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, 2023 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 of state is still compatible with observations, this uncertainty can be overcome to a large extent ...
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Neutron stars for undergraduates [PDF]
American Journal of Physics, 2004 The calculation of the structure of white dwarf and neutron stars is a suitable topic for an undergraduate thesis or an advanced special topics or independent study course. The subject is rich in many different areas of physics, ranging from thermodynamics to quantum statistics to nuclear physics to special and general relativity.
Sanjay Reddy, Richard R. Silbar
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Using Gravitational-wave Observations and Quasi-universal Relations to Constrain the Maximum Mass of Neutron Stars [PDF]
, 2017 Combining the GW observations of merging systems of binary neutron stars and quasi-universal relations, we set constraints on the maximum mass that can be attained by nonrotating stellar models of neutron stars.
L. Rezzolla, E. Most, L. R. Weih
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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
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What can neutron stars reveal about the equation of state of dense matter? [PDF]
EPJ Web of Conferences, 2020 Neutron stars are astrophysical objects of extremes, reaching the highest densities we can observe in the cosmos, and probing matter under conditions that cannot be recreated in terrestrial experiments.
Tews Ingo
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Many Aspects of Magnetic Fields in Neutron Stars
Universe, 2018 In this work, we explore different aspects in which strong magnetic fields play a role in the composition, structure and evolution of neutron stars. More specifically, we discuss (i) how strong magnetic fields change the equation of state of dense matter,
Rodrigo Negreiros +3 more
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Thermal properties of hot and dense matter: Influence of rapid rotation on protoneutron stars, hot neutron stars, and neutron star merger remnants [PDF]
EPJ Web of Conferences, 2021 The knowledge of the equation of state is a key ingredient for many dynamical phenomena that depend sensitively on the hot and dense nuclear matter, such as the formation of protoneutron stars and hot neutron stars.
Koliogiannis Polychronis +1 more
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SUPERFLUID NEUTRON STARS [PDF]
The Ninth Marcel Grossmann Meeting, 2002 2 pages, "mprocl.sty" with LaTeX 2.09; contribution to the 9th Marcel Grossmann Meeting (MG9), Rome, July ...
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Physica Scripta, 2000 15 pages, LaTeX2e, 3 eps figures, to appear in Physica ...
Ilona Bednarek, Ryszard Manka
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Strangeness in neutron stars [PDF]
Nuclear Physics A, 2005 Invited review talk at the VIII International Conference on Hypernuclear and Strange Particle Physics, Jefferson Lab, Newport News, Virginia, October 14-18, 2003.
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