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Prayush Kumar

37 papers hereh-index 192.7k citations57 works total

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

author position
  • sole author1
  • first author5
  • middle author29
  • last author2

Across the 37 of 37 papers where every author was matched, so the position is known.

fields
  • gr-qc36
  • astro-ph.HE1
same name
  • Prayush Kumar — 9 papers, h 2
  • Prayush Kumar — 7 papers, h 24
  • Prayush Kumar — 5 papers
  • Prayush Kumar — 3 papers
  • Prayush Kumar — 2 papers
  • Prayush Kumar — 1 paper, h 1

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
20122025
most citedAn improved effective-one-body model of spinning, nonprecessing binary black holes for the era of gravitational-wave astrophysics with advanced detectors

615 citations · 2.6k across the 37 of their papers we have counts for

collaborators
Showing 2012 · gr-qcShow all

3 papers · 2 filters

gr-qc2012★ 64 cited

Template banks to search for low-mass binary black holes in advanced gravitational-wave detectors

Duncan A. Brown, Prayush Kumar, Alexander H. Nitz

Coalescing binary black holes (BBHs) are among the most likely sources for the Laser Interferometer Gravitational-wave Observatory (LIGO) and its international partners Virgo and K…

gr-qc2012

Search for the PN coefficients for the Energy flux through Gravitational Waves from Black-Hole Binaries using Markov Chain Monte Carlo

Prayush Kumar

In this work, the focus is on the improvement of the existing post-Newtonian approximation for the gravitational flux from Super Massive Black Hole Binaries. In order to improve th…

gr-qc2012★ 12 cited

Accurate modeling of intermediate-mass-ratio inspirals: Exploring the form of the self-force in the intermediate-mass-ratio regime

E. A. Huerta, Prayush Kumar, Duncan A. Brown

In this paper we develop a waveform model that accurately reproduces the dynamical evolution of intermediate-mass-ratio inspirals, as predicted by the effective-one-body (EOB) mode…

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