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C. Rodriguez

70 papers hereh-index 509k citations111 works total

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

author position
  • sole author1
  • first author16
  • middle author44
  • last author8

Across the 69 of 70 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE37
  • astro-ph.GA20
  • astro-ph.SR5
  • astro-ph.IM3
  • gr-qc3
  • astro-ph.CO2
same name
  • C. Rodriguez — 6 papers, h 3
  • C. Rodriguez — 5 papers, h 5
  • C. Rodriguez — 5 papers, h 2
  • C. Rodriguez — 3 papers, h 3
  • C. Rodriguez — 2 papers, h 2
  • C. Rodriguez — 2 papers, h 2

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
20112023
most citedBinary Black Hole Mergers from Globular Clusters: Masses, Merger Rates, and the Impact of Stellar Evolution

581 citations · 8k across the 70 of their papers we have counts for

collaborators
Showing 2015Show all

3 papers · 1 filter

astro-ph.IM2015★ 15 cited

A New Hybrid Technique for Modeling Dense Star Clusters

Carl L. Rodriguez, Bharath Pattabiraman, Sourav Chatterjee +4

The "gravitational million-body problem," to model the dynamical evolution of a self-gravitating, collisional N-body system with ~10^6 particles over many relaxation times, remains…

astro-ph.GA2015★ 228 cited

Black hole mergers and blue stragglers from hierarchical triples formed in globular clusters

Fabio Antonini, Sourav Chatterjee, Carl L. Rodriguez +4

Hierarchical triple-star systems are expected to form frequently via close binary-binary encounters in the dense cores of globular clusters. In a sufficiently inclined triple, grav…

astro-ph.HE2015★ 411 cited

Binary Black Hole Mergers from Globular Clusters: Implications for Advanced LIGO

Carl L. Rodriguez, Meagan Morscher, Bharath Pattabiraman +3

The predicted rate of binary black hole mergers from galactic fields can vary over several orders of magnitude and is extremely sensitive to the assumptions of stellar evolution. B…

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