Constraining Forces Stabilizing Superconductivity in Bismuth

被引:4
|
作者
Krueger, Ekkehard [1 ]
机构
[1] Univ Stuttgart, Inst Mat Wissensch, Mat Phys, D-70569 Stuttgart, Germany
来源
SYMMETRY-BASEL | 2018年 / 10卷 / 02期
关键词
superconductivity; bismuth at ambient pressure; Bi-I; bismuth at high pressure; Bi-V; constraining forces; nonadiabatic Heisenberg model; NARROW ENERGY-BANDS; CONDUCTION; PRESSURE;
D O I
10.3390/sym10020044
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
As shown in former papers, the nonadiabatic Heisenberg model presents a mechanism of Cooper pair formation generated by the strongly correlated atomic-like motion of the electrons in narrow, roughly half-filled "superconducting bands" of special symmetry. The formation of Cooper pairs is not only the result of an attractive electron-electron interaction but is additionally the outcome of quantum mechanical constraining forces. There is theoretical and experimental evidence that only these constraining forces operating in superconducting bands may produce eigenstates in which the electrons form Cooper pairs. Here, we report evidence that also the experimentally found superconducting state in bismuth at ambient as well as at high pressure is stabilized by constraining forces.
引用
收藏
页数:13
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