Reduced photothermal heating in diamonds enriched with H3 point defects

Author:

Pant Anupum1,Gupta Chaman1ORCID,Senkalla Katharina2ORCID,Felsted Greg3,Xia Xiaojing4,Spohn Tobias2,Dunham Scott T.5,Jelezko Fedor2,Pauzauskie Peter J.16ORCID

Affiliation:

1. Department of Materials Science and Engineering, University of Washington, Seattle, Washington 98195, USA

2. Institute for Quantum Optics, Ulm University, Albert-Einstein-Allee 11, 89081 Ulm, Germany

3. Department of Chemistry, University of Washington, Seattle, Washington 98195, USA

4. Molecular Engineering & Sciences Institute, University of Washington, Seattle, Washington 98195, USA

5. Department of Electrical and Computer Engineering, University of Washington, Seattle, Washington 98195, USA

6. Physical & Computational Sciences Directorate, Pacific Northwest National Laboratory, Richland, Washington 99354, USA

Abstract

Solid-state laser refrigeration of semiconductors remains an outstanding experimental challenge. In this work, we show that, following excitation with a laser wavelength of 532 nm, bulk diamond crystals doped with H3 centers both emit efficient up-conversion (anti-Stokes) photoluminescence and also show significantly reduced photothermal heating relative to crystals doped with nitrogen–vacancy (NV) centers. The H3 center in diamond is a highly photostable defect that avoids bleaching at high laser irradiances of 10–70 MW/cm[Formula: see text] and has been shown to exhibit laser action, tunable over the visible band of 500–600 nm. The observed reduction of photothermal heating arises due to a decrease in the concentration of absorbing point defects, including NV-centers. These results encourage future exploration of techniques for H3 enrichment in diamonds under high-pressure, high-temperature conditions for the simultaneous anti-Stokes fluorescence cooling and radiation balanced lasing in semiconductor materials. Reducing photothermal heating in diamond through the formation of H3 centers also opens up new possibilities in quantum sensing via optically detected magnetic resonance spectroscopy at ambient conditions.

Funder

Fedor Jelezko acknowledges additional support from the following sources: ERC, DFG, and BMBF.

Publisher

AIP Publishing

Subject

General Physics and Astronomy

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