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Y. Kojima

66 papers hereh-index 275.8k citations140 works total

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

author position
  • sole author9
  • first author24
  • middle author7
  • last author18

Across the 58 of 66 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE26
  • gr-qc20
  • astro-ph16
  • astro-ph.IM2
  • astro-ph.CO1
  • physics.ins-det1
same name
  • Y. Kojima — 4 papers, h 4
  • Y. Kojima — 4 papers, h 8
  • Y. Kojima — 2 papers, h 8
  • Y. Kojima — 1 paper, h 10
  • Y. Kojima — 1 paper
  • Y. Kojima — 1 paper, h 50

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
19952026
most citedKAGRA: 2.5 Generation Interferometric Gravitational Wave Detector

535 citations · 2k across the 66 of their papers we have counts for

collaborators
Showing 2000 · astro-phShow all

4 papers · 2 filters

astro-ph2000★ 25 cited

General Relativistic Modification of a Pulsar Electromagnetic Field

Kohkichi Konno, Yasufumi Kojima

We consider an exterior electromagnetic field surrounding a rotating star endowed with a dipole magnetic field in the context of general relativity. The analytic solution for a sta…

astro-ph2000★ 6 cited

Profiles and Polarization Properties of Emission Lines from Relativistic Disks

Jun Ogura, Nobuyori Ohuo, Yasufumi Kojima

We examined the profiles and polarization properties of emission lines originating from the extremely relativistic region of Kepler disks. Because the emission region is more local…

astro-ph2000

Stability of Relativistic Blast Waves

Jun Ogura, Yasufumi Kojima

A spherical blast wave with relativistic velocity can be described by a similarity solution, that is used for theoretical models of gamma-ray bursts. We consider the linear stabili…

astro-ph2000

Flattening modulus of a neutron star by rotation and magnetic field

K. Konno, T. Obata, Y. Kojima

We calculated the ellipticity of the deformed star due to the rotation or magnetic field. These two effects are compared to each other within general relativity. It turned out that…

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