Nested Fermi surface and electronic instability in Ca3Ru2O7

被引:66
作者
Baumberger, F [1 ]
Ingle, NJC
Kikugawa, N
Hossain, MA
Meevasana, W
Perry, RS
Shen, KM
Lu, DH
Damascelli, A
Rost, A
Mackenzie, AP
Hussain, Z
Shen, ZX
机构
[1] Stanford Univ, Dept Appl Phys, Stanford, CA 94305 USA
[2] Stanford Univ, Dept Phys, Stanford, CA 94305 USA
[3] Stanford Univ, Stanford Synchrotron Radiat Lab, Stanford, CA 94305 USA
[4] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z4, Canada
[5] Univ St Andrews, Dept Phys & Astron, Scottish Univ Phys Alliance, St Andrews KY16 9SS, Fife, Scotland
[6] Kyoto Univ, Dept Phys, Kyoto 6068501, Japan
[7] Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA
基金
英国工程与自然科学研究理事会;
关键词
D O I
10.1103/PhysRevLett.96.107601
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
High-resolution angular resolved photoemission data reveal well-defined quasiparticle bands of unusually low weight, emerging in line with the metallic phase of Ca3Ru2O7 below similar to 30 K. At the bulk structural phase transition temperature of 48 K, we find clear evidence for an electronic instability, gapping large parts of the underlying Fermi surface that appears to be nested. Metallic pockets are found to survive in the small, non-nested sections, constituting a low-temperature Fermi surface with 2 orders of magnitude smaller volume than in all other metallic ruthenates. The Fermi velocities and volumes of these pockets are in agreement with the results of complementary quantum oscillation measurements on the same crystal batches.
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页码:1 / 4
页数:4
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