Radiation and Scattering of Massive Photons

With the aid of a modified Planck’s law for massive photons, it is shown that the ratio of the mean value of the photon mass equivalent to its rest (invariant) mass tends to be one with a decrease in temperature. A modified Stefan - Boltzmann law is obtained at different temperature regimes, as well as the Wien’s displacement law. At high temperatures the modified Planck’ s law approaches the standard Planck’ s law. It is also shown that the cross-section of the Thomson scattering slightly increases opacity of the scattering medium. The Compton shift in frequency for a massive photon appears to be frequency-dependent and slightly less than its value for a massless photon, except in the case of forward scattering when no change in frequency takes place. Astrophysical aspects of the massive photon hypothesis are discussed with regard to standard stellar models, early stages of the Universe, and the Breit-Weeler process, as well as active galactic nuclei. Estimates of the spreading time of the wave packet of the massive photon show that for frequencies ν ≥ 4.052 × 109Hz(λ ≤ 7.4) it exceeds the age of the Universe.

Authors

Publication Details

Journal
Communications of the Byurakan Astrophysical Observatory
Published
2024-12-27
DOI
https://doi.org/10.52526/25792776-24.71.2-307
Citations
1
Primary Topic
Quantum Electrodynamics and Casimir Effect
Type
article
Field-Weighted Citation Impact
0.34
Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

Radiation and Scattering of Massive Photons

G. A. Saiyan
1 citations
Communications of the Byurakan Astrophysical Observatory
Quantum Electrodynamics and Casimir Effect
0.34
article

Radiation and Scattering of Massive Photons

G. A. Saiyan
article en
1 citations

Abstract

With the aid of a modified Planck’s law for massive photons, it is shown that the ratio of the mean value of the photon mass equivalent to its rest (invariant) mass tends to be one with a decrease in temperature. A modified Stefan - Boltzmann law is obtained at different temperature regimes, as well as the Wien’s displacement law. At high temperatures the modified Planck’ s law approaches the standard Planck’ s law. It is also shown that the cross-section of the Thomson scattering slightly increases opacity of the scattering medium. The Compton shift in frequency for a massive photon appears to be frequency-dependent and slightly less than its value for a massless photon, except in the case of forward scattering when no change in frequency takes place. Astrophysical aspects of the massive photon hypothesis are discussed with regard to standard stellar models, early stages of the Universe, and the Breit-Weeler process, as well as active galactic nuclei. Estimates of the spreading time of the wave packet of the massive photon show that for frequencies ν ≥ 4.052 × 109Hz(λ ≤ 7.4) it exceeds the age of the Universe.

Communications of the Byurakan Astrophysical Observatory
Peace, Justice and strong institutions
Openalex Percentile: Top 37%
Quantum Electrodynamics and Casimir Effect
0.34
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.

Radiation and Scattering of Massive Photons — G. A. Saiyan · Communications of the Byurakan Astrophysical Observatory (2024) | TGRS Research Map | TGRS