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If dark matter interacts with quarks or gluons, the mediator of these interactions is either directly accessible at the LHC or is so heavy that its effects are encoded in contact operators. We find that the self-consistency of a contact…

High Energy Physics - Phenomenology · Physics 2013-05-30 Ian M. Shoemaker , Luca Vecchi

Recent results from direct detection experiments (Dama, CoGeNT), though subject to debate, seem to point toward a low mass (few GeV) dark matter (DM) particle. However, low mass DM candidates are not easily achieved in the MSSM nor NMSSM.…

High Energy Physics - Phenomenology · Physics 2011-06-13 Timur Delahaye , David Cerdeño , Julien Lavalle

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…

High Energy Physics - Phenomenology · Physics 2011-10-07 Jia-Ming Zheng , Zhao-Huan Yu , Jun-Wen Shao , Xiao-Jun Bi , Zhibing Li , Hong-Hao Zhang

Various dark matter models predict annual and diurnal modulations of dark matter interaction rates in Earth-based experiments as a result of the Earth's motion in the halo. Observation of such features can provide generic evidence for…

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…

High Energy Physics - Phenomenology · Physics 2010-11-16 R. Foot

Recently, the DAMA/LIBRA collaboration has repeated and reinforced their claim to have detected an annual modulation in their signal rate, and have interpreted this observation as evidence for dark-matter particles at the 8.2 sigma…

High Energy Physics - Phenomenology · Physics 2009-02-26 Dan Hooper , Frank Petriello , Kathryn M. Zurek , Marc Kamionkowski

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…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-03 R. Foot

Savage et al. have recently put forward the claim that results from the XENON10 experiment are incompatible with the totality of both DAMA/LIBRA and CoGeNT experimental regions. In this brief note the source of this erroneous conclusion is…

Cosmology and Nongalactic Astrophysics · Physics 2010-06-11 J. I. Collar

The channeling of the ion recoiling after a collision with a WIMP in direct dark matter crystalline detectors produces a larger scintillation or ionization signal than otherwise expected. Channeling is a directional effect which depends on…

Cosmology and Nongalactic Astrophysics · Physics 2015-03-17 Nassim Bozorgnia , Graciela B. Gelmini , Paolo Gondolo

Diverse astrophysical observations suggest the existence of cold dark matter that interacts only gravitationally with radiation and ordinary baryonic matter. Any nonzero coupling between dark matter and baryons would provide a significant…

The CoGeNT collaboration has recently published results from a fifteen month data set which indicate an annual modulation in the event rate similar to what is expected from weakly interacting massive particle interactions. It has been…

High Energy Physics - Experiment · Physics 2013-03-14 MINOS Collaboration

Dark matter which interacts through a magnetic or electric dipole moment is an interesting possibility which may help to resolve the discrepancy between the DAMA annual modulation signal and the null results of other searches. In this…

High Energy Physics - Phenomenology · Physics 2013-05-30 Jean-François Fortin , Tim M. P. Tait

We investigate the constraints on the scalar, vector and spin-3/2 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…

High Energy Physics - Phenomenology · Physics 2012-03-14 Zhao-Huan Yu , Jia-Ming Zheng , Xiao-Jun Bi , Zhibing Li , Dao-Xin Yao , Hong-Hao Zhang

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…

Astrophysics · Physics 2010-04-21 Paolo Ciarcelluti , Robert Foot

We investigate singlet scalar dark matter (DM) candidate in a left-right symmetric gauge model with two Higgs bidoublets (2HBDM) in which the stabilization of the DM particle is induced by the discrete symmetries P and CP. According to the…

High Energy Physics - Phenomenology · Physics 2010-12-13 Wan-Lei Guo , Yue-Liang Wu , Yu-Feng Zhou

Measurements from the Gaia satellite have greatly increased our knowledge of the dark matter velocity distributions in the Solar neighborhood. There is evidence for multiple cold structures nearby, including a high-velocity stream…

High Energy Physics - Phenomenology · Physics 2019-10-03 Matthew R. Buckley , Gopolang Mohlabeng , Christopher W. Murphy

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…

Astrophysics · Physics 2007-05-23 Saibal Mitra

We consider the hypothesis that Dark Matter (DM) has tree-level interactions only with leptons. Such a framework, where DM recoils against electrons bound in atoms, has been proposed as an explanation for the annually modulated…

High Energy Physics - Phenomenology · Physics 2010-01-15 Joachim Kopp , Viviana Niro , Thomas Schwetz , Jure Zupan

Previous work has argued that, in the framework of plasma dark matter models, the DAMA annual modulation signal can be consistently explained with electron recoils. In the specific case of mirror dark matter, that explanation requires an…

High Energy Physics - Phenomenology · Physics 2018-12-19 R. Foot

We extract at redshift z=0 a Milky Way sized object including gas, stars and dark matter (DM) from a recent, high-resolution cosmological N-body simulation with baryons. Its resolution is sufficient to witness the formation of a rotating…

Astrophysics of Galaxies · Physics 2014-11-20 F. -S. Ling , E. Nezri , E. Athanassoula , R. Teyssier