Cosmic Microwave Background

Details Cosmic Microwave Background Cosmic Microwave Background

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aps..apr.r9008b&link_type=abstract

American Physical Society, April Meeting, 2003, April 5-8, 2003 Philadelphia, Pennsylvania, MEETING ID: APR03, abstract #R9.008

Mathematics

Logic

Scientific paper

Large plasma redshifts of photons in hot, sparse plasma are given by ln ( 1+z )=3.326ot 10-25ot int_0^R N_eot dx., provided the wavelength λ ≤ λ_0.5 =3.185ot 10-6ot ( 1+1.296ot 10^5ot B^2/Ne )ot √ N_e/T cm, where Ne is the electron density in cm-3, T the temperature in K, R the distance in cm to the emitter, and B the magnetic field in Gauss. The cut-off at λ _0.5 means that the redshift is 50% of its full value. The theory is based on an overlooked interaction of photons with hot sparse electron plasma. It has been overlooked, because the necessary conditions (high temperature and low densities over extended dimensions) cannot be created in the laboratory. The plasma redshifts help explain: the heating of the transition to the corona, the coronal heating, solar redshifts (which invalidate the equivalence principle), galactic redshifts, the heating of galactic corona, the redshifts of white dwarfs and quasars, the cosmological redshifts, and the recently discovered dimming of distant super nova. This presentation will show how plasma redshift also helps explain the cosmic microwave background.

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