Spin-Up of Hot Neutron Stars Just Born by the Subsequent Cooling

Details Spin-Up of Hot Neutron Stars Just Born by the Subsequent Cooling Spin-Up of Hot Neutron Stars Just Born by the Subsequent Cooling

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pthph..85..427t&link_type=abstract

Progress of Theoretical Physics, Vol. 85, No. 3, pp. 427-432

Physics

5

Scientific paper

Extent of spin-up of hot neutron stars just born, during the subsequent
cooling stage due to neutrino diffusion, is studied. As a result of the
cooling down to cold normal (pion-condensed) stars, about (20 ~ 25) ((50
~ 90))% increase of rotation rate is found. A comment on the maximum
rotation rate is given.

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