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The Nuclear Physics of Neutron Stars
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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.
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Keywords
- Astrophysical jets
- binary mergers
- binary neutron star merger
- Cheshire Cat Principle
- compact stars
- EOS
- equation of state
- extragalactic
- GnEFT
- Gogny interaction
- gravitational redshift
- gravitational waves
- GW190814
- hadron-quark continuity
- hidden symmetries
- hidden symmetries dual to gluons
- Higgs inflationary model
- incompressibility of nuclear matter
- interior solutions
- landau parameters
- lepto-hadronic model
- Massive compact stars
- maximum mass
- moment of inertia
- n/a
- Neutron Star
- neutron star properties
- Neutron stars
- nuclear matter
- nuclear matter saturation properties
- photo-pion production
- psuedo-conformality
- relativistic fluids
- scalar-tensor gravity
- spherically symmetric sources
- symmetry energy
- thema EDItEUR::P Mathematics and Science
- thema EDItEUR::P Mathematics and Science::PH Physics
- thema EDItEUR::P Mathematics and Science::PH Physics::PHN Nuclear physics
- tidal deformability
- topology change
- topology for baryons
- ultra dense matter
- unified equation of state
- X17
- XRBs
- γ-ray emission
Links
DOI: 10.3390/books978-3-7258-1600-2Editions