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physics, is to highlight the main features of neutron stars making them unique cosmic bodies. It does not pretend to be comprehensive, bearing in mind the thousands of publications devoted to neutron stars, and is designed first and foremost to present the author’s personal view of the problem. Fundamentals of neutron star physics
Neutron stars are the dense remnants of the cores of high-mass stars which have undergone gravitational collapse. Shortly after the discovery of the neutron, Landau [1] proposed the idea of compact objects with densities greater than white dwarf stars.
Neutron Stars: The History. 1932 Landau suggests the existence of giant nucleus stars. 1932 Chadwick discovers the neutron. 1934 Baade & Zwicky predict the existence of neutron stars (NSs) as the end products of supernovae.
1 Μαΐ 2004 · Neutron stars are some of the densest manifestations of massive objects in the universe. They are ideal astrophysical laboratories for testing theories of dense matter physics and provide...
28 Φεβ 2011 · Topical problems in the physics of and basic facts about neutron stars are reviewed. The observational manifestations of neutron stars, their core and envelope structure, magnetic fields,...
The notes are divided into three parts: (1) the struc-ture of the neutron star crust and core and the mass-radius relation, (2) neutron star cooling, and (3) a brief discussion of neutron star magnetic field evolution. Chapter 1.
Neutron stars are laboratories for dense matter physics, since they contain the highest densities of cold matter in the universe. Combining laboratory experiments with observations of neutron stars will constrain the equation of state of relatively cold and dense matter.
