Possible evidence for a variable fine-structure constant from QSO absorption lines: systematic errors

被引:113
作者
Murphy, MT [1 ]
Webb, JK
Flambaum, VV
Churchill, CW
Prochaska, JX
机构
[1] Univ New S Wales, Sch Phys, Sydney, NSW 2052, Australia
[2] Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA
[3] Observ Carnegie Inst Washington, Pasadena, CA 91101 USA
关键词
atomic data; line : profiles; instrumentation : spectrographs; methods : data analysis; techniques : spectroscopic; quasars : absorption lines;
D O I
10.1046/j.1365-8711.2001.04841.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Comparison of quasar (QSO) absorption spectra with laboratory spectra allows us to probe possible variations in the fundamental constants over cosmological time-scales. In a companion paper we present an analysis of Keck/HIRES spectra and report possible evidence suggesting that the fine-structure constant, alpha, may have been smaller in the past: Delta alpha/alpha = (-0.72 +/- 0.18) x 10(-5) over the redshift range 0.5 < z < 3.5. In this paper we describe a comprehensive investigation into possible systematic effects. Most of these do not significantly influence our results. When we correct for those which do produce a significant systematic effect in the data, the deviation of Delta alpha/alpha from zero becomes more significaut. We are led increasingly to the interpretation that alpha was slightly smaller in the past.
引用
收藏
页码:1223 / 1236
页数:14
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