Quantum chemistry of the excited state: recent trends in methods developments and applications

Advances (2016–2017) in Quantum Chemistry of the Excited State (QCEX) are presented in this book chapter focusing firstly on developments of methodology and excited-state reaction-path computational strategies and secondly on the applications of QCEX to study light–matter interaction in distinct fields of biology, (nano)-technology, medicine and the environment. We highlight in this contribution developments of static and dynamic electron-correlation methods and methodological approaches to determine dynamical properties, recent examples of the roles of conical intersections, novel DNA spectroscopy and photochemistry findings, photo-sensitisation mechanisms in biological structures and the current knowledge on chemi-excitation mechanisms that give rise to light emission (in the chemiluminescence and bioluminescence phenomena)

Photochemistry of oxidized Hg(I) and Hg(II) species suggests missing mercury oxidation in the troposphere

Mercury (Hg), a global contaminant, is emitted mainly in its elemental form Hg0 to the atmosphere where it is oxidized to reactive HgII compounds, which efficiently deposit to surface ecosystems. Therefore, the chemical cycling between the elemental and oxidized Hg forms in the atmosphere determines the scale and geographical pattern of global Hg deposition. Recent advances in the photochemistry of gas-phase oxidized HgI and HgII species postulate their photodissociation back to Hg0 as a crucial step in the atmospheric Hg redox cycle. However, the significance of these photodissociation mechanisms on atmospheric Hg chemistry, lifetime, and surface deposition remains uncertain. Here we implement a comprehensive and quantitative mechanism of the photochemical and thermal atmospheric reactions between Hg0, HgI, and HgII species in a global model and evaluate the results against atmospheric Hg observations. We find that the photochemistry of HgI and HgII leads to insufficient Hg oxidation globally. The combined efficient photoreduction of HgI and HgII to Hg0 competes with thermal oxidation of Hg0, resulting in a large model overestimation of 99% of measured Hg0 and underestimation of 51% of oxidized Hg and ∼66% of HgII wet deposition. This in turn leads to a significant increase in the calculated global atmospheric Hg lifetime of 20 mo, which is unrealistically longer than the 3–6-mo range based on observed atmospheric Hg variability. These results show that the HgI and HgII photoreduction processes largely offset the efficiency of bromine-initiated Hg0 oxidation and reveal missing Hg oxidation processes in the troposphere

Experimental and theoretical studies on thymine photodimerization mediated by oxidatively generated DNA lesions and epigenetic intermediates

Support from the Université de Lorraine, CNRS, regional (Prometeo/2017/075) and Spanish Government (PGC2018-096684-B-I00, CTQ2017-87054-C2-2-P) is kindly acknowledged. A. F.-M. is grateful to Generalitat Valenciana and the European Social Fund (postdoctoral contract APOSTD/2019/149 and project GV/2020/226) for financial support. M. L.-R. acknowledges the Universitat Politècnica de València for the FPI grant. All calculations have been performed on the local LPCT computer center and on the Explor regional center in the framework of the project “Dancing under the light”

Mechanism of excited state deactivation of indan-1-ylidene and fluoren-9-ylidene malononitriles

A joint experimental and computational study on the non-radiative double bond isomerisation decay channel of indan-1-ylidene malononitrile and fluoren-9-ylidene malononitrile is presented in this work.</p

Triplet stabilization for enhanced drug photorelease from sunscreen-based photocages

Recently, sunscreen-based drug photocages have been introduced to provide UV protection to photoactive drugs, thus increasing their photosafety. Here, combined experimental and theoretical studies performed on a photocage based on the commercial UVA filter avobenzone (AB) and on the photosensitizing non-steroidal anti-inflammatory drug ketoprofen (KP) are presented unveiling the photophysical processes responsible for the light-triggered release. Particular attention is paid to solvent stabilization of the drug and UV filter excited states, respectively, which leads to a switching between the triplet excited state energies of the AB and KP units. Most notably, we show that the stabilization of the AB triplet excited state in ethanol solution is the key requirement for an efficient photouncaging. By contrast, in apolar solvents, in particular hexane, KP has the lowest triplet excited state, hence acting as an energy acceptor quenching the AB triplet manifold, thus inhibiting the desired photoreaction.Support from the Université de Lorraine, CNRS, regional (Prometeo/2017/075) and Spanish Government (PGC2018-096684-B-I00, CTQ2017-87054-C2-2-P) is kindly acknowledged. A. F.-M. is grateful to Generalitat Valenciana and the European Social Fund (postdoctoral contract APOSTD/2019/149 and project GV/2020/226) for financial support. M. L.-R. acknowledges the Universitat Politècnica de València for the FPI grant. All calculations have been performed on the local LPCT computer center and on the Explor regional center in the framework of the project “Dancing under the light”

Theoretical study on the photo-oxidation and photoreduction of an azetidine derivative as a model of dna repair

Photocycloreversion plays a central role in the study of the repair of DNA lesions, reverting them into the original pyrimidine nucleobases. Particularly, among the proposed mechanisms for the repair of DNA (6-4) photoproducts by photolyases, it has been suggested that it takes place through an intermediate characterized by a four-membered heterocyclic oxetane or azetidine ring, whose opening requires the reduction of the fused nucleobases. The specific role of this electron transfer step and its impact on the ring opening energetics remain to be understood. These processes are studied herein by means of quantum-chemical calculations on the two azetidine stereoisomers obtained from photocycloaddition between 6-azauracil and cyclohexene. First, we analyze the efficiency of the electron-transfer processes by computing the redox properties of the azetidine isomers as well as those of a series of aromatic photosensitizers acting as photoreductants and photo-oxidants. We find certain stereodifferentiation favoring oxidation of the cis-isomer, in agreement with previous experimental data. Second, we determine the reaction profiles of the ring-opening mechanism of the cationic, neutral, and anionic systems and assess their feasibility based on their energy barrier heights and the stability of the reactants and products. Results show that oxidation largely decreases the ring-opening energy barrier for both stereoisomers, even though the process is forecast as too slow to be competitive. Conversely, one-electron reduction dramatically facilitates the ring opening of the azetidine heterocycle. Considering the overall quantum-chemistry findings, N,N-dimethylaniline is proposed as an efficient photosensitizer to trigger the photoinduced cycloreversion of the DNA lesion model.This work has been funded by the Generalitat Valenciana and the European Social Fund through the postdoctoral contract APOSTD/2019/149 and the project GV/2020/226. It also was funded by the Spanish Ministerio de Ciencia e Innovación (MICINN), projects CTQ2017-87054-C2-2-P and PGC2018-096684-B-I00, and a 2019 Leonardo Grant for Researchers and Cultural Creators, BBVA Foundation. The Foundation takes no responsibility for the opinions, statements, and contents of this project, which are entirely the responsibility of its authors. D.R.-S. is grateful to the Spanish MICINN for the “Ramón y Cajal” grant (Ref. RYC-2015-19234). M.N.-M. acknowledges the Generalitat Valenciana for the predoctoral grant (Ref. ACIF/2020/075).Peer reviewe

Photochromic System among Boron Hydrides: The Hawthorne Rearrangement

Photoswitchable molecules have attracted wide interest for many applications in chemistry, physics, and materials science. In this work, we revisit the reversible photochemical and thermal rearrangements of the two BH isomers reported by Hawthorne and Pilling in 1966, whose mechanism had not been understood so far. We investigate the rearrangements by means of a joint experimental and computational study with the outcome that BH represents the first boron-based photochromic system ever reported. Both photochemical and thermal isomerizations occur through the same intermediate and involve a diamond-square-diamond (DSD) mechanism. Given the absence within boron chemistry of named chemical reactions as opposed to organic chemistry, we propose to label the BH photo- A nd thermal isomerization processes as the Hawthorne rearrangement

Photochemical and thermochemical pathways to S2 and polysulfur formation in the atmosphere of Venus

8 pags., 3 figs.Polysulfur species have been proposed to be the unknown near-UV absorber in the atmosphere of Venus. Recent work argues that photolysis of one of the (SO) isomers, cis-OSSO, directly yields S with a branching ratio of about 10%. If correct, this pathway dominates polysulfur formation by several orders of magnitude, and by addition reactions yields significant quantities of S, S, and S. We report here the results of high-level ab-initio quantum-chemistry computations that demonstrate that S is not a product in cis-OSSO photolysis. Instead, we establish a novel mechanism in which S is formed in a two-step process. Firstly, the intermediate SO is produced by the coupling between the S and Cl atmospheric chemistries (in particular, SO reaction with ClS) and in a lesser extension by O-abstraction reactions from cis-OSSO. Secondly, SO reacts with SO. This modified chemistry yields S and subsequent polysulfur abundances comparable to the photolytic cis-OSSO mechanism through a more plausible pathway. Ab initio quantification of the photodissociations at play fills a critical data void in current atmospheric models of Venus.Calculations have been partially conducted at the local QCEXVAL cluster and the Lluis Vives v2 and Tirant v3 superclusters of the Servei d’Informàtica (University of Valencia), and at the local LPCT cluster and the regional ExpLor center (University of Lorraine, France). A.F.-M. thanks Generalitat Valenciana and the European Social Fund for the post-doctoral contract APOSTD/2019/149 and the project GV/2020/226, and the Ministerio de Ciencia e Innovación (MICINN) for the Juan de la Cierva contract IJC2019-039297-I. D.R.-S. is grateful to the MICINN for the project CTQ2017-87054-C2-2-P and the Ramón y Cajal grant RYC2015- 19234. The project that gave rise to these results received also the support of a fellowship for J.C.-G. from “la Caixa” Foundation (ID 100010434); the fellowship code is LCF/BQ/DR20/11790027

Photochemistry of HOSO2and SO3and Implications for the Production of Sulfuric Acid

9 pags., 5 figs.Sulfur trioxide (SO3) and the hydroxysulfonyl radical (HOSO2) are two key intermediates in the production of sulfuric acid (H2SO4) on Earth's atmosphere, one of the major components of acid rain. Here, the photochemical properties of these species are determined by means of high-level quantum chemical methodologies, and the potential impact of their light-induced reactivity is assessed within the context of the conventional acid rain generation mechanism. Results reveal that the photodissociation of HOSO2 occurs primarily in the stratosphere through the ejection of hydroxyl radicals (•OH) and sulfur dioxide (SO2). This may decrease the production rate of H2SO4 in atmospheric regions with low O2 concentration. In contrast, the photostability of SO3 under stratospheric conditions suggests that its removal efficiency, still poorly understood, is key to assess the H2SO4 formation in the upper atmosphere.The project that gave rise to these results received the support of a fellowship for J.C.-G. from “la Caixa” Foundation (ID 100010434); the fellowship code is LCF/BQ/DR20/11790027. This work was supported by the Spanish “Ministerio de Ciencia e Innovación (MICINN)” (Project ref. CTQ2017-87054-C2-2-P) and Unit of Excellence María de Maeztu CEX2019-000919-M). D.R.-S. is grateful to the Spanish MICINN for the “Ramón y Cajal” grant (ref. RYC2015-19234). A.F.-M. is grateful to the Generalitat Valenciana and the European Social Fund for the postdoctoral contract APOSTD/2019/149 and the project GV/2020/226, and to the MICINN for the “Juan de la Cierva” contract IJC2019-039297-I. Computations have been partially conducted at the local QCEXVAL cluster and the Tirant v3 supercluster (Servei d’Informatica of the University of Valencia)

Triplet Stabilization for Enhanced Drug Photorelease from Sunscreen-Based Photocages

The importance of the relative triplet excited state energies of avobenzone (our phenacyl-like photolabile group) and ketoprofen (our photocaged drug) has been demonstrated by means of spectroscopic experiments and theoretical calculations. , Recently, sunscreen-based drug photocages have been introduced to provide UV protection to photoactive drugs, thus increasing their photosafety. Here, combined experimental and theoretical studies performed on a photocage based on the commercial UVA filter avobenzone (AB) and on the photosensitizing non-steroidal anti-inflammatory drug ketoprofen (KP) are presented unveiling the photophysical processes responsible for the light-triggered release. Particular attention is paid to solvent stabilization of the drug and UV filter excited states, respectively, which leads to a switching between the triplet excited state energies of the AB and KP units. Most notably, we show that the stabilization of the AB triplet excited state in ethanol solution is the key requirement for an efficient photouncaging. By contrast, in apolar solvents, in particular hexane, KP has the lowest triplet excited state, hence acting as an energy acceptor quenching the AB triplet manifold, thus inhibiting the desired photoreaction