π-condensation and neutron star cooling

Details π-condensation and neutron star cooling π-condensation and neutron star cooling

Sep 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972phla...41..129k&link_type=abstract

Physics Letters A, Volume 41, Issue 2, p. 129-131.

Physics

23

Scientific paper

We show, within the context of an independent particle model, that π- condensation should occur in neutron stars having baryon densities exceeding~0.4 - 0.5 fm-3. This high concentration of π- implies a very fast cooling rate for `hot' neutron stars.
Work supported by the Air Force Office of Scientific Research, Office of Aerospace Research, United States Air Force, under AFOSR Grant 70-1866A.

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