Could pulsar glitch recovery phenomenon be a function of the dynamics of neutron star components involved in the glitch ?
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The pulsar glitch recovery times are too long that they suggest the involvement of frictionless fluid (superfluid) with the inner-crust of the neutron star in the glitch process. This inner-crust fluid is regarded as one component, while the rest of the neutron star components is regarded as the other component. These two component rotate differential - a process that accumulate to glitch. The glitch size is expected to constrain the magnitude of the components.
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Could pulsar glitch recovery phenomenon be a function of the dynamics of neutron star components involved in the glitch?
The pulsar glitch recovery times are too long that they suggest the involvement of frictionless fluid (superfluid) with the inner-crust of the neutron star in the glitch process. This inner-crust fluid is regarded as one component, while the rest of the neutron star components is regarded as the other component. These two component rotate differential - a process that accumulate to glitch. The glitch size is expected to constrain the magnitude of the components.
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