Homogeneous linewidth behavior of narrow optical emitters at sub-kelvin temperatures

X X. Lin (Department of Engineering, University of Cambridge 1 , 9 JJ Thomson Avenue, Cambridge CB3 0FA,) M M. T. Hartman (Laboratoire Temps Espace (LNE-OP), Observatoire de Paris, Université PSL, Sorbonne Université, Université de Lille, LNE, CNRS 1 , 61 avenue de l’Observatoire, Paris 75014,) P P. Goldner (Chimie ParisTech, Université PSL, CNRS, Institut de Recherche de Chimie Paris 2 , 75005 Paris,) B B. Fang Y Y. Le Coq (LNE-SYRTE, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université 1 , Paris,) S S. Seidelin (University Grenoble Alpes, CNRS, Grenoble INP and Institut Néel 5 , 38000 Grenoble,)

Abstract

We explore the properties of ultranarrow spectral holes in ensembles of solid-state emitters in crystals over a range of sub-kelvin temperatures, as a new step toward leveraging their exceptional coherence properties more effectively. As an example, we consider the potential gain observed in their application in frequency stabilization schemes. We investigate how the parameters used to burn the spectral hole impact its shape, and how these factors determine the minimum achievable linewidth. In addition to the stability of the hole's center frequency, the linewidth and contrast play a crucial role in frequency locking. At sub-kelvin temperatures, the temperature-dependent T7 broadening from two-phonon Raman scattering is expected to be negligible, and the spectral hole's linewidth should therefore remain constant in this interval. We observe however a linear broadening with increasing temperature, highlighting the need for further investigation into the mechanisms governing the linewidth at ultra-low temperatures.

Article Details

Volume / Issue Vol. 126, Issue 5
Published February 03, 2025
ISSN 0003-6951
Publisher American Institute of Physics

Journal Info

Applied Physics Letters

American Institute of Physics

ISSN: 0003-6951 Physical Sciences

Authors (6)

X

X. Lin

Department of Engineering, University of Cambridge 1 , 9 JJ Thomson Avenue, Cambridge CB3 0FA,

M

M. T. Hartman

Laboratoire Temps Espace (LNE-OP), Observatoire de Paris, Université PSL, Sorbonne Université, Université de Lille, LNE, CNRS 1 , 61 avenue de l’Observatoire, Paris 75014,

P

P. Goldner

Chimie ParisTech, Université PSL, CNRS, Institut de Recherche de Chimie Paris 2 , 75005 Paris,

B

B. Fang

Y

Y. Le Coq

LNE-SYRTE, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université 1 , Paris,

S

S. Seidelin

University Grenoble Alpes, CNRS, Grenoble INP and Institut Néel 5 , 38000 Grenoble,