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    Gas-Phase Cytosine and Cytosineā€‘N<sub>1</sub>ā€‘Derivatives Have 0.1ā€“1 ns Lifetimes Near the S<sub>1</sub> State Minimum

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    Ultraviolet radiative damage to DNA is inefficient because of the ultrafast S<sub>1</sub> ā‡ S<sub>0</sub> internal conversion of its nucleobases. Using picosecond pumpā€“ionization delay measurements, we find that the S<sub>1</sub>(<sup>1</sup><i>Ļ€Ļ€</i>*) state vibrationless lifetime of gas-phase keto-amino cytosine (Cyt) is Ļ„ = 730 ps or āˆ¼700 times longer than that measured by femtosecond pumpā€“probe ionization at higher vibrational excess energy, <i>E</i><sub>exc</sub>. N<sub>1</sub>-Alkylation increases the S<sub>1</sub> lifetime up to Ļ„ = 1030 ps for N<sub>1</sub>-ethyl-Cyt but decreases it to 100 ps for N<sub>1</sub>-isopropyl-Cyt. Increasing the vibrational energy to <i>E</i><sub>exc</sub> = 300ā€“550 cm<sup>ā€“1</sup> decreases the lifetimes to 20ā€“30 ps. The nonradiative dynamics of S<sub>1</sub> cytosine is not solely a property of the amino-pyrimidinone chromophore but is strongly influenced by the N<sub>1</sub>-substituent. Correlated excited-state calculations predict that the gap between the S<sub>2</sub>(<sup>1</sup><i>n</i><sub>O</sub>Ļ€*) and S<sub>1</sub>(<sup>1</sup><i>Ļ€Ļ€</i>*) states decreases along the series of N<sub>1</sub>-derivatives, thereby influencing the S<sub>1</sub> state lifetime
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