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Algebraically special space-time in relativity, black holes, and pulsar modelsThe entire field of astronomy is in very rapid flux, and at the center of interest are problems relating to the very dense, rotating, neutron stars observed as pulsars. the hypothesized collapsed remains of stars known as black holes, and quasars. Degenerate metric form, or Kerr-Schild metric form, was used to study several problems related to intense gravitational fields.
Document ID
19730024009
Acquisition Source
Legacy CDMS
Document Type
Technical Memorandum (TM)
Authors
Adler, R. J.
(NASA Ames Research Center Moffett Field, CA, United States)
Sheffield, C.
(NASA Ames Research Center Moffett Field, CA, United States)
Date Acquired
September 2, 2013
Publication Date
August 1, 1973
Subject Category
Space Sciences
Report/Patent Number
NASA-TM-X-62298
Report Number: NASA-TM-X-62298
Accession Number
73N32742
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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