2019
DOI: 10.1103/physreva.100.052702
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Universal three-body parameter of heavy-heavy-light systems with a negative intraspecies scattering length

Abstract: The three-body parameter (3BP) a (1) − is crucial for understanding Efimov physics, and a universal 3BP has been shown in experiments and theory in ultracold homonuclear gases. The 3BP of heteronuclear systems has been predicted to possess much richer properties than its homonuclear counterparts due to the larger parameter space. In this work, we investigate the universal properties of a (1) − for heavy-heavy-light (HHL) systems with a negative intraspecies scattering length a HH . We find that a (1) − follows… Show more

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Cited by 9 publications
(6 citation statements)
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“…The few-body aspects of heteronuclear mixtures attracted significant interest in the last decade, both theoretical [11][12][13][14][15][16][17][18][19][20][21] and experimental [22][23][24][25][26][27][28][29]. The 6 Li-133 Cs mixture is the most extreme mass imbalanced system in which Efimov features were observed up to date making it favorable for the attempt to reveal the few-body physics at a narrow Feshbach resonance.…”
Section: Introductionmentioning
confidence: 99%
“…The few-body aspects of heteronuclear mixtures attracted significant interest in the last decade, both theoretical [11][12][13][14][15][16][17][18][19][20][21] and experimental [22][23][24][25][26][27][28][29]. The 6 Li-133 Cs mixture is the most extreme mass imbalanced system in which Efimov features were observed up to date making it favorable for the attempt to reveal the few-body physics at a narrow Feshbach resonance.…”
Section: Introductionmentioning
confidence: 99%
“…Apart from this, mass-imbalanced ensembles offer a large parameter space, such as the particles' mass ratio, the sign and magnitude of the inter-and intra-species scattering lengths, which provide fertile ground to investigate the pristine attributes of the Efimov states. Specifically, theoretical and experimental efforts have mapped out a large portion of the parameter space, addressing the underlying physics of recombination processes in heavy-heavy-light (HHL) systems [26,27,[29][30][31][32]. The particular case that stands out corresponds to HHL systems that possess inter-and intra-species scattering lengths of opposite sign, i.e., a HL < 0 and a HH > 0, respectively.…”
Section: Introductionmentioning
confidence: 99%
“…Apart from that, mass-imbalanced ensembles offer a large parameter space, such as the particles' mass-ratio, the sign and magnitude of the interand intra-species scattering lengths, which provide fertile ground to investigate pristine attributes of the Efimov states. Specifically, theoretical and experimental efforts have mapped out a large portion of the parameter space addressing the underlying physics of recombination processes in heavy-heavy-light (HHL) systems [27,28,[30][31][32][33]. The particular case which stands out corresponds to HHL systems that possess inter-and intraspecies scattering lengths of opposite sign, i.e.…”
Section: Introductionmentioning
confidence: 99%