Month-long-lifetime microwave spectral holes in an erbium-doped scheelite crystal at millikelvin temperature

Fuente: arXiv
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Autori principali: Wang, Zhiren, Lin, Sen, Dantec, Marianne Le, Rančić, Miloš, Goldner, Philippe, Bertaina, Sylvain, Chanelière, Thierry, Liu, Ren-Bao, Esteve, Daniel, Vion, Denis, Flurin, Emmanuel, Bertet, Patrice
Natura: Preprint
Pubblicazione: 2024
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author Wang, Zhiren
Lin, Sen
Dantec, Marianne Le
Rančić, Miloš
Goldner, Philippe
Bertaina, Sylvain
Chanelière, Thierry
Liu, Ren-Bao
Esteve, Daniel
Vion, Denis
Flurin, Emmanuel
Bertet, Patrice
author_facet Wang, Zhiren
Lin, Sen
Dantec, Marianne Le
Rančić, Miloš
Goldner, Philippe
Bertaina, Sylvain
Chanelière, Thierry
Liu, Ren-Bao
Esteve, Daniel
Vion, Denis
Flurin, Emmanuel
Bertet, Patrice
contents Rare-earth-ion (REI) ensembles in crystals have remarkable optical and spin properties characterized by narrow homogeneous linewidths relative to the inhomogeneous ensemble broadening. This makes it possible to precisely tailor the ensemble spectral density and therefore the absorption profile by applying narrow-linewidth radiation to transfer population into auxiliary levels, a process broadly known as spectral hole burning (SHB). REI-doped crystals find applications in information processing, both classical (pattern recognition, filtering, spectral analysis) and quantum (photon storage), all protocols requiring suitable ensemble preparation by SHB as a first step. In Er$^{3+}$-doped materials, the longest reported hole lifetime is one minute, and longer lifetimes are desirable. Here, we report SHB and accumulated echo measurements in a scheelite crystal of CaWO$_4$ by pumping the electron spin transition of Er$^{3+}$ ions at microwave frequencies and millikelvin temperatures, with nuclear spin states of neighboring $^{183}$W atoms serving as the auxiliary levels. The lifetime of the holes and accumulated echoes rises steeply as the sample temperature is decreased, exceeding a month at 10 mK. Our results demonstrate that millikelvin temperatures can be beneficial for signal processing applications requiring long spectral hole lifetimes.
format Preprint
id arxiv_https___arxiv_org_abs_2408_12758
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Month-long-lifetime microwave spectral holes in an erbium-doped scheelite crystal at millikelvin temperature
Wang, Zhiren
Lin, Sen
Dantec, Marianne Le
Rančić, Miloš
Goldner, Philippe
Bertaina, Sylvain
Chanelière, Thierry
Liu, Ren-Bao
Esteve, Daniel
Vion, Denis
Flurin, Emmanuel
Bertet, Patrice
Quantum Physics
Mesoscale and Nanoscale Physics
Rare-earth-ion (REI) ensembles in crystals have remarkable optical and spin properties characterized by narrow homogeneous linewidths relative to the inhomogeneous ensemble broadening. This makes it possible to precisely tailor the ensemble spectral density and therefore the absorption profile by applying narrow-linewidth radiation to transfer population into auxiliary levels, a process broadly known as spectral hole burning (SHB). REI-doped crystals find applications in information processing, both classical (pattern recognition, filtering, spectral analysis) and quantum (photon storage), all protocols requiring suitable ensemble preparation by SHB as a first step. In Er$^{3+}$-doped materials, the longest reported hole lifetime is one minute, and longer lifetimes are desirable. Here, we report SHB and accumulated echo measurements in a scheelite crystal of CaWO$_4$ by pumping the electron spin transition of Er$^{3+}$ ions at microwave frequencies and millikelvin temperatures, with nuclear spin states of neighboring $^{183}$W atoms serving as the auxiliary levels. The lifetime of the holes and accumulated echoes rises steeply as the sample temperature is decreased, exceeding a month at 10 mK. Our results demonstrate that millikelvin temperatures can be beneficial for signal processing applications requiring long spectral hole lifetimes.
title Month-long-lifetime microwave spectral holes in an erbium-doped scheelite crystal at millikelvin temperature
topic Quantum Physics
Mesoscale and Nanoscale Physics
url https://arxiv.org/abs/2408.12758