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Katsuhiko Sato

81 papers hereh-index 427.7k citations266 works total

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

author position
  • first author2
  • middle author16
  • last author59

Across the 77 of 81 papers where every author was matched, so the position is known.

fields
  • astro-ph50
  • nucl-th9
  • astro-ph.HE6
  • hep-ph6
  • astro-ph.CO4
  • gr-qc3
same name
  • Katsuhiko Sato — 9 papers, h 6
  • Katsuhiko Sato — 6 papers, h 12
  • Katsuhiko Sato — 1 paper
  • Katsuhiko Sato — 1 paper, h 2

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
19952020
most citedExplosion Mechanism, Neutrino Burst, and Gravitational Wave in Core-Collapse Supernovae

313 citations · 3.7k across the 81 of their papers we have counts for

collaborators
Showing 2001Show all

4 papers · 1 filter

nucl-th2001★ 1 cited

Microscopic Study of Nuclear "Pasta" by Quantum Molecular Dynamics

Gentaro Watanabe, Katsuhiko Sato, Kenji Yasuoka +1

Structure of cold dense stellar matter at subnuclear densities is investigated with quantum molecular dynamics (QMD). We succeeded in showing that the phases with slab-like and rod…

hep-ph2001★ 24 cited

Determining the Supernova Direction by its Neutrinos

Shin'ichiro Ando, Katsuhiko Sato

Supernova neutrinos, which arrive at Earth earlier than light, allow for the earliest determination of the direction of the supernova. The topic of this paper is to study how accur…

nucl-th2001★ 17 cited

Formation of Nuclear "Pasta" in Cold Neutron Star Matter

Kei Iida, Gentaro Watanabe, Katsuhiko Sato

Formation and decay of rod-like and slab-like nuclei, as may be encountered in the outer parts of neutron stars, are examined within a zero-temperature stability analysis with resp…

astro-ph2001★ 18 cited

Propagation of UHECRs from the Sources in the Super-Galactic Plane

Y. Ide, S. Nagataki, S. Tsubaki +2

We have performed the detailed numerical simulations on the propagation of the UHE protons in the energy range E=(1019.5−1022.0) eV in the relatively strong extra-galacti…

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