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Non-linear hydrodynamical evolution of rotating relativistic stars: numerical methods and code tests

✍ Scribed by José A. Font; Nikolaos Stergioulas; Kostas D. Kokkotas

Book ID: 104465500
Publisher: John Wiley and Sons
Year: 2000
Tongue: English
Weight: 485 KB
Volume: 313
Category: Article
ISSN: 0035-8711
DOI: 10.1046/j.1365-8711.2000.03254.x

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## Abstract A simple and efficient numerical method is proposed to investigate deformations and stresses in elastic–plastic rotating solid shafts. Using the assumption of plane strain, the governing equation is derived from the geometric relation, equilibrium equation, deformation theory, von Mises