Results 81 to 90 of about 766,537 (359)

Constraining the Maximum Mass of Neutron Stars from Multi-messenger Observations of GW170817 [PDF]

open access: yes, 2017
We combine electromagnetic (EM) and gravitational-wave (GW) information on the binary neutron star (NS) merger GW170817 in order to constrain the radii and maximum mass of NSs.
B. Margalit, B. Metzger
semanticscholar   +1 more source

Quarkyonic Matter and Neutron Stars. [PDF]

open access: yesPhysical Review Letters, 2018
We consider quarkyonic matter to naturally explain the observed properties of neutron stars. We argue that such matter might exist at densities close to that of nuclear matter, and at the onset, the pressure and the sound velocity in quarkyonic matter ...
L. McLerran, S. Reddy
semanticscholar   +1 more source

Neutron star properties with relativistic equations of state [PDF]

open access: yes, 1997
We study the properties of neutron stars adopting relativistic equations of state of neutron star matter, calculated in the framework of the relativistic Brueckner-Hartree-Fock approximation for electrically charge neutral neutron star matter in beta ...
Bodmer A. R.   +29 more
core   +3 more sources

The Magnetospheres of (Accreting) Neutron Stars

open access: yesEPJ Web of Conferences, 2014
I give an overview of the most important observational tools to study the magnetospheres of accreting neutron stars, with a focus on accreting neutron stars in high mass X-ray binary systems.
Wilms J.
doaj   +1 more source

The cosmic merger rate of neutron stars and black holes [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2018
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]

open access: yesOld and New Concepts of Physics, 2007
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

On magnetized neutron stars [PDF]

open access: yesJournal of Cosmology and Astroparticle Physics, 2015
6 Figures + Appendix.
Débora P. Menezes   +2 more
openaire   +3 more sources

Herschel and Spitzer observations of slowly rotating, nearby isolated neutron stars

open access: yes, 2014
Supernova fallback disks around neutron stars have been discussed to influence the evolution of the diverse neutron star populations. Slowly rotating neutron stars are most promising to find such disks.
Pavlov, G. G.   +3 more
core   +1 more source

Evolution of Neutron Stars and Observational Constraints

open access: yesEPJ Web of Conferences, 2010
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

Dark halos around neutron stars and gravitational waves [PDF]

open access: yesJournal of Cosmology and Astroparticle Physics, 2018
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

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