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researcher

B. Krishnan

111 papers hereh-index 7835.7k citations275 works total

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

author position
  • sole author4
  • first author2
  • middle author49
  • last author21

Across the 76 of 111 papers where every author was matched, so the position is known.

fields
  • gr-qc97
  • astro-ph5
  • astro-ph.HE4
  • astro-ph.IM2
  • astro-ph.SR2
  • astro-ph.CO1
same name
  • B. Krishnan — 45 papers
  • B. Krishnan — 17 papers, h 22
  • B. Krishnan — 8 papers, h 3
  • B. Krishnan — 2 papers, h 3
  • B. Krishnan — 1 paper, h 19
  • B. Krishnan — 1 paper, h 3

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
20002023
most citedCharacterization of the LIGO detectors during their sixth science run

1.3k citations · 17.1k across the 110 of their papers we have counts for

collaborators
Showing 2010Show all

3 papers · 1 filter

gr-qc2010★ 1.1k cited

Sensitivity Studies for Third-Generation Gravitational Wave Observatories

S. Hild, M. Abernathy, F. Acernese +136

Advanced gravitational wave detectors, currently under construction, are expected to directly observe gravitational wave signals of astrophysical origin. The Einstein Telescope, a…

gr-qc2010★ 36 cited

The slicing dependence of non-spherically symmetric quasi-local horizons in Vaidya Spacetimes

Alex B. Nielsen, Michael Jasiulek, Badri Krishnan +1

It is well known that quasi-local black hole horizons depend on the choice of a time coordinate in a spacetime. This has implications for notions such as the surface of the black h…

gr-qc2010★ 498 cited

Matching post-Newtonian and numerical relativity waveforms: systematic errors and a new phenomenological model for non-precessing black hole binaries

L. Santamaria, F. Ohme, P. Ajith +10

We present a new phenomenological gravitational waveform model for the inspiral and coalescence of non-precessing spinning black hole binaries. Our approach is based on a frequency…

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