ds 2 = A(r )dt 2 − B (r )dr 2 − C (r )(d θ2 sin 2 θ d ϕ2 ) A, B, C > 0∀r ≠ ro. RELATIVISTIC GEOMETRY AND ITS IMPLICATIONS FOR BLACK HOLES AND COSMOLOGY - Anti-de Sitter space - Document - PDFSEARCH.IO

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	ds 2 = A(r )dt 2 − B (r )dr 2 − C (r )(d θ2 + sin 2 θ d ϕ2 ) A, B, C > 0∀r ≠ ro. RELATIVISTIC GEOMETRY AND ITS IMPLICATIONS FOR BLACK HOLES AND COSMOLOGY Add to Reading List Document Date: 2009-04-18 05:20:10 Open Document File Size: 146,45 KB Share Result on Facebook City Leipzig / / Company Schwarzschild / Eddington A. S. / Cambridge University Press / / Country Australia / / / Facility The centre / / IndustryTerm actual solution / symmetric solutions / valid solution / correct particular solution / / Organization Cambridge University / / Person Schwarzschild / Stephen J. Crothers / / Position General / / ProvinceOrState Queensland / / PublishedMedium Progress in Physics / / Technology Microwave / / URL www.ptep-online.com / www.geocities.com/theometria/McVittie.pdf / www.geocities.com/theometria/schwarzschild.pdf / www.geocities.com/theometria/Droste.pdf / / SocialTag Geometry Kerr–Newman metric Anti de Sitter space Metric tensor Reissner–Nordström metric Polar coordinate system Proper time Exact solutions in general relativity Physics Theoretical physics

ds 2 = A(r )dt 2 − B (r )dr 2 − C (r )(d θ2 + sin 2 θ d ϕ2 ) A, B, C > 0∀r ≠ ro. RELATIVISTIC GEOMETRY AND ITS IMPLICATIONS FOR BLACK HOLES AND COSMOLOGYAdd to Reading List