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T. Kawano

30 papers hereh-index 3212k citations376 works total

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

author position
  • sole author2
  • first author5
  • middle author18
  • last author4

Across the 29 of 30 papers where every author was matched, so the position is known.

fields
  • nucl-th21
  • astro-ph.HE3
  • nucl-ex3
  • astro-ph.SR2
  • astro-ph1
same name
  • T. Kawano — 35 papers, h 17
  • T. Kawano — 15 papers, h 13
  • T. Kawano — 13 papers, h 9
  • T. Kawano — 11 papers, h 14
  • T. Kawano — 4 papers, h 2
  • T. Kawano — 3 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
20082026
most citedReference Database for Photon Strength Functions

164 citations · 1k across the 30 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

3 papers · 1 filter

astro-ph.HE2020★ 6 cited

Characterizing r-Process Sites through Actinide Production

Erika M. Holmbeck, Rebecca Surman, Anna Frebel +6

Of the variations in the elemental abundance patterns of stars enhanced with r-process elements, the variation in the relative actinide-to-lanthanide ratio is among the most sign…

astro-ph.HE2019★ 24 cited

Neutrino self-interaction and MSW effects on the supernova neutrino-process

Heamin Ko, Myung-Ki Cheoun, Eunja Ha +13

We calculate the abundances of 7Li, 11B, 92Nb, 98Tc, 138La, and 180Ta produced by neutrino (ν) induced reactions in a core-collapse supernova explos…

astro-ph.HE2018★ 95 cited

Californium-254 and kilonova light curves

Y. Zhu, R. T. Wollaeger, N. Vassh +13

Neutron star mergers offer unique conditions for the creation of the heavy elements and additionally provide a testbed for our understanding of this synthesis known as the r-proc…

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