[PDF] Top 20 Searching for dark matter with superheated liquid detectors
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Searching for dark matter with superheated liquid detectors
... of dark matter which comprises 85% of the total mass of the ...the superheated liquid or bubble chamber technique to search for dark ...technique for dark mat- ter ... Voir le document complet
295
Searching for Light Scalar Dark Matter with Gravitational Waves Detectors
... Models with a single outburst underestimate the excess emission observed in the Galactic ...order for the gamma-ray emissions to exhibit roughly the same spectral shape at all relevant latitudes as observed ... Voir le document complet
206
Coherent neutrino scattering in dark matter detectors
... noble liquid detector [ 2 , 3 ] or other dark matter detector technology), for concreteness we consider the specific example of a set of GEODM-derived detectors with ...source. ... Voir le document complet
9
Dark Matter, what is it?
... Latin for light, and is also the acronym for the Large Underground Xenon ...collide with one of the xenon atoms, producing a flash of light, which will be ...now for about three years and as ... Voir le document complet
2
Dark Matter Direct Detection using Cryogenic Detectors
... g detectors, it appears important to increase the individual detector mass of discriminating experiments, presently in the 250-320 g range, to ∼ 1 ...rapidly. For example, it seems difficult at present to ... Voir le document complet
48
Boosted dark matter at neutrino experiments
... Cherenkov detectors like Super-Kamiokande (Super-K) [10] and Hyper-Kamiokande (Hyper-K) [11] , and liquid argon time projection chambers (LArTPCs) like the upcoming Deep Underground Neutrino Experiment ... Voir le document complet
13
Neutralino Dark Matter beyond CMSSM Universality
... models with non-universal Higgs soft masses m 2 H 2 = m 0 and m 2 H 1 = ...and with A 0 = 0, tan β = 45, µ > ...7.64) for RGE’s and SUSY spectrum calculation (instead of Suspect in this work) ... Voir le document complet
24
Minimal dark matter: model and results
... particle with a ...present for signals from the galactic center, which is possible if DM clumps are tidally disrupted in the central regions of the Milky ...tension with state-of-the-art numerical ... Voir le document complet
33
Dark Matter constraints on composite Higgs models
... viable dark matter ...except for corrections due to the explicit breaking of ...observed dark matter component of the ...pNGB. For a model based on the coset SO(7)/G2, see ... Voir le document complet
42
Constraining Dark Matter with the Long-Term Variability of Quasars
... that all variability is due to mi rolensing and omparing the predi tions from mi rolensing s enarios to the observed amplitudes of quasar light urves, upp er limits to the osmologi al density of ompa t obje t may ... Voir le document complet
3
Search for dark matter towards the Galactic Centre with 11 years of ANTARES data
... term for antineu- trinos. The detector effective area increases with energy due to the raise with energy of the CC cross section, combined with the better track definition of high-energy ... Voir le document complet
7
Analysis method for detecting topological defect dark matter with a global magnetometer network
... ordinary matter in a variety of ways. For example, fermion spins may couple to the gradient of the axion field ...fermionic matter crosses a region with an axion field gradient, such as a ... Voir le document complet
12
DAEδALUS and dark matter detection
... [79] with a simplified model of the DAE δALUS target geometry and generated the DM kinematics by decaying the pions as predicted by the dark photon model; details are given below and in ...agreement ... Voir le document complet
21
About dark matter and gravitation
... beginning with Andromeda, by looking at their outermost material, and observed flat rotation curves: the outermost components of the galaxy were moving as quickly as those close to the ...by dark ... Voir le document complet
17
Searching for stochastic gravitational waves using data from the two colocated LIGO Hanford detectors
... Institute for Advanced Research, the Brazilian Ministry of Science, Technology, Innovations, and Commu- nications, the International Center for Theoretical Physics South American Institute for ... Voir le document complet
59
Dark matter from dynamical SUSY breaking
... 4 Dark matter from a quantum moduli space In addition to the chiral models discussed in ...theories with a QMS, e.g. the ITIY model [18]. In these models, SUSY QCD with a QMS is coupled to ... Voir le document complet
24
Dark Matter Accretion into Supermassive Black Holes
... the dark matter accretion process into black holes is ...cross-section for capture by a black hole of non-relativistic and non-interacting par- ...inside dark mat- ter halos issued from ... Voir le document complet
8
Composite dark matter and direct-search experiments
... underground detectors. To go further with this idea, one could even imagine that dark particles are not elementary but consist of structures made of exotic particles, that we could generically call ... Voir le document complet
70
Effective theory of self-interacting dark matter
... mechanism for electroweak symmetry ...potential for this type of indirect detection has gained attention recently due to possible anomalies in the positron fluxes measured by pamela [1], Fermi [2] and ... Voir le document complet
26
Light dark matter annihilations into two photons
... a dark matter source (and the response to it by SPI) has been studied in detail in ...only dark matter scenario which can explain SPI observa- tion requires a Navarro-Frenk-White profile (NFW) ... Voir le document complet
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