Fine-structure constant variability: surprises for laboratory atomic spectroscopy and cosmological evolution of quasar spectra

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

RevTeX, 4 pages

Scientific paper

Calculation of the Dirac hydrogen atom spectrum in the framework of dynamical fine structure constant (alpha) variability discloses a small departure in the laboratory from Sommerfeld's formula for the fine structure shifts, possibly measurable today. And for a distant object in the universe, the wavelength shift of a spectral line specifically ascribable to cosmological alpha variation is found to depend differently on the quantum numbers than in the conventional view. This last result clashes with the conventional wisdom that an atom's spectrum can change with cosmological time only through evolution of the alpha parameter in the energy eigenvalue formula, and thus impacts on the Webb group's analysis of fine structure intervals in quasar absorption lines (which has been claimed to disclose cosmological alpha evolution). In particular, analyzing together a mix of quasar absorption lines from different fine structure multiplets can bias estimates of cosmological alpha variability.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Fine-structure constant variability: surprises for laboratory atomic spectroscopy and cosmological evolution of quasar spectra does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Fine-structure constant variability: surprises for laboratory atomic spectroscopy and cosmological evolution of quasar spectra, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Fine-structure constant variability: surprises for laboratory atomic spectroscopy and cosmological evolution of quasar spectra will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-679289

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.