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researcher

P. Taylor

4 papers hereh-index 232.2k citations180 works total

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

author position
  • first author2
  • middle author1
  • last author1

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE2
  • astro-ph1
  • astro-ph.IM1
same name
  • P. Taylor — 20 papers, h 26
  • P. Taylor — 20 papers, h 12
  • P. Taylor — 18 papers, h 22
  • P. Taylor — 17 papers, h 10
  • P. Taylor — 15 papers, h 13
  • P. Taylor — 12 papers, h 5

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
20032012
most citedLong duration gamma-ray bursts: hydrodynamic instabilities in collapsar disks

29 citations · 62 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.HE2012★ 22 cited

An analytic toy model for relativistic accretion in Kerr spacetime

Emilio Tejeda, Paul A. Taylor, John C. Miller

We present a relativistic model for the stationary axisymmetric accretion flow of a rotating cloud of non-interacting particles falling onto a Kerr black hole. Based on a ballistic…

astro-ph.IM2011★ 10 cited

Measuring the Effects of Artificial Viscosity in SPH Simulations of Rotating Fluid Flows

Paul A. Taylor, John C. Miller

A commonly cited drawback of SPH is the introduction of spurious shear viscosity by the artificial viscosity term in situations involving rotation. Existing approaches for quantify…

astro-ph.HE2010★ 29 cited

Long duration gamma-ray bursts: hydrodynamic instabilities in collapsar disks

Paul A. Taylor, John C. Miller, Philipp Podsiadlowski

We present 3D numerical simulations of the early evolution of long-duration gamma-ray bursts in the collapsar scenario. Starting from the core-collapse of a realistic progenitor mo…

astro-ph2003★ 1 cited

Migration of Asteroidal Dust

S. I. Ipatov, J. C. Mather, P. A. Taylor

We numerically investigate the migration of dust particles with initial orbits close to those of the numbered asteroids. The fraction of silicate particles that collided with the E…

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