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Collinear Jahn-Teller Ordering Induces Monoclinic Distortion in "Defect-Free" LiNiO<sub>2</sub>. [PDF]

open access: yesJ Am Chem Soc
Phillips GS   +12 more
europepmc   +1 more source

Enhanced production of 60Fe in massive stars. [PDF]

open access: yesNat Commun
Spyrou A   +25 more
europepmc   +1 more source

Kilonova simulations: connecting observations with the underlying physics. [PDF]

open access: yesPhilos Trans A Math Phys Eng Sci
Collins C, Shingles L, Vijayan V.
europepmc   +1 more source
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Neutron Stars

, 2022
Neutron stars are highly compact astrophysical objects and therefore of utmost relevance to learn about theories of gravity. Whereas the proper equation of state of the nuclear matter inside neutron stars is not yet known, and a wide range of equations ...
J. Kunz
semanticscholar   +2 more sources

Neutron star crusts

Physical Review Letters, 1993
We calculate properties of neutron star matter at subnuclear densities using an improved nuclear Hamiltonian. Nuclei disappear and the matter becomes uniform at a density of about 0.6n(s), where n(s) of about 0.16/cu fm is the saturation density of nuclear matter. As a consequence, the mass of matter in the crusts of neutron stars is only about half as
, Lorenz, , Ravenhall, , Pethick
openaire   +2 more sources

Neutron star matter

Nuclear Physics A, 1971
Abstract The matter in neutron stars is essentially in its ground state and ranges in density up to and beyond 3 × 10 14 g/cm 3 , the density of nuclear matter. Here we determine the constitution of the ground state of matter and its equation of state in the regime from 4.3 × 10 11 g/cm 3 where free neutrons begin to “drip” out of the nuclei, up ...
GORDON BAYM   +2 more
openaire   +1 more source

Identification of strontium in the merger of two neutron stars

Nature, 2019
Half of all of the elements in the Universe that are heavier than iron were created by rapid neutron capture. The theory underlying this astrophysical r-process was worked out six decades ago, and requires an enormous neutron flux to make the bulk of the
D. Watson   +17 more
semanticscholar   +1 more source

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