Dense nuclear matter equation of state from heavy-ion collisions
The nuclear equation of state (EOS) is at the center of numerous theoretical and
experimental efforts in nuclear physics. With advances in microscopic theories for nuclear …
experimental efforts in nuclear physics. With advances in microscopic theories for nuclear …
Neutron-star tidal deformability and equation-of-state constraints
K Chatziioannou - General Relativity and Gravitation, 2020 - Springer
Despite their long history and astrophysical importance, some of the key properties of
neutron stars are still uncertain. The extreme conditions encountered in their interiors …
neutron stars are still uncertain. The extreme conditions encountered in their interiors …
Population of merging compact binaries inferred using gravitational waves through GWTC-3
R Abbott, TD Abbott, F Acernese, K Ackley, C Adams… - Physical Review X, 2023 - APS
We report on the population properties of compact binary mergers inferred from gravitational-
wave observations of these systems during the first three LIGO-Virgo observing runs. The …
wave observations of these systems during the first three LIGO-Virgo observing runs. The …
[HTML][HTML] Observation of gravitational waves from two neutron star–black hole coalescences
R Abbott, TD Abbott, S Abraham… - The Astrophysical …, 2021 - iopscience.iop.org
The radius of PSR J0740+ 6620 from NICER and XMM-Newton data
MC Miller, FK Lamb, AJ Dittmann… - The Astrophysical …, 2021 - iopscience.iop.org
PSR J0740+ 6620 has a gravitational mass of 2.08±0.07 M⊙, which is the highest reliably
determined mass of any neutron star. As a result, a measurement of its radius will provide …
determined mass of any neutron star. As a result, a measurement of its radius will provide …
A NICER view of the massive pulsar PSR J0740+ 6620 informed by radio timing and XMM-Newton spectroscopy
We report on Bayesian estimation of the radius, mass, and hot surface regions of the
massive millisecond pulsar PSR J0740+ 6620, conditional on pulse-profile modeling of …
massive millisecond pulsar PSR J0740+ 6620, conditional on pulse-profile modeling of …
Constraints on the dense matter equation of state and neutron star properties from NICER's mass–radius estimate of PSR J0740+ 6620 and multimessenger …
G Raaijmakers, SK Greif, K Hebeler… - The Astrophysical …, 2021 - iopscience.iop.org
In recent years our understanding of the dense matter equation of state (EOS) of neutron
stars has significantly improved by analyzing multimessenger data from radio/X-ray pulsars …
stars has significantly improved by analyzing multimessenger data from radio/X-ray pulsars …
A horizon study for cosmic explorer: science, observatories, and community
This Horizon Study describes a next-generation ground-based gravitational-wave
observatory: Cosmic Explorer. With ten times the sensitivity of Advanced LIGO, Cosmic …
observatory: Cosmic Explorer. With ten times the sensitivity of Advanced LIGO, Cosmic …
[HTML][HTML] GW190814: Gravitational waves from the coalescence of a 23 solar mass black hole with a 2.6 solar mass compact object
R Abbott, TD Abbott, S Abraham… - The Astrophysical …, 2020 - iopscience.iop.org
Strongly interacting matter exhibits deconfined behavior in massive neutron stars
E Annala, T Gorda, J Hirvonen, O Komoltsev… - Nature …, 2023 - nature.com
Neutron-star cores contain matter at the highest densities in our Universe. This highly
compressed matter may undergo a phase transition where nuclear matter melts into …
compressed matter may undergo a phase transition where nuclear matter melts into …