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Title: Constraint on a cosmological variation in the proton-to-electron mass ratio from electronic co absorption

Journal Article · · Astrophysical Journal
; ; ;  [1]
  1. Department of Physics and Astronomy, LaserLaB, Vrije Universiteit University, De Boelelaan 1081, 1081 HV Amsterdam (Netherlands)

Carbon monoxide (CO) absorption in the sub-damped Lyα absorber at redshift z{sub abs}≃2.69 toward the background quasar SDSS J123714.60+064759.5 (J1237+0647) was investigated for the first time in order to search for a possible variation of the proton-to-electron mass ratio, μ, over a cosmological timescale. The observations were performed with the Very Large Telescope/Ultraviolet and Visual Echelle Spectrograph with a signal-to-noise ratio of 40 per 2.5 km s{sup −1} per pixel at ∼5000 Å. Thirteen CO vibrational bands in this absorber are detected: the A{sup 1}Π − X{sup 1}Σ{sup +} (ν{sup ′}, 0) for ν{sup ′}=0--8, B{sup 1}Σ{sup +} − X{sup 1}Σ{sup +} (0, 0), C{sup 1}Σ{sup +} − X{sup 1}Σ{sup +} (0, 0), and E{sup 1}Π − X{sup 1}Σ{sup +} (0, 0) singlet–singlet bands and the d{sup 3}Δ − X{sup 1}Σ{sup +} (5, 0) singlet–triplet band. An updated database including the most precise molecular inputs needed for a μ-variation analysis is presented for rotational levels J = 0–5, consisting of transition wavelengths, oscillator strengths, natural lifetime damping parameters, and sensitivity coefficients to a variation of the proton-to-electron mass ratio. A comprehensive fitting method was used to fit all the CO bands at once and an independent constraint of Δμ/μ=(0.7±1.6{sub stat}±0.5{sub syst})×10{sup −5} was derived from CO only. A combined analysis using both molecular hydrogen and CO in the same J1237+0647 absorber returned a final constraint on the relative variation of Δμ/μ=(−5.6±5.6{sub stat}±3.1{sub syst})×10{sup −6}, which is consistent with no variation over a look-back time of ∼11.4 Gyr.

OSTI ID:
22868842
Journal Information:
Astrophysical Journal, Vol. 826, Issue 2; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 0004-637X
Country of Publication:
United States
Language:
English