dorsal/arxiv
View SchemaCosmological Variation of the Fine Structure Constant versus a new Interaction
| Authors | E. J. Angstmann, V. V. Flambaum, S. G. Karshenboim |
|---|---|
| Categories | |
| ArXiv ID | physics/0403009 |
| URL | https://arxiv.org/abs/physics/0403009 |
| DOI | 10.1103/PhysRevA.70.044104 |
Abstract
We show why a dynamically varying fine structure constant does not impact on the Webb group's analysis as suggested by Bekenstein. We also provide a limit on the size of a possible correction to the Dirac Hamiltonian caused by a perturbation due to a dynamically varying alpha in hydrogen.
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"abstract": "We show why a dynamically varying fine structure constant does not impact on\nthe Webb group\u0027s analysis as suggested by Bekenstein. We also provide a limit\non the size of a possible correction to the Dirac Hamiltonian caused by a\nperturbation due to a dynamically varying alpha in hydrogen.",
"arxiv_id": "physics/0403009",
"authors": [
"E. J. Angstmann",
"V. V. Flambaum",
"S. G. Karshenboim"
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"doi": "10.1103/PhysRevA.70.044104",
"title": "Cosmological Variation of the Fine Structure Constant versus a new Interaction",
"url": "https://arxiv.org/abs/physics/0403009"
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