Fundamental limitations on photoisomerization from thermodynamic resource theories
- Creators
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Yunger Halpern, Nicole
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Limmer, David T.
Abstract
Small, out-of-equilibrium, and quantum systems defy simple thermodynamic expressions. Such systems are exemplified by molecular switches, which exchange heat with a bath. These molecules can photoisomerize, or change conformation, or switch, on absorbing light. The photoisomerization probability depends on kinetic details that couple the molecule's energetics to its dissipation. Therefore, a simple, general, thermodynamic-style bound on the photoisomerization probability seems out of reach. We derive such a bound using a resource theory. The resource-theory framework is a set of mathematical tools, developed in quantum information theory, used to generalize thermodynamics to small and quantum settings. From this toolkit has been derived a generalization of the second law, the thermomajorization preorder. We use thermomajorization to upper-bound the photoisomerization probability. Then, we compare the bound with an equilibrium prediction and with a Lindbladian model. We identify a realistic parameter regime in which the Lindbladian evolution saturates the thermomajorization bound. We also quantify the energy coherence in the electronic degree of freedom, and we argue that this coherence cannot promote photoisomerization. This work illustrates how quantum-information-theoretic thermodynamics can elucidate complex quantum processes in nature, experiments, and synthetics.
Additional Information
© 2020 American Physical Society. Received 9 December 2019; revised manuscript received 9 March 2020; accepted 13 March 2020; published 17 April 2020. N.Y.H. thanks Bassam Helou, David Jennings, Christopher Perry, and Mischa Woods for helpful conversations. N.Y.H. is grateful for funding from the Institute for Quantum Information and Matter, an NSF Physics Frontiers Center (NSF Grant No. PHY-1125565) with support from the Gordon and Betty Moore Foundation (GBMF-2644), for a Barbara Groce Graduate Fellowship, for a KITP Graduate Fellowship (the KITP receives support from the NSF under Grant No. NSF PHY-1125915), and for an NSF grant for the Institute for Theoretical Atomic, Molecular, and Optical Physics at Harvard University and the Smithsonian Astrophysical Observatory. D.T.L. was initially supported by the UC Berkeley College of Chemistry and by the Kavli Energy NanoSciences Institute. The later stage of this work was supported by the U.S. Department of Energy, Office of Science, Basic Energy Sciences, CPIMS Program Early Career Research Program under Award No. DE-FOA-0002019.Attached Files
Published - PhysRevA.101.042116.pdf
Submitted - 1811.06551.pdf
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Additional details
- Eprint ID
- 92769
- Resolver ID
- CaltechAUTHORS:20190207-150038978
- NSF
- PHY-1125565
- Gordon and Betty Moore Foundation
- GBMF-2644
- Barbara Groce Graduate Fellowship, Caltech
- Kavli Institute for Theoretical Physics
- NSF
- PHY-1125915
- Harvard University
- Smithsonian Astrophysical Observatory
- University of California, Berkeley
- Kavli Energy NanoSciences Institute
- Department of Energy (DOE)
- DE-FOA-0002019
- Created
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2019-02-15Created from EPrint's datestamp field
- Updated
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2021-11-16Created from EPrint's last_modified field
- Caltech groups
- Institute for Quantum Information and Matter