在原子极限中,一维扩展的哈伯德模型的半满带中出现了不寻常的低温行为
Onofre Rojas1, S M de Souza1, J Torrico2
1Departamento de Física, <a href="https://ror.org/0122bmm03">Universidade Federal de Lavras</a>, CP 3037, 37200-900 Lavras-MG, Brazil.
Physical review. E
|September 19, 2024
概括
这项研究分析了一维扩展的哈伯德模型,揭示了交替对 (AP) 和偏磁 (PM) 阶段之间的异常行为. 这种伪转换模仿真实相位转换,但在有限的温度下不会发生.
科学领域:
- 凝聚物质物理学 凝聚物质物理学
- 统计力学 统计力学
- 量子多体系统是一个量子多体系统.
背景情况:
- 在准一维模型中观察到的有限温度伪转换.
- 原子极限中的一维扩展的哈伯德模型是一个长期研究的系统,具有复杂的特性.
研究的目的:
- 在磁场下研究一个1D扩展的哈伯德模型的低温行为.
- 澄清半满频段出现异常行为的性质.
- 区分伪转换与真正的相位转换.
主要方法:
- 转移矩阵技术用于严格的低温分析.
- 精确的数值模拟.
- 涉及立方方程解决方案的分析调查.
主要成果:
- 在零度温度下,在交替对 (AP) 和偏磁 (PM) 阶段之间确认了异常行为.
- 确定了一种模仿第一和第二阶段过渡的伪过渡.
- 该模型不表现出有限温度相位过渡.
结论:
- 半满带中的异常行为是一种伪转换,而不是真正的相位转换.
- 由于立方方程,分析解决方案是复杂的.
- 对1D模型的进一步研究可以揭示微妙的现象.
相关概念视频
Band Theory
15.0K
When two or more atoms come together to form a molecule, their atomic orbitals combine and molecular orbitals of distinct energies result. In a solid, there are a large number of atoms, and therefore a large number of atomic orbitals that may be combined into molecular orbitals. These groups of molecular orbitals are so closely placed together to form continuous regions of energies, known as the bands.
The energy difference between these bands is known as the band gap.
Conductor, Semiconductor,...
The energy difference between these bands is known as the band gap.
Conductor, Semiconductor,...
15.0K
Fermi Level
533
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,...
533
Energy Bands in Solids
764
Isolated atoms have discrete energy levels that are well described by the Bohr model. And, it quantifies the energy of an electron in a hydrogen atom as En. Higher quantum numbers 'n' yield less negative, closer electron energy levels.
Band Formation:
When atoms are brought close together, as in a solid, these discrete energy levels begin to split due to the overlap of electron orbitals from adjacent atoms. This split occurs because of the Pauli exclusion principle, which states...
Band Formation:
When atoms are brought close together, as in a solid, these discrete energy levels begin to split due to the overlap of electron orbitals from adjacent atoms. This split occurs because of the Pauli exclusion principle, which states...
764
Atomic Nuclei: Nuclear Spin State Population Distribution
962
Near absolute zero temperatures, in the presence of a magnetic field, the majority of nuclei prefer the lower energy spin-up state to the higher energy spin-down state. As temperatures increase, the energy from thermal collisions distributes the spins more equally between the two states. The Boltzmann distribution equation gives the ratio of the number of spins predicted in the spin −½ (N−) and spin +½ (N+) states.
962
IR Spectroscopy: Hooke's Law Approximation of Molecular Vibration
1.2K
A covalently bonded heteronuclear diatomic molecule can be modeled as two vibrating masses connected by a spring. The vibrational frequency of the bond can be expressed using an equation derived from Hooke's law, which describes how the force applied to stretch or compress a spring is proportional to the displacement of the spring. In this case, the atoms behave like masses, and the bond acts like a spring.
According to Hooke's law, the vibrational frequency is directly proportional to...
According to Hooke's law, the vibrational frequency is directly proportional to...
1.2K
The Bohr Model
51.6K
Following the work of Ernest Rutherford and his colleagues in the early twentieth century, the picture of atoms consisting of tiny dense nuclei surrounded by lighter and even tinier electrons continually moving about the nucleus was well established. This picture was called the planetary model since it pictured the atom as a miniature “solar system” with the electrons orbiting the nucleus like planets orbiting the sun. The simplest atom is hydrogen, consisting of a single proton as...
51.6K


