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[PDF] Top 20 Probing decaying heavy dark matter with the 4-year IceCube HESE data

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Probing decaying heavy dark matter with the 4-year IceCube HESE data

Probing decaying heavy dark matter with the 4-year IceCube HESE data

... of the 2-year IceCube HESE dataset [ 57 ] (considering the energy spectrum of the events in this dataset) has been studied in ...agreement with the data for ... Voir le document complet

37

Update on decaying and annihilating heavy dark matter with the 6-year IceCube HESE data

Update on decaying and annihilating heavy dark matter with the 6-year IceCube HESE data

... of the neutrino flux seems to be compatible with a galactic disc origin [ 31 – 34 ...that the limits on the galactic contribution are usually obtained using spatial and energy templates for ... Voir le document complet

37

Boosted Dark Matter and its implications for the features in IceCube HESE data

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 PeV, attributed to ... Voir le document complet

41

Dark matter assimilation into the baryon asymmetry

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 ... Voir le document complet

29

Current dark matter annihilation constraints from CMB and low-redshift data

Current dark matter annihilation constraints from CMB and low-redshift data

... taking the expansion of the Universe into account, using an improved version of the code first described in .... The spectra of photons and electrons below this energy are stored —many of ... Voir le document complet

11

Dark matter dynamics in the early universe

Dark matter dynamics in the early universe

... In section 6, we turn on both the annihilation and catalytic reactions and solve the Boltzmann's equation numerically, and discuss how their combined effect affects d[r] ... Voir le document complet

39

Search for dark matter produced with an energetic jet or a hadronically decaying W or Z boson at $ \sqrt{s}=13 $ TeV

Search for dark matter produced with an energetic jet or a hadronically decaying W or Z boson at $ \sqrt{s}=13 $ TeV

... for dark matter particles is performed using events with large miss- ing transverse momentum, at least one energetic jet, and no leptons, in proton-proton collisions at √ s = 13 TeV collected ... Voir le document complet

50

Almost closing the νMSM sterile neutrino dark matter window with NuSTAR

Almost closing the νMSM sterile neutrino dark matter window with NuSTAR

... analysis with 0-bounce photons Because the solid-angle aperture for 0-bounce photons is over 2 orders of magnitude larger than the FOV for focused photons, observations of diffuse emission that ... Voir le document complet

13

Constraints on Galactic Neutrino Emission with Seven Years of IceCube Data

Constraints on Galactic Neutrino Emission with Seven Years of IceCube Data

... Abstract The origins of high-energy astrophysical neutrinos remain a mystery despite extensive searches for their ...of IceCube Neutrino Observatory muon data on the neutrino flux coming from ... Voir le document complet

12

Unifying inflation with the axion, dark matter, baryogenesis and the seesaw mechanism

Unifying inflation with the axion, dark matter, baryogenesis and the seesaw mechanism

... extra matter content was recently proposed in [6], where it was emphasized that in addition to solving the strong CP problem, provid- ing a good dark matter candidate (the axion), ... Voir le document complet

7

Exceptional Composite Dark Matter

Exceptional Composite Dark Matter

... detection data could in principle test the model with improved sensi- tivity in the range of f that is relevant for ...DM. The Cherenkov Telescope Array CTA [ 51 ], which should start ... Voir le document complet

33

Dark Matter Indirect Detection with charged cosmic rays

Dark Matter Indirect Detection with charged cosmic rays

... Since the J-factor grows as the DM density squared, the best targets are the ones with a high concentration of DM, such as the GC, clusters, dwarf spheroidal galaxies and ... Voir le document complet

175

Constraining a Thin Dark Matter Disk with Gaia

Constraining a Thin Dark Matter Disk with Gaia

... over the nuisance parameters. From the likelihood profiles, we compute the 95% one- sided limit on Σ DD , which is shown in ...to the expectation under the null hypothesis, which is ... Voir le document complet

8

Inhomogeneous cosmology : an answer to the Dark Matter and Dark Energy problems?

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 principle should ... Voir le document complet

204

Results from the search for dark matter in the Milky Way with 9 years of data of the ANTARES neutrino telescope

Results from the search for dark matter in the Milky Way with 9 years of data of the ANTARES neutrino telescope

... 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 the Zhao profile [12] , which ... Voir le document complet

7

About dark matter and gravitation

About dark matter and gravitation

... of the model. At the time of Newton, nothing was known about atoms and ...that the cohesion of matter and gravity might share the same ...1748. The theory proposed a mechanical ... Voir le document complet

17

Dark matter at the LHC: WIMPs and beyond

Dark matter at the LHC: WIMPs and beyond

... of the characteristic features of thermal freeze-out is that, given that dark matter is required to interact relatively strongly with the Standard Model particles, thermal equilibrium ... Voir le document complet

9

DAEδALUS and dark matter detection

DAEδALUS and dark matter detection

... Note the inclusion of the helicity-suppressed pion decay modes to electrons and positrons, which will in fact pose the main backgrounds above 250 ...estimate the beam-on backgrounds, we used ... Voir le document complet

21

Search for dark matter produced in association with heavy-flavor quark pairs in proton-proton collisions at $\sqrt{s}=13$ TeV

Search for dark matter produced in association with heavy-flavor quark pairs in proton-proton collisions at $\sqrt{s}=13$ TeV

... background The sources of uncer- tainty in the misidentified-lepton background for the dileptonic search stem from the uncertainty in the mea- sured misidentification rate, and from ... Voir le document complet

36

Indirect Search for Dark Matter

Indirect Search for Dark Matter

... Possible dark matter candidates are reviewed as well as indirect search methods based on annihilation or decay channels of these ...presently the best particle candidate and its annihilation produces ... Voir le document complet

9

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