From Microphysics to Gravitational Waves: Modeling Neutron Star and Signatures

dc.rights.license	CC-BY-NC-ND
dc.contributor.advisor	Stoof, H.T.C.
dc.contributor.author	Hertogh, Timo Hertogh
dc.date.accessioned	2025-08-22T00:01:37Z
dc.date.available	2025-08-22T00:01:37Z
dc.date.issued	2025
dc.identifier.uri	https://studenttheses.uu.nl/handle/20.500.12932/49967
dc.description.sponsorship	Utrecht University
dc.language.iso	EN
dc.subject	In this research, the 2- and 3- body interactions of particles inside neutron stars are modelled. From these interactions, the equation of state is obtained. The Tolman Oppenheimer Volkov equations are then calculated with the equation of state to acquire the mass and radius of a neutron star in this framework. Additionally, we calculated multiple moments of the electric and magnetic deformations that arise in binary neutron stars, which are of interest in gravitational wave research.
dc.title	From Microphysics to Gravitational Waves: Modeling Neutron Star and Signatures
dc.type.content	Master Thesis
dc.rights.accessrights	Open Access
dc.subject.courseuu	Theoretical Physics
dc.thesis.id	52473