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S. Woosley

164 papers hereh-index 9946.7k citations624 works total

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

author position
  • sole author8
  • first author18
  • middle author77
  • last author43

Across the 146 of 164 papers where every author was matched, so the position is known.

fields
  • astro-ph96
  • astro-ph.HE42
  • astro-ph.SR18
  • astro-ph.CO5
  • astro-ph.GA1
  • nucl-ex1
same name
  • S. Woosley — 45 papers, h 23
  • S. Woosley — 5 papers, h 4
  • S. Woosley — 2 papers, h 4

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
19942023
most citedCollapsars - Gamma-Ray Bursts and Explosions in "Failed Supernovae"

2.3k citations · 32.2k across the 163 of their papers we have counts for

collaborators
Showing 2000 · astro-phShow all

4 papers · 2 filters

astro-ph2000★ 201 cited

Presupernova Evolution with Improved Rates for Weak Interactions

A. Heger, S. E. Woosley, G. Martinez-Pinedo +1

Recent shell-model calculations of weak-interaction rates for nuclei in the mass range A = 45 - 65 have resulted in substantial revisions to the hitherto standard set of Fuller, Fo…

astro-ph2000★ 11 cited

Nucleosynthesis in massive stars revisited

T. Rauscher, A. Heger, R. D. Hoffman +1

We have performed the first calculations to follow the evolution of all stable nuclei and their radioactive progenitors in a finely-zoned stellar model computed from the onset of c…

astro-ph2000★ 182 cited

On the stability of very massive primordial stars

I. Baraffe, A. Heger, S. E. Woosley

The stability of metal-free very massive stars (Z = 0; $M = 120 - 500 \msol$) is analyzed and compared with metal-enriched stars. Such zero-metal stars are unstable to nuclear-po…

astro-ph2000★ 487 cited

Pair-Instability Supernovae, Gravity Waves, and Gamma-Ray Transients

C. L. Fryer, S. E. Woosley, A. Heger

Growing theoretical evidence suggests that the first generation of stars may have been quite massive (~100-300 solar masses). If they retain their high mass until death, such stars…

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