Using gravitational-wave observations and quasi-universal relations to constrain the maximum mass of neutron stars
Combining the GW observations of merging systems of binary neutron stars and quasi-
universal relations, we set constraints on the maximum mass that can be attained by …
universal relations, we set constraints on the maximum mass that can be attained by …
Gravitational-wave signature of core-collapse supernovae
D Vartanyan, A Burrows, T Wang, MSB Coleman… - Physical Review D, 2023 - APS
We calculate the gravitational-wave (GW) signatures of detailed three-dimensional (3D) core-
collapse supernova simulations spanning a range of massive stars. Most of the simulations …
collapse supernova simulations spanning a range of massive stars. Most of the simulations …
Core collapse supernova gravitational wave emission for progenitors of 9.6, 15, and
A Mezzacappa, P Marronetti, RE Landfield, EJ Lentz… - Physical Review D, 2023 - APS
We present gravitational wave emission predictions based on three core collapse
supernova simulations corresponding to three different progenitor masses. The masses …
supernova simulations corresponding to three different progenitor masses. The masses …
The next generation global gravitational wave observatory: the science book
V Kalogera, BS Sathyaprakash, M Bailes… - arXiv preprint arXiv …, 2021 - arxiv.org
The next generation of ground-based gravitational-wave detectors will observe
coalescences of black holes and neutron stars throughout the cosmos, thousands of them …
coalescences of black holes and neutron stars throughout the cosmos, thousands of them …
Nuclear reactions in astrophysics: a review of useful probes for extracting reaction rates
Astrophysical simulations require knowledge of a wide array of reaction rates. For a number
of reasons, many of these reaction rates cannot be measured directly and instead are …
of reasons, many of these reaction rates cannot be measured directly and instead are …
The gravitational wave signal from core-collapse supernovae
V Morozova, D Radice, A Burrows… - The Astrophysical …, 2018 - iopscience.iop.org
We study gravitational waves (GWs) from a set of 2D multigroup neutrino radiation
hydrodynamic simulations of core-collapse supernovae (CCSNe). Our goal is to systematize …
hydrodynamic simulations of core-collapse supernovae (CCSNe). Our goal is to systematize …
Detecting and reconstructing gravitational waves from the next galactic core-collapse supernova in the advanced detector era
We performed a detailed analysis of the detectability of a wide range of gravitational waves
derived from core-collapse supernova simulations using gravitational-wave detector noise …
derived from core-collapse supernova simulations using gravitational-wave detector noise …
Three dimensional magnetorotational core-collapse supernova explosions of a 39 solar mass progenitor star
We perform three-dimensional simulations of magnetorotational supernovae using a
progenitor star with two different initial magnetic field strengths of 1010 and 1012 G in the …
progenitor star with two different initial magnetic field strengths of 1010 and 1012 G in the …
Three-dimensional core-collapse supernova simulations of massive and rotating progenitors
We present 3D simulations of the core-collapse of massive rotating and non-rotating
progenitors performed with the general relativistic neutrino hydrodynamics code coconut …
progenitors performed with the general relativistic neutrino hydrodynamics code coconut …
Gravitational wave emission from 3D explosion models of core-collapse supernovae with low and normal explosion energies
Understanding gravitational wave emission from core-collapse supernovae will be essential
for their detection with current and future gravitational wave detectors. This requires a …
for their detection with current and future gravitational wave detectors. This requires a …