2017
DOI: 10.1103/physrevb.95.195116
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Electronic properties of Ba1xSrxV13O18

Abstract: We have studied the electronic structure of Ba1−xSrxV13O18(x = 0, 0.2, and 1) at different temperatures across the trimerization and charge order transitions by using hard x-ray photoemission spectroscopy (HAXPES) experiment. The V 2p HAXPES indicates V 2+ /V 3+ charge order and fluctuation in the high-temperature tetramer phase, low-temperature trimer phase, and intermediatetemperature charge order phase in the series of x = 0, 0.2, and 1. In the valence-band HAXPES, although the spectral weight at the Fermi … Show more

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Cited by 11 publications
(3 citation statements)
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“…However, the V 3d spectral distribution is rather broad in the experimental result and is not separated into V 2+ and V 3+ bands. Also the spectral weight near the Fermi level is rather large compared to the metallic phase of BaV 10 O 15 [32] and Ba 1−x Sr x V 13 O 18 [33]. Here, we speculate that the V 2+ and V 3+ components are highly mixed due to strong charge fluctuation along the face sharing bond.…”
Section: (B)mentioning
confidence: 75%
“…However, the V 3d spectral distribution is rather broad in the experimental result and is not separated into V 2+ and V 3+ bands. Also the spectral weight near the Fermi level is rather large compared to the metallic phase of BaV 10 O 15 [32] and Ba 1−x Sr x V 13 O 18 [33]. Here, we speculate that the V 2+ and V 3+ components are highly mixed due to strong charge fluctuation along the face sharing bond.…”
Section: (B)mentioning
confidence: 75%
“…In Since the superexchange pathways for the xy, yz, and zx orbitals are all active in the face sharing V-O-V bond, the V 3+ and V 2+ sites should have the antiferromagnetic coupling in agreement with the neutron result [13]. This situation is different from the ferromagnetic coupling between the face sharing V 3+ and V 2+ in BaV 10 O 15 and related systems where the a 1g orbital is unoccupied at the V 3+ site [22][23][24].…”
Section: Resultsmentioning
confidence: 99%
“…As O 1s spectral features change only slightly in the opposite direction at the lower binding edge between 300 K and 180 K, this indicates that the change between 300 K and 180 K is different from that at 120 K. The asymmetry parameter (α) is obtained with the Doniach-Sunjic function fitted to the O 1s spectra at 70, 180, 245, and 300 K, similarly adopted to O 1s in Ba 1x Sr x V 13 O 18 (Supplemental Material in ref. 31). The Doniach-Sunjic profile can be written as…”
Section: Resultsmentioning
confidence: 99%