Probing the Gravitational Dependence of the Fine-Structure Constant from Observations of White Dwarf Stars
Hot white dwarf stars are the ideal probe for a relationship between the fine-structure constant and strong gravitational fields, providing us with an opportunity for a direct observational test. We study a sample of hot white dwarf stars, combining far-UV spectroscopic observations, atomic physics,...
Main Authors: | , , , , , , , , , , , , , , |
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Other Authors: | |
Language: | en |
Published: |
MDPI AG
2017
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Subjects: | |
Online Access: | http://hdl.handle.net/10150/625061 http://arizona.openrepository.com/arizona/handle/10150/625061 |