - 唯象学 · 物理学 2019-11-21 Manuel Drees , Rahul Mehra

The direct detection rate for supersymmetric cold dark matter (CDM) particles is calculated for a number of suitable nuclear targets. Both the coherent and spin contributions are considered. By considering representative phenomenologically…

高能物理 - 唯象学 · 物理学 2014-11-17 J. D. Vergados , T. S. Kosmas

In this paper, we investigate the possibility of testing the weakly interacting massive particle (WIMP) dark matter (DM) models by applying the simplest phenomenological model which introduces an interaction term between dark energy (DE)…

宇宙学与河外天体物理 · 物理学 2021-09-15 Wei Cheng , Yuan He , Jin-Wang Diao , Yu Pan , Jun Zeng , Jia-Wei Zhang

The only coupling dark matter is guaranteed to have with the standard model is through gravity. Here we propose a concept for direct dark matter detection using only this gravitational coupling. We suggest that an array of quantum-limited…

高能物理 - 唯象学 · 物理学 2021-08-25 Daniel Carney , Sohitri Ghosh , Gordan Krnjaic , Jacob M. Taylor

Conventional approaches to describe dark matter phenomenology at collider and (in)direct detection experiments in the form of dark matter effective field theory or simplified models suffer in general from drawbacks regarding validity at…

高能物理 - 唯象学 · 物理学 2018-03-23 Tommi Alanne , Florian Goertz

So far all evidences of dark matter (DM) come from astrophysical and cosmological observations, due to gravitational interactions of the DM. It is possible that the true DM particle in the universe joins gravitational interactions only, but…

高能物理 - 唯象学 · 物理学 2015-03-30 Jing Ren , Hong-Jian He

Identifying the nature of dark matter (DM) has long been a pressing question for particle physics. In the face of ever-more-powerful exclusions and null results from large-exposure searches for TeV-scale DM interacting with nuclei, a…

高能物理 - 唯象学 · 物理学 2022-05-31 Yonatan Kahn , Tongyan Lin

The search for sub-GeV dark matter (DM) particles via electronic transitions in underground detectors attracted much theoretical and experimental interest in the past few years. A still open question in this field is whether experimental…

高能物理 - 唯象学 · 物理学 2023-04-05 Riccardo Catena , Daniel Cole , Timon Emken , Marek Matas , Nicola Spaldin , Walter Tarantino , Einar Urdshals

We present the projected sensitivity to non-relativistic Effective Field Theory (EFT) operators for Dark Matter (DM) direct detection using the QUEST-DMC experiment. QUEST-DMC employs superfluid Helium-3 as a target medium and measures…

We apply effective field theory methods to compute bino-nucleon scattering, in the case where tree-level interactions are suppressed and the leading contribution is at loop order via heavy flavor squarks or sleptons. We find that leading…

高能物理 - 唯象学 · 物理学 2016-05-31 Asher Berlin , Denis S. Robertson , Mikhail P. Solon , Kathryn M. Zurek

Direct detection of dark matter with directional sensitivity is a promising concept for improving the search for weakly interacting massive particles. With information on the direction of WIMP induced nuclear recoils one has access to the…

高能物理 - 唯象学 · 物理学 2015-10-15 Ciaran A. J. O'Hare

The WIMP proposed here yields the observed abundance of dark matter, and is consistent with the current limits from direct detection, indirect detection, and collider experiments, if its mass is $\sim 72$ GeV/$c^2$. It is also consistent…