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Rotational cooling anisotropic

Neutron stars are thought to form in supernova explosions. The outer layers of the star crystallize as the newborn neutron star cools by neutrino emission. Estimates, based on the expected breaking strain of the crystal lattice, suggest that anisotropic stresses, which build up as the pulsar loses rotational energy, could lead to e < 10 the exact value depends on the breaking strain of the neutron... [Pg.103]

See other pages where Rotational cooling anisotropic is mentioned: [Pg.227]    [Pg.97]    [Pg.354]    [Pg.135]    [Pg.40]    [Pg.354]    [Pg.165]    [Pg.253]    [Pg.393]    [Pg.261]    [Pg.103]    [Pg.100]    [Pg.387]    [Pg.16]    [Pg.394]    [Pg.196]    [Pg.393]    [Pg.946]    [Pg.255]    [Pg.14]   
See also in sourсe #XX -- [ Pg.227 ]



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