在重超导体CeSb_{2}中出现的铁磁梯激发
Zhaoyang Shan1, Yangjie Jiao1, Jiayu Guo1
1Zhejiang University, Center for Correlated Matter and School of Physics, Hangzhou 310058, China.
Physical review letters
|April 7, 2025
概括
沉重费米离子超导体CeSb2中几乎一维的旋转波动表明了一个旋转三重组对联状态. 这些磁刺激可能会驱动在这种材料中观察到的不寻常的压力诱导超导.
科学领域:
- 凝聚物质物理学 凝聚物质物理学
- 材料科学 材料科学 材料科学
- 量子磁力 量子磁力 量子磁力
背景情况:
- 在非传统的超导体中,低维的旋转波动至关重要.
- 几乎一维的旋转激发可能表明旋转三元超导.
- 沉重费米离子超导体CeSb2显示了一个不寻常的上临界场,暗示了三重配对.
研究的目的:
- 研究CeSb2.2中自旋激发的性质.
- 确定CeSb2.2中磁刺激和超导之间的关系.
- 探索低维磁体在非传统超导中的作用.
主要方法:
- 无弹性中子散射被用来探测磁刺激.
- 分析包括将数据与铁磁旋转梯模型相匹配.
- 描述了磁体结构和动态.
主要成果:
- 在CeSb2.2中发现了几乎一维的磁刺激.
- 激发源于几乎正方形的Ce层与正方形变形.
- 铁磁自旋梯模型准确地描述了观察到的磁刺激.
- 分散磁激发在尼尔温度 (T_N) 以上持续存在.
结论:
- 在CeSb2.2,几乎存在一维的旋转波动.
- 这些由旋转梯模型描述的波动与材料的结构有关.
- 铁磁性paramagnons可能通过影响磁性秩序抑制来促进压力诱导的超导.
更多相关视频
04:51Comparison of Two Different Synthesis Methods of Single Crystals of Superconducting Uranium Ditelluride
Published on: July 8, 2021
2.7K
06:49Radio Frequency Magnetron Sputtering of GdBa2Cu3O7âˆ'ÃŽ ´/ La0.67Sr0.33MnO3 Quasi-bilayer Films on SrTiO3 STO Single-crystal Substrates
Published on: April 12, 2019
7.6K
相关概念视频
Types Of Superconductors
889
A superconductor is a substance that offers zero resistance to the electric current when it drops below a critical temperature. Zero resistance is not the only interesting phenomenon as materials reach their transition temperatures. A second effect is the exclusion of magnetic fields. This is known as the Meissner effect. A light, permanent magnet placed over a superconducting sample will levitate in a stable position above the superconductor. High-speed trains that levitate on strong...
889
Ferromagnetism
2.4K
Materials like iron, nickel, and cobalt consist of magnetic domains, within which the magnetic dipoles are arranged parallel to each other. The magnetic dipoles are rigidly aligned in the same direction within a domain by quantum mechanical coupling among the atoms. This coupling is so strong that even thermal agitation at room temperature cannot break it. The result is that each domain has a net dipole moment. However, some materials have weaker coupling, and are ferromagnetic at lower...
2.4K
Colors and Magnetism
11.4K
Color in Coordination Complexes
When atoms or molecules absorb light at the proper frequency, their electrons are excited to higher-energy orbitals. For many main group atoms and molecules, the absorbed photons are in the ultraviolet range of the electromagnetic spectrum, which cannot be detected by the human eye. For coordination compounds, the energy difference between the d orbitals often allows photons in the visible range to be absorbed and emitted, which is seen as colors by the human...
When atoms or molecules absorb light at the proper frequency, their electrons are excited to higher-energy orbitals. For many main group atoms and molecules, the absorbed photons are in the ultraviolet range of the electromagnetic spectrum, which cannot be detected by the human eye. For coordination compounds, the energy difference between the d orbitals often allows photons in the visible range to be absorbed and emitted, which is seen as colors by the human...
11.4K
Superconductor
1.0K
A substance that reaches superconductivity, a state in which magnetic fields cannot penetrate, and there is no electrical resistance, is referred to as a superconductor. In 1911, Heike Kamerlingh Onnes of Leiden University, a Dutch physicist, observed a relation between the temperature and the resistance of the element mercury. The mercury sample was then cooled in liquid helium to study the linear dependence of resistance on temperature. It was observed that, as the temperature decreased, the...
1.0K
The Born-Haber Cycle
21.5K
Lattice Energy
21.5K
Fermi Level
404
The Fermi-Dirac function is represented by an S-shaped curve indicating the probability of an energy state being occupied by an electron at a given temperature. The Fermi level is the energy level at which there is a fifty percent chance of finding an electron, and it is positioned between the lower-energy valence band and the higher-energy conduction band.
At absolute zero temperature, electrons fill all energy states up to the Fermi level, leaving upper states empty. As the temperature rises,...
At absolute zero temperature, electrons fill all energy states up to the Fermi level, leaving upper states empty. As the temperature rises,...
404
