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 …
Astrophysics with the laser interferometer space antenna
Abstract The Laser Interferometer Space Antenna (LISA) will be a transformative experiment
for gravitational wave astronomy, and, as such, it will offer unique opportunities to address …
for gravitational wave astronomy, and, as such, it will offer unique opportunities to address …
Precision Determination of the Neutral Weak Form Factor of
We report a precise measurement of the parity-violating (PV) asymmetry A PV in the elastic
scattering of longitudinally polarized electrons from Ca 48. We measure A PV= 2668±106 …
scattering of longitudinally polarized electrons from Ca 48. We measure A PV= 2668±106 …
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 …
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 …
Accurate Determination of the Neutron Skin Thickness of through Parity-Violation in Electron Scattering
We report a precision measurement of the parity-violating asymmetry A PV in the elastic
scattering of longitudinally polarized electrons from Pb 208. We measure A PV= 550±16 …
scattering of longitudinally polarized electrons from Pb 208. We measure A PV= 550±16 …
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 …
Pulsar magnetospheres and their radiation
The discovery of pulsars opened a new research field that allows studying a wide range of
physics under extreme conditions. More than 3,000 pulsars are currently known, including …
physics under extreme conditions. More than 3,000 pulsars are currently known, including …
Implications of PREX-2 on the equation of state of neutron-rich matter
Laboratory experiments sensitive to the equation of state of neutron rich matter in the vicinity
of nuclear saturation density provide the first rung in a “density ladder” that connects …
of nuclear saturation density provide the first rung in a “density ladder” that connects …