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a cooling process. Because of the short muon lifetime (2.2 |$\mu$|s), muon cooling is challenging and various innovative methods are under development [22–25]. One such method is to thermalize the surface ...
with the longitudinal velocity profile then determines the profiles along the jet of the number density, and global magnetic field strength. Specifically, the cross-sectional radius R at any height z along the jet ...
The core of the star, consisting of the neutron superfluid and plasma of electrons, muons , superconducting protons, and, probably, charged and neutral hyperons responds to the glitch via magnetic, viscous ...
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