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B. Owen

82 papers hereh-index 9547.1k citations399 works total

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

author position
  • sole author6
  • first author10
  • middle author23
  • last author21

Across the 60 of 82 papers where every author was matched, so the position is known.

fields
  • gr-qc43
  • hep-lat13
  • astro-ph10
  • astro-ph.HE6
  • astro-ph.IM4
  • astro-ph.SR4
same name
  • B. Owen — 16 papers, h 16
  • B. Owen — 1 paper, h 8
  • B. Owen — 1 paper, h 7
  • B. Owen — 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
19952025
most citedLIGO: The Laser Interferometer Gravitational-Wave Observatory

1.2k citations · 9.7k across the 81 of their papers we have counts for

collaborators
Showing 2005 · astro-phShow all

4 papers · 2 filters

astro-ph2005★ 90 cited

R-modes of accreting hyperon stars as persistent sources of gravitational waves

Mohit Nayyar, Benjamin J. Owen

The r-modes of accreting neutron stars could be a detectable source of persistent gravitational waves if the bulk viscosity of the stellar matter can prevent a thermal runaway. T…

astro-ph2005★ 110 cited

Upper Limits on a Stochastic Background of Gravitational Waves

LIGO Scientific Collaboration, B. Abbott

The Laser Interferometer Gravitational Wave Observatory (LIGO) has performed a third science run with much improved sensitivities of all three interferometers. We present an analys…

astro-ph2005★ 211 cited

Observational constraints on hyperons in neutron stars

Benjamin D. Lackey, Mohit Nayyar, Benjamin J. Owen

The possibility that neutron stars may contain substantial hyperon populations has important implications for neutron-star cooling and, through bulk viscosity, the viability of the…

astro-ph2005★ 237 cited

Maximum elastic deformations of compact stars with exotic equations of state

Benjamin J. Owen

I make the first estimates of maximum elastic quadrupole deformations sustainable by alternatives to conventional neutron stars. Solid strange quark stars might sustain maximum ell…

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