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相关论文: Detecting reconnection sites using the Lorentz Tra…

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Magnetic reconnection is a fundamental mechanism of driving eruptive phenomena of different scales and may be coupled with turbulence as suggested by recent remote-sensing and in-situ observations. However, the specific physics behind the…

太阳与恒星天体物理 · 物理学 2025-04-08 Yulei Wang , Xin Cheng , Mingde Ding

We investigate the generation of magnetic fields from non-linear effects around recombination. As tight-coupling is gradually lost when approaching $z\simeq 1100$, the velocity difference between photons and baryons starts to increase,…

宇宙学与河外天体物理 · 物理学 2016-06-01 Christian Fidler , Guido Pettinari , Cyril Pitrou

We study in this paper the possible occurrence of orbital magnetim for two-dimensional electrons confined by a harmonic potential in various regimes of temperature and magnetic field. Standard coherent state families are used for…

统计力学 · 物理学 2009-11-07 J. P. Gazeau , P. Y. Hsiao , A. Jellal

This paper describes a particularly didactic and transparent derivation of basic properties of the Lorentz group. The generators for rotations and boosts along an arbitrary direction, as well as their commutation relations, are written as…

综合物理 · 物理学 2011-12-12 Bernard R. Durney

Due to the phase interference of electromagnetic wave, one can recover the total image of one object from a small piece of holograph, which records the interference pattern of two laser light reflected from it. Similarly, the quantum…

量子物理 · 物理学 2014-11-18 Shi-Jian Gu , Guang-Shan Tian , Hai-Qing Lin

Altermagnetism is a compensated magnetic phase characterized by zero net magnetization and exchange-driven spin splitting. However, identifying altermagnets among collinear antiferromagnets usually requires full magnetic-space-group or…

材料科学 · 物理学 2026-05-27 Ying Chen , Qiushi Huang , Yu Wu , Xiaolan Yan , Su-Huai Wei

The current understanding of MHD turbulence envisions turbulent eddies which are anisotropic in all three directions. In the plane perpendicular to the local mean magnetic field, this implies that such eddies become current-sheet-like…

等离子体物理 · 物理学 2017-06-21 N. F. Loureiro , S. Boldyrev

This paper was concerned with the spin-momentum correlation in single-particle quantum states, which is described by the mixed states under Lorentz transformations. For convenience, instead of using the superposition of momenta we use only…

量子物理 · 物理学 2010-08-05 M. A. Jafarizadeha , M. Mahdian

We consider electromagnetic fields having an angular momentum density in a locally non-rotating reference frame in Schwarzschild, Kerr, and Kerr-Newman spacetimes. The nature of such fields is assessed with two families of observers, the…

广义相对论与量子宇宙学 · 物理学 2022-06-02 H. Vargas-Rodríguez , H. C. Rosu , M. G. Medina-Guevara , A. Gallegos , M. A. Muñiz-Torres

Transverse electron focusing in two-dimensional electron gases (2DEGs) with strong spin-orbit coupling is revisited. The transverse focusing is related to the transmission between two contacts at the edge of a 2DEG when a perpendicular…

介观与纳米尺度物理 · 物理学 2015-06-25 Andres A. Reynoso , Gonzalo Usaj , C. A. Balseiro

Light bridges, the bright structure dividing umbrae in sunspot regions, show various activity events. In Paper I, we reported on analysis of multi-wavelength observations of a light bridge in a developing active region (AR) and concluded…

太阳与恒星天体物理 · 物理学 2015-10-07 Shin Toriumi , Mark C. M. Cheung , Yukio Katsukawa

The evolution of the photospheric magnetic field plays a key role in the energy transport into the chromosphere and the corona. In active regions, newly emerging magnetic flux interacts with the pre-existent magnetic field, which can lead…

太阳与恒星天体物理 · 物理学 2021-04-07 C. J. Díaz Baso , J. de la Cruz Rodríguez , J. Leenaarts

We perform a magneto-optical study of a two-dimensional electron systems (2DES) in the regime of the Stoner ferromagnetic instability for even quantum Hall filling factors on Mg$_x$Zn$_{1-x}$O/ZnO heterostructures. Under conditions of…

介观与纳米尺度物理 · 物理学 2017-12-06 A. B. Van'kov , B. D. Kaysin , I. V. Kukushkin

Electron dynamics and energization are one of the key components of magnetic field dissipation in collisionless reconnection. In 2D numerical simulations of magnetic reconnection, the main mechanism that limits the current density and…

等离子体物理 · 物理学 2019-10-09 F. Pucci , S. Usami , H. Ji , X. Guo , R. Horiuchi , S. Okamura , W. Fox , J. Jara-Almonte , M. Yamada , J. Yoo

Observations of galaxy clusters show radio emission extended over almost the system scale, necessitating mechanisms for particle acceleration. Previous models for acceleration such as diffusive shock acceleration and that due to turbulence…

宇宙学与河外天体物理 · 物理学 2025-01-30 Subham Ghosh , Pallavi Bhat

The extended BMS group includes supertranslation, dual supertranslation and Lorentz transformations. The generators of these symmetries can be classified according to their parity into "electric" and "magnetic" types. Using a multipole…

高能物理 - 理论 · 物理学 2021-08-18 Uri Kol

Magnetic separators, which lie on the boundary between four topologically-distinct flux domains, are prime locations in three-dimensional magnetic fields for reconnection, especially in the magnetosphere between the planetary and…

等离子体物理 · 物理学 2016-01-29 Julie E. H. Stevenson , Clare E. Parnell

Although magnetic reconnection takes place in three-dimensional space, reconnection theory has focused on two-dimensional models for more than sixty years. Well-posed three-dimensional mathematics associated with the theory of fluid mixing…

等离子体物理 · 物理学 2020-02-12 Allen H Boozer

Magnetic fields without a direction of continuous symmetry have the generic feature that neighboring field lines exponentiate away from each other and become stochastic, hence the ideal constraint of preserving magnetic field line…

太阳与恒星天体物理 · 物理学 2014-09-16 Yi-Min Huang , A. Bhattacharjee , Allen H. Boozer

There is growing evidence that when magnetic reconnection occurs in high Lundquist number plasmas such as in the Solar Corona or the Earth's Magnetosphere it does so within a fragmented, rather than a smooth current layer. Within the extent…

太阳与恒星天体物理 · 物理学 2016-07-12 Peter F. Wyper , Michael Hesse