Ultrafast excited-state dynamics of promising nucleobase ancestor 2,4,6-triaminopyrimidine

Quantum mechanics/molecular mechanics studies on mechanistic photophysics of cytosine aza-analogues: 2,4-diamino-1,3,5-triazine and 2-amino-1,3,5-triazine in aqueous solution

The excited-state properties and photophysics of cytosine aza-analogues, i.e., 2,4-diamino-1,3,5-triazine (2,4-DT) and 2-amino-1,3,5-triazine (2-AT) in solution have been systematically explored using the QM(MS-CASPT2//CASSCF)/MM approach. The excited-state nonradiative relaxation mechanisms for the initially photoexcited S₁(ππ*) state decay back to the S₀ state are proposed in terms of the present computed minima, surface crossings (conical intersections and singlet-triplet crossings), and excited-state decay paths in the S₁, S₂, T₁, T₂, and S₀ states. Upon photoexcitation to the bright S₁(ππ*) state, 2,4-DT quickly relaxes to its S₁ minimum and then overcomes a small energy barrier of 5.1 kcal mol^-1 to approach a S₁/S₀ conical intersection, where the S₁ system hops to the S₀ state through S₁ → S₀ internal conversion (IC). In addition, at the S₁ minimum, the system could partially undergo intersystem crossing (ISC) to the T₁ state, followed by further ISC to the S₀ state via the T₁/S₀ crossing point. In the T₁ state, an energy barrier of 7.9 kcal mol^-1 will trap 2,4-DT for a while. In parallel, for 2-AT, the system first relaxes to the S₁ minimum and then S₁ → S₀ IC or S₁ → T₁ → S₀ ISCs take place to the S₀ state by surmounting a large barrier of 15.3 kcal mol^-1 or 11.9 kcal mol^-1, respectively, which heavily suppress electronic transition to the S₀ state. Different from 2,4-DT, upon photoexcitation in the Franck-Condon region, 2-AT can quickly evolve in an essentially barrierless manner to nearby S₂/S₁ conical intersection, where the S₂ and T₁ states can be populated. Once it hops to the S₂ state, the system will overcome a relatively small barrier (6.6 kcal mol^-1vs. 15.3 kcal mol^-1) through IC to the S₀ state. Similarly, an energy barrier of 11.9 kcal mol^-1 heavily suppresses the T₁ state transformation to the S₀ state. The present work manifests that the amination/deamination of the triazine rings can affect some degree of different vertical and adiabatic excitation energies and nonradiative decay pathways in solution. It not only rationalizes excited-state decay dynamics of 2,4-DT and 2-AT in aqueous solution but could also provide insights into the understanding of the photophysics of aza-nucleobases.

Solvent assisted excited-state deactivation pathways in isolated 2,7-diazaindole-S1-3 (S = Water and Ammonia) complexes

The role of solvent molecules in the deactivation of photo-excited 2,7-diazaindole (DAI) - (H₂O)_1-3 and DAI - (NH₃)_1-3 complexes were computationally investigated. An excited-state proton transfer (ESPT) path from the solvent to the DAI molecule was followed using the TD-DFT-D4 (B3LYP) level of theory. The computed potential energy profile of ESPT process has shown intersection between ππ* and nπ* states facilitated via relative stabilization of the nπ* state with decreasing N(7)-H_b bond length. The ESPT process, starting from the DAI-S_n (ππ*) state, crosses through a barrier ranging from 27 to 36 kJmol^-1 for water complexes and 26-30 kJmol^-1 for ammonia complexes. The energy of the excited state was rapidly decreased with a shorter N(7)-H_b bond length. Subsequently, a significant trend of finding a second intersection between the ground and the excited state was observed for all the complexes. The results firmly suggested a significant deactivation channel of excited azaindole derivatives. In the present system, two competing channels, ESPT and ESHT, were found to be energetically accessible. The energy barriers associated with the ESPT barriers for DAI-(H₂O)_1-3 complexes are similar to the ESHT barrier, depicting equal dominance of both processes. The increased basicity of the N(7) atom in the excited state resulted a facile ESPT process from the water to N(7) of the DAI molecule. However, DAI-(NH₃)_1-3 complexes show clear preference for ESHT over ESPT process owing to its higher gas-phase pK_a value making it a poor proton donor. The above systems can be used as a model to computationally and experimentally investigate the competing radiative and deactivation pathways of photo-excited solvated complexes of N-H-bearing bio-relevant molecules via proton and hydrogen transfer reactions.

On the Photostability of Cyanuric Acid and Its Candidature as a Prebiotic Nucleobase

Cyanuric acid is a triazine derivative that has been identified from reactions performed under prebiotic conditions and has been proposed as a prospective precursor of ancestral RNA. For cyanuric acid to have played a key role during the prebiotic era, it would have needed to survive the harsh electromagnetic radiation conditions reaching the Earth’s surface during prebiotic times (≥200 nm). Therefore, the photostability of cyanuric acid would have been crucial for its accumulation during the prebiotic era. To evaluate the putative photostability of cyanuric acid in water, in this contribution, we employed density functional theory (DFT) and its time-dependent variant (TD-DFT) including implicit and explicit solvent effects. The calculations predict that cyanuric acid has an absorption maximum at ca. 160 nm (7.73 eV), with the lowest-energy absorption band extending to ca. 200 nm in an aqueous solution and exhibiting negligible absorption at longer wavelengths. Excitation of cyanuric acid at 160 nm or longer wavelengths leads to the population of S_5,6 singlet states, which have ππ* character and large oscillator strengths (0.8). The population reaching the S_5,6 states is expected to internally convert to the S_1,2 states in an ultrafast time scale. The S_1,2 states, which have nπ* character, are predicted to access a conical intersection with the ground state in a nearly barrierless fashion (ca. ≤ 0.13 eV), thus efficiently returning the population to the ground state. Furthermore, based on calculated spin–orbit coupling elements of ca. 6 to 8 cm⁻¹, the calculations predict that intersystem crossing to the triplet manifold should play a minor role in the electronic relaxation of cyanuric acid. We have also calculated the vertical ionization energy of cyanuric acid at 8.2 eV, which predicts that direct one-photon ionization of cyanuric acid should occur at ca. 150 nm. Collectively, the quantum-chemical calculations predict that cyanuric acid would have been highly photostable under the solar radiation conditions reaching the Earth’s surface during the prebiotic era in an aqueous solution. Of relevance to the chemical origin of life and RNA-first theories, these observations lend support to the idea that cyanuric acid could have accumulated in large quantities during the prebiotic era and thus strengthens its candidature as a relevant prebiotic nucleobase.