[PDF] Top 20 Boosted Dark Matter and its implications for the features in IceCube HESE data
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Boosted Dark Matter and its implications for the features in IceCube HESE data
... consider the case where this heavy particle constitutes a significant part of the dark matter (DM) density of the ...Universe. Its late-time decay produces a highly energetic ... Voir le document complet
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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
Exceptional Composite Dark Matter
... account the dependence of the abundance Ω h 2 of η on its mass (or, equivalently, on the scale f ), as shown in Figure 1 .... The weakest indirect detection bounds that we ... Voir le document complet
33
Reconciling neutrino flux from heavy dark matter decay and recent events at IceCube
... data in the near future will serve as an important test for the consistency of the observa- tions with the astrophysical flux predicted from standard ...with the ... Voir le document complet
15
Minimal dark matter: model and results
... recap the main features of minimal dark matter (MDM) and assess its status in the light of recent experimental ...data. The theory selects an ... Voir le document complet
33
Boosted dark matter at neutrino experiments
... bound the Lorentz factor from below. We performed two analyses, one for BDM originating from the GC and one in which we stacked signals from ...Super-K in the case of ... Voir le document complet
13
Update on decaying and annihilating heavy dark matter with the 6-year IceCube HESE data
... ] and even violates the unitarity bound [ 80 , 81 ] in most ...Nevertheless, for low DM masses and for final state leptons, previous works found results more restrictive than ... Voir le document complet
37
Probing decaying heavy dark matter with the 4-year IceCube HESE data
... panels). For all panels, τ DM = 10 27 s. Note that the average over neutrino flavors results in fluxes which are identical with or without neutrino ...Earth for two DM masses m DM = 200 TeV ... Voir le document complet
37
Results from the search for dark matter in the Milky Way with 9 years of data of the ANTARES neutrino telescope
... model and the “McMillan” [10] profile. The parameters for these models are taken from [11] and [10] and are shown in Table 1 .... The McMillan profile is a variant of ... Voir le document complet
7
Tools for model-independent bounds in direct dark matter searches
... Now, Dark Matter being a particle physics problem, any ‘model’ of the interactions of DM with ordinary matter will be expressed in terms of operators involving the degrees of ... Voir le document complet
48
A Correlation between the Higgs Mass and Dark Matter
... from the behavior of 𝜆(𝐸) with 𝑚 퐻 = 126 GeV in Figure ...however the factor of ℎ 4 makes it vary by many orders of magnitude as we explore a large field ...of the resulting potential will be ... Voir le document complet
9
Detecting the invisible universe with neutrinos and dark matter
... Black points show nuclear recoil candidates; grey shading shows Monte Carlo generated nuclear recoil candidates; blue line shows predicted (3D) range-energy function f[r] ... Voir le document complet
118
Dark matter assimilation into the baryon asymmetry
... of the time, heavy stable charged particles simply exit the detector, but if they are produced with a small enough β factor, they can loose sufficient energy through ionization that they stop inside ... Voir le document complet
29
Inhomogeneous cosmology : an answer to the Dark Matter and Dark Energy problems?
... to the cosmological principle, it is impossible for the ΛCDM model to describe any structure under a scale between 100h ´1 and 700h ´1 ...Mpc. The re- strictions introduced by this ... Voir le document complet
204
Analysis of vacuum and argon gas fill data from the MiniCLEAN dark matter experiment
... The MiniCLEAN dark matter experiment is a single-phase liquid argon scintil- lation detector which uses the wavelength-shifting fluor tetraphenyl butadiene and cryogen[r] ... Voir le document complet
193
Direct Search for Dark Matter with the DarkSide Experiment
... on the results of a large statistics FLUKA [92] simulation (34 years of cosmic muons irradiation of the detector) and particular attention has been devoted to the validation of the ... Voir le document complet
192
First Search for Dark Matter Annihilation in the Sun Using the ANTARES Neutrino Telescope
... downwards in order to optimise their acceptance to upgoing light and to avoid the effect of sedimentation and biofouling [ 18 ...]. The length of a line is 450 m and the ... Voir le document complet
22
Constraints on mediator-based dark matter and scalar dark energy models using $\sqrt s = 13$ TeV $pp$ collision data collected by the ATLAS detector
... 20(a) and 20(b) present the exclusion limits dependence on the mixing angle, sin θ, for a low-mass and high-mass a hypothesis, as evaluated in the third ...scenario. ... Voir le document complet
84
Neutrino indirect detection of neutralino dark matter in the CMSSM
... adopt the central value. Lowering m t implies that the top Yukawa coupling Y t is smaller so that the RG decreasing of m 2 H u is less efficient and the region where EWSB does not occur ... Voir le document complet
16
Searching for dark matter with superheated liquid detectors
... indefinitely and shortly after the passage of par- ticles the pressure is raised to condensate the vapor to ...liquid. The operation of bubble chambers has rapidly evolved since ... Voir le document complet
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