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P. Duffell

15 papers hereh-index 263.4k citations58 works total

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

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

Across the 14 of 15 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE9
  • astro-ph.SR3
  • astro-ph.EP2
  • astro-ph.IM1
same name
  • P. Duffell — 23 papers, h 7

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
20152023
most citedThe Effect of Jet-Ejecta Interaction on the Viewing Angle Dependence of Kilonova Light Curves

32 citations · 34 across the 3 of their papers we have counts for

collaborators
Showing 2019Show all

4 papers · 1 filter

astro-ph.SR2019

Circumbinary Disks: Accretion and Torque as a Function of Mass Ratio and Disk Viscosity

Paul C. Duffell, Daniel D'Orazio, Andrea Derdzinski +4

Using numerical hydrodynamics calculations and a novel method for densely sampling parameter space, we measure the accretion and torque on a binary system from a circumbinary disk.…

astro-ph.HE2019

How Dense a CSM is Sufficient to Choke a Jet?

Paul C. Duffell, Anna Y. Q. Ho

The progenitor stars of stripped-envelope high-velocity supernovae (Ic-BL SNe) can explode inside a dense circumstellar medium (CSM) that extends out to many times the progenitor r…

astro-ph.EP2019

An empirically-derived formula for the shape of planet-induced gaps in protoplanetary disks

Paul C. Duffell

This study uses numerical hydrodynamics calculations and a novel method for densely sampling parameter space to measure the precise shape of a gap opened by a planet in a gaseous d…

astro-ph.HE2019

ALMA Detection of a Linearly Polarized Reverse Shock in GRB 190114C

Tanmoy Laskar, Kate D. Alexander, Ramandeep Gill +11

We present ALMA 97.5 GHz total intensity and linear polarization observations of the mm-band afterglow of GRB 190114C spanning 2.2 to 5.2 hours after the burst. We detect linear po…

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