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帕邢-巴克效应

1912
  • Friedrich Paschen
  • Ernst Back
物理学家在强磁场中进行光谱实验。

(图片仅供参考)

The Paschen-Back effect occurs in the presence of a very strong magnetic field, where the Zeeman splitting energy becomes much larger than the fine-structure (spin-orbit) interaction energy. In this regime, the coupling between orbital ([latex]\vec{L}[/latex]) and spin ([latex]\vec{S}[/latex]) angular momentum is broken. They precess independently around the strong external magnetic field, simplifying the spectral pattern.

帕申-巴克效应代表了高场极限 Zeeman effect反常塞曼效应描述的是外场相对于内部自旋轨道耦合而言扰动较小的情况,而帕邢-巴克效应则描述了相反的情况。当磁场足够强时,磁矩与外场的相互作用能[latex]hat{H}_Z[/latex]将远大于自旋轨道相互作用能。 Hamiltonian, [latex]\hat{H}_{SO}[/latex].

As a result, [latex]\vec{L}[/latex] and [latex]\vec{S}[/latex] are effectively decoupled. The ‘good’ quantum numbers are no longer J and [latex]m_J[/latex], but rather [latex]m_L[/latex] and [latex]m_S[/latex], which describe the independent projections of orbital and spin angular momentum along the magnetic field axis. The first-order energy shift is then given by the sum of the independent interactions: [latex]\Delta E = (m_L + g_s m_S)\mu_B B[/latex]. With [latex]g_s \approx 2[/latex], this leads to a splitting pattern that closely resembles the normal Zeeman triplet, although the fine-structure interaction, now treated as a small perturbation, causes each of these lines to have a small residual substructure. The transition from the anomalous Zeeman regime to the Paschen-Back regime is continuous and can be calculated using intermediate-field theories.

UNESCO Nomenclature: 2202
– Atomic and molecular physics

类型

Physical Phenomenon

中断

Incremental

用法

Niche/Specialized

前体

  • 弱场中的塞曼效应
  • 精细结构和自旋轨道耦合理论
  • 产生强磁场的技术,例如魏斯磁场,已经出现。 electromagnet
  • advances in high-resolution 光谱学

应用程序

  • spectroscopy of astrophysical objects with immense magnetic fields (e.g., neutron stars, white dwarfs)
  • 使用超导磁体在高场物理实验室进行研究
  • 了解极端物理条件下的原子结构
  • 在强场极限下测试量子电动力学(qed)
  • 高密度等离子体诊断

专利:

NA

潜在创新理念

  • a diagnostic tool for inertial confinement fusion that uses the paschen-back effect to measure the intense magnetic fields generated during implosion
  • 一种通过施加强外部场来诱导周围电子的帕申-巴克效应来控制核磁共振成像的核自旋态的方法
  • 一种通过选择性激发帕申-巴克态的原子态来产生高度极化的粒子束的技术
  • 利用与磁星强磁场相互作用的星际探测器的拟议驱动
  • 通过重建帕申-巴克条件来模拟天体物理环境的实验室装置
  • 一种基于帕申背分裂能级跃迁的新型激光器
  • 一种用于敏感文件的安全功能,使用含有原子的墨水,其帕申-巴克光谱独特且难以复制
  • 一种利用强磁场破坏反应物自旋轨道耦合来操纵化学反应路径的方法
  • 一项基础物理实验,通过寻找与预测的帕申-巴克分裂的微小偏差来寻找新的力量
  • 一种稳健的量子计算量子比特设计,在帕申-巴克机制下运行,以最大限度地减少自旋轨道波动造成的退相干
Related to: Paschen-Back effect, strong magnetic field, fine structure, spin-orbit decoupling, spectroscopy, atomic physics, high-field limit, quantum mechanics, energy levels, decoupling.

历史背景

帕邢-巴克效应

1907
1909
1910
1912
1915
1915-11
1916
1907
1909
1910
1911-04-08
1913
1915
1916
1917

(如果日期未知或不相关,例如“流体力学”,则提供其显著出现的近似估计)

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