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相关论文: Geometric concepts for stellarator permanent magne…

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Magnetars (SGRs and AXPs) are one of the most evolutionary paths of a neutron star. These objects have an ultra-strong magnetic field $B \sim 10^{15}$ G at their surface and show persistent X-ray pulsations and transient bursts. Till date…

天体物理学 · 物理学 2008-01-10 Nirvikar Prasad

Tokamaks and stellarators are the leading magnetic-confinement concepts for fusion, but they rely on complementary design principles. Tokamaks use simple axisymmetric coils and plasma current, whereas stellarators use externally generated…

Models of rotating relativistic stars with a toroidal magnetic field have been computed for a sample of eight equations of state of cold dense matter. Non-rotating models admit important levels of magnetization and quadrupole distortion…

广义相对论与量子宇宙学 · 物理学 2015-06-18 Joachim Frieben , Luciano Rezzolla

A model of magnetic field structure is presented to help test the prevalence of flux freezing in star-forming clouds of various shapes, orientations, and degrees of central concentration, and to estimate their magnetic field strength. The…

星系天体物理 · 物理学 2018-11-28 Philip C. Myers , Shantanu Basu , Sayantan Auddy

To search for a conceptual picture describing the magnetization plateau phenomenon, we surveyed the crystal structures and the spin lattices of those magnets exhibiting plateaus in their magnetization vs. magnetic field curves by probing…

材料科学 · 物理学 2024-10-24 Myung-Hwan Whangbo , Hyun-Joo Koo , Reinhard K. Kremer , Alexander N. Vasiliev

The magnetic domain configuration of a system reveals a wealth of information about the fundamental magnetic properties of that system and can be a critical factor in the operation of magnetic devices. Not only are the details of the domain…

介观与纳米尺度物理 · 物理学 2018-07-02 Robert M. Reeve , Hans-Joachim Elmers , Felix Büttner , Mathias Kläui

We study the magnetic interactions experimentally in nanostructures of nanowire arrays. The intensity value obtained from the interactions provides information about its magnetic behavior. We observed two types of experimental magnetic…

The steady-state structure of self-gravitating, magnetized accretion disks is studied using a set of self-similar solutions which are appropriate in the outer regions. The disk is assumed to be isothermal and the magnetic field outside of…

天体物理学 · 物理学 2009-11-13 Mohsen Shadmehri , Fazeleh Khajenabi

There is currently no agreed-upon methodology for characterizing a stellarator magnetic field geometry, and yet modern stellarator designs routinely attain high levels of magnetic-field quasi-symmetry through careful flux-surface shaping.…

等离子体物理 · 物理学 2026-01-01 M. J. Gerard , M. J. Pueschel , S. Stewart , H. O. M. Hillebrecht , B. Geiger

The ongoing development of electromagnets based on High Temperature Superconductors has led to the conceptual exploration of high-magnetic-field fusion reactors of the tokamak type, operating at on-axis fields above 10 T. In this work we…

等离子体物理 · 物理学 2022-01-19 J. A. Alonso , I. Calvo , D. Carralero , J. L. Velasco , J. M. García-Regaña , I. Palermo , D. Rapisarda

We apply topological methods to better understand how the magnetic field in the stellarator edge can be diverted away from the confined region. Our primary method is calculating the winding numbers of closed contours, which gives…

等离子体物理 · 物理学 2025-01-31 Robert Davies , Christopher B. Smiet , Alkesh Punjabi , Allen Boozer , Sophia A. Henneberg

We review the results in our recent works on the generation of strong magnetic fields in compact stars driven by the parity violating electroweak interactions between background fermions. The cases of a neutron star, a hybrid star, and a…

高能天体物理现象 · 物理学 2017-12-21 Maxim Dvornikov

We perform cosmological, hydrodynamic simulations of magnetic fields in galaxy clusters. The computational code combines the special-purpose hardware Grape for calculating gravitational interaction, and smooth-particle hydrodynamics for the…

天体物理学 · 物理学 2007-05-23 Klaus Dolag , Matthias Bartelmann , Harald Lesch

Geospace phenomena such as the aurora, plasma motion, ionospheric currents and associated magnetic field disturbances are highly organized by Earth's main magnetic field. This is due to the fact that the charged particles that comprise…

空间物理 · 物理学 2016-12-01 K. M. Laundal , A. D. Richmond

This paper concerns the investigation of the critical (HC) and the saturation (HS) magnetic fields behavior of the studied system as a function of different physical parameters. The Monte Carlo method has been used to study the magnetic…

软凝聚态物质 · 物理学 2021-09-06 H. Eraki , Z. Fadil , N. Maaouni , A. Mhirech , B. Kabouchi , L. Bahmad , W. Ousi Benomar

We find numerical solutions of the coupled system of Einstein-Maxwell's equations with a linear approach, in which the magnetic field acts as a perturbation of a spherical neutron star. In our study, magnetic fields having both poloidal and…

天体物理学 · 物理学 2009-11-13 A. Colaiuda , V. Ferrari , L. Gualtieri , J. A. Pons

The generation of zonal magnetic fields in laboratory fusion plasmas is predicted by theoretical and numerical models and was recently observed experimentally. It is shown that the modification of the current density gradient associated…

等离子体物理 · 物理学 2009-11-13 F. Militello , M. Romanelli , R. J. Hastie , N. F. Loureiro

X-ray polarimetry promises us an unprecedented look at the structure of magnetic fields and on the processes at the base of acceleration of particles up to ultrarelativistic energies in relativistic jets. Crucial pieces of information are…

高能天体物理现象 · 物理学 2021-05-19 Fabrizio Tavecchio

In high-temperature plasma physics, a strong magnetic field is usually used to confine charged particles. Therefore, for studying the classical mathematical models of the physical problems it needs to consider the effect of external…

数值分析 · 数学 2025-09-05 Anjiao Gu , Yajuan Sun

We demonstrate the use of model order reduction and neural networks for estimating the hysteresis properties of nanocrystalline permanent magnets from microstructure. With a data-driven approach, we learn the demagnetization curve from…