Buchdahl-like transformations for perfect fluid spheres

dc.creatorBoonserm, Petarpa
dc.creatorVisser, Matt
dc.date2007-07-02
dc.date.accessioned2026-07-07T11:17:24Z
dc.date.available2026-07-07T11:17:24Z
dc.descriptionIn two previous articles [Phys. Rev. D71 (2005) 124307 (gr-qc/0503007), and gr-qc/0607001] we have discussed several "algorithmic" techniques that permit one (in a purely mechanical way) to generate large classes of general relativistic static perfect fluid spheres. Working in Schwarzschild curvature coordinates, we used these algorithmic ideas to prove several "solution-generating theorems" of varying levels of complexity. In the present article we consider the situation in other coordinate systems: In particular, in general diagonal coordinates we shall generalize our previous theorems, in isotropic coordinates we shall encounter a variant of the so-called "Buchdahl transformation", while in other coordinate systems (such as Gaussian polar coordinates, Synge isothermal coordinates, and Buchdahl coordinates) we shall find a number of more complex "Buchdahl-like transformations" and "solution-generating theorems" that may be used to investigate and classify the general relativistic static perfect fluid sphere. Finally by returning to general diagonal coordinates and making a suitable ansatz for the functional form of the metric components we place the Buchdahl transformation in its most general possible setting.
dc.description23 pages
dc.identifierhttps://arxiv.org/abs/0707.0146
dc.identifierhttp://arxiv.org/abs/0707.0146
dc.identifierInt.J.Mod.Phys.D17:135-163,2008
dc.identifierdoi:10.1142/S0218271808011912
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/192994
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleBuchdahl-like transformations for perfect fluid spheres
dc.typetext

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