TY - JOUR
T1 - An observational determination of the proton to electron mass ratio in the early universe
AU - Thompson, Rodger I.
AU - Bechtold, Jill
AU - Black, John H.
AU - Eisenstein, Daniel
AU - Fan, Xiaohui
AU - Kennicutt, Robert C.
AU - Martins, Carlos
AU - Prochaska, J. Xavier
AU - Shirley, Yancey L.
PY - 2009
Y1 - 2009
N2 - In an effort to resolve the discrepancy between two measurements of the fundamental constant μ, the proton to electron mass ratio, at early times in the universe we reanalyze the same data used in the earlier studies. Our analysis of the molecular hydrogen absorption lines in archival Very Large Telescope/Ultraviolet and Visible Echelle Spectrometer (UVES) spectra of the damped Lyman alpha systems in the quasi-stellar objects Q0347-383 and Q0405-443 yields a combined measurement of a Δμ/μ value of (-7 8) × 10-6, consistent with no change in the value of μ over a time span of 11.5 Gyr. Here, we define Δμ as (μz - μ0) where μz is the value of μ at a redshift of z and μ0 is the present-day value. Our null result is consistent with the recent measurements of King etal., Δμ/μ = (2.6 3.0) × 10-6, and inconsistent with the positive detection of a change in μ by Reinhold etal. Both of the previous studies and this study are based on the same data but with differing analysis methods. Improvements in the wavelength calibration over the UVES pipeline calibration is a key element in both of the null results. This leads to the conclusion that the fundamental constant μ is unchanged to an accuracy of 10-5 over the last 80% of the age of the universe, well into the matter dominated epoch. This limit provides constraints on models of dark energy that invoke rolling scalar fields and also limits the parameter space of supersymmetric or string theory models of physics. New instruments, both planned and under construction, will provide opportunities to greatly improve the accuracy of these measurements.
AB - In an effort to resolve the discrepancy between two measurements of the fundamental constant μ, the proton to electron mass ratio, at early times in the universe we reanalyze the same data used in the earlier studies. Our analysis of the molecular hydrogen absorption lines in archival Very Large Telescope/Ultraviolet and Visible Echelle Spectrometer (UVES) spectra of the damped Lyman alpha systems in the quasi-stellar objects Q0347-383 and Q0405-443 yields a combined measurement of a Δμ/μ value of (-7 8) × 10-6, consistent with no change in the value of μ over a time span of 11.5 Gyr. Here, we define Δμ as (μz - μ0) where μz is the value of μ at a redshift of z and μ0 is the present-day value. Our null result is consistent with the recent measurements of King etal., Δμ/μ = (2.6 3.0) × 10-6, and inconsistent with the positive detection of a change in μ by Reinhold etal. Both of the previous studies and this study are based on the same data but with differing analysis methods. Improvements in the wavelength calibration over the UVES pipeline calibration is a key element in both of the null results. This leads to the conclusion that the fundamental constant μ is unchanged to an accuracy of 10-5 over the last 80% of the age of the universe, well into the matter dominated epoch. This limit provides constraints on models of dark energy that invoke rolling scalar fields and also limits the parameter space of supersymmetric or string theory models of physics. New instruments, both planned and under construction, will provide opportunities to greatly improve the accuracy of these measurements.
KW - Early universe
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U2 - 10.1088/0004-637X/703/2/1648
DO - 10.1088/0004-637X/703/2/1648
M3 - Article
AN - SCOPUS:70549087073
SN - 0004-637X
VL - 703
SP - 1648
EP - 1662
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 2
ER -