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L. Paiella

11 papers hereh-index 14922 citations40 works total

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

author position
  • first author2
  • middle author9

Across the 11 of 11 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA5
  • astro-ph.IM3
  • astro-ph.HE2
  • gr-qc1
same name
  • L. Paiella — 7 papers
  • L. Paiella — 3 papers
  • L. Paiella — 1 paper
  • L. Paiella — 1 paper
  • L. Paiella — 1 paper
  • L. Paiella — 1 paper

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
20232026
most citedOpportunities and limits of lunar gravitational-wave detection

15 citations · 24 across the 10 of their papers we have counts for

collaborators
Showing 2025 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2025★ 6 cited

Seeds to success: growing heavy black holes in dense star clusters

Lavinia Paiella, Manuel Arca Sedda, Benedetta Mestichelli +1

The observational dearth of black holes (BHs) with masses between ∼100 and 100,000 M⊙​ raises questions about the nature of intermediate-mass black holes (IMBHs). Propos…

astro-ph.GA2025

Assembling GW231123 in star clusters through the combination of stellar binary evolution and hierarchical mergers

Lavinia Paiella, Cristiano Ugolini, Mario Spera +2

GW231123 is the most massive binary black hole (BBH) merger detected to date by the LIGO-Virgo-KAGRA collaboration. With at least one black hole (BH) in the upper-mass gap and both…

astro-ph.GA2025★ 1 cited

Black Hole - Neutron Star and Binary Neutron Star Mergers from Population III and II stars

Benedetta Mestichelli, Michela Mapelli, Filippo Santoliquido +9

Population III (Pop. III) stars are expected to be massive and to undergo minimal mass loss due to their lack of metals, making them ideal progenitors of black holes and neutron…

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