[PDF] Top 20 Reconciling neutrino flux from heavy dark matter decay and recent events at IceCube
Has 10000 "Reconciling neutrino flux from heavy dark matter decay and recent events at IceCube" found on our website. Below are the top 20 most common "Reconciling neutrino flux from heavy dark matter decay and recent events at IceCube".
Reconciling neutrino flux from heavy dark matter decay and recent events at IceCube
... The IceCube detector has recently reported the observation of 28 events at previously unexplored ...observed events are still low, these events hint at the existence of a ... Voir le document complet
15
Boosted Dark Matter and its implications for the features in IceCube HESE data
... this heavy particle constitutes a significant part of the dark matter (DM) density of the ...late-time decay produces a highly energetic flux of light dark matter (LDM) ... Voir le document complet
41
Minimal dark matter: model and results
... particles, at a given energy, that on average would emerge from their Earth crossing in the charged state and therefore would leave detectable tracks in the neutrino ...that, at high ... Voir le document complet
33
All-flavour search for neutrinos from dark matter annihilations in the Milky Way with IceCube/DeepCore
... Signal and background simulations In order to keep the analysis general we will assume that WIMPs annihilate with 100 % branching ratio into a few benchmark channels (b ¯ b, W + W − , ν ¯ν, μ + μ − and τ + ... Voir le document complet
15
Probing decaying heavy dark matter with the 4-year IceCube HESE data
... τ and ¯ ν τ and neutral-current interactions of all ...4-year IceCube HESE data, with a threshold of 10 TeV, contains 54 events, with ∼21 of them expected to be associated to atmospheric muons ... Voir le document complet
37
Charm decay in slow-jet supernovae as the origin of the IceCube ultra-high energy neutrino events
... of events at E > 2.1 PeV at the IC, and in contrast to the ∼ 4 events predicted by a uniform E −2 flux with normalization set by ...PeV from SJS is only about 1 in 10 ... Voir le document complet
14
Update on decaying and annihilating heavy dark matter with the 6-year IceCube HESE data
... starting events (HESE) sam- ple, we revisit the possibility that the updated data may be better explained by a combination of neutrino fluxes from dark matter decay and an ... Voir le document complet
37
The Direct Detection of Boosted Dark Matter at High Energies and PeV events at IceCube
... DM at high energies in neutrino detectors by performing a flux and cross-section ...broader and more general study, vis a vis choices of a mediator (scalar versus a vector boson, for ... Voir le document complet
14
Reconciling $B$-meson decay anomalies with neutrino masses, dark matter and constraints from flavour violation
... data and pre- dicting new phenomena, three independent observations signal the need to consider New Physics (NP) scenarios: neutrino oscillations, the baryon asymmetry of the Universe (BAU), and the ... Voir le document complet
39
DAEδALUS and dark matter detection
... luminosity and larger acceptance compared to previous experiments, a light DM search at DAE δALUS=LENA would not require a separate running mode, such as the off-target mode used for ...geometry, and ... Voir le document complet
21
First Search for Dark Matter Annihilation in the Sun Using the ANTARES Neutrino Telescope
... of dark matter ...5 and 6 , where for each WIMP mass and channel the values of the optimised angular separation, the average 90% CL upper limit computed from the background without ... Voir le document complet
22
Atomic ionization by sterile-to-active neutrino conversion and constraints on dark matter sterile neutrinos with germanium detectors
... of matter during the conversion of sterile to active neutrinos via their transition magnetic ...massless neutrino has almost zero four momentum so the square of 4-momentum transfer is simply ∼m 2 s ), ... Voir le document complet
11
Antiprotons from Dark Matter: current constraints and future sensitivities
... current and foreseen cosmic ray antiproton measurements on the properties of Dark Matter ...data from Pamela impose constraints on annihilating and decaying DM which are similar to (or ... Voir le document complet
17
Dark matter
... 12 WHAT’S NEW? In 2015 Massey et al. found a discrepancy between the observed mass distribution in Abell 3827 galaxy cluster and that predicted within standard cold DM model. They attributed the effect to ... Voir le document complet
19
Current dark matter annihilation constraints from CMB and low-redshift data
... Nonbaryonic matter is a crucial ingredient in our current understanding of the cosmological history of the ...“dark matter” that interacts only very weakly (if at all) with ordinary ... Voir le document complet
11
About dark matter and gravitation
... follows from very interesting observations made by the americano- swiss astronomer Fritz Zwicky around 1930 and reported in the two basic papers [13, ...luminous matter compared to the calculated ... Voir le document complet
17
Dark matter dynamics
... out and accelerate the ...called dark energy; the scientists who made the observations leading to dark energy’s discovery have recently been awarded the Nobel ...scales and re- veal that ... Voir le document complet
150
Exceptional Composite Dark Matter
... dot-dashed) and ZZ (black ...abundance at 95 % ...− from observations of the Galactic center by ...estimate and its comparison to the results of [ 48 ] also apply ...bound and the ... Voir le document complet
33
Constraints on Galactic Neutrino Emission with Seven Years of IceCube Data
... Physics and Center for Relativistic Astrophysics, Georgia Institute of Technology, Atlanta, GA 30332, USA Received 2017 July 11; revised 2017 September 3; accepted 2017 September 11; published 2017 October 31 ... Voir le document complet
12
Search for dark matter produced in association with heavy-flavor quark pairs in proton-proton collisions at $\sqrt{s}=13$ TeV
... data, and prefit and fitted background-only p miss T dis- tributions in two control regions (hadB and hadC in Table 2 ) for the 0,1 RTT hadronic tt + p T miss signal region with 0 leptons (upper) ... Voir le document complet
36
Sujets connexes