Propagation of light: Coherent or Monte-Carlo computation ?
Jacques Moret-Bailly

TL;DR
This paper argues that coherent optical effects, rather than Monte Carlo methods, better explain light propagation in nebulae, accounting for observed phenomena without invoking new physics.
Contribution
It introduces the use of coherent interactions in astrophysical contexts, replacing Monte Carlo calculations to improve accuracy and explain observations.
Findings
Superradiance causes the nebula's limb to appear as a dotted circle.
Coherent effects explain frequency shifts in solar and stellar spectra.
No need for new physics to account for observed astrophysical phenomena.
Abstract
Wrong Monte-Carlo computations are used to study the propagation of light in low pressure gas of nebulae. We recall that the incoherent interactions required for Monte Carlo calculations and hindering coherent interactions are due to collisions that disappear at low pressure. Incoherent interactions blur the images while coherent do not. We introduce coherent optical effects or substitute them for Monte Carlo calculations in published papers, improving the results and avoiding the introduction of "new physics". The spectral radiance of novae has the magnitude of the radiance of lasers, and large column densities are available in the nebulae. Several types of coherent interactions (superradiance, multiphoton effects, etc..), well studied using lasers, work in nebulae as in laboratories. The relatively thin shell of plasma containing atoms around a Str\^omgren sphere is…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Geophysics and Sensor Technology · Astro and Planetary Science
