Speaker
Mr
Souvik Priyam Adhya
(Saha Institute of Nuclear Physics)
Description
In this present work we have incorporated the non-Fermi liquid behavior into the expression of the neutron star kick velocity due to assymetric neutrino emission. We have studied leading order as well as next-to-leading order corrections to the velocity and compared the results with the Fermi liquid case. We have also approximated our results for the case of large magnetic field found in neutron stars.
Author
Mr
Souvik Priyam Adhya
(Saha Institute of Nuclear Physics)
Co-authors
Prof.
Abhee K. Dutt-Mazumder
(Saha Institute of Nuclear Physics)
Prof.
Pradip Kumar Roy
(Saha Institute of Nuclear Physics)
