Portent of Heine's Reciprocal Square Root Identity

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dc.creatorCohl, Howard S.
dc.date2003-03-10
dc.date.accessioned2026-07-07T02:07:51Z
dc.date.available2026-07-07T02:07:51Z
dc.descriptionPrecise 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.
dc.description6 pages, newpasp.sty cohl_new.tex
dc.identifierhttps://arxiv.org/abs/astro-ph/0303205
dc.identifierhttp://arxiv.org/abs/astro-ph/0303205
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5835
dc.subjectAstrophysics
dc.titlePortent of Heine's Reciprocal Square Root Identity
dc.typetext

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