Plasma Redshift of Photons

Mathematics – Logic

Scientific paper

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Scientific paper

Plasma redshift of photons in extended, hot, sparse plasma is given by ln ( 1+z )=3.326\cdot 10-25\cdot int_0^R N_e\cdot dx., provided that the wavelength λ <= λ _cut-off≈ 7.12\cdot 10-6\cdot √ N_e/T cm, where Ne is the electron density in cm-3, T in ^0K, and R the distance in cm to the emitter. The theory is based on an overlooked interaction of photons with hot sparse electron plasma. It has been overlooked, because the conditions (high temperature and low densities over extended dimensions) necessary for its observation cannot be created in laboratory experiments. Its large magnitude when integrated over astronomical dimensions, nevertheless, has profound implications for our understanding of many astrophysical phenomena, including: the solar redshift, solar corona, transition to the corona and the outer limits of the heliosphere, the redshift of white dwarfs and quasars, and the cosmological redshift. A long series of experiments, including the recently discovered dimming of distant super nova, confirm the theory.

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