Singlet
fission (SF) has the potential to dramatically increase
solar cell efficiency by converting one singlet exciton to two free
triplet excitons via a correlated triplet pair intermediate. Identification
and characterization of excited states involved in SF are of great
importance for understanding the fundamentals of SF. Despite their
importance, it is still nontrivial to distinguish various species
in transient absorption spectra due to their spectral overlaps and
ultrashort lifetimes. Theoretical modeling of SF and its electronically
excited state absorption (ESA) is generally challenging due to the
multiexciton nature of the correlated triplet pair, which usually
requires description by expensive high-level ab initio methods. In this work, taking the bis((triisopropylsilyl)ethynyl)
(TIPS)-pentacene monomer and its covalently linked dimer as representative
examples, we demonstrate the use of single-reference DFT-based approaches
to simulate the ESA spectra during SF. In particular, the singlet
and triplet ESA are evaluated by TDDFT, QR-TDDFT, SLR-TDDFT, SF-TDDFT,
and UTDDFT, in combination with ten different exchange–correlation
functionals. The correlated triplet pair and its ESA are characterized
by broken-symmetry DFT and TDDFT, and the role of orbital relaxation
is highlighted. With a rational choice of exchange–correlation
functionals, we found the resulting spectra to show good agreement
with transient absorption experiments and certain improvements over
high-order CI methods.