[PDF] Top 20 Direct Search for Dark Matter with the DarkSide Experiment
Has 10000 "Direct Search for Dark Matter with the DarkSide Experiment" found on our website. Below are the top 20 most common "Direct Search for Dark Matter with the DarkSide Experiment".
Direct Search for Dark Matter with the DarkSide Experiment
... within the geometry of the detector is affected by the optical properties of each detector volume and of the interfaces between ...implement the optical simulation. In some cases ... Voir le document complet
192
Study of the single electron charge signals in the XENON100 direct Dark Matter search experiment
... assembled: the DarkSide experiment [95] in LNGS and the ArDM [96] experiment in Canfranc, and have started to acquire data for dark matter ...detectors The ... Voir le document complet
258
Search for dark matter produced in association with bottom or top quarks in $\sqrt{s}=13$ TeV pp collisions with the ATLAS detector
... this search is the case of colour-charged scalar mediators [ 22 ]. The model assumes bottom-flavoured dark matter (b-FDM) and was proposed to explain the excess of gamma rays ... Voir le document complet
52
Combined search for neutrinos from dark matter self-annihilation in the Galactic Center with ANTARES and IceCube
... optimised for a previ- ous dark matter search based on the same dataset ...to the number of strings with triggered PMTs, two different reconstruction algorithms are ... Voir le document complet
12
Search for dark matter towards the Galactic Centre with 11 years of ANTARES data
... in the indirect search for the fundamental constituents of dark matter (DM) in form of weakly interacting massive particles ...in the Northern Hemisphere, is able to ... Voir le document complet
7
Contribution to the energy and time measurement of electrons and photons in the ATLAS experiment and search for dark matter production is association to a Higgs boson
... inside the Milky Way galactic center (GC). In the FERMI-LAT paper [ 93 ], interstellar emission models (IEM’s) are developed to determine the galactic back- ground γ-ray emissions, together ... Voir le document complet
278
All-flavour search for neutrinos from dark matter annihilations in the Milky Way with IceCube/DeepCore
... a. For a cascade reconstruction there are seven degrees of freedom, while an infinite track reconstruc- tion has only six since the point x 0 can be chosen arbitrarily along the ...track. The ... Voir le document complet
15
Search for dark matter in association with an energetic photon in $pp$ collisions at $\sqrt{s}$ = 13 TeV with the ATLAS detector
... CERN for the very successful operation of the LHC, as well as the support staff from our institutions without whom ATLAS could not be operated ...acknowledge the support of ANPCyT, ... Voir le document complet
46
Results from the search for dark matter in the Milky Way with 9 years of data of the ANTARES neutrino telescope
... acknowledge the financial support of the fund- ing agencies: Centre National de la Recherche Scientifique (CNRS), Commissariat à l’énergie atomique et aux énergies alternatives (CEA), Commission Européenne ... Voir le document complet
7
Search for dark matter candidates and large extra dimensions in events with a jet and missing transverse momentum with the ATLAS detector
... The value of using an effective field theory approach to WIMP-SM particle coupling is that only two parameters, M ∗ and m χ , are needed to describe WIMP pair production at the LHC, WIMP-nucleon scattering ... Voir le document complet
59
Search for dark matter in association with a Higgs boson decaying to two photons at $\sqrt{s}$ = 13 TeV with the ATLAS detector
... CERN for the very successful operation of the LHC, as well as the support staff from our institutions without whom ATLAS could not be operated e ...acknowledge the support of ANPCyT, ... Voir le document complet
45
Dark matter effective field theory scattering in direct detection experiments
... show the limit calculated assuming the alternate velocity distribution function discussed ...above. The SuperCDMS Soudan, CDMS II Ge (reanalysis), and CDMS II Si limits use the candidate ... Voir le document complet
14
Stellar streams as probes of dark matter : search and dynamical analysis
... is, the velocity vector of a stream star in the Galaxy’s rest frame must be a tangent vector to the orbit of this extended structure at that stellar ...to the orbital path of the stream ... Voir le document complet
163
Composite dark matter and direct-search experiments
... 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 “composite dark ...posite ... Voir le document complet
70
Tools for model-independent bounds in direct dark matter searches
... Cdms-Ge The Cryogenic Dark Matter Search (Cdms II) experiment is located at the Soudan Un- derground Laboratory in ...measure the energy deposited by incident particles in ... Voir le document complet
48
Optimization of spherical proportional counter backgrounds and response for low mass dark matter search
... toward the center of the sphere. Close to the anode, an avalanche occurs, creating a large number of secondary ion-electron ...pairs. The motions of the secondary ions then induces ... Voir le document complet
239
Search for photon line-like signatures from Dark Matter annihilations with H.E.S.S
... In the last few years, imaging atmospheric Cherenkov telescopes (IACTs) have been used to search for dark matter (DM) signals in very-high-energy (VHE; E γ > 100 GeV) γ rays ... Voir le document complet
7
Searching for Light Scalar Dark Matter with Gravitational Waves Detectors
... to the previous one is the absence of contamination effects together with the fact that the mass distribution is derived directly without any assumption about the dark ... Voir le document complet
206
Identification of backgrounds in the EDELWEISS-I dark matter search experiment
... associated with incomplete charge collection due to surface interactions, it is difficult to explain why we observe a constant value of Q ∼ ...efficiency for alpha interactions in Ge is similar to that of ... Voir le document complet
23
Indirect Search for Dark Matter
... rate. The expected low event rate demands a very low radioactive and cosmic ray background, which is one of the major difficulties of a direct search for dark matter ... Voir le document complet
9
Sujets connexes