280 citations · 1.2k across the 22 of their papers we have counts for
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On the Dynamics of Proto-Neutron Star Winds and r-Process Nucleosynthesis
I. V. Panov, H. -Th. Janka
We study here the formation of heavy r-process nuclei in the high-entropy environment of rapidly expanding neutrino-driven winds from compact objects. In particular, we explore the…
Ejecta and progenitor of the low-luminosity Type IIP supernova 2003Z
V. P. Utrobin, N. N. Chugai, A. Pastorello
The origin of low-luminosity Type IIP supernovae is unclear: they have been proposed to originate either from massive (about 25 Msun) or low-mass (about 9 Msun) stars. We wish to d…
Permafrost - An Alternative Target Material for Ultra High Energy Neutrino Detection?
R. Nahnhauer, A. A. Rostovtsev, D. Tosi
The detection of cosmic neutrinos with energies above 1017 eV got growing interest during recent years. Possible target materials for in-matter arrays of ~100 km3 size under discus…
Theoretical light curves for deflagration models of Type Ia supernova
S. I. Blinnikov, F. K. Roepke, E. I. Sorokina +5
We present synthetic bolometric and broad-band UBVRI light curves of SNe Ia, for four selected 3-D deflagration models of thermonuclear supernovae. The light curves are computed wi…
Dynamics and Radiation of Young Type-Ia Supernova Remnants: Important Physical Processes
E. I. Sorokina, S. I. Blinnikov, D. I. Kosenko +1
We examine and analyze the physical processes that should be taken into account when modeling young type-Ia SNRs, with ages of several hundred years. It is shown, that energy losse…
The type IIn supernova 1994W: evidence for the explosive ejection of a circumstellar envelope
Nikolai N. Chugai, Sergei I. Blinnikov, Robert J. Cumming +6
We present and analyse spectra of the Type IIn supernova 1994W obtained between 18 and 203 days after explosion. During the luminous phase (first 100 d) the line profiles are compo…
Energy exchange inside SN ejecta and light curves of SNe Ia
E. I. Sorokina, S. I. Blinnikov
A treatment of line opacity in expanding medium is most crucial for the light curve (LC) modeling of Type Ia supernovae (SNe Ia). Spectral lines are the main source of opacity insi…