Thermodynamic Explanation for the Cosmic Ubiquity of Organic Pigments
Karo Michaelian, Aleksandar Simeonov

TL;DR
This paper proposes a thermodynamic framework explaining the widespread presence of organic pigments in the cosmos, emphasizing their role in dissipating stellar radiation and increasing entropy, which may also relate to dark matter and the origins of life.
Contribution
It introduces a non-equilibrium thermodynamic explanation for the cosmic ubiquity of organic pigments based on their catalytic properties in photon dissipation.
Findings
Organic molecules are abundant in various cosmic environments.
Pigments' absorption spectra relate to local stellar radiation.
Some dark matter may consist of undetected infrared-emitting molecules.
Abstract
There is increasingly more evidence being accumulated for the occurrence of large amounts of organic material in the cosmos, particularly in the form of aromatic compounds. These molecules can be found on the surface of Earth and Mars, in the atmospheres of the larger planets and on many of their satellites, on asteroids, comets, meteorites, the atmospheres of red giant stars, interstellar nebulae, and in the spiral arms of galaxies. Many of these environments are expected to be of low temperature and pressure, implying that the Gibbs free energy for the formation of these complex molecules should be positive and large, suggesting that their existence could only be attributed to non-equilibrium thermodynamic processes. In this article we first review the evidence for the abundance of these molecules in the cosmos and then describe how the ubiquity can be explained from within the…
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