Discrete Self-Similarity Of RR Lyrae Stars II. Period Spectrum For A Very Large Sample
| dc.creator | Oldershaw, R. L. | |
| dc.date | 2006-06-06 | |
| dc.date.accessioned | 2026-07-07T07:12:08Z | |
| dc.date.available | 2026-07-07T07:12:08Z | |
| dc.description | A recent paper demonstrated a considerable degree of self-similarity between RR Lyrae stars and their atomic scale analogues: excited helium atoms undergoing single-level transition between n = 7 and n = 10. Discrete self-similarity between these fractal analogues was indentified in terms of their masses, radii, oscillation periods, basic morphologies and kinematics. In this second paper on the subject, an extremely large and carefully analyzed sample of RR Lyrae oscillation periods provides further evidence for a unique match between the predicted set of discrete periods, based exclusively on the known helium spectrum and the discrete scaling equations of a fractal cosmological paradigm, and the observed period spectra of RR Lyrae stars. | |
| dc.description | 8 Pages, 1 Figure, 2 Tables, comments/criticism welcome | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0606128 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0606128 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/111982 | |
| dc.subject | Astrophysics | |
| dc.title | Discrete Self-Similarity Of RR Lyrae Stars II. Period Spectrum For A Very Large Sample | |
| dc.type | text |