Cosmological Variation of the Fine Structure Constant versus a new Interaction
英文摘要：
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.
机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。
