Microscopic dissipative structuring and proliferation at the origin of life


Por: Michaelian, Karo

Publicada: 1 oct 2017
Categoría: Multidisciplinary

Resumen:
Some fundamental molecules of life are suggested to have been formed, proliferated, and evolved through photochemical microscopic dissipative structuring and autocatalytic proliferation under the UV-C/UV-B solar environment prevalent at Earth's surface throughout the Archean. Evidence is given in the numerous salient characteristics of these, including their strong absorption in this spectral region and their rapid non-radiative excited state decay through inherent conical intersections. The examples of the dissipative structuring and dissipative proliferation of the purines and of single strand DNA are given. UV-C and UV-B induced stationary state isomerizations and tautomerizations are shown to be crucial to the formation of the purines from hydrogen cyanide in an aqueous environment under UV-C light, while UV-C induced phosphorylation of nucleosides and denaturing of double helix RNA and DNA are similarly important to the production and proliferation of single strand DNA. This thermodynamic dissipation perspective provides a physical-chemical foundation for understanding the origin and evolution of life.

Filiaciones:
Michaelian, Karo:
 Department of Nuclear Physics and Application of Radiations, Instituto de Física, Universidad Nacional Autónoma de México, Apartado Postal 20–364, Cuidad de México, Mexico

 Univ Nacl Autonoma Mexico, Inst Fis, Dept Nucl Phys & Applicat Radiat, Apartado Postal 20-364, Cuidad De Mexico, Mexico
ISSN: 24058440
Editorial
Elsevier Ltd, THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, OXON, ENGLAND, Estados Unidos America
Tipo de documento: Article
Volumen: 3 Número: 10
Páginas:
WOS Id: 000432026800010
ID de PubMed: 29062973