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researcher

S. Blinnikov

16 papers hereh-index 10908 citations34 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author1
  • middle author10
  • last author4

Across the 15 of 16 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE12
  • astro-ph2
  • astro-ph.CO1
  • astro-ph.SR1
same name
  • S. Blinnikov — 81 papers, h 32
  • S. Blinnikov — 25 papers, h 21
  • S. Blinnikov — 9 papers, h 7
  • S. Blinnikov — 9 papers, h 2
  • S. Blinnikov — 4 papers, h 3
  • S. Blinnikov — 3 papers, h 0

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20062022
most citedPulsational pair instability as an explanation for the most luminous supernovae

672 citations · 1.3k across the 16 of their papers we have counts for

collaborators
Showing 2015Show all

3 papers · 1 filter

astro-ph.SR2015★ 8 cited

Multicolor light curves simulations of Population III core-collapse supernovae: from shock breakout to 56Co decay

Alexey Tolstov, Ken'ichi Nomoto, Nozomu Tominaga +3

The properties of the first generation of stars and their supernova (SN) explosions remains unknown due to the lack of their actual observations. Recently many transient surveys ar…

astro-ph.HE2015★ 35 cited

On physical and numerical instabilities arising in simulations of non-stationary radiatively cooling shocks

D. A. Badjin, S. I. Glazyrin, K. V. Manukovskiy +1

We describe our modelling of the radiatively cooling shocks and their thin shells with various numerical tools in different physical and calculational setups. We inspect structure…

astro-ph.HE2015★ 47 cited

Can pair-instability supernova models match the observations of superluminous supernovae?

Alexandra Kozyreva, S. Blinnikov

An increasing number of so-called superluminous supernovae (SLSNe) are discovered. It is believed that at least some of them with slowly fading light curves originate in stellar ex…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.