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Intrinsic magnetic polarizability contribution to susceptibility of dense neutron matter

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dc.contributor.author	Bernabeu Alberola, José
dc.contributor.author	Ericson, Torleif E.O.
dc.contributor.author	Ferro Fontán, Constantino
dc.date.accessioned	2016-05-03T11:48:39Z
dc.date.available	2016-05-03T11:48:39Z
dc.date.issued	1975
dc.identifier.citation	Bernabeu Alberola, José; Ericson, Torleif E.O.; Ferro Fontán, Constantino (1975) Intrinsic magnetic polarizability contribution to susceptibility of dense neutron matter Astrophysical Letters & Communications 16 2 57 59
dc.identifier.uri	http://hdl.handle.net/10550/53327
dc.description.abstract	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.
dc.language.iso	eng
dc.relation.ispartof	Astrophysical Letters & Communications, 1975, vol. 16, num. 2, p. 57-59
dc.subject	Física
dc.title	Intrinsic magnetic polarizability contribution to susceptibility of dense neutron matter
dc.type	journal article	es_ES
dc.date.updated	2016-05-03T11:48:39Z
dc.identifier.idgrec	069116
dc.rights.accessRights	open access	es_ES