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相关论文: Mirror dark matter explanation of the DAMA, CoGeNT…

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We examine data from the DAMA, CoGeNT, CRESST-II and CDMS/Si direct detection experiments in the context of multi-component hidden sector dark matter. The models considered feature a hidden sector with two or more stable particles charged…

高能物理 - 唯象学 · 物理学 2013-08-09 R. Foot

Mirror dark matter offers a framework to explain the existing dark matter direct detection experiments. Here we confront this theory with the most recent experimental data, paying attention to the various known systematic uncertainties, in…

高能物理 - 唯象学 · 物理学 2010-11-11 R. Foot

Recently, the CDMS/Si experiment has observed a low energy excess of events in their dark matter search. In light of this new result we update the mirror dark matter explanation of the direction detection experiments. We find that the DAMA,…

宇宙学与河外天体物理 · 物理学 2015-06-16 R. Foot

The CRESST-II collaboration have announced evidence for the direct detection of dark matter in 730 kg-days exposure of a CaWO$_4$ target. We examine these new results, along with DAMA and CoGeNT data, in the context of the mirror dark…

高能物理 - 唯象学 · 物理学 2015-06-04 R. Foot

Three dark matter direct detection experiments (DAMA/LIBRA, CoGeNT, and CRESST-II) have each reported signals which are not consistent with known backgrounds, but resemble that predicted for a dark matter particle with a mass of roughly…

宇宙学与河外天体物理 · 物理学 2013-05-30 Chris Kelso , Dan Hooper , Matthew R. Buckley

Mirror and more generic hidden sector dark matter models can simultaneously explain the DAMA, CoGeNT and CRESST dark matter signals consistently with the null results of the other experiments. This type of dark matter can be captured by the…

高能物理 - 唯象学 · 物理学 2015-05-30 R. Foot

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

The CoGeNT collaboration has recently reported a rising low energy spectrum in their ultra low noise germanium detector. This is particularly interesting as the energy range probed by CoGeNT overlaps with the energy region in which DAMA has…

高能物理 - 唯象学 · 物理学 2010-11-16 R. Foot

Dark matter in the form of particles from a hidden mirror sector has recently been proposed as an explanation for the DAMA annual modulation signal. Here one assumes that there exists a small mixing between photons and mirror photons. We…

天体物理学 · 物理学 2007-05-23 Saibal Mitra

We explore the dark matter interpretation of the anomalies claimed by the DAMA and CoGeNT experiments, in conjunction with the various null direct-detection experiments. An independent analysis of the CoGeNT data is employed and several…

高能物理 - 唯象学 · 物理学 2015-05-28 Marco Farina , Duccio Pappadopulo , Alessandro Strumia , Tomer Volansky

A mirror sector of particles and forces provides a simple explanation of the inferred dark matter of the Universe. The status of this theory is reviewed - with emphasis on how the theory explains the impressive DAMA/NaI annual modulation…

高能物理 - 唯象学 · 物理学 2008-11-26 R. Foot

We examine the possibility that dark matter may be the manifestation of dark forces of a hidden sector, i.e. "Dark Force = Dark Matter." As an illustrative and minimal example we consider the hidden SU(2)_h x U(1)_h gauge group. The hidden…

高能物理 - 唯象学 · 物理学 2014-04-02 Hooman Davoudiasl , Ian M. Lewis

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

Mirror atoms are expected to be a significant component of the galactic dark matter halo if mirror matter is identified with the non-baryonic dark matter in the Universe. Mirror matter can interact with ordinary matter via gravity and via…

高能物理 - 唯象学 · 物理学 2008-11-26 R. Foot

A simple way to accommodate dark matter is to postulate the existence of a hidden sector. That is, a set of new particles and forces interacting with the known particles predominantly via gravity. In general this leads to a large set of…

宇宙学与河外天体物理 · 物理学 2014-05-13 R. Foot

Mirror dark matter, where dark matter resides in a hidden sector exactly isomorphic to the standard model, can be probed via direct detection experiments by both nuclear and electron recoils if the kinetic mixing interaction exists. In…

高能物理 - 唯象学 · 物理学 2017-01-04 J. D. Clarke , R. Foot

Mirror dark matter is a dissipative and self-interacting multiparticle dark matter candidate which can explain the DAMA, CoGeNT and CRESST-II direct detection experiments. This explanation requires photon-mirror photon kinetic mixing of…

宇宙学与河外天体物理 · 物理学 2015-06-11 R. Foot

Mirror matter is a stable self-collisional dark matter candidate. If exact mirror parity is a conserved symmetry of nature, there could exist a parallel hidden (mirror) sector of the Universe which has the same kind of particles and the…

宇宙学与河外天体物理 · 物理学 2014-11-20 Paolo Ciarcelluti

Mirror dark matter interacting with ordinary matter via photon-mirror photon kinetic mixing can explain the DAMA, CoGeNT and CRESSTII direct detection experiments. This explanation requires kinetic mixing of strength $\epsilon \sim…

宇宙学与河外天体物理 · 物理学 2015-06-03 R. Foot

Mirror dark matter offers a framework to explain the existing dark matter direct detection experiments, including the impressive DAMA annual modulation signal. Here we examine the implications of mirror dark matter for experiments like…

高能物理 - 唯象学 · 物理学 2010-11-16 R. Foot
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