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Computer simulations of biotic chiral selection scenarios

Published online by Cambridge University Press:  14 March 2022

Savino Longo*
Affiliation:
Dipartimento di Chimica, Università degli Studi di Bari Aldo Moro, Via Orabona 4–70125, Bari, Italy Istituto per la Scienza e Tecnologia dei Plasmi – Consiglio Nazionale delle Ricerche, Bari Section – Via Amendola 122/D – 70125, Bari, Italy
Carmela Mundo
Affiliation:
Dipartimento di Bioscienze Biotecnologie e Biofarmaceutica, Università degli Studi di Bari Aldo Moro, Via Orabona 4–70125, Bari, Italy
Gaia Micca Longo
Affiliation:
Dipartimento di Chimica, Università degli Studi di Bari Aldo Moro, Via Orabona 4–70125, Bari, Italy Istituto per la Scienza e Tecnologia dei Plasmi – Consiglio Nazionale delle Ricerche, Bari Section – Via Amendola 122/D – 70125, Bari, Italy
*
Author for correspondence: Savino Longo, E-mail: savino.longo@uniba.it
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Abstract

The biotic scenario of the selection of biological homochirality is one of the most interesting applications of computer modelling to astrobiology. These scenarios have been studied for more than 70 years, yet there are plenty of studies to better assess them, in particular in the development of models of the selective extinction process. In this paper, we review former studies performed by biology-grounded models of this process and present a new class of computer programs: they further demonstrate the complexity of the selective extinction dynamics and the role played into it by non-trivial chemical-physical concepts. Indeed, the results display large and persistent differences between the populations of the two different chiral types, made possible by the freedom of individual populations to fluctuate wildly while the total population is stabilized by the limited availability of chemical energy. Such strong differences ultimately lead to the selective extinction of one of the two types. This way, computer simulations provide increasing evidence in favour of the biotic scenario.

Information

Type
Research Article
Creative Commons
Creative Common License - CCCreative Common License - BY
This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted re-use, distribution and reproduction, provided the original article is properly cited.
Copyright
Copyright © The Author(s), 2022. Published by Cambridge University Press
Figure 0

Fig. 1. An artistic interpretation of the alpha-helix in proteins: a spring-shaped structure formed by amino acids, linked by the peptide bond between carbon and nitrogen, and by the hydrogen bonds between oxygen and hydrogen. For good stability of the alpha-helix, the bulky R groups do not occupy the same space: this is possible when the amino acids are either all L or all D.

Figure 1

Fig. 2. The evolutionary Palmiter model as a model of the genesis of homochirality: one of the two chiral types colonize the source of nutrition at the centre; the other type become extinct. On the right, the interpretation of the phenomenon as instability, which randomly chooses one of the two types. Figure from (Longo and Coppola, 2013).

Figure 2

Fig. 3. Top: the population of each of two replicator types L (deep blue) and D (cyan) in a typical run of the simulation code. Bottom: the average availability of chemical energy. All simulations end with a selective extinction event. Note, in this case, the persistent advantage of the deep blue types in the second half of the simulation, and their sudden arising at about t  =  800 after a chaotic stage.

Figure 3

Fig. 4. Two stages of the simulation are shown in Fig. 3. The central circle in any square of the boards represents one of the two types (cyan or deep blue), or an empty square (white). The periphery of each square displays the available chemical energy: purple corresponds to the lowest level, green to the highest level (abundance of nutrients).