PIRSA:08070008

Quasar absorption line constraints on variable fundamental constants

(2008). Quasar absorption line constraints on variable fundamental constants. Perimeter Institute. https://pirsa.org/08070008

Quasar absorption line constraints on variable fundamental constants. Perimeter Institute, Jul. 14, 2008, https://pirsa.org/08070008 

          @misc{ pirsa_PIRSA:08070008,
            doi = {10.48660/08070008},
            url = {https://pirsa.org/08070008},
            author = {},
            keywords = {Particle Physics, Cosmology},
            language = {en},
            title = {Quasar absorption line constraints on variable fundamental constants},
            publisher = {Perimeter Institute},
            year = {2008},
            month = {jul},
            note = {PIRSA:08070008 see, \url{https://pirsa.org}}
          }
Talk number
PIRSA:08070008
Collection
Talk Type
Subject
Abstract
I will review the published quasar absorption line constraints on variations in the fine-structure constant, alpha, focusing on the apparent disagreement between those derived from Keck/HIRES and VLT/UVES spectra which have provided evidence for and against alpha variation, respectively. I demonstrate simple yet fundamental flaws in the UVES constraints which preclude reliable comparison with those from HIRES. I will outline our program to obtain a definitive UVES measurement. I will also present several new absorption line constraints on variations in the proton-to-electron mass ratio, mu. For the two molecular hydrogen absorbers from which previous authors found tentative evidence for mu-variation, we find robustly null results. A further two molecular hydrogen absorbers, including an entirely new system, also yield tight, null constraints. Finally, I present new, detailed comparison of a radio absorption system containing ammonia inversion and molecular rotational transitions which yields the strongest current astrophysical constraint on mu-variation, dmu/mu=[mu(z)-mu(lab)]/mu(lab)=[+0.74+/-0.47(stat)+/-0.76(sys)]x10^-6, at redshift z=0.685.