Theoretical Study of Neutron Stars using Cyclotron Resonance Scattering Features
International Journal of Development Research
Theoretical Study of Neutron Stars using Cyclotron Resonance Scattering Features
Received 13th November, 2017; Received in revised form 06th December, 2017; Accepted 23rd January, 2018; Published online 28th February, 2018.
Copyright © 2018, Pratyush Ranjan. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
Neutron stars and black holes are among the most exotic objects in the universe. Neutron stars are ancient remnants of stars that have reached the end of their evolutionary journey through space and time. Neutron stars comprise one of the possible evolutionary end-points of high mass stars. Neutron stars are thought to form by the gravitational collapse of the remnant of a massive star after a supernova explosion. Magnetic field strength is one of the most important physical parameters of neutron star. In Present paper we have done a comparative study to measure the magnetic field strength of a neutron star. Present Paper is the theoretical Study of Neutron Stars using Cyclotron Resonance Scattering Features (CRSF) as cyclotron re-emitting processes is equal to scattering and one might expect Cyclotron Resonant Scattering Features as absorption in the spectrum.
