[PDF] Top 20 The Direct Detection of Boosted Dark Matter at High Energies and PeV events at IceCube
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The Direct Detection of Boosted Dark Matter at High Energies and PeV events at IceCube
... study the possibility of detecting dark matter directly via a small but energetic component that is allowed within present-day ...upon the fact that neutral current neutrino nucleon ... Voir le document complet
14
Dark Matter Direct Detection using Cryogenic Detectors
... among the developments that might mark a fur- ther progress in discrimination performances, are the identification with high efficiency of surface events, and most notably heavy ... Voir le document complet
48
Reconciling neutrino flux from heavy dark matter decay and recent events at IceCube
... Introduction The IceCube detector (IC) at the South Pole has recently observed 28 events at energies 30 ...TeV–1.2 PeV [ 1 ]. This marks the first ever ... Voir le document complet
15
Dark matter effective field theory scattering in direct detection experiments
... examine the effects of the different possible interactions for experiments with similar fiducial masses, we also plot the event rate per time per target mass ...Ge and Si SuperCDMS ... Voir le document complet
14
Boosted Dark Matter and its implications for the features in IceCube HESE data
... on the other hand, is designed to explain only the event excess at 50–100 TeV energies as being due to DM scattering on ice, with the other events, including those above 1 ... Voir le document complet
41
Direct Observation of the Surface Topography at High Temperature with SEM
... use the 3D reconstructions is to focus more specifically on the volume variations of a particular area of the sample ...In the present case, particular attention was paid onto ... Voir le document complet
21
Combined search for neutrinos from dark matter self-annihilation in the Galactic Center with ANTARES and IceCube
... consists of events recorded over 9 years between 2007 and 2015, resulting in an effec- tive livetime of ...composed of up-going track-like events and was optimised for a ... Voir le document complet
12
On the importance of electroweak corrections for Majorana dark matter indirect detection
... show the fluxes of charged cosmic rays for the representative choice of model parameters already used in Section 5 (namely, M χ = 1 TeV and M S = 4 ...for the annihilation cross ... Voir le document complet
27
Saturation regimes at LHC energies
... curve and the circles represent the above cases for Γ 2 ...where the BDL is smooth. First of all, we can continue the Γ = 1 plateau by a Gaussian which connects quickly to ... Voir le document complet
6
Thermal dileptons at SPS energies
... of the excess referred to the Collins Soper frame is found to be ...with the interpretation of the excess as thermal ...study the hot and dense QCD matter ... Voir le document complet
8
Phenomenology of LFV at low-energies and at the LHC: strategies to probe the SUSY seesaw
... Extending the Standard Model to accommo- date ν data naturally opens the possibility of many other new ...theoretical and experimentally shortcomings of the Standard Model can be ... Voir le document complet
7
Probing the supersymmetric type III seesaw: LFV at low-energies and at the LHC
... Under the hypothesis that neutrinos are Majorana particles, the smallness of their masses, as well as their mixings, can be explained via seesaw-like mechanisms due to the exchange of ... Voir le document complet
20
Broadband and Resonant Approaches to Axion Dark Matter Detection
... in the mass range m a ∈ ½10 −14 ; 10 −6 eV. Most existing axion detection proposals use some kind of resonant enhancement, but we have shown that broadband circuits can have superior sensitivity ... Voir le document complet
7
Constraints on the MSSM from the Higgs Sector - A pMSSM Study of Higgs Searches, Bs -> mu+ mu- and Dark Matter Direct Detection
... view of the negative results of the searches in chan- nels with M ET conducted by the ATLAS and CMS ex- periments on more than 1 fb −1 of statistics at 7 TeV [1–5], ... Voir le document complet
11
Evolution of the phase-space density of dark matter haloes and mixing effects in merger events
... spite of these impressive successes, there are still discrepan- cies between simulations and observations at scales 1 Mpc, which have been extensively discussed in the literature in ... Voir le document complet
7
All-flavour search for neutrinos from dark matter annihilations in the Milky Way with IceCube/DeepCore
... is the product of the self-annihilation cross sec- tion, σ A , and the WIMP velocity, v, averaged over the velocity distribution of WIMPS in the halo, which we ... Voir le document complet
15
On inverse scattering at high energies for the multidimensional Newton equation in electromagnetic field
... inversion of the X-ray transform P we obtain that for n ≥ 2 the velocity valued component of the scattering operator at high ener- gies uniquely determines (∇V, ... Voir le document complet
38
The structure and analytic properties of the scattering amplitude at LHC energies
... that the TOTEM data at 7 TeV for the differential cross sections seem to be somewhat inconsistent with their determination of σ tot (s) and ρ(s, t = 0) ...compare the data ... Voir le document complet
5
Dark Matter Indirect Detection with charged cosmic rays
... that Dark Matter indirect detection with antiprotons has revealed itself to be a more difficult exercise than expected: with more sensitive data, the energy spectrum starts to discriminate ... Voir le document complet
175
Constraints on Dynamical Dark Energy Models from the Abundance of Massive Galaxies at High Redshifts
... 3.1. The Stellar Mass function at z = 6 from CAN- DELS We first compare with the observed stellar mass distribution of massive, distant ...to the details of the star ... Voir le document complet
17
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