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  1. Neutron stars are not the sole objects in whose depth matter is compressed to high densities inaccessible in laboratory. Other representatives of the class of compact stars are white dwarfs and hypothetical quark stars [2]. While the size of a neutron star mainly depends on the balance between gravity force and degenerate neutron

  2. 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...

  3. 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 connections among nuclear physics, particle physics, and astrophysics.

  4. 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,...

  5. 31 Δεκ 2010 · 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, thermal evolution, and masses and radii are briefly discussed, along with the underlying microphysics.

  6. This book summarizes the recent progress in the physics and astrophysics of neutron stars. It provides an overview of neutron star formation in supernovae, pulsars, equations of state of neutron stars, super dense matter, gravitational wave emission and alternative theories of gravity.

  7. 6 Οκτ 2022 · Neutron starscompact objects with masses similar to that of our Sun but radii comparable to the size of a city—contain the densest form of matter in the universe that can be probed in terrestrial laboratories as well as in earth- and space-based observatories.

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