2021
DOI: 10.1103/physrevlett.127.046401
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Charge Density Waves and Electronic Properties of Superconducting Kagome Metals

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Cited by 373 publications
(325 citation statements)
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“…The observed kink in the energy dispersion and the peak-dip-hump structure in EDCs are reminiscent of those from the electron–boson coupling in simple metal 46 and high-temperature superconductors 47 . The phonon frequency of the vanadium vibrations in AV 3 Sb 5 can reach up to ~36 meV 32 that is consistent with the mode energy we have observed. Therefore, we have observed significant self-energy effects in KV 3 Sb 5 .…”
Section: Resultssupporting
confidence: 91%
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“…The observed kink in the energy dispersion and the peak-dip-hump structure in EDCs are reminiscent of those from the electron–boson coupling in simple metal 46 and high-temperature superconductors 47 . The phonon frequency of the vanadium vibrations in AV 3 Sb 5 can reach up to ~36 meV 32 that is consistent with the mode energy we have observed. Therefore, we have observed significant self-energy effects in KV 3 Sb 5 .…”
Section: Resultssupporting
confidence: 91%
“…Besides the Fermi surface nesting, the CDW phase can also be driven by the concerted action of electronic and ionic subsystems where a q -dependent electron–phonon coupling plays an indispensable part 49 , 50 . In AV 3 Sb 5 system, the driving force for the CDW formation remains under debate 15 , 17 , 25 , 32 , 33 , 37 , 38 . Based on our observations, we found that the electron–phonon coupling plays a major role in generating the CDW phase in KV 3 Sb 5 .…”
Section: Discussionmentioning
confidence: 99%
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“…Previous first-principles calculation [28,41] in AV 3 Sb 5 has also confirmed that the 2 × 2 charge order is a bulk effect and is consistent with a hexamer and trimer formation [28] (or termed as inverse star of David formation [41]) in the V kagome lattice. The chirality feature of the charge order, however, is beyond the current first-principles calculation.…”
Section: Transport and Tunneling Resultssupporting
confidence: 61%
“…4(d)], with the leading instability at the L point. These phonon instabilities are B 1u modes, corresponding to a CDW state with a star of David (or its inverse) deformation of the kagome lattice [45], consistent with previous calculations for AV 3 Sb 5 [39,44]. Increasing pressure to 10 GPa in RbV 3 Sb 5 and 5 GPa in KV 3 Sb 5 [Figs.…”
Section: First-principles Calculations Of Phonon Spectrasupporting
confidence: 88%