Prediction of photodynamics of 200 nm excited cyclobutanone with linear response electronic structure and ab initio multiple spawning

Author:

Hait Diptarka12ORCID,Lahana Dean12ORCID,Fajen O. Jonathan12ORCID,Paz Amiel S. P.12ORCID,Unzueta Pablo A.12ORCID,Rana Bhaskar12ORCID,Lu Lixin12ORCID,Wang Yuanheng12ORCID,Kjønstad Eirik F.123ORCID,Koch Henrik3ORCID,Martínez Todd J.12ORCID

Affiliation:

1. Department of Chemistry and The PULSE Institute, Stanford University 1 , Stanford, California 94305, USA

2. SLAC National Accelerator Laboratory 2 , Menlo Park, California 94024, USA

3. Department of Chemistry, Norwegian University of Science and Technology 3 , Trondheim 7491, Norway

Abstract

Simulations of photochemical reaction dynamics have been a challenge to the theoretical chemistry community for some time. In an effort to determine the predictive character of current approaches, we predict the results of an upcoming ultrafast diffraction experiment on the photodynamics of cyclobutanone after excitation to the lowest lying Rydberg state (S2). A picosecond of nonadiabatic dynamics is described with ab initio multiple spawning. We use both time dependent density functional theory (TDDFT) and equation-of-motion coupled cluster singles and doubles (EOM-CCSD) theory for the underlying electronic structure theory. We find that the lifetime of the S2 state is more than a picosecond (with both TDDFT and EOM-CCSD). The predicted ultrafast electron diffraction spectrum exhibits numerous structural features, but weak time dependence over the course of the simulations.

Funder

Basic Energy Sciences

Stanford Science Fellows Program

Advanced Scientific Computing Research

Directorate for Mathematical and Physical Sciences

National Energy Research Scientific Computing Center

Norwegian Research Council

Horizon 2020 Framework Program

Publisher

AIP Publishing

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