NASA NTRS · 19740061137
Analytic pulsar models
Abstract
An analytical procedure is given for solving the Einstein equations of a rotating fluid body. It is demonstrated that an analytic model of uniform denisty, representing a slowly rotating neutron star, can describe both differentially and uniformly rotating stars.
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Adams, R. C., Cohen, J. M., Adler, R. J., Sheffield, C.. 1974-09-01. Analytic pulsar models. https://ntrs.nasa.gov/citations/19740061137
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