TY - JOUR
T1 - Compressibility of the HgBa2Can-1CunO2n+2+δ (n=1,2,3) high-temperature superconductors
AU - Eggert, J. H.
AU - Hu, J. Z.
AU - Mao, H. K.
AU - Beauvais, L.
AU - Meng, R. L.
AU - Chu, C. W.
N1 - Copyright:
Copyright 2015 Elsevier B.V., All rights reserved.
PY - 1994
Y1 - 1994
N2 - The transition temperatures (Tc) of the homologous series HgBa2Can-1CunO2n+2+δ of high-temperature superconductors show very large (∼30 K) pressure enhancements, saturating at 118, 154, and 164 K for Hg1201, Hg1212, and Hg1223, respectively. We have measured the compressibility of the first three mercury superconductors in a diamond-anvil cell using energy-dispersive synchrotron x-ray diffraction. We report the tetragonal-cell parameters a and c up to 30 GPa. We find ambient-pressure bulk moduli, KV0==-V0(P/V)0, of 65.4(3.0), 91.6(4.7), and 83.8(10.5) GPa for Hg1201, Hg1212, and Hg1223, respectively. The Hg superconductors are highly compressible compared to other high-temperature superconductors which generally show bulk moduli in the range of 100-200 GPa. The relation c=A+B(n-1) holds for the c-axis cell parameter at ambient pressure, however, the relation breaks down at high pressures.
AB - The transition temperatures (Tc) of the homologous series HgBa2Can-1CunO2n+2+δ of high-temperature superconductors show very large (∼30 K) pressure enhancements, saturating at 118, 154, and 164 K for Hg1201, Hg1212, and Hg1223, respectively. We have measured the compressibility of the first three mercury superconductors in a diamond-anvil cell using energy-dispersive synchrotron x-ray diffraction. We report the tetragonal-cell parameters a and c up to 30 GPa. We find ambient-pressure bulk moduli, KV0==-V0(P/V)0, of 65.4(3.0), 91.6(4.7), and 83.8(10.5) GPa for Hg1201, Hg1212, and Hg1223, respectively. The Hg superconductors are highly compressible compared to other high-temperature superconductors which generally show bulk moduli in the range of 100-200 GPa. The relation c=A+B(n-1) holds for the c-axis cell parameter at ambient pressure, however, the relation breaks down at high pressures.
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U2 - 10.1103/PhysRevB.49.15299
DO - 10.1103/PhysRevB.49.15299
M3 - Article
AN - SCOPUS:0001388242
VL - 49
SP - 15299
EP - 15304
JO - Physical Review B
JF - Physical Review B
SN - 0163-1829
IS - 21
ER -