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Title: Portent of Heine's Reciprocal Square Root Identity

Conference ·
OSTI ID:15003144

Precise efforts in theoretical astrophysics are needed to fully understand the mechanisms that govern the structure, stability, dynamics, formation, and evolution of differentially rotating stars. Direct computation of the physical attributes of a star can be facilitated by the use of highly compact azimuthal and separation angle Fourier formulations of the Green's functions for the linear partial differential equations of mathematical physics.

Research Organization:
Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
Sponsoring Organization:
US Department of Energy (US)
DOE Contract Number:
W-7405-ENG-48
OSTI ID:
15003144
Report Number(s):
UCRL-JC-150467-REV-1; TRN: US200420%%383
Resource Relation:
Conference: 3-D Stellar Evolution Workshop, Department of Applied Science (DAS), Livermore, CA (US), 07/22/2002--07/26/2002; Other Information: PBD: 13 Jan 2003
Country of Publication:
United States
Language:
English