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Induced p-wave superfluidity in strongly interacting imbalanced Fermi gases
Induced p-wave superfluidity imbalanced Fermi gases
2010/11/24
The induced interaction among the majority spin species, due to the presence of the minority
species, is computed for the case of a population-imbalanced resonantly-interacting Fermi gas.
Rapid Cooling of the Neutron Star in Cassiopeia A Triggered by Neutron Superfluidity in Dense Matter
Rapid Cooling of the Neutron Star Cassiopeia Neutron Superfluidity
2011/1/10
We propose that the recently observed cooling of the neutron star in Cassiopeia A is due to
enhanced neutrino emission from the onset of the breaking and formation of neutron Cooper pairs
in the 3P2...
Superfluidity in neutron matter and symmetric nuclear matter and the effect of a microscopic three-body force
neutron matter symmetric nuclear matter superfluidity three-body force BCS theory BHF approach
2009/8/14
The neutron 3PF2 pairing gap in pure neutron matter, neutron 3PF2 gap and neutron-proton 3SD1 gap in symmetric nuclear matter have been studied by using the Brueckner-Hartree-Fock(BHF) approach and th...