The Composition, Structure and Evolution of Neutron Stars

Details The Composition, Structure and Evolution of Neutron Stars The Composition, Structure and Evolution of Neutron Stars

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aps..dnp.ja004p&link_type=abstract

American Physical Society, Division of Nuclear Physics Meeting, 27-30 October, 2004, Chicago, IL. MEETING ID: DNP04., abstract #

Physics

Nuclear Physics

Scientific paper

Neutron stars are the densest manifestations of massive objects in the universe. Neutron stars may exhibit conditions and phenomena not observed elsewhere, such as hyperon-dominated matter, Bose-condensed matter, deconfined quark matter, superfluidity and superconductivity with critical temperatures near 10^10 K, opaqueness to neutrinos, and magnetic fields in excess of 10^13 Gauss. Observations, including studies of binary pulsars, thermal emission from isolated neutron stars, glitches from pulsars, quasi-periodic oscillations from accreting neutron stars and neutrinos released when a neutron star is born, provide information about neutron star masses, radii, temperatures, ages and internal compositions.

Affiliated with

Also associated with

No associations

Rating

The Composition, Structure and Evolution of Neutron Stars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The Composition, Structure and Evolution of Neutron Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Composition, Structure and Evolution of Neutron Stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-898655