activity
20012011
most citedRole of dense matter in collective supernova neutrino transformations

174 citations · 1.9k across the 30 of their papers we have counts for

collaborators

30 papers

astro-ph.HE2011★ 73 cited

ELMAG: A Monte Carlo simulation of electromagnetic cascades on the extragalactic background light and in magnetic fields

M. Kachelriess, S. Ostapchenko, R. Tomas

A Monte Carlo program for the simulation of electromagnetic cascades initiated by high-energy photons and electrons interacting with extragalactic background light (EBL) is present…

hep-ph2011★ 94 cited

Analysis of matter suppression in collective neutrino oscillations during the supernova accretion phase

Sovan Chakraborty, Tobias Fischer, Alessandro Mirizzi +2

The usual description of self-induced neutrino flavor conversions in core collapse supernovae (SNe) is based on the dominance of the neutrino density n_nu over the net electron den…

hep-ph2011★ 124 cited

No collective neutrino flavor conversions during the supernova accretion phase

Sovan Chakraborty, Tobias Fischer, Alessandro Mirizzi +2

The large neutrino fluxes emitted with a distinct flavor hierarchy from core-collapse supernovae (SNe) during the post-bounce accretion phase, offer the best opportunity to detect…

astro-ph.HE2011★ 30 cited

Antimatter production in supernova remnants

M. Kachelriess, S. Ostapchenko, R. Tomas

We calculate the energy spectra of cosmic rays (CR) and their secondaries produced in a supernova remnant (SNR), taking into account the time-dependence of the SNR shock. We model…

hep-ph2010★ 36 cited

Multi-angle effects in self-induced oscillations for different supernova neutrino fluxes

Alessandro Mirizzi, Ricard Tomàs

The non-isotropic nature of the neutrino emission from a supernova (SN) core might potentially affect the flavor evolution of the neutrino ensemble, via neutrino-neutrino interacti…

astro-ph.HE2010★ 1 cited

Antimatter spectra from a time-dependent modeling of supernova remnants

M. Kachelriess, S. Ostapchenko, R. Tomas

We calculate the energy spectra of cosmic rays (CR) and their secondaries produced in a supernova remnant (SNR), taking into account the time-dependence of the SNR shock. We model…