Date of Award
Master of Science
Effrain J. Ferrer
Neutron stars (NSs) are the windows to check the validation of physical laws at extreme conditions, for example, at very high densities and strong magnetic fields and thus to reach the equations of state (EoS) for a better understanding of the structure as well as the composition of the NSs. In our investigations, it is found that the system's (NSs) pressure becomes anisotropic due to the breaking of rotational symmetry in the presence of strong magnetic fields, which even can be significantly sufficient to lead into the deformation of NSs or to destroy itself.
Received from ProQuest
Masud, Md, "Equation of State of a Dense and Magnetized Neutron System" (2016). Open Access Theses & Dissertations. 694.