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相关论文: A `fast-burning' mechanism for magnetic diffusion

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We investigate wave propagation and energy transport in magnetic elements, which are representatives of small scale magnetic flux concentrations in the magnetic network on the Sun. This is a continuation of earlier work by Hasan et al.…

太阳与恒星天体物理 · 物理学 2015-05-14 G. Vigeesh , S. S. Hasan , O. Steiner

The present paper seeks to determine the mechanism of flame acceleration and transition to detonation when a turbulent flame preceded by a shock interacts with a single obstruction in its path, taken as a cylindrical obstacle or a wall in…

流体动力学 · 物理学 2018-06-12 Willstrong Rakotoarison , Brian Maxwell , Andrzej Pekalski , Matei I. Radulescu

Fast Radio Bursts (FRBs), characterized by strong bursts of radiation intensity at radio wavelengths lasting on the order of a millisecond, have yet to be firmly associated with a family, or families, of astronomical sources. It follows…

高能天体物理现象 · 物理学 2018-01-31 Martin Houde , Abhilash Mathews , Fereshteh Rajabi

Magnetar bursts can be emitted by Alfv\'en waves growing in the outer magnetosphere to nonlinear amplitudes, $\delta B/B\sim 1$, and triggering magnetic reconnection. Similar magnetic flares should occur quasi-periodically in a magnetized…

高能天体物理现象 · 物理学 2021-11-17 Andrei M. Beloborodov

The evolution of a dilute electron-positron fireball is calculated in the regime of strong magnetization and very high compactness (l ~10^3-10^8). Heating is applied at a low effective temperature (< 25 keV), and the fireball is allowed to…

高能天体物理现象 · 物理学 2015-06-17 Christopher Thompson , Ramandeep Gill

We propose a new model for the origin of Fast Radio Bursts (FRBs), attributing these phenomena to sudden discharges of accumulated electric charge in the accretion disk of compact objects such as black holes. Our framework demonstrates how…

高能天体物理现象 · 物理学 2025-08-06 Parsa Kafashi , Sohrab Rahvar

Highly energetic ions that impact materials have applications from semiconductor industry to medicine, and are fundamentally interesting as they trigger multi-length and time-scale processes. In particular, they excite electrons into…

材料科学 · 物理学 2025-07-24 Cheng-Wei Lee , André Schleife

Sharp fronts observed by Chandra satellite between dense cool cluster cores moving with near-sonic velocity through the hotter intergalactic gas, require strong suppression of thermal conductivity across the boundary. This may be due to…

天体物理学 · 物理学 2009-11-11 Maxim Lyutikov

Charged particles in a magnetosphere are spontaneously attracted to a planet while increasing their kinetic energy via inward diffusion process. A constraint on particles' micro-scale adiabatic invariants restricts the class of motions…

等离子体物理 · 物理学 2016-11-08 Y. Ushida , Y. Kawazura , N. Sato , Z. Yoshida

Despite that gamma-ray bursts is a phenomenon quite different from accreting compact objects, it could be that their hard X-ray emission is associated with a very similar mechanism of energy dissipation. In both cases, we could deal with…

天体物理学 · 物理学 2007-05-23 Boris Stern

The fast (ms) radio bursts reported by Thornton, {\it et al.} have extremely high brightness temperatures if at the inferred cosmological distances. This implies coherent emission by "bunches" of charges. We model the emission region as a…

高能天体物理现象 · 物理学 2015-06-17 J. I. Katz

The solidification process during squeeze casting is analyzed based on the classical solidification and plastic deformation theory. The linear relationship between punch velocity and the solidification rate is established if the density…

材料科学 · 物理学 2009-09-30 Xiao-Hui Chen , Xu Huang , Xue-Ping. Ren

A model is developed for magnetic `propeller'-driven outflows which cause a rapidly rotating magnetized star accreting from a disk to spin-down. Energy and angular momentum lost by the star goes into expelling most of the accreting disk…

天体物理学 · 物理学 2009-10-31 R. V. E. Lovelace , M. M. Romanova , G. S. Bisnovatyi-Kogan

Merger of a white dwarf binary creates a differentially rotating object which is expected to generate strong magnetic fields. Kinetic energy stored in differential rotation is partially dissipated in the magnetically dominated corona, which…

高能天体物理现象 · 物理学 2015-06-17 Andrei M. Beloborodov

The transport of magnetic flux to outside of collapsing molecular clouds is a required step to allow the formation of stars. Although ambipolar diffusion is often regarded as a key mechanism for that, it has been recently argued that it may…

太阳与恒星天体物理 · 物理学 2015-05-27 E. M. de Gouveia Dal Pino , R. Santos-Lima , A. Lazarian , M. R. M. Leão , D. Falceta-Gonçalves , G. Kowal

Turbulence is ubiquitous in astrophysical fluids. Therefore it is necessary to study magnetic reconnection in turbulent environments. The model of fast turbulent reconnection proposed in Lazarian & Vishniac 1999 has been successfully tested…

星系天体物理 · 物理学 2011-12-16 A. Lazarian

We examine the possibility that fast radio bursts (FRBs) are emitted inside the magnetosphere of a magnetar. On its way out, the radio wave must interact with a low-density $e^\pm$ plasma in the outer magnetosphere at radii…

高能天体物理现象 · 物理学 2021-11-24 Andrei M. Beloborodov

Fast Ignition Inertial Confinement Fusion is a variant of inertial fusion in which DT fuel is first compressed to high density and then ignited by a relativistic electron beam generated by a fast (< 20 ps) ultra-intense laser pulse, which…

Fast Magnetic Reconnection is currently regarded as an important process also beyond the solar system, specially in magnetically dominated regions of galactic and extragalactic sources like the surrounds of black holes and relativistic…

We examine four candidate mechanisms that could explain the high surface temperatures of magnetars. (1) Heat flux from the liquid core heated by ambipolar diffusion. It could sustain the observed surface luminosity $L_s\approx 10^{35}$…

高能天体物理现象 · 物理学 2016-12-28 Andrei M. Beloborodov , Xinyu Li