activity
20082026
most citedLight Sterile Neutrinos: A White Paper

454 citations · 5.6k across the 116 of their papers we have counts for

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Showing 2014Show all

5 papers · 1 filter

astro-ph.HE2014★ 71 cited

High-energy gamma-ray and neutrino backgrounds from clusters of galaxies and radio constraints

Fabio Zandanel, Irene Tamborra, Stefano Gabici +1

Cosmic-ray protons accumulate for cosmological times in clusters of galaxies as their typical radiative and diffusive escape times are longer than the Hubble time. Their hadronic i…

astro-ph.SR2014★ 55 cited

Impact of neutrino flavor oscillations on the neutrino-driven wind nucleosynthesis of an electron-capture supernova

Else Pllumbi, Irene Tamborra, Shinya Wanajo +2

Neutrino oscillations, especially to light sterile states, can affect the nucleosynthesis yields because of their possible feedback effect on the electron fraction (Ye). For the fi…

astro-ph.SR2014★ 155 cited

Neutrino emission characteristics and detection opportunities based on three-dimensional supernova simulations

Irene Tamborra, Georg Raffelt, Florian Hanke +2

The neutrino emission characteristics of the first full-scale three-dimensional supernova simulations with sophisticated three-flavor neutrino transport for three models with masse…

astro-ph.HE2014★ 200 cited

Star-forming galaxies as the origin of diffuse high-energy backgrounds: Gamma-ray and neutrino connections, and implications for starburst history

Irene Tamborra, Shin'ichiro Ando, Kohta Murase

Star-forming galaxies have been predicted to contribute considerably to the diffuse gamma-ray background as they are guaranteed reservoirs of cosmic rays. Assuming that the hadroni…

astro-ph.SR2014★ 179 cited

Self-sustained asymmetry of lepton-number emission: A new phenomenon during the supernova shock-accretion phase in three dimensions

Irene Tamborra, Florian Hanke, Hans-Thomas Janka +3

During the stalled-shock phase of our 3D hydrodynamical core-collapse simulations with energy-dependent, 3-flavor neutrino transport, the lepton-number flux (nue minus antinue) eme…