NewEvery arXiv paper, its researchers & institutions — mapped.
papers

Publications (14)

nucl-ex2010

Transition probabilities in the X(5) candidate $^{122}$Ba

P. G. Bizzeti, A. M. Bizzeti-Sona, D. Tonev +30

astro-ph.HE2019

Light-curve models of black hole - neutron star mergers: steps towards a multi-messenger parameter estimation

C. Barbieri, O. S. Salafia, A. Perego +2

gr-qc2019

All-sky search for short gravitational-wave bursts in the second Advanced LIGO and Advanced Virgo run

The LIGO Scientific Collaboration, the Virgo Collaboration, B. P. Abbott +1186

astro-ph.HE2009

Dual black holes in merger remnants. II: spin evolution and gravitational recoil

M. Dotti, M. Volonteri, A. Perego +3

astro-ph.SR2015

Pushing 1D CCSNe to explosions: model and SN 1987A

A. Perego, M. Hempel, C. Fröhlich +5

astro-ph.HE2014

MODA: a new algorithm to compute optical depths in multi-dimensional hydrodynamic simulations

A. Perego, E. Gafton, R. Cabezon +2

physics.ins-det2012

AGATA - Advanced Gamma Tracking Array

S. Akkoyun, A. Algora, B. Alikhani +351

gr-qc2018

GW170817: Measurements of Neutron Star Radii and Equation of State

The LIGO Scientific Collaboration, the Virgo Collaboration, B. P. Abbott +1149

astro-ph.CO2012

On the orientation and magnitude of the black hole spin in galactic nuclei

M. Dotti, M. Colpi, S. Pallini +2

astro-ph.HE2010

A path to radio-loudness through gas-poor galaxy mergers and the role of retrograde accretion

M. Dotti, M. Colpi, L. Maraschi +2

astro-ph.CO2009

Mass and spin coevolution during the alignment of a black hole in a warped accretion disc

A. Perego, M. Dotti, M. Colpi +1

astro-ph.HE2019

Compact radio emission indicates a structured jet was produced by a binary neutron star merger

G. Ghirlanda, O. S. Salafia, Z. Paragi +33

astro-ph.HE2017

The role of weak interactions in dynamic ejecta from binary neutron star mergers

D. Martin, A. Perego, W. Kastaun +1

astro-ph.HE2012

Neutrino processes in partially degenerate neutron matter

S. Bacca, K. Hally, M. Liebendörfer +3