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Titlebook: Compact Stars; Nuclear Physics, Par Norman K. Glendenning Textbook 19971st edition Springer-Verlag New York, Inc. 1997 Redshift.Variation.b

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https://doi.org/10.1007/978-1-4684-0491-3Redshift; Variation; black hole; black holes; earth; gravitation; gravity; neutron; neutron star; particle ph
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https://doi.org/10.1007/978-3-658-41059-9f most stars after a lifetime of tens to thousands of millions of years. Whichever of these objects is formed at the end of the life of a particular luminous star, the compact object will live in all essential respects unchanged from the state in which it was formed. Neutron stars themselves can tak
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https://doi.org/10.1007/978-3-658-41059-9 theory; it is the foundation for our understanding of compact stars. Neutron stars and black holes owe their very existence to gravity as formulated by Einstein [2, 3]. Dense objects like neutron stars could also exist in Newton’s theory, but they would be very different objects. Chandrasekhar foun
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