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B. S. Sathyaprakash

3 papers hereh-index 133 citations2 works total

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

author position
  • first author1
  • last author2

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • gr-qc2
  • astro-ph1
same name
  • B. S. Sathyaprakash — 65 papers
  • B. S. Sathyaprakash — 5 papers
  • B. S. Sathyaprakash — 2 papers
  • B. S. Sathyaprakash — 2 papers
  • B. S. Sathyaprakash — 2 papers
  • B. S. Sathyaprakash — 1 paper

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
19942019
most citedComparison of post-Newtonian mode amplitudes with numerical relativity simulations of binary black holes

39 citations · 85 across the 3 of their papers we have counts for

collaborators

3 papers

gr-qc2019★ 39 cited

Comparison of post-Newtonian mode amplitudes with numerical relativity simulations of binary black holes

Ssohrab Borhanian, K. G. Arun, Harald P. Pfeiffer +1

Gravitational waves from the coalescence of two black holes carry the signature of the strong field dynamics of binary black holes. In this work we have used numerical relativity s…

gr-qc2004★ 15 cited

New class of post-Newtonian approximants to the waveform templates of inspiralling compact binaries: Test-mass in the Schwarzschild spacetime

P. Ajith, Bala R. Iyer, C. A. K. Robinson +1

(Abridged): The standard adiabatic approximation to phasing of gravitational waves from inspiralling compact binaries uses the post-Newtonian expansions of the binding energy and g…

astro-ph1994★ 31 cited

Gravitational instability in the strongly nonlinear regime: A study of various approximations

B. S. Sathyaprakash, V. Sahni, D. Munshi +2

We study the development of gravitational instability in the strongly non-linear regime. For this purpose we use a number of statistical indicators such as filamentary statistics,…

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