Hydrogen Cyanide at the Onset of Prebiotic Chemical Reactivity
Doktorsavhandling, 2026

Hydrogen cyanide (HCN) is a unique molecule. It is ubiquitous in the universe, highly reactive, and capable of forming a diverse range of life's building blocks through self-reaction. Its solid phase is equally intriguing, as it has been observed to glow and exhibit electric discharges, likely driven by its strong polarity. While investigating these exceptional properties is crucial for astrochemistry and the origin of life, HCN's high toxicity and tendency to form intractable polymers have left its rich chemistry relatively unexplored. In this thesis, I employ quantum chemical methods to unravel the reactivity and solid-state properties of HCN.
 
The first part of this thesis focuses on the reactivity of HCN. An exploration of the thermodynamic landscape of its self-reaction reveals that while most products are thermodynamically favorable, several proposed polymerization pathways are endergonic. Among the most favored products are highly conjugated polymers and the nucleobase adenine. The kinetics of adenine formation is further investigated by comparing proposed base-catalyzed pathways in an HCN-rich environment. These results provide a kinetic explanation for the low adenine yields typically observed in experiments.
 
The second part concerns the HCN crystal, with a particular focus on Titan, where HCN ice is abundant. In this part of the thesis, crystal morphology and polar surface properties are investigated. The results suggest a high anisotropy of the crystal, making it grows into needle-shaped structures, whose tips can exert strong electric fields. These electric fields arise from the uncompensated electrostatic potential at the polar surfaces and are suggested to facilitate chemical transformations. Furthermore, the electronic structure of HCN polar surfaces shows the emergence of localized metallic surface states. This metallicity is transferred to chemisorbed water molecules, suggesting enhanced reactivity at the interface. This thesis provides insights into the exceptional properties of HCN in the context of prebiotic chemistry and astrochemistry.

Computational Chemistry

Diaminomaleonitrile

Origin of Life

Hydrogen Cyanide

Titan

Adenine

HCN-derived products

FB salen, Fysik huset
Opponent: Assistant Professor Thanja Lamberts, Leiden University, Leiden, Netherlands

Författare

Marco Cappelletti

Chalmers, Kemi och kemiteknik, Kemi och biokemi

A Thermodynamic Landscape of Hydrogen Cyanide-Derived Molecules and Polymers

ACS Earth and Space Chemistry,;Vol. 8(2024)p. 1272-1280

Artikel i vetenskaplig tidskrift

How Does Adenine Form from Hydrogen Cyanide?

Journal of the American Chemical Society,;Vol. 148(2026)p. 3949-3961

Artikel i vetenskaplig tidskrift

Electric Fields Can Assist Prebiotic Reactivity on Hydrogen Cyanide Surfaces

ACS Central Science,;Vol. 12(2026)p. 111-121

Artikel i vetenskaplig tidskrift

Cappelletti, M., Rahm, M., Hydrogen Cyanide Surfaces Can Turn Water Metallic

How did life emerge from non-living matter? This is the central puzzle of prebiotic chemistry, the study of the chemistry that led to life. At the heart of this mystery lies Hydrogen Cyanide (HCN), a molecule that is paradoxically a deadly poison to modern life, yet a central precursor to its origins. Uncovering its role in the origin of life is, however, difficult: not only is HCN highly toxic, but it also creates an unmanageable black "tar" that challenges experimental analysis. Thankfully, modern computer simulations allow us to bypass these problems. In this thesis, I use these computational tools to safely explore the reactions at the onset of prebiotic chemistry. I reveal how HCN can successfully form adenine, an essential letter in our genetic alphabet. Furthermore, I show that in cold environments HCN crystallizes into needle-shaped structures that generate intense electric fields capable of catalyzing chemical reactions. These findings are particularly relevant for cold worlds like Saturn’s moon Titan, suggesting that prebiotic chemistry can also take place in cold, alien environments.

Undersökning av prebiotiska ursprung för polypeptider och fasttillståndskemi på titan

Vetenskapsrådet (VR) (2024-05049), 2025-01-01 -- 2028-12-31.

Beräkning av astrobiologi: makromolekylernas uppkomst

Vetenskapsrådet (VR) (2020-04305), 2021-01-01 -- 2024-12-31.

Ämneskategorier (SSIF 2025)

Teoretisk kemi

Fysikalisk kemi

DOI

10.63959/chalmers.dt/5822

ISBN

978-91-8103-365-6

Doktorsavhandlingar vid Chalmers tekniska högskola. Ny serie: 5822

Utgivare

Chalmers

FB salen, Fysik huset

Opponent: Assistant Professor Thanja Lamberts, Leiden University, Leiden, Netherlands

Mer information

Senast uppdaterat

2026-01-27