Generalized Doppler formula in a nonstatic universe

Details Generalized Doppler formula in a nonstatic universe Generalized Doppler formula in a nonstatic universe

Jul 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977amjph..45..642g&link_type=abstract

American Journal of Physics, Volume 45, Issue 7, pp. 642-644 (1977).

Physics

1

Special Relativity

Scientific paper

The general Doppler formula in a nonstatic universe is derived, relating the expansion of the universe and the peculiar velocity of the light-emitting object to the shift of spectral lines measured by a fundamental observer. No reference to the Riemannian metric of general relativity is required; the only assumptions needed are special relativity, homogeneity, and isotropy of the universe. A few examples of applications to physical cosmology are given.

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