Exotic bulk viscosity and its influence on neutron star r-modes Debades Bandyopadhyay Saha Institute of Nuclear Physics, Kolkata, India Collaborator: Debarati.
Acoustic waves (case k = 0 ) -- Important for non-magnetized regions in the low solar atmosphere: Eqs. (10),(6) = (12) Fig. 3: Defined by Eq(12) variation.
Debades Bandyopadhyay Saha Institute of Nuclear Physics Kolkata, India With Debarati Chatterjee (SINP) Bulk viscosity and r-modes of neutron stars.
Fig.4: Typical values of the collisional and viscous damping time ratios for propagating a) Alfvén and fast magnetoacoustic waves and b) acoustic wave.
