Cosmic microwave background constraints on the strong equivalence principle
| dc.creator | Boucher, V. | |
| dc.creator | Gerard, J. -M. | |
| dc.creator | Vandergheynst, P. | |
| dc.creator | Wiaux, Y. | |
| dc.date | 2004-07-10 | |
| dc.date | 2004-10-26 | |
| dc.date.accessioned | 2026-07-07T02:13:49Z | |
| dc.date.available | 2026-07-07T02:13:49Z | |
| dc.description | We study the effect of a violation of the strong equivalence principle (SEP) on the cosmic microwave background (CMB). Such a violation would modify the weight of baryons in the primordial gravitational potentials and hence their impact in the establishment of the photon-baryon plasma acoustic oscillations before recombination. This cosmological Nordtvedt effect alters the odd peaks height of the CMB temperature anisotropy power spectrum. A gravitational baryonic mass density of the universe may already be inferred at the first peak scale from the analysis of WMAP data. Experimental constraints on a primordial SEP violation are derived from a comparison with the universe's inertial baryonic mass density measured either in a full analysis of the CMB, or in the framework of the standard big bang nucleosynthesis (BBN). | |
| dc.description | Version accepted for publication in Phys. Rev. D, 8 pages, Revtex 4; discussion of "Experimental constraints" extended, references added, typos corrected | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0407208 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0407208 | |
| dc.identifier | Phys.Rev. D70 (2004) 103528 | |
| dc.identifier | doi:10.1103/PhysRevD.70.103528 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/7940 | |
| dc.subject | Astrophysics | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Cosmic microwave background constraints on the strong equivalence principle | |
| dc.type | text |