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Ellipsoidal Universe and Cosmic Shear

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arxiv 2409.07509 v1 pith:FLI7FMLR submitted 2024-09-11 gr-qc astro-ph.COhep-th

Ellipsoidal Universe and Cosmic Shear

classification gr-qc astro-ph.COhep-th
keywords cosmicshearuniverseeccentricitybianchiconnectionconsiderellipsoidal
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We consider a Bianchi I geometry of the Universe. We obtain a cosmic shear expression related with the eccentricity of the Universe. In particular we study the connection among cosmic shear, eccentricity and CMB. The equation are self-contained with only two parameters.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background

    astro-ph.CO 2026-07 conditional novelty 6.0

    An analytic weak-shear Bianchi I calculation bounds the low-redshift luminosity-distance quadrupole to |Aμ(0.15)|≲2.4×10^-11 mag under BBN shear limits, ruling out shear-only resolution of the Hubble tension.