Bounds are derived on the cross section, flux and energy density of new particles that may be responsible for the atmospheric neutrino anomaly. $4.6 primordial homogeneous dark matter can be excluded
We derive new constraints on combination of dark matter - electron cross-section ($\sigma_{\chi e}$)...
We consider dark matter annihilation into Standard Model particles and show that the least detectabl...
High-energy neutrinos, arising from decays of mesons that were produced through the cosmic rays coll...
Dark matter (DM) annihilations in the Galaxy may produce high-energy neutrinos, which can be detecte...
In order to facilitate the identification of possible new physics signatures in neutrino telescopes,...
The atmospheric neutrino anomaly is the apparent reduction of the either a reduction in the muon neu...
In the TeV energy region and above, the uncertainty in the level of prompt atmospheric neutrinos wou...
In this talk I review measurements and calculations of the flux of neutrinos produced by interaction...
We show that the canonical oscillation-based (nonresonant) production of sterile neutrino dark matte...
Abstract: Neutrino telescopes are looking to detect neutrinos produced by the annihilation of weakly...
Ultrahigh energy cosmic neutrinos are incisive probes of both astrophysical sources and new TeV-scal...
International audienceWe present joint constraints on the number of effective neutrino speciesN_eff ...
We consider dark matter annihilation into standard model particles and show that the least detectabl...
The recent results of the EDGES Collaboration indicate that during the era of reionization, the prim...
AbstractWe review the status of sterile neutrino dark matter and discuss astrophysical and cosmologi...
We derive new constraints on combination of dark matter - electron cross-section ($\sigma_{\chi e}$)...
We consider dark matter annihilation into Standard Model particles and show that the least detectabl...
High-energy neutrinos, arising from decays of mesons that were produced through the cosmic rays coll...
Dark matter (DM) annihilations in the Galaxy may produce high-energy neutrinos, which can be detecte...
In order to facilitate the identification of possible new physics signatures in neutrino telescopes,...
The atmospheric neutrino anomaly is the apparent reduction of the either a reduction in the muon neu...
In the TeV energy region and above, the uncertainty in the level of prompt atmospheric neutrinos wou...
In this talk I review measurements and calculations of the flux of neutrinos produced by interaction...
We show that the canonical oscillation-based (nonresonant) production of sterile neutrino dark matte...
Abstract: Neutrino telescopes are looking to detect neutrinos produced by the annihilation of weakly...
Ultrahigh energy cosmic neutrinos are incisive probes of both astrophysical sources and new TeV-scal...
International audienceWe present joint constraints on the number of effective neutrino speciesN_eff ...
We consider dark matter annihilation into standard model particles and show that the least detectabl...
The recent results of the EDGES Collaboration indicate that during the era of reionization, the prim...
AbstractWe review the status of sterile neutrino dark matter and discuss astrophysical and cosmologi...
We derive new constraints on combination of dark matter - electron cross-section ($\sigma_{\chi e}$)...
We consider dark matter annihilation into Standard Model particles and show that the least detectabl...
High-energy neutrinos, arising from decays of mesons that were produced through the cosmic rays coll...
DOI
Add to ORKG