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Simulations of astrophysical disks in the shearing box that are subject to the magnetorotational instability (MRI) show that activity appears to be reduced as the magnetic Prandtl number (Pm) is lowered. On the other hand, calculations for…

太阳与恒星天体物理 · 物理学 2015-05-18 O. M. Umurhan

The intracluster medium (ICM) is the low-density diffuse magnetized plasma in galaxy clusters, which reaches virial temperatures of up to 10^8 K. Under these conditions, the plasma is weakly collisional and therefore has an anisotropic…

宇宙学与河外天体物理 · 物理学 2024-03-11 Y. Rappaz , J. Schober

The magnetorotational instability (MRI) is thought to be a powerful source of turbulence in Keplerian accretion disks. Motivated by recent laboratory experiments, we study the MRI driven by an azimuthal magnetic field in an electrically…

太阳与恒星天体物理 · 物理学 2017-11-21 Anna Guseva , Ashley P. Willis , Rainer Hollerbach , Marc Avila

Differential rotation is known to suppress linear instabilities in fusion plasmas. However, even in the absence of growing eigenmodes, subcritical fluctuations that grow transiently can lead to sustained turbulence. Here transient growth of…

等离子体物理 · 物理学 2015-08-26 A. A. Schekochihin , E. G. Highcock , S. C. Cowley

By performing ideal magnetohydrodynamical (MHD) simulations with weak vertical magnetic fields in unstratified cylindrical shearing boxes with modified boundary treatment, we investigate MHD turbulence excited by magnetorotational…

高能天体物理现象 · 物理学 2023-11-06 Takeru K. Suzuki

We propose a scheme to entangle two magnon modes via Kerr nonlinear effect when driving the systems far-from-equilibrium. We consider two macroscopic yttrium iron garnets (YIGs) interacting with a single-mode microcavity through the…

量子物理 · 物理学 2019-09-25 Zhedong Zhang , Marlan O. Scully , Girish S. Agarwal

Transverse oscillations of coronal loops are often observed and have been theoretically interpreted as kink magnetohydrodynamic (MHD) modes. Numerical simulations by Terradas et al. (2008, ApJ 687, L115) suggest that shear flows generated…

太阳与恒星天体物理 · 物理学 2014-11-20 R. Soler , J. Terradas , R. Oliver , J. L. Ballester , M. Goossens

New unstable temperature gradient driven modes in an inhomogeneous plasma are identified. These modes represent transient $\omega \simeq k_{\Vert }v_{th}^{(e,i)}$ sound oscillations in magnetized plasma that are kinetically destabilized via…

等离子体物理 · 物理学 2007-05-23 A. I. Smolyakov , M. Yagi , Y. Kishimoto

The quasilinear particle flux arising from gyrokinetic instabilities is calculated in the electrostatic and collisionless approximation, keeping the geometry of the magnetic field arbitrary. In particular, the flux of electrons and heavy…

等离子体物理 · 物理学 2018-08-01 Per Helander , Alessandro Zocco

Gyrokinetic theory is a basis for treating magnetised plasma dynamics slower than particle gyrofrequencies where the scale of the background is larger than relevant gyroradii. The energy of field perturbations can be comparable to the…

等离子体物理 · 物理学 2024-05-29 Bruce D. Scott

The magnetic phase variations under hydrostatic pressure on multiferroic BiMnO3 have been examined by the dc magnetization [Mg(T)], magnetic hysteresis [Ueff(H)], and ac susceptibility [X'g(T)]. Three magnetic transitions, manifested as…

The Global Magnetorotational Instability (MRI) is investigated for a configuration in which the rotation frequency changes only in a narrow transition region. If the vertical wavelength of the unstable mode is of the same order or smaller…

天体物理仪器与方法 · 物理学 2011-02-11 J. Pino , S. M. Mahajan

We simulate Lattice QED in a constant external magnetic field using the RHMC algorithm. We seek evidence for chiral symmetry breaking predicted by truncated Schwinger-Dyson methods. Since the predicted values of the dynamical electron mass…

高能物理 - 格点 · 物理学 2022-10-21 D. K. Sinclair , J. B. Kogut

(Abridged) We analyse the stability and evolution of power-law accretion disc models. These have midplane densities that follow radial power-laws, and have either temperature or entropy distributions that are power-law functions of…

地球与行星天体物理 · 物理学 2015-06-11 Richard P. Nelson , Oliver Gressel , Orkan M. Umurhan

Recent experimental observations at JET show evidence of reduced ion temperature profile stiffness, hypothesised to be due to concomitant low magnetic shear (s) and significant toroidal rotational flow shear. Non-linear gyrokinetic…

We have investigated the effect of sheared equilibrium flows on the $m = 1, n = 1$ resistive internal kink mode in the framework of a reduced magnetohydrodynamic model in a periodic cylindrical geometry. Our numerical studies show that…

等离子体物理 · 物理学 2018-02-13 Jervis Mendonca , Debasis Chandra , Abhijit Sen , Anantanarayanan Thyagaraja

With strong gradients in the pedestal of high confinement mode (H-mode) fusion plasmas, gyrokinetic simulations are carried out for the trapped electron and ion temperature gradient modes. A broad class of unconventional mode structures is…

等离子体物理 · 物理学 2015-09-16 H. S. Xie , Y. Xiao

Magnetic reconnection (MR) in Earth's magnetotail is usually followed by a systemwide redistribution of explosively released kinetic and thermal energy. Recently, multispacecraft observations from the THEMIS mission were used to study…

地球与行星天体物理 · 物理学 2014-11-20 Z. Voros , M. P. Leubner , A. Runov , V. Angelopoulos , W. Baumjohann

Recently, it was shown that strongly correlated metallic fermionic systems [Nature Phys. 3, 168 (2007)] generically display kinks in the dispersion of single fermions without the coupling to collective modes. Here we provide compelling…

强关联电子 · 物理学 2009-02-24 Carsten Raas , Patrick Grete , Götz S. Uhrig

The relationship between a decaying strong turbulence and kinetic instabilities in a slowly expanding plasma is investigated using two-dimensional (2-D) hybrid expanding box simulations. We impose an initial ambient magnetic field…

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