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M. Kimura

33 papers hereh-index 293.8k citations337 works total

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

author position
  • sole author3
  • first author5
  • middle author16
  • last author8

Across the 32 of 33 papers where every author was matched, so the position is known.

fields
  • gr-qc17
  • hep-th10
  • astro-ph4
  • astro-ph.IM1
  • hep-ph1
same name
  • M. Kimura — 29 papers, h 29
  • M. Kimura — 20 papers, h 11
  • M. Kimura — 11 papers, h 22
  • M. Kimura — 7 papers, h 12
  • M. Kimura — 5 papers
  • M. Kimura — 2 papers, h 18

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
20062022
most citedAnisotropic Inflation from Vector Impurity

131 citations · 870 across the 25 of their papers we have counts for

collaborators
Showing 2018Show all

4 papers · 1 filter

gr-qc2018

Stability analysis of black holes by the S-deformation method for coupled systems

Masashi Kimura, Takahiro Tanaka

We propose a simple method to prove the linear mode stability of a black hole when the perturbed field equations take the form of a system of coupled Schrödinger equations. The lin…

gr-qc2018

Stability analysis of Schwarzschild black holes in dynamical Chern-Simons gravity

Masashi Kimura

Dynamical Chern-Simons gravity has an interesting feature that the parity violating term exists, and the coupling is determined by a dynamical scalar field. When the spacetime has…

gr-qc2018

Black holes, gravitational waves and fundamental physics: a roadmap

Leor Barack, Vitor Cardoso, Samaya Nissanke +203

The grand challenges of contemporary fundamental physics---dark matter, dark energy, vacuum energy, inflation and early universe cosmology, singularities and the hierarchy problem-…

gr-qc2018

Robustness of the S-deformation method for black hole stability analysis

Masashi Kimura, Takahiro Tanaka

The S-deformation method is a useful way to show the linear mode stability of a black hole when the perturbed field equation takes the form of the Schrödinger equation. While pre…

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