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27 April 2024 |
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A possible mechanism of effective decoupling of hadronic superfluids in precessing neutron stars | | Egor Babaev
; | | Date: |
28 Jan 2009 | | Abstract: | I consider the standard neutron star interior model: a strongly interacting
mixture of neutronic superfluid and protonic superconductor under rotation and
carrying magnetic field. Recently the model was cast in doubt because in its
framework a strong interaction between protonic and neutronic vortices could
not be constrained with the long-period precession found in some pulsars. Here
I propose a mechanism which at the hydrodynamic level, in a narrow range of
parameters leads to a greatly reduced coupling between the superfluid and
magnetic-field carrying superconducting components. | | Source: | arXiv, 0901.4380 | | Services: | Forum | Review | PDF | Favorites | |
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