A Spectral Approach to the Relativistic Inverse Stellar Structure Problem

A Spectral Approach to the Relativistic Inverse Stellar Structure Problem

We present a new method for solving the inverse stellar structure problem, which determines an expression for the high density range of the neutron star equation of state (EOS) based on observations of total masses, M, and radii, R of these stars. This approach determines spectral representations of...

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Bibliographic Details
Main Author:	Indik, Nathaniel Michael
Published:	2012
Online Access:	Indik, Nathaniel Michael (2012) A Spectral Approach to the Relativistic Inverse Stellar Structure Problem. Senior thesis (Major), California Institute of Technology. doi:10.7907/829S-BX59. https://resolver.caltech.edu/CaltechTHESIS:02132018-113201713 <https://resolver.caltech.edu/CaltechTHESIS:02132018-113201713>

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