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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 are expounded in the excellent textbook by Shapiro and Teukolsky [24]. More detailed descriptions of develop-ments in selected branches of neutron star astrophysics
- The Nuclear Physics of Neutron Stars
Neutron stars—compact objects with masses similar to that of...
- The Nuclear Physics of Neutron Stars
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...
Download book PDF. Download book EPUB. Overview. Editors: Luciano Rezzolla, Pierre Pizzochero, David Ian Jones, Nanda Rea, Isaac Vidaña. Offers an authoritative and current overview of the physics and astrophysics of neutron stars. Discusses testing of gravity with the aid of pulsars.
31 Δεκ 2010 · Physics. 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. View on IOP Publishing. [PDF] Semantic Reader.
TLDR. Observations that include studies of pulsars in binary systems, thermal emission from isolated neutron stars, glitches from pulsars, and quasi-periodic oscillations from accreting neutron stars provide information about neutron star masses, radii, temperatures, ages, and internal compositions. Expand.
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.
6 Οκτ 2022 · Neutron stars—compact 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.
