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arxiv: 0711.3459 · v1 · submitted 2007-11-22 · 🌌 astro-ph

A Test of the Copernican Principle

classification 🌌 astro-ph
keywords copernicancosmicprinciplespectrumvoidaccelerationcentermeasurements
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The blackbody nature of the cosmic microwave background (CMB) radiation spectrum is used in a modern test of the Copernican Principle. The reionized universe serves as a mirror to reflect CMB photons, thereby permitting a view of ourselves and the local gravitational potential. By comparing with measurements of the CMB spectrum, a limit is placed on the possibility that we occupy a privileged location, residing at the center of a large void. The Hubble diagram inferred from lines-of-sight originating at the center of the void may be misinterpreted to indicate cosmic acceleration. Current limits on spectral distortions are shown to exclude the largest voids which mimic cosmic acceleration. More sensitive measurements of the CMB spectrum could prove the existence of such a void or confirm the validity of the Copernican Principle.

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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. CMB dipoles and other low-order multipoles in the quasispherical Szekeres model

    astro-ph.CO 2019-07 unverdicted novelty 5.0

    Quasispherical Szekeres models allow a small but less special observer region for CMB dipole consistency and can accommodate significant quadrupole unlike LTB voids.