6 citations · 8 across the 3 of their papers we have counts for
6 papers · 1 filter
The impact of nuclear equations of state on the dynamics and multi-messenger emission of magnetorotational stellar explosions
Andrea Celati, Matteo Bugli, Luca Del Zanna +2
The gravitational collapse of massive stars at the end of their life leads to powerful supernova explosions that produce compact objects, regulate the dynamics of host galaxies, an…
Impact of the equation of state on core collapse supernovae I: the low- instability
Marco Cusinato, Martin Obergaulinger, Miguel Ángel Aloy
Rapidly rotating core-collapse supernovae are promising sources of multimessenger emission, as non-axisymmetric dynamics in the newly formed proto-neutron star can leave characteri…
Convection signatures in early-time gravitational waves from core-collapse supernovae
Marco Cusinato, Martin Obergaulinger, Miguel-Ángel Aloy
Gravitational waves emitted from core-collapse supernova explosions are critical observables for extracting information about the dynamics and properties of both the progenitor and…
Resonant amplification of multimessenger emission in rotating stellar core collapse
Marco Cusinato, Martin Obergaulinger, Miguel-Ángel Aloy +1
In a series of axisymmetric core-collapse supernova simulations extending up to , we identify a regime of pre-collapse central rotation rates ($\sim 1\,\mathrm{…
Efficient Stochastic Template Bank using Inner Product Inequalities
Keisi Kacanja, Alexander H. Nitz, Shichao Wu +5
Gravitational wave searches are crucial for studying compact sources like neutron stars and black holes. Many sensitive modeled searches use matched filtering to compare gravitatio…
Search for Eccentric Black Hole Coalescences during the Third Observing Run of LIGO and Virgo
The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1772
Despite the growing number of confident binary black hole coalescences observed through gravitational waves so far, the astrophysical origin of these binaries remains uncertain. Or…