Reprint

The Nuclear Physics of Neutron Stars

Edited by
July 2024
192 pages
  • ISBN978-3-7258-1599-9 (Hardback)
  • ISBN978-3-7258-1600-2 (PDF)

This is a Reprint of the Special Issue The Nuclear Physics of Neutron Stars that was published in

Biology & Life Sciences
Chemistry & Materials Science
Computer Science & Mathematics
Physical Sciences
Summary

Neutron stars are considered extraordinary astronomical laboratories for the physics of nuclear matter as they have the most fascinating constitution of energy and matter in the universe. Recently, the detection of gravitational waves from the merger of two neutron stars, in a binary neutron star system, has opened a new window to explore the physics of neutron stars. The following Special Issue is a collection of various contributions dedicated to modern applications of the theory of nuclear matter in neutron stars and its main purpose is to shed light on some of the open problems concerning the nuclear physics of neutron stars and how they can possibly be addressed or even answered.

Format
  • Hardback
License and Copyright
© 2024 by the authors; CC BY-NC-ND license
Keywords
equation of state; neutron star; GW190814; maximum mass; tidal deformability; nuclear matter; neutron star; equation of state; gravitational waves; binary mergers; unified equation of state; Gogny interaction; neutron star; symmetry energy; tidal deformability; moment of inertia; neutron stars; scalar-tensor gravity; Higgs inflationary model; XRBs; astrophysical jets; photo-pion production; extragalactic; γ-ray emission; lepto-hadronic model; topology for baryons; hidden symmetries; ultra dense matter; compact stars; X17; EoS; neutron star; Massive compact stars; EoS; topology change; hadron-quark continuity; Cheshire Cat Principle; hidden symmetries dual to gluons; GnEFT; psuedo-conformality; nuclear matter saturation properties; landau parameters; incompressibility of nuclear matter; neutron star properties; binary neutron star merger; gravitational redshift; relativistic fluids; interior solutions; spherically symmetric sources; n/a

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