Transport model comparison studies of intermediate-energy heavy-ion collisions
Transport models are the main method to obtain physics information on the nuclear equation
of state and in-medium properties of particles from low to relativistic-energy heavy-ion …
of state and in-medium properties of particles from low to relativistic-energy heavy-ion …
Searches for continuous-wave gravitational radiation
K Riles - Living Reviews in Relativity, 2023 - Springer
Now that detection of gravitational-wave signals from the coalescence of extra-galactic
compact binary star mergers has become nearly routine, it is intriguing to consider other …
compact binary star mergers has become nearly routine, it is intriguing to consider other …
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 …
Refined mass and geometric measurements of the high-mass PSR J0740+ 6620
We report results from continued timing observations of PSR J0740+ 6620, a high-mass, 2.8
ms radio pulsar in orbit with a likely ultracool white dwarf companion. Our data set consists …
ms radio pulsar in orbit with a likely ultracool white dwarf companion. Our data set consists …
[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
A NICER view of PSR J0030+ 0451: millisecond pulsar parameter estimation
We report on Bayesian parameter estimation of the mass and equatorial radius of the
millisecond pulsar PSR J0030+ 0451, conditional on pulse-profile modeling of Neutron Star …
millisecond pulsar PSR J0030+ 0451, conditional on pulse-profile modeling of Neutron Star …
PSR J0030+ 0451 mass and radius from NICER data and implications for the properties of neutron star matter
MC Miller, FK Lamb, AJ Dittmann… - The Astrophysical …, 2019 - iopscience.iop.org
Neutron stars are not only of astrophysical interest, but are also of great interest to nuclear
physicists because their attributes can be used to determine the properties of the dense …
physicists because their attributes can be used to determine the properties of the dense …
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 nicer view of the nearest and brightest millisecond pulsar: Psr j0437–4715
We report Bayesian inference of the mass, radius, and hot X-ray emitting region properties—
using data from the Neutron Star Interior Composition ExploreR (NICER)—for the brightest …
using data from the Neutron Star Interior Composition ExploreR (NICER)—for the brightest …
Discovery of a radio-emitting neutron star with an ultra-long spin period of 76 s
The radio-emitting neutron star population encompasses objects with spin periods ranging
from milliseconds to tens of seconds. As they age and spin more slowly, their radio emission …
from milliseconds to tens of seconds. As they age and spin more slowly, their radio emission …