activity
20132026
most citedVery massive stars, pair-instability supernovae and intermediate-mass black holes with the SEVN code

344 citations · 1.8k across the 27 of their papers we have counts for

collaborators
Showing 2020Show all

11 papers · 1 filter

gr-qc202071 cited

All-sky search in early O3 LIGO data for continuous gravitational-wave signals from unknown neutron stars in binary systems

The LIGO Scientific Collaboration, the Virgo Collaboration, R. Abbott +1369

Rapidly spinning neutron stars are promising sources of persistent, continuous gravitational waves. Detecting such a signal would allow probing of the physical properties of matter…

astro-ph.GA202022 cited

From hydrodynamics to N-body simulations of star clusters: mergers and rotation

Alessandro Ballone, Stefano Torniamenti, Michela Mapelli +5

We present a new method to obtain more realistic initial conditions for N-body simulations of young star clusters. We start from the outputs of hydrodynamical simulations of molecu…

astro-ph.SR2020

Formation of GW190521 from stellar evolution: the impact of the hydrogen-rich envelope, dredge-up and C(, )O rate on the pair-instability black hole mass gap

Guglielmo Costa, Alessandro Bressan, Michela Mapelli +3

Pair-instability (PI) is expected to open a gap in the mass spectrum of black holes (BHs) between M and M. The existence of the mass…

astro-ph.EP2020

The ominous fate of exomoons around hot Jupiters in the high-eccentricity migration scenario

Alessandro A. Trani, Adrian S. Hamers, Aaron Geller +1

All the giant planets in the solar system host a large number of natural satellites. Moons in extrasolar systems are difficult to detect, but a Neptune-sized exomoon candidate has…

astro-ph.HE2020137 cited

Exploring the Lower Mass Gap and Unequal Mass Regime in Compact Binary Evolution

Michael Zevin, Mario Spera, Christopher P. L. Berry +1

On August 14, 2019, the LIGO and Virgo detectors observed GW190814, a gravitational-wave signal originating from the merger of a black hole with a $\simeq 2.6 M…

astro-ph.HE2020

Populating the upper black hole mass gap through stellar collisions in young star clusters

Kyle Kremer, Mario Spera, Devin Becker +6

Theoretical modeling of massive stars predicts a gap in the black hole (BH) mass function above for BHs formed through single star evolution, arising from (…