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14 October 2024
 
  » arxiv » astro-ph/0510147

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Self-Similarity Between RR Lyrae Stars And Their Constituent Helium Atoms
R. L. Oldershaw ;
Date 5 Oct 2005
Subject Astrophysics; Chaotic Dynamics; Atomic Physics | astro-ph nlin.CD physics.atom-ph
AbstractThe masses, radii and oscillation periods of RR Lyrae variable stars and the counterpart parameters of helium atoms undergoing single-level transitions between Rydberg states are shown to obey discrete self-similar scaling relations. The agreement between observed period distributions for the two classes of systems appears to be unique.
Source arXiv, astro-ph/0510147
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