Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
2008-07-21
Phys.Rev.Lett.101:241101,2008
Physics
High Energy Physics
High Energy Physics - Phenomenology
4 pages; comments and refs. added; it matches with published version
Scientific paper
10.1103/PhysRevLett.101.241101
Dissipative processes acting in rotating neutron stars are essential in preventing the growth of the r-mode instability. We estimate the damping time of r-modes of an hypothetical compact quark star made up by color flavor locked quark matter at a temperature $T \lesssim 0.01$ MeV. The dissipation that we consider is due to the the mutual friction force between the normal and the superfluid component arising from the elastic scattering of phonons with quantized vortices. This process is the dominant one for temperatures $T \lesssim 0.01$ MeV where the mean free path of phonons due to their self-interactions is larger than the radius of the star and they can be described as an ideal bosonic gas. We find that r-modes oscillations are efficiently damped by this mechanism for pulsars rotating at frequencies of the order of 1 Hz at most. Our analysis rules out the possibility that cold pulsars rotating at higher frequencies are entirely made up by color flavor locked quark matter.
Mannarelli Massimo
Manuel Cristina
Sa'd Basil A.
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