“…A computational study by Safaei et al 20 In this work, we study the reactions of the nitrene intermediates (denoted here as sfGFP 66nF and Venus 66nF ) as part of the photochemistry of the phenyl azide variants of sfGFP and Venus using modern computational molecular modeling methods. Specifically, we use quantum mechanics/molecular mechanics (QM/MM) 21 and molecular dynamics (MD) with QM/MM potentials (QM/MM MD) 22 to estimate the reaction energy profiles and to reveal mechanisms of formation of the phenylamine chromophores.…”
A photochemical transformation to arylnitrene occurs in GFP variants with a non-canonical amino acid residue, p-azidophenylalanine, that replaces Tyr66. The arylnitrene reduction is coupled with the oxidation of the nearby His148 side chain.
“…A computational study by Safaei et al 20 In this work, we study the reactions of the nitrene intermediates (denoted here as sfGFP 66nF and Venus 66nF ) as part of the photochemistry of the phenyl azide variants of sfGFP and Venus using modern computational molecular modeling methods. Specifically, we use quantum mechanics/molecular mechanics (QM/MM) 21 and molecular dynamics (MD) with QM/MM potentials (QM/MM MD) 22 to estimate the reaction energy profiles and to reveal mechanisms of formation of the phenylamine chromophores.…”
A photochemical transformation to arylnitrene occurs in GFP variants with a non-canonical amino acid residue, p-azidophenylalanine, that replaces Tyr66. The arylnitrene reduction is coupled with the oxidation of the nearby His148 side chain.
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