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R. Capuzzo-Dolcetta

117 papers hereh-index 282.7k citations170 works total

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

author position
  • sole author9
  • first author26
  • middle author30
  • last author28

Across the 93 of 117 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA40
  • astro-ph37
  • astro-ph.EP9
  • astro-ph.IM9
  • astro-ph.CO7
  • astro-ph.HE7
same name
  • R. Capuzzo-Dolcetta — 9 papers, h 4
  • R. Capuzzo-Dolcetta — 5 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
19932026
most citedDissipationless Formation and Evolution of the Milky Way Nuclear Star Cluster

204 citations · 2.4k across the 113 of their papers we have counts for

collaborators
Showing 1996Show all

4 papers · 1 filter

astro-ph1996

Force Evaluation in Particle Methods for Self-Gravitating Multi-Phase Systems

R. Capuzzo-Dolcetta, R. Di Lisio, P. Miocchi

A modern approach to the evolution of a mixed (stars and gas) self-gravitating system is the fully Lagrangian particle approach. The gaseous (particle) phase differs from the compa…

astro-ph1996

Can Galactic Nuclei Activity be Explained by Globular Cluster Mass Accretion?

Roberto Capuzzo-Dolcetta

Globular clusters can decay to the center of their mother galaxy carrying a quantity of mass sufficient to sustain the gravitational activity of a small pre-existing nucleus and to…

astro-ph1996

Force Error Optimization in Smooth Particle Hydrodynamics

R. Capuzzo-Dolcetta, R. Di Lisio

We discuss capability of Smooth Particle Hydrodynamics to represent adequately the dynamics of self-gravitating systems, in particular for what regards the quality of approximation…

astro-ph1996

The Evolution of Embedded Small Clusters

R. Capuzzo-Dolcetta, F. Sori

A young open cluster is a 2-phase system: an ensemble of stars move in a gaseous medium (the mother molecular cloud). The dynamics and thermodynamics of the system, and so its evol…

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