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Our research is focused on theoretical modeling of open-shell
molecules. Since chemical transformations involve bond-breaking,
radicals and diradicals are often encountered as reaction intermediates
or transition states. Therefore, they play a central role in mechanistic
understanding of processes important in the environment, synthetic
chemistry, material science, biochemistry, etc. Since these open-shell
species are often very reactive and short-lived, their experimental
observations are difficult. That is why electronic structure theory is
a valuable tool for studying their properties.
Equation-of-motion (EOM) is a versatile electronic structure approach
that allows one to describe many multi-configurational wave functions
within a single-reference formalism. For example, EOM for excitation
energies (EOM-EE) method accurately describes electronically excited
states, while ionized/electron attached EOM models (EOM-IP/EA) can
tackle doublet radicals, including notorious cases of symmetry breaking.
We have extended EOM approach to diradicals, triradicals, and
bond-breaking.
In our approach, which is called the Spin-Flip (SF method) problematic
low-spin states are treated as spin-flipping excitations from the
high-spin reference state.
We are fascinated by electronic structure and bonding in triradicals,
species with three unpaired electrons.
To model angular distributions of photoelectrons, we implemented the
calculation of Dyson orbitals using EOM-EE/IP/EA-CCSD.
Electron transfer reactions are common in biological and synthetic
polymers. The rates of these processes can be related to the coupling
between the diabatic electronic states that correspond to reactant and
product states. Calculations on these systems are difficult due
to the propensity of Hartree-Fock solutions to overlocalize charge and
break symmetry.
As a part of spectroscopy modeling unit of programs, we develop a code for wavepacket propagation.
We characterized the ground and electronically excited states of cyclic N3+ at
the equilibrium D3h geometry and along Jahn-Teller distortions.

Electronic structure of radicals that play important role in atmosphere,
combustion, and catalysis
Radicals are ubiquitous in chemistry, and it is not surprising that
they play an important role in atmosphere (think ozone) and in catalysis
(after all, it is all about breaking and making bonds).
We are studying
the electronic structure of small halogen-containing radicals
(CH2Cl, CH2F, etc.) that are involved into the
ozone depletion process in collaboration with the
experimental group of
Prof. Hanna Reisler (USC).
In collaboration with
Prof. Andrei Vilesov group
(USC), we investigate bond activation in prototypical systems,
e. g., Al-ethylene clusters.
Vinyl radicals are of great practical and theoretical interest. They
are important intermediates in high-temperature combustion,
photochemistry of interstellar nebulae, and photochemical smog
formation in the Earth's atmosphere. Recent experiments done by
the Laurie Butler
group at Chicago have found that photolysis of halogenated precursors
produces these radicals in an electronically excited state.
Take it or leave it, but real chemistry does happen in condensed
phases! In particular, aqueous radicals are implicated in atmospheric
chemistry (HOO, ClO, NO3), radiation chemistry
(water coolant in nuclear reactors), and enzymatic processes (Tyr).
In collaboration with several experimental and theoretical groups,
complex photodissociation dynamics of the NO dimer were uncovered.
(NO)2 is unstable at room temperature, but exists in cold
atmospheres and on cold surfaces, where it behaves differently than
the NO radical. It strongly absorbs UV radiation and falls apart.
Carbon trioxide plays an important role in atmospheric chemistry and
has been detected in interstellar ices. However, its ground state
symmetry has eluded both experimental and computational chemists
for decades.
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