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Near-infrared absorption and radiative cooling of naphthalene dimers (C10H8)2
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Number of Authors: 132024 (English)In: Physical Chemistry, Chemical Physics - PCCP, ISSN 1463-9076, E-ISSN 1463-9084, Vol. 26, no 27, p. 18571-18583Article in journal (Refereed) Published
Abstract [en]

The radiative cooling of naphthalene dimer cations, (C10H8)2+ was studied experimentally through action spectroscopy using two different electrostatic ion-beam storage rings, DESIREE in Stockholm and Mini-Ring in Lyon. The spectral characteristics of the charge resonance (CR) band were observed to vary significantly with a storage time of up to 30 seconds in DESIREE. In particular, the position of the CR band shifts to the blue, with specific times (inverse of rates) of 0.64 s and 8.0 s in the 0–5 s and 5–30 s storage time ranges, respectively. These long-time scales indicate that the internal energy distribution of the stored ions evolves by vibrational radiative cooling, which is consistent with the absence of fast radiative cooling via recurrent fluorescence for (C10H8)2+. Density functional based tight binding calculations with local excitations and configuration interactions (DFTB-EXCI) were used to simulate the absorption spectrum for ion temperatures between 10 and 500 K. The evolution of the bandwidth and position with temperature is in qualitative agreement with the experimental findings. Furthermore, these calculations yielded linear temperature dependencies for both the shift and the broadening. Combining the relationship between the CR band position and the ion temperature with the results of the statistical model, we demonstrate that the observed blue shift can be used to determine the radiative cooling rate of (C10H8)2+.

Place, publisher, year, edition, pages
2024. Vol. 26, no 27, p. 18571-18583
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Physical Chemistry
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URN: urn:nbn:se:su:diva-238613DOI: 10.1039/d4cp01200cISI: 001260103800001PubMedID: 38949429Scopus ID: 2-s2.0-85197394465OAI: oai:DiVA.org:su-238613DiVA, id: diva2:1933019
Available from: 2025-01-30 Created: 2025-01-30 Last updated: 2025-01-30Bibliographically approved

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Ji, MingChaoZettergren, HenningCederquist, HenrikStockett, Mark H.Indrajith, Suvasthika

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