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One of the most popular classes of candidates for dark matter are Weakly Interacting Massive Particles (WIMPs), i.e. particles possessing masses and couplings falling roughly within the electroweak scale. Apart from offering a natural…

高能物理 - 唯象学 · 物理学 2011-06-21 Andreas Goudelis

We investigate a possible dark matter origin of the high-energy nuclear-recoil-like events in XENONnT and LZ data, which cannot be explained by standard elastic spin-independent WIMP scattering. Using our unified DIAMX framework, built on…

高能物理 - 唯象学 · 物理学 2025-12-10 Haipeng An , Fei Gao , Jia Liu , Minghao Liu , Haoming Nie , Changlong Xu

A search for Weakly Interacting Massive Particles (WIMPs) was conducted with the single-phase liquid-xenon detector XMASS through inelastic scattering in which $^{129}$Xe nuclei were excited, using an exposure ($\rm 327\; kg \times 800.0 \;…

Self-interacting dark matter (SIDM) is a simple and well-motivated scenario that could explain long-standing puzzles in structure formation on small scales. If the required self-interaction arises through a light mediator (with mass $\sim…

高能物理 - 唯象学 · 物理学 2015-11-04 Eugenio Del Nobile , Manoj Kaplinghat , Hai-Bo Yu

An ever-increasing body of evidence suggests that weakly interacting massive particles (WIMPs) constitute the bulk of the matter in the Universe. Experimental data, dimensional analysis and Standard Model particle physics are sufficient to…

高能物理 - 唯象学 · 物理学 2007-05-23 F. Halzen

Liquid Xe TPCs are among the most popular choices for double beta decay and WIMP dark matter searches. Gaseous Xe has intrinsic advantages when compared to Liquid Xe, specifically, tracking capability and better energy resolution for double…

仪器与探测器 · 物理学 2015-05-15 Y. Nakajima , A. Goldschmidt , H. S. Matis , D. Nygren , C. Oliveira , J. Renner

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

The next generation of large scale WIMP direct detection experiments have the potential to go beyond the discovery phase and reveal detailed information about both the particle physics and astrophysics of dark matter. We report here on…

宇宙学与河外天体物理 · 物理学 2014-02-05 Jayden L. Newstead , Thomas D. Jacques , Lawrence M. Krauss , James B. Dent , Francesc Ferrer

We provide a new way of constraining the relative scintillation efficiency L_eff for liquid xenon. Using a simple estimate for the electronic and nuclear stopping powers together with an analysis of recombination processes we predict both…

天体物理仪器与方法 · 物理学 2011-08-23 Fedor Bezrukov , Felix Kahlhoefer , Manfred Lindner

The recent WMAP data have confirmed that exotic dark matter together with the vacuum energy (cosmological constant) dominate in the flat Universe. Modern particle theories naturally provide viable cold dark matter candidates with masses in…

宇宙学与河外天体物理 · 物理学 2009-12-17 J. D. Vergados , Ch. C. Moustakidis

The landscape of dark matter direct detection has been profoundly altered by the slew of recent experiments. While some have claimed signals consistent with dark matter, others have seen few, if any, events consistent with dark matter. The…

高能物理 - 唯象学 · 物理学 2014-05-28 Patrick J. Fox , Gabriel Jung , Peter Sorensen , Neal Weiner

Coherent scattering of solar, atmospheric and diffuse supernovae neutrinos creates an irreducible background for direct dark matter experiments with sensitivities to WIMP-nucleon spin-independent scattering cross-sections of…

高能物理 - 唯象学 · 物理学 2014-10-01 Philipp Grothaus , Malcolm Fairbairn , Jocelyn Monroe

Light WIMP dark matter and hidden sector dark matter have been proposed to explain the DAMA, CoGeNT and CRESST-II data. Both of these approaches feature spin independent elastic scattering of dark matter particles on nuclei. Light WIMP dark…

高能物理 - 唯象学 · 物理学 2012-11-15 R. Foot

The direct search for dark matter is entering a period of increased sensitivity to the hypothetical Weakly Interacting Massive Particle (WIMP). One such technology that is being examined is a scintillation only noble liquid experiment,…

A strong anti-correlation between ionization and scintillation signals produced by MeV gamma-rays in liquid xenon has been measured and used to improve the energy resolution by combining the two signals. The improvement is explained by…

天体物理学 · 物理学 2007-07-30 E. Aprile , K. L. Giboni , P. Majewski , K. Ni , M. Yamashita

An overview of non-directional direct detection methods is given. The currently leading experiments for spin independent WIMPs interactions are using simultaneous measurement of two quantities for event-by-event background discrimination in…

宇宙学与河外天体物理 · 物理学 2015-05-30 Benjamin Censier

We investigate the implication of different spin-dependent (SD) operators on both the direct and indirect detections of the Weakly Interacting Massive Particle (WIMP). Six representative building blocks of SD operators, together with their…

高能物理 - 唯象学 · 物理学 2014-02-26 Zheng-Liang Liang , Yue-Liang Wu

Dual phase xenon time projection chambers (TPCs) detect both the scintillation photons and ionization electrons created by energy depositions within the liquid xenon (LXe) volume. The electrons are extracted from the interaction site…

仪器与探测器 · 物理学 2025-02-24 Jianyang Qi , Kaixuan Ni , Haiwen Xu , Yue Ma , Yuechen Liu

We propose new signals for the direct detection of ultralight dark matter such as the axion. Axion or axion like particle (ALP) dark matter may be thought of as a background, classical field. We consider couplings for this field which give…

高能物理 - 唯象学 · 物理学 2013-09-11 Peter W. Graham , Surjeet Rajendran

We extend the study of the performance of a prototype two-phase liquid xenon WIMP dark matter detector to recoil energies below 20 keV. We demonstrate a new method for obtaining the best estimate of the energies of events using a calibrated…

天体物理学 · 物理学 2008-11-26 T. Shutt , C. E. Dahl , J. Kwong , A. Bolozdynya , P. Brusov
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