activity
19942026
most citedInstability of a stalled accretion shock: evidence for the advective-acoustic cycle

264 citations · 1.9k across the 40 of their papers we have counts for

collaborators

40 papers

astro-ph.HE2026

Analytic insight into the physics of SASI II. Spiral instability of the prograde mode in a rotating stellar core

T. Foglizzo

During the core-collapse of a rotating massive star, the standing accretion shock instability (SASI) favours the development of non-axisymmetric motions which can imprint specific…

astro-ph.HE2024

Analytic insight into the physics of SASI I. Shock instability in a non-rotating stellar core

T. Foglizzo

During the core collapse of a massive star just before its supernova explosion, the amplification of asymmetric motions by the standing accretion shock instability (SASI) imprints…

astro-ph.SR2024

Convective vortices in collapsing stars

Yerassyl Telman, Ernazar Abdikamalov, Thierry Foglizzo

Recent studies show that non-radial structures arising from massive star shell convection play an important role in shaping core-collapse supernova explosions. During the collapse…

astro-ph.HE2023

Prospects for realtime characterization of core-collapse supernova and neutrino properties

Meriem Bendahman, Isabel Goos, Joao Coelho +9

Core-collapse supernovae (CCSNe) offer extremely valuable insights into the dynamics of galaxies. Neutrino time profiles from CCSNe, in particular, could reveal unique details abou…

astro-ph.HE2023★ 9 cited

Detectability of Late-time Supernova Neutrinos with Fallback Accretion onto Protoneutron star

Ryuichiro Akaho, Hiroki Nagakura, Thierry Foglizzo

We investigate the late-time neutrino emission powered by fallback mass accretion onto proto-neutron star (PNS), using neutrino radiation-hydrodynamic simulations with full Boltzma…

astro-ph.HE2023★ 17 cited

Effect of stellar rotation on the development of post-shock instabilities during core-collapse supernovae

A. -C. Buellet, T. Foglizzo, J. Guilet +1

The growth of instabilities is key to trigger a supernova explosion during the phase of stalled shock, immediately after the birth of a proto-neutron star (PNS). We assess the effe…