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تسجيل مستخدم جديدThe UVES Large Program for Testing Fundamental Physics II: Constraints on a Change in {mu} Towards Quasar HE 0027-1836
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We present an accurate analysis of the H2 absorption lines from the zabs ~ 2.4018 damped Ly{alpha} system towards HE 0027-1836 observed with the Very Large Telescope Ultraviolet and Visual Echelle Spectrograph (VLT/UVES) as a part of the European Southern Observatory Large Programme The UVES large programme for testing fundamental physics to constrain the variation of proton-to-electron mass ratio, {mu} = mp/me. We perform cross-correlation analysis between 19 individual exposures taken over three years and the combined spectrum to check the wavelength calibration stability. We notice the presence of a possible wavelength dependent velocity drift especially in the data taken in 2012. We use available asteroids spectra taken with UVES close to our observations to confirm and quantify this effect. We consider single and two component Voigt profiles to model the observed H2 absorption profiles. We use both linear regression analysis and Voigt profile fitting where {Delta}{mu}/{mu} is explicitly considered as an additional fitting parameter. The two component model is marginally favored by the statistical indicators and we get {Delta}{mu}/{mu} = (-2.5 +/- 8.1(stat) +/- 6.2(sys)) ppm. When we apply the correction to the wavelength dependent velocity drift we find {Delta}{mu}/{mu} = (-7.6 +/- 8.1(stat) +/- 6.3(sys)) ppm. It will be important to check the extent to which the velocity drift we notice in this study is present in UVES data used for previous {Delta}{mu}/{mu} measurements.
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Absorption line systems detected in quasar spectra can be used to compare the value of the fine-structure constant, {alpha}, measured today on Earth with its value in distant galaxies. In recent years, some evidence has emerged of small temporal and
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