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25 April 2024
 
  » arxiv » astro-ph/0106194

 Article overview



A new constraint on cosmological variability of the proton-to-electron mass ratio
S. A. Levshakov ; M. Dessauges-Zavadsky ; S. D’Odorico ; P. Molaro ;
Date 12 Jun 2001
Journal Mon.Not.Roy.Astron.Soc. 333 (2002) 373
Subject astro-ph
AffiliationNAOJ, Mitaka, Tokyo; ESO, Garching, Germany; Osservatorio Astronomico di Trieste, Italy
AbstractExotic cosmologies predict variability of the fundamental physical constants over the cosmic time. Using the VLT/UVES high resolution spectra of the quasar Q0347-3819 and unblended electronic - vibrational - rotational lines of the H2 molecule identified at z = 3.025 we test possible changes in the proton - to - electron mass ratio mu_0 = m_p/m_e over the period of 11 Gyr. We obtained a new constraint on the time - averaged variation rate of mu_0 of |d mu /d t /mu_0| < 5 10^{-15} yr^{-1} (1 sigma c.l.). The estimated 1 sigma uncertainty interval of the |Delta mu/mu_0| ratio of about 0.004% implies that since the time when the H2 spectrum was formed at z = 3.025, mu_0 has not changed by more than a few thousands of a percent.
Source arXiv, astro-ph/0106194
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