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Ugo N Di Carlo

3 papers here

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

author position
  • middle author2
  • last author1

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA2
  • astro-ph.SR1
ORCID 0000-0003-2654-5239

identity via Semantic Scholar / OpenAlex

most citedDynamics of intermediate mass black holes in globular clusters. Wander radius and anisotropy profiles

7 citations · 8 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.GA2024

MAGICS II. Seed black holes stripped of their surrounding stars do not sink

Yihao Zhou, Diptajyoti Mukherjee, Nianyi Chen +7

MBH seed mergers are expected to be among the loudest sources of gravitational waves detected by the Laser Interferometer Space Antenna (LISA), providing a unique window into the b…

astro-ph.SR2023★ 1 cited

Dynamical formation of Gaia BH1 in a young star cluster

Sara Rastello, Giuliano Iorio, Michela Mapelli +5

Gaia BH1, the first quiescent black hole (BH) detected from Gaia data, poses a challenge to most binary evolution models: its current mass ratio is ≈0.1, and its orbi…

astro-ph.GA2023★ 7 cited

Dynamics of intermediate mass black holes in globular clusters. Wander radius and anisotropy profiles

Pierfrancesco Di Cintio, Mario Pasquato, Luca Barbieri +2

We recently introduced a new method for simulating collisional gravitational N-body systems with approximately linear time scaling with N, based on the Multi-Particle Collision (…

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