High-density Equation of State of Neutron Stars

Details High-density Equation of State of Neutron Stars High-density Equation of State of Neutron Stars

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000eaa..booke2123w&link_type=abstract

"Encyclopedia of Astronomy and Astrophysics, Edited by Paul Murdin, article 2123. Bristol: Institute of Physics Publishing, 2001

Astronomy and Astrophysics

Astrophysics

Stars, Stellar Models And Concepts

Scientific paper

The enormous gravitational pull that binds NEUTRON STARS compresses most of their matter to densities that are up to an order of magnitude higher than the mass density of atomic nuclei, 2.5×1014 g cm-3. This provides a high pressure environment in which numerous subatomic particle processes, ranging from the generation of new BARYON particles (Σ,Λ,Ξ,Δ), to QUARK deconfinement, to the formation o...

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