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Evolution of Neutron Stars and Observational Constraints
The structure and evolution of neutron stars is discussed with a view towards constraining the properties of high density matter through observations.
Lattimer J.
doaj +1 more source
Radii of neutron drops probed via the neutron skin thickness of nuclei [PDF]
Multi-neutron systems are crucial to understanding the physics of neutron-rich nuclei and neutron stars. Neutron drops, neutrons confined in an external field, are investigated systematically in both non-relativistic and relativistic density functional theories and with ab initio calculations.
arxiv +1 more source
The cosmic merger rate of neutron stars and black holes [PDF]
Six gravitational wave detections have been reported so far, providing crucial insights on the merger rate of double compact objects. We investigate the cosmic merger rate of double neutron stars (DNSs), neutron star-black hole binaries (NSBHs) and black
M. Mapelli, N. Giacobbo
semanticscholar +1 more source
Neutrostriction in Neutron Stars [PDF]
It is demonstrated that not only gravity, but also neutrostriction forces due to optical potential created by coherent elastic neutron-neutron scattering can hold a neutron star together. The latter forces can be stronger than gravitational ones. The effect of these forces on mass, radius and structure of the neutron star is estimated.
openaire +3 more sources
Fallback supernova assembly of heavy binary neutron stars and light black hole-neutron star pairs and the common stellar ancestry of GW190425 and GW200115 [PDF]
The detection of the unusually heavy binary neutron star merger GW190425 marked a stark contrast to the mass distribution from known Galactic pulsars in double neutron star binaries and gravitational-wave source GW170817. We suggest here a formation channel for heavy binary neutron stars and light black hole - neutron star binaries in which massive ...
arxiv +1 more source
On the minimum mass of neutron stars [PDF]
We investigate remnant neutron star masses (in particular, the minimum allowed mass) by performing advanced stellar evolution calculations and neutrino-radiation hydrodynamics simulations for core-collapse supernova explosions.
Y. Suwa+4 more
semanticscholar +1 more source
Dark halos around neutron stars and gravitational waves [PDF]
We find that models of MeV-GeV dark matter in which dark matter interacts strongly can be constrained by the observation of gravitational waves from binary neutron star (BNS) mergers.
A. Nelson, S. Reddy, Dake Zhou
semanticscholar +1 more source
This is a review of X-ray emission from all types of isolated neutron stars, with an emphasis on rotation-powered pulsars. Topics include magnetospheric and thermal emission, as well as pulsar wind nebulae.
Mallory S. E. Roberts+2 more
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On magnetized neutron stars [PDF]
6 Figures + Appendix.
Débora P. Menezes+2 more
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Effects of dark matter on the spontaneous scalarization in neutron stars
Dark matter, an important portion of compact objects, can influence different phenomena in neutron stars. The spontaneous scalarization in the scalar-tensor gravity has been proposed for neutron stars.
Fahimeh Rahimi, Zeinab Rezaei
doaj +1 more source