The physics of fast radio bursts

B Zhang - Reviews of Modern Physics, 2023 - APS
Fast radio bursts (FRBs), millisecond-duration bursts prevailing in the radio sky, are the
latest large puzzle in the Universe and have been a subject of intense observational and …

The dynamics of binary neutron star mergers and GW170817

D Radice, S Bernuzzi, A Perego - Annual Review of Nuclear …, 2020 - annualreviews.org
With the first observation of a binary neutron star merger through gravitational waves and
light, GW170817, compact binary mergers have now taken the center stage in nuclear …

Using gravitational-wave observations and quasi-universal relations to constrain the maximum mass of neutron stars

L Rezzolla, ER Most, LR Weih - The Astrophysical Journal …, 2018 - iopscience.iop.org
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 …

Constraining the maximum mass of neutron stars from multi-messenger observations of GW170817

B Margalit, BD Metzger - The Astrophysical Journal Letters, 2017 - iopscience.iop.org
Constraining the Maximum Mass of Neutron Stars from Multi-messenger Observations of
GW170817 - IOPscience This site uses cookies. By continuing to use this site you agree to our …

The THESEUS space mission concept: science case, design and expected performances

L Amati, P O'Brien, D Götz, E Bozzo, C Tenzer… - Advances in Space …, 2018 - Elsevier
THESEUS is a space mission concept aimed at exploiting Gamma-Ray Bursts for
investigating the early Universe and at providing a substantial advancement of multi …

Maximum mass, moment of inertia and compactness of relativistic stars

C Breu, L Rezzolla - Monthly Notices of the Royal Astronomical …, 2016 - academic.oup.com
A number of recent works have highlighted that it is possible to express the properties of
general-relativistic stellar equilibrium configurations in terms of functions that do not depend …

A luminous precursor in the extremely bright GRB 230307A

S Dichiara, D Tsang, E Troja, D Neill… - The Astrophysical …, 2023 - iopscience.iop.org
GRB 230307A is an extremely bright long-duration GRB with an observed gamma-ray
fluence of≳ 3× 10− 3 erg cm− 2 (10–1000 keV), second only to GRB 221009A. Despite its …

The evolution of binary neutron star post-merger remnants: a review

N Sarin, PD Lasky - General Relativity and Gravitation, 2021 - Springer
Two neutron stars merge somewhere in the Universe approximately every 10 to 100 s,
creating violent explosions potentially observable in gravitational waves and across the …

The gravitational-wave physics II: Progress

L Bian, RG Cai, S Cao, Z Cao, H Gao, ZK Guo… - Science China Physics …, 2021 - Springer
It has been a half-decade since the first direct detection of gravitational waves, which
signifies the coming of the era of the gravitational-wave astronomy and gravitational-wave …

Equation of state constraints from the threshold binary mass for prompt collapse of neutron star mergers

A Bauswein, S Blacker, V Vijayan, N Stergioulas… - Physical Review Letters, 2020 - APS
Using hydrodynamical simulations for a large set of high-density matter equations of state
(EOSs), we systematically determine the threshold mass M thres for prompt black-hole …