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N. Nishimura

41 papers hereh-index 191.8k citations72 works total

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

author position
  • first author11
  • middle author22
  • last author5

Across the 38 of 41 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR17
  • astro-ph.HE13
  • nucl-th4
  • astro-ph.GA3
  • astro-ph2
  • astro-ph.CO1
same name
  • N. Nishimura — 15 papers, h 23
  • N. Nishimura — 4 papers, h 23
  • N. Nishimura — 2 papers, h 9
  • N. Nishimura — 2 papers, h 1
  • N. Nishimura — 1 paper, h 3
  • N. Nishimura — 1 paper, 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
20052025
most citedProduction of all the r-process nuclides in the dynamical ejecta of neutron star mergers

624 citations · 2.8k across the 38 of their papers we have counts for

collaborators
Showing 2014Show all

3 papers · 1 filter

astro-ph.HE2014

Production of 92Nb, 92Mo, and 146Sm in the gamma-process in SNIa

T. Rauscher, C. Travaglio, R. Gallino +2

The knowledge of the production of extinct radioactivities like 92Nb and 146Sm by photodisintegration processes in ccSN and SNIa models is essential for interpreting abundances in…

astro-ph.SR2014★ 54 cited

Code dependencies of pre-supernova evolution and nucleosynthesis in massive stars: Evolution to the end of core helium burning

Samuel Jones, Raphael Hirschi, Marco Pignatari +5

Massive stars are key sources of radiative, kinetic, and chemical feedback in the universe. Grids of massive star models computed by different groups each using their own codes, in…

astro-ph.SR2014★ 624 cited

Production of all the r-process nuclides in the dynamical ejecta of neutron star mergers

Shinya Wanajo, Yuichiro Sekiguchi, Nobuya Nishimura +3

Recent studies suggest that binary neutron star (NS-NS) mergers robustly produce the heavy r-process nuclei above the atomic mass number A ~ 130 because of their ejecta consisting…

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