Colloquium: Machine learning in nuclear physics
Advances in machine learning methods provide tools that have broad applicability in
scientific research. These techniques are being applied across the diversity of nuclear …
scientific research. These techniques are being applied across the diversity of nuclear …
Neutron stars and the nuclear matter equation of state
JM Lattimer - Annual Review of Nuclear and Particle Science, 2021 - annualreviews.org
Neutron stars provide a window into the properties of dense nuclear matter. Several recent
observational and theoretical developments provide powerful constraints on their structure …
observational and theoretical developments provide powerful constraints on their structure …
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 …
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 …
Origin of the heaviest elements: The rapid neutron-capture process
JJ Cowan, C Sneden, JE Lawler, A Aprahamian… - Reviews of Modern …, 2021 - APS
The production of about half of the heavy elements found in nature is assigned to a specific
astrophysical nucleosynthesis process: the rapid neutron-capture process (r process) …
astrophysical nucleosynthesis process: the rapid neutron-capture process (r process) …
Multimessenger constraints on the neutron-star equation of state and the Hubble constant
Observations of neutron-star mergers with distinct messengers, including gravitational
waves and electromagnetic signals, can be used to study the behavior of matter denser than …
waves and electromagnetic signals, can be used to study the behavior of matter denser than …
On the sound speed in neutron stars
Determining the sound speed cs in compact stars is an important open question with
numerous implications on the behavior of matter at large densities and hence on …
numerous implications on the behavior of matter at large densities and hence on …
Strongly interacting matter exhibits deconfined behavior in massive neutron stars
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 …
How perturbative QCD constrains the equation of state at neutron-star densities
We demonstrate in a general and analytic way how high-density information about the
equation of state (EOS) of strongly interacting matter obtained using perturbative quantum …
equation of state (EOS) of strongly interacting matter obtained using perturbative quantum …
Multimessenger constraints for ultradense matter
Recent rapid progress in neutron-star (NS) observations offers great potential to constrain
the properties of strongly interacting matter under the most extreme conditions. In order to …
the properties of strongly interacting matter under the most extreme conditions. In order to …