Speaker
Mr
SOUVIK PRIYAM ADHYA
(SAHA INSTITUTE OF NUCLEAR PHYSICS, KOLKATA)
Description
In this work we have studied the non-Fermi liquid behavior that enters into the expression of the
pulsar kick velocity due to assymetric neutrino emission. We have incorporated leading order as
well as next-to-leading order corrections to the velocity and compared the results with the simple
Fermi liquid case. The relation between quark phase radius and temperature
has been shown.
We have also approximated our results for the case of large magnetic field present
in neutron stars.
Primary author
Mr
SOUVIK PRIYAM ADHYA
(SAHA INSTITUTE OF NUCLEAR PHYSICS, KOLKATA)
Co-authors
Prof.
ABHEE K. DUTT-MAZUMDER
(SAHA INSTITUTE OF NUCLEAR PHYSICS, KOLKATA)
Prof.
PRADIP K. ROY
(SAHA INSTITUTE OF NUCLEAR PHYSICS, KOLKATA)
