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researcher

S. Goriely

135 papers hereh-index 6717.4k citations573 works total

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

author position
  • first author15
  • middle author76
  • last author26

Across the 117 of 135 papers where every author was matched, so the position is known.

fields
  • nucl-th40
  • astro-ph.SR26
  • nucl-ex23
  • astro-ph22
  • astro-ph.HE20
  • astro-ph.CO1
same name
  • S. Goriely — 48 papers, h 14
  • S. Goriely — 10 papers, h 6
  • S. Goriely — 9 papers, h 5
  • S. Goriely — 5 papers, h 4
  • S. Goriely — 2 papers, h 45
  • S. Goriely — 1 paper

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
19972026
most citedThe r-process of stellar nucleosynthesis: Astrophysics and nuclear physics achievements and mysteries

904 citations · 9.5k across the 133 of their papers we have counts for

collaborators
Showing 2003Show all

4 papers · 1 filter

nucl-th2003★ 194 cited

Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. II: Role of the effective mass

S. Goriely, M. Samyn, M. Bender +1

We have constructed four new complete mass tables, referred to as HFB-4 to HFB-7, each one including all the 9200 nuclei lying between the two drip lines over the range of Z and N>…

astro-ph2003★ 1 cited

Pre-suprenova evolution of rotating massive stars

Raphael Hirschi, Georges Meynet, Andre Maeder +1

The Geneva evolutionary code has been modified to study the advanced stages (Ne, O, Si burnings) of rotating massive stars. Here we present the results of four 20 solar mass stars…

nucl-th2003★ 302 cited

Microscopic HFB+QRPA predictions of dipole strength for astrophysics applications

S. Goriely, E. Khan, M. Samyn

Large-scale QRPA calculations of the E1 strength are performed on top of HFB calculations in order to derive the radiative neutron capture cross sections for the whole nuclear char…

astro-ph2003★ 121 cited

More lead stars

S. Van Eck, S. Goriely, A. Jorissen +1

The standard model for the operation of the s-process in asymptotic giant branch (AGB) stars predicts that low-metallicity ([Fe/H] <= -1) AGB stars should exhibit large overabundan…

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