Chand, H. ; Srianand, R. ; Petitjean, P. ; Aracil, B. (2005) Probing the variation of the fine-structure constant using QSO absorption lines Proceedings of the International Astronomical Union, 1 . pp. 409-411. ISSN 1743-9213
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Related URL: http://dx.doi.org/10.1017/S1743921305002917
Abstract
Search for the time variation of the fundamental constants is motivated by various unification theories. Here we present constraints on the variation of the fine-structure constant α≡2/ ħc) obtained using UVES/VLT samples of QSO absorption systems. We find < Δα/α >w = (-0.06 ± 0.06) × 10-5 using 23 Mg II systems and the many-multiplet (MM) method. Well selected 15 Si IV systems provide < Δα/α >w = (0.15 ± 0.43) ×10-5. Absence of detectable variation in α is also confirmed by our new very high resolution (R ~ 100,000) observation of zabs = 1.1508 toward HE 0515-4414 using HARPS on the ESO 3.6m telescope.
Item Type: | Article |
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Source: | Copyright of this article belongs to Cambridge University Press. |
ID Code: | 55281 |
Deposited On: | 18 Aug 2011 07:58 |
Last Modified: | 18 May 2016 07:36 |
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