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Bernabeu Alberola, José; Ericson, Torleif E.O.; Ferro Fontán, Constantino | |||
Aquest document és un/a article, creat/da en: 1975 | |||
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It is shown that, apart from the neutron interaction contribution to the susceptibility of neutron stars, there is an additional contribution coming from the magnetic polarizability beta /sub n/ of individual neutrons. For beta /sub n/ approximately=10/sup -4/fm/sup 3 /, this part overwhelms the interaction contribution for k/sub F/>or approximately=3.5fm/sup -1/. No transition to ferromagnetic state is predicted in the interesting density region. | |||
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