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Constraining the Topology of the Universe

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arxiv astro-ph/0310233 v1 pith:5GR2Q7TD submitted 2003-10-08 astro-ph gr-qc

classification astro-phgr-qc
keywords universecirclepairstopologyback-to-backcirclesnearlysearch
verification ladder T0 review T1 audit T2 compute T3 formal
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The first year data from the Wilkinson Microwave Anisotropy Probe are used to place stringent constraints on the topology of the Universe. We search for pairs of circles on the sky with similar temperature patterns along each circle. We restrict the search to back-to-back circle pairs, and to nearly back-to-back circle pairs, as this covers the majority of the topologies that one might hope to detect in a nearly flat universe. We do not find any matched circles with radius greater than 25 degrees. For a wide class of models, the non-detection rules out the possibility that we live in a universe with topology scale smaller than 24 Gpc.

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Cited by 2 Pith papers

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

  1. Inflation and topology from the no-boundary state

    hep-th 2026-05 unverdicted novelty 7.0 of 10

    The no-boundary wavefunction on the 3-torus, summed over SL(3,Z) geometries using GL(3) automorphic forms, favors large inflating universes with N ≳ 250 e-folds and induces torus-moduli corrections to the CMB spectrum.

  2. Quantum stress-energy at timelike boundaries: testing a new beyond-$\Lambda$CDM parameter with cosmological data

    astro-ph.CO 2025-06 conditional novelty 6.0 of 10

    Timelike boundaries sourcing negative, 1/a-scaling vacuum energy fit CMB+BAO data slightly better than LCDM and relax the neutrino-mass constraint, though the preference is only about 2 sigma.

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