Equations of state for supernovae and compact stars
M Oertel, M Hempel, T Klähn, S Typel - Reviews of Modern Physics, 2017 - APS
A review is given of various theoretical approaches for the equation of state (EoS) of dense
matter, relevant for the description of core-collapse supernovae, compact stars, and compact …
matter, relevant for the description of core-collapse supernovae, compact stars, and compact …
Quantum Monte Carlo methods for nuclear physics
Quantum Monte Carlo methods have proved valuable to study the structure and reactions of
light nuclei and nucleonic matter starting from realistic nuclear interactions and currents …
light nuclei and nucleonic matter starting from realistic nuclear interactions and currents …
Neutron and weak-charge distributions of the 48Ca nucleus
What is the size of the atomic nucleus? This deceivably simple question is difficult to answer.
Although the electric charge distributions in atomic nuclei were measured accurately already …
Although the electric charge distributions in atomic nuclei were measured accurately already …
Future of nuclear fission theory
There has been much recent interest in nuclear fission, due in part to a new appreciation of
its relevance to astrophysics, stability of superheavy elements, and fundamental theory of …
its relevance to astrophysics, stability of superheavy elements, and fundamental theory of …
Evidence of hexadecapole deformation in uranium-238 at the relativistic heavy ion collider
State-of-the-art hydrodynamic simulations of the quark-gluon plasma are unable to
reproduce the elliptic flow of particles observed at the BNL Relativistic Heavy Ion Collider …
reproduce the elliptic flow of particles observed at the BNL Relativistic Heavy Ion Collider …
Combining electromagnetic and gravitational-wave constraints on neutron-star masses and radii
We perform a joint Bayesian inference of neutron-star mass and radius constraints based on
GW170817, observations of quiescent low-mass x-ray binaries (QLMXBs), photospheric …
GW170817, observations of quiescent low-mass x-ray binaries (QLMXBs), photospheric …
Bayesian approach to model-based extrapolation of nuclear observables
Background: The mass, or binding energy, is the basis property of the atomic nucleus. It
determines its stability and reaction and decay rates. Quantifying the nuclear binding is …
determines its stability and reaction and decay rates. Quantifying the nuclear binding is …
Neutron drip line in the Ca region from Bayesian model averaging
The region of heavy calcium isotopes forms the frontier of experimental and theoretical
nuclear structure research where the basic concepts of nuclear physics are put to stringent …
nuclear structure research where the basic concepts of nuclear physics are put to stringent …
Sound velocity bound and neutron stars
P Bedaque, AW Steiner - Physical review letters, 2015 - APS
It has been conjectured that the velocity of sound in any medium is smaller than the velocity
of light in vacuum divided by 3. Simple arguments support this bound in nonrelativistic …
of light in vacuum divided by 3. Simple arguments support this bound in nonrelativistic …
Three-nucleon forces: Implementation and applications to atomic nuclei and dense matter
K Hebeler - Physics Reports, 2021 - Elsevier
Recent advances in nuclear structure theory have significantly enlarged the accessible part
of the nuclear landscape via ab initio many-body calculations. These developments open …
of the nuclear landscape via ab initio many-body calculations. These developments open …