Author

Woosley, Stanford Earl

INSPIRE profile983190 ORCID0000-0002-3352-7437

9 papers·1,132 citations in this corpus

	Paper	Category
Mar 16, 2021#92103.07933	The Pair-Instability Mass Gap for Black Holes S. E. Woosley (1)🇺🇸 · Alexander Heger (2 and 3 and 4 and 5) ((1) UCSC, (2) Monash, (3) OzGrav, (4) ASTRO-3D, (5) JINA-CEE)🇦🇺	↳ astro-ph.SR	ApJL	266
Mar 27, 2015#31503.07522	A two-parameter criterion for classifying the explodability of massive stars by the neutrino-driven mechanism T. Ertl (1,2) · H.-Th. Janka (1) · S.E. Woosley (3) · T. Sukhbold (3) · M. Ugliano (4) ((1) MPI Astrophysics, Garching, (2) Physik Dept., TUM, Garching, (3) UC Santa Cruz, (4) TU Darmstadt)	↳ astro-ph.SR	ApJ	388
Aug 1, 2003#4*astro-ph/0307546	Neutrino Nucleosynthesis A. Heger (1,2) · E. Kolbe (3) · W. C. Haxton (4) · K. Langanke (5) · G.Martinez-Pinedo (6,7) · S. E. Woosley (8) ((1) U Chicago, (2) LANL, (3) U Basel, (4) INT, U Washington, (5) U Aarhus, (6) IEEC, (7) ICREA, (8) UCSC)	↳ astro-ph	PLB	195
Jun 18, 2001#4*astro-ph/0106289	Nuclear Aspects of the s- and n-Processes in Massive Stars T. Rauscher (1) · A. Heger (2) · S. E. Woosley (2) · R. D. Hoffman (3) ([1] Dept. of Physics and Astronomy, University of Basel, Switzerland; [2] Dept. of Astronomy and Astrophysics, UCSC, USA; [3] Lawrence Livermore National Laboratory, USA)	↳ astro-ph	—	1
Nov 29, 2000#5*astro-ph/0011507	Presupernova Evolution with Improved Rates for Weak Interactions A. Heger (1)🇺🇸 · S. E. Woosley (1)🇺🇸 · G. Martinez-Pinedo (2)🇺🇸 · K. Langanke(2) ((1)UCSC, (2)Aarhus Universitet, Denmark)🇺🇸	↳ astro-ph	ApJ	161
Sep 1, 2000#2*nucl-th/0008065	Nuclear Aspects of Nucleosynthesis in Massive Stars T. Rauscher (1,2)🇨🇭 · R.D. Hoffman (3)🇺🇸 · A. Heger (2)🇺🇸 · S.E. Woosley (2) ((1) University of Basel, Switzerland; (2) UCSC, USA; (3) Lawrence Livermore National Laboratory, USA)🇺🇸	nucl-th	—	1
Aug 1, 2000#6*astro-ph/0007453	Prediction of Astrophysical Reaction Rates: Methods, Data Needs, and Consequences for Nucleosynthesis Studies T. Rauscher (1)🇨🇭 · R. D. Hoffman (2)🇺🇸 · S. E. Woosley (2,3)🇺🇸 · F.-K. Thielemann(1) ((1) Dept. of Physics and Astronomy, Univ. of Basel, Switzerland; (2) Lawrence Livermore National Laboratory, Livermore, CA, USA; (3) Dept. of Astron. and Astroph., Univ. of California, Santa Cruz, CA, USA)🇨🇭	↳ astro-ph	AIP Conf.Proc.	2
Jul 28, 2000#7*astro-ph/0007412	Presupernova collapse models with improved weak-interaction rates A. Heger (1)🇺🇸 · K. Langanke (2)🇩🇰 · G. Martinez-Pinedo (2)🇩🇰 · S.E. Woosley (1) ((1) UCO/Lick Observatory, University of California; (2) Institut for Fysik og Astronomi, Aarhus Universitet)🇺🇸	↳ astro-ph	PRL	116
Jun 27, 2000#4*astro-ph/0006350	Nucleosynthesis in Massive Stars - Including All Stable Isotopes A. Heger (1)🇺🇸 · R. D. Hoffman (2)🇺🇸 · T. Rauscher (1,3)🇺🇸 · S. E. Woosley (1) ((1) UCSC, (2) LLNL, (3) Uni. Basel)🇺🇸	↳ astro-ph	—	2

The Pair-Instability Mass Gap for Black Holes
S. E. Woosley (1)🇺🇸 · Alexander Heger (2 and 3 and 4 and 5) ((1) UCSC, (2) Monash, (3) OzGrav, (4) ASTRO-3D, (5) JINA-CEE)🇦🇺
Mar 16, 2021#9↳ astro-ph.SRApJL266 citations
A two-parameter criterion for classifying the explodability of massive stars by the neutrino-driven mechanism
T. Ertl (1,2) · H.-Th. Janka (1) · S.E. Woosley (3) · T. Sukhbold (3) · M. Ugliano (4) ((1) MPI Astrophysics, Garching, (2) Physik Dept., TUM, Garching, (3) UC Santa Cruz, (4) TU Darmstadt)
Mar 27, 2015#3↳ astro-ph.SRApJ388 citations
Neutrino Nucleosynthesis
A. Heger (1,2) · E. Kolbe (3) · W. C. Haxton (4) · K. Langanke (5) · G.Martinez-Pinedo (6,7) · S. E. Woosley (8) ((1) U Chicago, (2) LANL, (3) U Basel, (4) INT, U Washington, (5) U Aarhus, (6) IEEC, (7) ICREA, (8) UCSC)
Aug 1, 2003#4*↳ astro-phPLB195 citations
Nuclear Aspects of the s- and n-Processes in Massive Stars
T. Rauscher (1) · A. Heger (2) · S. E. Woosley (2) · R. D. Hoffman (3) ([1] Dept. of Physics and Astronomy, University of Basel, Switzerland; [2] Dept. of Astronomy and Astrophysics, UCSC, USA; [3] Lawrence Livermore National Laboratory, USA)
Jun 18, 2001#4*↳ astro-ph1 citation
Presupernova Evolution with Improved Rates for Weak Interactions
A. Heger (1)🇺🇸 · S. E. Woosley (1)🇺🇸 · G. Martinez-Pinedo (2)🇺🇸 · K. Langanke(2) ((1)UCSC, (2)Aarhus Universitet, Denmark)🇺🇸
Nov 29, 2000#5*↳ astro-phApJ161 citations
Nuclear Aspects of Nucleosynthesis in Massive Stars
T. Rauscher (1,2)🇨🇭 · R.D. Hoffman (3)🇺🇸 · A. Heger (2)🇺🇸 · S.E. Woosley (2) ((1) University of Basel, Switzerland; (2) UCSC, USA; (3) Lawrence Livermore National Laboratory, USA)🇺🇸
Sep 1, 2000#2*nucl-th1 citation
Prediction of Astrophysical Reaction Rates: Methods, Data Needs, and Consequences for Nucleosynthesis Studies
T. Rauscher (1)🇨🇭 · R. D. Hoffman (2)🇺🇸 · S. E. Woosley (2,3)🇺🇸 · F.-K. Thielemann(1) ((1) Dept. of Physics and Astronomy, Univ. of Basel, Switzerland; (2) Lawrence Livermore National Laboratory, Livermore, CA, USA; (3) Dept. of Astron. and Astroph., Univ. of California, Santa Cruz, CA, USA)🇨🇭
Aug 1, 2000#6*↳ astro-phAIP Conf.Proc.2 citations
Presupernova collapse models with improved weak-interaction rates
A. Heger (1)🇺🇸 · K. Langanke (2)🇩🇰 · G. Martinez-Pinedo (2)🇩🇰 · S.E. Woosley (1) ((1) UCO/Lick Observatory, University of California; (2) Institut for Fysik og Astronomi, Aarhus Universitet)🇺🇸
Jul 28, 2000#7*↳ astro-phPRL116 citations
Nucleosynthesis in Massive Stars - Including All Stable Isotopes
A. Heger (1)🇺🇸 · R. D. Hoffman (2)🇺🇸 · T. Rauscher (1,3)🇺🇸 · S. E. Woosley (1) ((1) UCSC, (2) LLNL, (3) Uni. Basel)🇺🇸
Jun 27, 2000#4*↳ astro-ph2 citations

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