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相关论文: A Simple Explanation for DAMA with Moderate Channe…

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Recent results from the CoGeNT collaboration (as well as the annual modulation reported by DAMA/LIBRA) point toward dark matter with a light (5-10 GeV) mass and a relatively large elastic scattering cross section with nucleons (\sigma ~…

高能物理 - 唯象学 · 物理学 2011-08-09 Matthew R. Buckley , Dan Hooper , Tim M. P. Tait

If dark matter (DM) has non-zero direct or transition, electric or magnetic dipole moment then it can scatter nucleons electromagnetically in direct detection experiments. Using the results from experiments like XENON, CDMS, DAMA and COGENT…

高能物理 - 唯象学 · 物理学 2009-09-02 Eduard Masso , Subhendra Mohanty , Soumya Rao

The annual modulation in the rate of WIMP recoils observed by the DAMA collaboration at high significance is often analyzed in the context of an isothermal Maxwell-Boltzmann velocity distribution. While this is the simplest model, there is…

宇宙学与河外天体物理 · 物理学 2011-02-23 Aravind Natarajan

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 DAMA experiment clearly observes a small oscillatory signal. The observed yearly modulation is in phase with the Earth's motion around the Sun. Recent reference [Vavra, 2014] suggested that the DAMA experiment observes a WIMP of much…

天体物理仪器与方法 · 物理学 2014-01-28 J. Va'vra

We examine the dark matter interpretation of the modulation signal reported by the DAMA experiment from the perspective of effective field theories displaying Galilean invariance. We consider the most general effective coupling leading to…

高能物理 - 唯象学 · 物理学 2016-05-25 Riccardo Catena , Alejandro Ibarra , Sebastian Wild

Recently the CDMS collaboration has reported an excess of events in the signal region of a search for dark matter scattering with Silicon nuclei. Three events on an expected background of 0.4 have a significance of about 2 sigma, and it is…

高能物理 - 唯象学 · 物理学 2014-07-30 Randel C. Cotta , Arvind Rajaraman , Tim M. P. Tait , Alexander M. Wijangco

Recently, the CoGeNT experiment has reported events in excess of expected background. We analyze dark matter scenarios which can potentially explain this signal. Under the standard case of spin independent scattering with equal couplings to…

高能物理 - 唯象学 · 物理学 2014-11-20 Spencer Chang , Jia Liu , Aaron Pierce , Neal Weiner , Itay Yavin

Dark Matter annihilation (DMA) may yield an excess of gamma rays and antimatter particles, like antiprotons and positrons, above the background from cosmic ray interactions. Several signatures, ranging from the positron excess, as observed…

天体物理学 · 物理学 2009-11-13 W. de Boer

Exotic dark matter together with dark energy or cosmological constant seem to dominate in the Universe. An even higher density of such matter seems to be gravitationally trapped in our Galaxy. The nature of dark matter can be unveiled only,…

核理论 · 物理学 2009-09-29 J. D. Vergados

We re-analyse the implications of the DAMA/NaI experiment for mirror matter-type dark matter, taking into account information from the energy dependence of the DAMA annual modulation signal. This is combined with the null results from the…

天体物理学 · 物理学 2008-11-26 R. Foot

We study a Dirac Dark Matter particle interacting with ordinary matter via the exchange of a light pseudo-scalar, and analyze its impact on both direct and indirect detection experiments. We show that this candidate can accommodate the…

高能物理 - 唯象学 · 物理学 2015-01-14 Chiara Arina , Eugenio Del Nobile , Paolo Panci

Dark Matter (DM) is generally assumed to be massive, cold and collisionless from the structure formation point of view. A more correct statement however is that DM indeed experiences collisional damping, but on a scale which is supposed to…

天体物理学 · 物理学 2007-05-23 C. Boehm , H. Mathis , J. Devriendt , J. Silk

We consider a model in which dark matter consists of a large self-interacting component (SIDM particles) and a small component with strong interactions with baryons (SIMPs). We show that the DAMA annual modulation signal can be caused by…

天体物理学 · 物理学 2007-05-23 Saibal Mitra

In this paper, we study the recent excess of low energy events observed by the CoGeNT collaboration and the annual modulation reported by the DAMA/LIBRA collaboration, and discuss whether these signals could both be the result of the same…

高能物理 - 唯象学 · 物理学 2010-12-24 Dan Hooper , J. I. Collar , Jeter Hall , Dan McKinsey , Chris Kelso

Directional detection can provide unambiguous observation of Dark Matter interactions even in presence of insidious backgrounds. The DM-TPC collaboration is developing a detector with the goal of measuring the direction and sense of nuclear…

Since the expected rates for neutralino-nucleus scattering are expected to be small, one should exploit all the characteristic signatures of this reaction. Such are: (i) In the standard recoil measurements the modulation of the event rate…

高能物理 - 唯象学 · 物理学 2007-05-23 J. D. Vergados

Mirror dark matter provides a simple framework for which to explain the DAMA/Libra annual modulation signal consistently with the null results of the other direct detection experiments. The simplest possibility involves ordinary matter…

天体物理学 · 物理学 2010-04-21 Paolo Ciarcelluti , Robert Foot

The channeling effect in crystals refers to the orientation dependence of charged ion penetration in crystals. In direct dark matter crystalline detectors, a channeled ion recoiling after a collision with a WIMP gives all its energy to…

天体物理仪器与方法 · 物理学 2011-09-06 Nassim Bozorgnia

Possible hints for WIMP dark matter with mass around 10 GeV coming from the DAMA, CoGeNT, and maybe also CRESST experiments are presented, and confronted with constraints from CDMS and XENON data. Focusing on spin-independent (SI)…

高能物理 - 唯象学 · 物理学 2010-11-29 Thomas Schwetz