General Relativistic Non-Radial Oscillations in Compact Stars
<p> Currently, we lack a means of identifying the type of matter at the core of compact stars, but in the future, we may be able to use gravitational wave signals produced by fluid oscillations inside compact stars to discover new phases of dense matter. To this end, we study the fluid perturb...
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| Language: | EN |
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California State University, Long Beach
2017
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| Online Access: | http://pqdtopen.proquest.com/#viewpdf?dispub=10604673 |