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Ko Nakamura

30 papers hereh-index 18993 citations63 works total

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

author position
  • first author11
  • middle author15
  • last author2

Across the 28 of 30 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE21
  • astro-ph.SR4
  • astro-ph3
  • astro-ph.IM1
  • nucl-th1

identity via Semantic Scholar / OpenAlex

activity
20042026
most citedSystematic Features of Axisymmetric Neutrino-Driven Core-Collapse Supernova Models in Multiple Progenitors

133 citations · 1.2k across the 30 of their papers we have counts for

collaborators
Showing 2018Show all

3 papers · 1 filter

astro-ph.HE2018★ 36 cited

Progenitor Mass Distribution of Core-Collapse Supernova Remnants in Our Galaxy and Magellanic Clouds based on Elemental Abundances

Satoru Katsuda, Tomoya Takiwaki, Nozomu Tominaga +2

We investigate a progenitor mass distribution of core-collapse supernova remnants (CCSNRs) in our Galaxy and the Large and Small Magellanic Clouds, for the first time. We count the…

astro-ph.HE2018★ 2 cited

Diagnosing the Structure of Massive Stars with Galactic Supernova Neutrinos

Shunsaku Horiuchi, Ko Nakamura, Tomoya Takiwaki +1

It has been suggested that whether a star explodes or not, and what kind of explosion properties it shows, is strongly dependent on the progenitor's core structure. We present the…

astro-ph.HE2018★ 76 cited

Impact of Neutrino Opacities on Core-Collapse Supernova Simulations

Kei Kotake, Tomoya Takiwaki, Tobias Fischer +2

Accurate description of neutrino opacities is central both to the core-collapse supernova (CCSN) phenomenon and to the validity of the explosion mechanism itself. In this work, we…

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