File:A-causal-diamond-in-a-maximally-symmetric-spacetime-for-a-ball-shaped-spacelike-region-S.png

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A-causal-diamond-in-a-maximally-symmetric-spacetime-for-a-ball-shaped-spacelike-region-S.png(456 × 496 pixels, file size: 15 KB, MIME type: image/png)

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English: A causal diamond in a maximally symmetric spacetime for a ball-shaped spacelike region Σ. The past and future vertices of the diamond are denoted by p and p´, respectively, and is the null boundary. The dashed arrows are the flow lines of the conformal Killing vector ζ, whose flow sends the boundary of the diamond into itself, and vanishes at ∂Σ,p and p´.
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Source Fig1 at https://www.researchgate.net/publication/337872130_Gravitational_thermodynamics_of_causal_diamonds_in_AdS Gravitational thermodynamics of causal diamonds in (A)dS
Author Theodore Jacobson, Manus Visser

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current11:18, 13 June 2022Thumbnail for version as of 11:18, 13 June 2022456 × 496 (15 KB)Ernsts (talk | contribs)Uploaded a work by Theodore Jacobson, Manus Visser from https://www.researchgate.net/publication/337872130_Gravitational_thermodynamics_of_causal_diamonds_in_AdS Gravitational thermodynamics of causal diamonds in (A)dS with UploadWizard

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