1984
DOI: 10.1016/0022-5088(84)90291-1
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High pressure electrical resistivity of HgCr2Se4

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Cited by 10 publications
(12 citation statements)
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“…A simple extrapolation of the existing curves yields zero E g values either at 80 GPa (dE g /dP = -0.0165 eV/GPa, AFM1) or 57 GPa (dE g /dP = -0.032 eV/GPa, AFM2). This electronic behavior is rather different compared to other Cr-spinels, where pressure-induced insulator-metal transitions at lower pressures are reported 18,21,24,25 .…”
Section: Figmentioning
confidence: 69%
See 1 more Smart Citation
“…A simple extrapolation of the existing curves yields zero E g values either at 80 GPa (dE g /dP = -0.0165 eV/GPa, AFM1) or 57 GPa (dE g /dP = -0.032 eV/GPa, AFM2). This electronic behavior is rather different compared to other Cr-spinels, where pressure-induced insulator-metal transitions at lower pressures are reported 18,21,24,25 .…”
Section: Figmentioning
confidence: 69%
“…The straightforward effect of compression is the reduction of the Cr-Cr distances, which in turn causes the enhancement of the AFM J 1 interactions over the FM J 2 ones. Besides from tuning the magnetic interactions, pressure can also lead to structural [18][19][20][21][22][23] , electronic 21,24,25 , and even magnetic 21 27 . A red-shift of E g was detected below T C 27 , but without any apparent complementary structural effect 5,28 .…”
Section: Introductionmentioning
confidence: 99%
“…20,23 Given this close interrelation between structural, vibrational, magnetic, and charge degrees of freedom, the variation of lattice by external pressure provides an appealing method for tuning the physical properties of these materials. Actually, several studies report structural [24][25][26] and electronic [26][27][28] transitions under pressure for various Cr-based spinels.…”
mentioning
confidence: 99%
“…In certain cases, electronic changes, e.g. insulator-to-metal [13][14][15][16] or semiconductor-to-semiconductor 17 transitions have been reported. On the other hand, the magnetic interactions of the oxide spinels with magnetic A 2+ cations are more complex, since one needs to consider also the A 2+ -Cr 3+ and the more distant A 2+ -A 2+ magnetic exchange interactions 2,4,18 .…”
Section: Introductionmentioning
confidence: 99%