abstract
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% \centering
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% \includegraphics[width=\linewidth]{TOC}
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We provide a global overview of the successive steps that made possible to obtain increasingly accurate excited-state energies and properties, eventually leading to chemically accurate excitation energies.
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We describe
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i) the evolution of ab initio reference methods, e.g., originally CASPT2 (Roos, Serrano-Andres in the 1990's), then high-level CCn (as in the
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acclaimed Thiel benchmark series in the 2000's), and now selected CI methods thanks to their resurgence in the past five years;
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ii) how these high-level methods have allowed to assess fairly and accurately the performances of lower-order methods, e.g., ADC,
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TD-DFT and BSE;
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iii) the current potentiality of these various methods from both an expert and non-expert points of view;
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iv) what we believe could be the future developments in the field.
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We provide a global overview of the successive steps that made possible to obtain increasingly accurate excited-state energies and properties, eventually leading to chemically-accurate excitation energies for small- and medium-size molecules.
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First, we describe the evolution of \textit{ab initio} state-of-the-art methods, with originally Roos' CASPT2 method, and then third-order coupled cluster methods as in the renowned Thiel set of excitation energies described in a remarkable series of papers in the 2000's.
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More recently, this quest for highly accurate excitation energies was reinitiated thanks to the resurgence of selected configuration interaction (SCI) methods and their efficient parallel implementation.
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These methods have been able to routinely deliver highly-accurate excitation energies for small molecules as well as medium-size molecules in small basis sets for single and double excitations.
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Second, we describe how these high-level methods and the creation of large, broad and accurate benchmark sets of excitation energies have allowed to assess fairly and accurately the performances of lower-order methods (\eg, TD-DFT, BSE, ADC, EOM-CC, etc) for different types of excited states.
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We conclude this \textit{Perspective} by discussing the current potentiality of these methods from both an expert and a non-expert point of view, and what we believe could be the future theoretical and technological developments in the field.
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\end{abstract}
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\maketitle
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@ -95,7 +93,7 @@ The factors that makes this quest for high accuracy particularly delicate are ve
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First of all (and maybe surprisingly), it is, in most cases, tricky to obtain reliable and accurate experimental data that one can straightforwardly compare to theoretical values.
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In the case of vertical excitation energies, \ie, excitation energies at a fixed geometry, band maxima does not usually match theoretical values as one needs to take into account geometric relaxation and zero-point vibrational energy motion.
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Even more problematic, experimental spectra might not be available in gas phase, and, in the worst-case scenario, wrong assignments may have occured.
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Even more problematic, experimental spectra might not be available in gas phase, and, in the worst-case scenario, wrong assignments may have occurred.
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For a more faithful comparison between theory and experiment, although more computationally demanding, the so-called 0-0 energies are definitely a safer playground. \cite{Loo19b}
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%However, they require, from a theoretical point of view, access to the optimised excited-state geometry as well as its harmonic vibration frequencies.
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