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Rigidly rotationg perfect fluids
Author(s) -
Kramer D.
Publication year - 1986
Publication title -
astronomische nachrichten
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.394
H-Index - 63
eISSN - 1521-3994
pISSN - 0004-6337
DOI - 10.1002/asna.2113070519
Subject(s) - limiting , physics , general relativity , perfect fluid , class (philosophy) , classical mechanics , tensor (intrinsic definition) , zero (linguistics) , theoretical physics , theory of relativity , limit (mathematics) , mathematical physics , mathematical analysis , mathematics , pure mathematics , computer science , philosophy , linguistics , mechanical engineering , engineering , artificial intelligence
A class of stationary rigidly rotating perfect fluids in General Relativity is investigated. This class which is characterized by zero Simon tensor contains only the Wahlquist solution and its limits. It is shown how a recently given solution follows from the Wahlquist solution by a limiting procedure.

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