2016
DOI: 10.1039/c6ra07835d
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Laser cooling of copper monofluoride: a theoretical study including spin–orbit coupling

Abstract: A laser cooling scheme is proposed for CuF by including the spin–orbit coupling effects, and based on our calculated radiative lifetimes and vibrational branching ratios.

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Cited by 10 publications
(4 citation statements)
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“…So far only a few molecules including SrF, CaF, and YO have been cooled to the ultracold temperature experimentally, and there is an urgent need to search for more suitable molecular candidates for laser cooling. Recently, a number of theoretical efforts have been made in searching for promising molecular laser cooling candidates (Wells and Lane, 2011a;Fu et al, 2016a;Cao et al, 2019;González-Sánchez et al, 2019;Xu et al, 2019). It is generally accepted (Di Rosa, 2004;Fu et al, 2016b) that, a suitable laser-cooling candidate must meet the following three criteria: highly diagonal Franck-Condon factors (FCFs), a short lifetime, and no intermediate electronic-state interference.…”
Section: Introductionmentioning
confidence: 99%
“…So far only a few molecules including SrF, CaF, and YO have been cooled to the ultracold temperature experimentally, and there is an urgent need to search for more suitable molecular candidates for laser cooling. Recently, a number of theoretical efforts have been made in searching for promising molecular laser cooling candidates (Wells and Lane, 2011a;Fu et al, 2016a;Cao et al, 2019;González-Sánchez et al, 2019;Xu et al, 2019). It is generally accepted (Di Rosa, 2004;Fu et al, 2016b) that, a suitable laser-cooling candidate must meet the following three criteria: highly diagonal Franck-Condon factors (FCFs), a short lifetime, and no intermediate electronic-state interference.…”
Section: Introductionmentioning
confidence: 99%
“…Radiative lifetimes of the same order of magnitude are also reported for other laser cooling candidates, such as CH 51,52 and CuF. 50 Moreover, the Doppler and recoil temperatures for the main cooling transition of AsH are 4.18 and 2.20 μK, respectively, and the corresponding values of SbH are 4.33 and 1.13 μK.…”
Section: Resultsmentioning
confidence: 53%
“…S3 (ESI†). Since the relative strengths of the photon loss pathways are more directly related to the vibrational branching ratios ( R ν ′ ν ) than f ν ′ ν in the laser cooling cycle, 50 we need to further check R ν ′ ν of the A 3 Π → X 3 Σ − transition. The Einstein A coefficients ( A ν ′ ν ) and R ν ′ ν of the A 3 Π 2 → X 3 Σ − 1 transition for AsH and SbH are calculated and presented in Tables 3 and 4, respectively.…”
Section: Resultsmentioning
confidence: 99%
“…The reason is that the relation between the relative strengths of the vibrational branching ratios and that between photon loss pathways are more direct than FCFs in the cooling cycle. [50][51][52] Thus, the cooling cycle with branching ratio R v v , which can be calculated by using the ratio of Einstein coefficients A v v for each vibronic transition, is expressed as…”
Section: Laser Cooling Of Chmentioning
confidence: 99%