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researcher

R. Penna

42 papers hereh-index 212.3k citations59 works total

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

author position
  • sole author17
  • first author8
  • middle author11
  • last author3

Across the 39 of 42 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE18
  • hep-th14
  • gr-qc5
  • astro-ph3
  • astro-ph.IM2
same name
  • R. Penna — 2 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
20042026
most citedGRMHD Simulations of Magnetized Advection Dominated Accretion on a Non-Spinning Black Hole: Role of Outflows

504 citations · 2.7k across the 41 of their papers we have counts for

collaborators
Showing 2015Show all

4 papers · 1 filter

hep-th2015★ 62 cited

BMS invariance and the membrane paradigm

Robert F. Penna

The Bondi-van der Burg-Metzner-Sachs (BMS) group is the asymptotic symmetry group of asymptotically flat spacetime. It is infinite dimensional and entails an infinite number of con…

gr-qc2015★ 19 cited

Strong-field tidal distortions of rotating black holes: II. Horizon dynamics from eccentric and inclined orbits

Stephen O'Sullivan, Scott A. Hughes

In a previous paper, we developed tools for studying the horizon geometry of a Kerr black hole that is tidally distorted by a binary companion using techniques that require large m…

astro-ph.HE2015★ 31 cited

Energy extraction from boosted black holes: Penrose process, jets, and the membrane at infinity

Robert F. Penna

Numerical simulations indicate that black holes carrying linear momentum and/or orbital momentum can power jets. The jets extract the kinetic energy stored in the black hole's moti…

astro-ph.HE2015★ 12 cited

Black hole jet power from impedance matching

Robert F. Penna

Black hole jet power depends on the angular velocity of magnetic field lines, ΩF​. Force-free black hole magnetospheres typically have ΩF​/ΩH​≈0.5, where ΩH​ is the a…

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