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researcher

K. Sugimura

30 papers hereh-index 17845 citations73 works total

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

author position
  • sole author1
  • first author12
  • middle author10
  • last author7

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

fields
  • astro-ph.GA24
  • astro-ph.CO3
  • astro-ph.SR1
  • gr-qc1
  • hep-th1
same name
  • K. Sugimura — 4 papers, h 18
  • K. Sugimura — 4 papers, h 6
  • K. Sugimura — 3 papers, h 4
  • K. Sugimura — 2 papers, 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
20112025
most citedThe critical radiation intensity for direct collapse black hole formation: dependence on the radiation spectral shape

155 citations · 894 across the 30 of their papers we have counts for

collaborators
Showing 2018Show all

3 papers · 1 filter

astro-ph.GA2018★ 23 cited

Gravitational stability and fragmentation condition for discs around accreting supermassive stars

Ryoki Matsukoba, Sanemichi Z. Takahashi, Kazuyuki Sugimura +1

Supermassive stars (SMSs) with mass ∼105 M⊙​ are promising candidates for the origin of supermassive black holes observed at redshift ≳6. They are suppos…

astro-ph.GA2018★ 32 cited

Super-Eddington accretion of dusty gas onto seed black holes: metallicity-dependent efficiency of mass growth

Daisuke Toyouchi, Takashi Hosokawa, Kazuyuki Sugimura +2

The super-Eddington accretion onto intermediate seed BHs is a potential formation mode of supermassive black holes exceeding 109 M⊙​ in the early universe. We here investiga…

astro-ph.GA2018★ 36 cited

Stunted accretion growth of black holes by combined effect of the flow angular momentum and radiation feedback

Kazuyuki Sugimura, Takashi Hosokawa, Hidenobu Yajima +2

Accretion on to seed black holes (BHs) is believed to play a crucial role in formation of supermassive BHs observed at high-redshift (z>6). Here, we investigate the combined effect…

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