Power Dependence of the Magnetic Field Effect on Triplet Fusion: A Quantitative Model.


Journal

The journal of physical chemistry letters
ISSN: 1948-7185
Titre abrégé: J Phys Chem Lett
Pays: United States
ID NLM: 101526034

Informations de publication

Date de publication:
25 May 2023
Historique:
medline: 15 5 2023
pubmed: 15 5 2023
entrez: 15 5 2023
Statut: ppublish

Résumé

Two strategies for improving solar energy efficiencies, triplet fusion and singlet fission, rely on the details of triplet-triplet interactions. In triplet fusion, there are several steps, each of which is a possible loss mechanism. In solution, the parameters describing triplet fusion collisions are difficult to inspect. Here we show that these parameters can be determined by examining the magnetic field dependence of triplet fusion upconversion. We show that there is a reduction of the magnetic field effect for perylene triplet fusion as the system moves from the quadratic to linear annihilation regimes with an increase in laser power. Our data are modeled with a small set of parameters that characterize the triplet fusion dynamics. These parameters are cross-validated with molecular dynamics simulations. This approach can be applied to both solution and solid state materials, providing a tool for screening potential annihilators for photon upconversion.

Identifiants

pubmed: 37184362
doi: 10.1021/acs.jpclett.3c00919
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Pagination

4742-4747

Auteurs

Roslyn Forecast (R)

ARC Centre of Excellence in Exciton Science, School of Science, RMIT University, Melbourne, VIC 3001, Australia.

Elham M Gholizadeh (EM)

ARC Centre of Excellence in Exciton Science, School of Chemistry, The University of Melbourne, Parkville, VIC 3010, Australia.

Shyamal K K Prasad (SKK)

ARC Centre of Excellence in Exciton Science, School of Chemistry, The University of New South Wales, Kensington, NSW 2052, Australia.

Simon Blacket (S)

Department of Chemistry, School of Physical Sciences, The University of Adelaide, Adelaide, SA 5005, Australia.

Patrick C Tapping (PC)

Department of Chemistry, School of Physical Sciences, The University of Adelaide, Adelaide, SA 5005, Australia.

Dane R McCamey (DR)

ARC Centre of Excellence in Exciton Science, School of Physics, The University of New South Wales, Kensington, NSW 2052, Australia.

Murad J Y Tayebjee (MJY)

School of Photovoltaic and Renewable Energy Engineering, The University of New South Wales, Kensington, NSW 2052, Australia.

David M Huang (DM)

Department of Chemistry, School of Physical Sciences, The University of Adelaide, Adelaide, SA 5005, Australia.

Jared H Cole (JH)

ARC Centre of Excellence in Exciton Science, School of Science, RMIT University, Melbourne, VIC 3001, Australia.

Timothy W Schmidt (TW)

ARC Centre of Excellence in Exciton Science, School of Chemistry, The University of New South Wales, Kensington, NSW 2052, Australia.

Classifications MeSH