Research

neutron star
In a strong magnetic field (such as generated by neutron stars), the H2 molecule tunnels between two equilvalent orientations.  The instanton pathway depicted passes through complex-valued positions.

Simulating the dynamics of large molecules has been one of the key goals of theoretical chemistry. Although classical molecular dynamics has been successful in many cases, it falls short in accounting for quantum-mechanical effects, such as tunnelling and nonadiabatic transitions. It is known that these effects can not only dramatically affect the rate of a chemical reaction but also change the reaction mechanism.

In principle, fully quantum-mechanical methods give exact results, but in practice, they are only applicable to small molecules or simplified models. The key challenge is thus to account for quantum-mechanical behaviour for large complex systems with a computational efficiency similar to that of classical approaches.

Semiclassical instanton theory

Representation of instanton

Calculating the rates of chemical reactions including quantum tunnelling effects and nonadiabatic transitions

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Tunnelling in water clusters

hexamer tunnelling dynamics

Simulating tunnelling dynamics in molecular clusters

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Nonadiabatic Rate Theory

Representation of nonadiabatic RPMD

Extending instanton theory to nonadiabatic processes such as Fermi's golden rule and beyond

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Mapping Approach to Surface Hopping (MASH)

mash_deniele

A rigorous mixed quantum–classical trajectory approach for nonadiabatic dynamics

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Polaritonic Chemistry

Molecules in mirrors!

Understanding quantum effects within a cavity

 

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