Results 41 to 50 of about 676,319 (287)
Constraining the Maximum Mass of Neutron Stars from Multi-messenger Observations of GW170817 [PDF]
, 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
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Constraint on the maximum mass of neutron stars using GW170817 event [PDF]
Physical Review D, 2019 We revisit the constraint on the maximum mass of cold spherical neutron stars coming from the observational results of GW170817. We develop a new framework for the analysis by employing both energy and angular momentum conservation laws as well as solid ...
M. Shibata +3 more
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From hadrons to quarks in neutron stars: a review [PDF]
Reports on progress in physics. Physical Society, 2017 In recent years our understanding of neutron stars has advanced remarkably, thanks to research converging from many directions. The importance of understanding neutron star behavior and structure has been underlined by the recent direct detection of ...
G. Baym +5 more
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The Mass Distribution of Galactic Double Neutron Stars [PDF]
Astrophysical Journal, 2019 The conventional wisdom, dating back to 2012, is that the mass distribution of Galactic double neutron stars (DNSs) is well-fit by a Gaussian distribution with a mean of 1.33 M⊙ and a width of 0.09 M⊙.
N. Farrow, X. Zhu 朱, E. Thrane
semanticscholar +1 more source
Capture of leptophilic dark matter in neutron stars [PDF]
Journal of Cosmology and Astroparticle Physics, 2019 Dark matter particles will be captured in neutron stars if they undergo scattering interactions with nucleons or leptons. These collisions transfer the dark matter kinetic energy to the star, resulting in appreciable heating that is potentially ...
N. Bell, G. Busoni, S. Robles
semanticscholar +1 more source
, 2008 6 pages, 12 figures, paper presented at the IX International Conference on Hypernuclear and Strange Particle Physics, 10-14 October 2006, Johannes Gutenberg-Universitaet Mainz, Mainz ...
Weber, Fridolin, Rosenfield, Philip
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Neutron skins and neutron stars [PDF]
AIP Conference Proceedings, 2013 The neutron-skin thickness of heavy nuclei provides a fundamental link to the equation of state of neutron-rich matter, and hence to the properties of neutron stars. The Lead Radius Experiment ("PREX") at Jefferson Laboratory has recently provided the first model-independence evidence on the existence of a neutron-rich skin in 208Pb.
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New Constraints on Radii and Tidal Deformabilities of Neutron Stars from GW170817. [PDF]
Physical Review Letters, 2018 We explore in a parameterized manner a very large range of physically plausible equations of state (EOSs) for compact stars for matter that is either purely hadronic or that exhibits a phase transition.
E. Most +3 more
semanticscholar +1 more source
, 2006 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.
Kaspi, V. M. +2 more
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The Astrophysical Journal, 2000 13 pages, 6 PostScript figures, accepted to ...
POPOV SB +5 more
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