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researcher

M. Campanelli

66 papers hereh-index 00 citations0 works total

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

author position
  • first author10
  • middle author40
  • last author12

Across the 62 of 66 papers where every author was matched, so the position is known.

fields
  • gr-qc38
  • astro-ph.HE22
  • astro-ph.GA2
  • hep-ex2
  • physics.comp-ph1
  • physics.ed-ph1
same name
  • M. Campanelli — 181 papers
  • M. Campanelli — 177 papers, h 0
  • M. Campanelli — 150 papers
  • M. Campanelli — 141 papers, h 21
  • M. Campanelli — 127 papers
  • M. Campanelli — 47 papers, h 51

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
19952026
most citedThe Einstein Toolkit: A Community Computational Infrastructure for Relativistic Astrophysics

587 citations · 4.2k across the 66 of their papers we have counts for

collaborators
Showing 2016Show all

3 papers · 1 filter

astro-ph.HE2016★ 78 cited

Relativistic Dynamics and Mass Exchange in Binary Black Hole Mini-Disks

Dennis B. Bowen, Manuela Campanelli, Julian H. Krolik +2

We present the first exploration of relativistic gas dynamics in the immediate vicinity of binary black holes as the system inspirals close to merger in the gravitational radiation…

gr-qc2016★ 5 cited

Spinning, Precessing, Black Hole Binary Spacetime via Asymptotic Matching

Hiroyuki Nakano, Brennan Ireland, Manuela Campanelli +1

We briefly discuss a method to construct a global, analytic, approximate spacetime for precessing, spinning binary black holes. The spacetime construction is broken into three part…

gr-qc2016★ 85 cited

Modeling the source of GW150914 with targeted numerical-relativity simulations

Geoffrey Lovelace, Carlos O. Lousto, James Healy +11

In fall of 2015, the two LIGO detectors measured the gravitational wave signal GW150914, which originated from a pair of merging black holes. In the final 0.2 seconds (about 8 grav…

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