Speaker
Manisha Kumari
(DR. B. R. AMBEDKAR NATIONAL INSTITUTE OF TECHNOLOGY, JALANDHAR)
Description
The medium modification in energies of kaon and antikaon at zero momentum in strongly magnetized asymmetric nuclear matter are explored using a chiral $\text{SU(3)}$ model. The parameters used in this calculation are fitted to nuclear matter saturation properties and with vacuum masses of baryon. We have investigated the possibility of antikaon condensation in neutron star with charge neutrality and $\beta-$equilibrium condition. By considering the effect of anomalous magnetic moments (AMM) in present study it is observed that the density effect is dominating in medium as compared to magnetic field and isospin asymmetry.
| First author | Manisha Kumari |
|---|---|
| maniyadav93@gmail.com | |
| Collaboration / Activity | no |
Primary authors
Manisha Kumari
(DR. B. R. AMBEDKAR NATIONAL INSTITUTE OF TECHNOLOGY, JALANDHAR)
Arvind Kumar
(Dr B R Ambedkar National Institute of Technology Jalandhar India)
