共查询到20条相似文献,搜索用时 46 毫秒
1.
在惯性约束聚变(ICF)电子束快点火物理方案中,需要超强拍瓦激光脉冲驱动MeV能量的强流电子束,并沉积数十kJ能量到压缩氘氚芯区。强流电子束的束流品质是影响点火成功的关键因素之一,为深入了解强流电子束产生物理过程,研制成了三维高性能、适应上万CPU核规模的并行粒子模拟程序,并开展了大规模数值模拟研究,探索了强流电子束的产生机制和输运规律。回顾了近几年来快点火研究团队围绕强流电子束产生和控制开展的研究,介绍了导致束流品质差的两大物理原因:预等离子体效应和束流不稳定性磁场的随机散射。针对这两个物理原因,提出了四种提高强流电子束品质的方法:(1)双层金锥靶减弱预等离子体的负面效应;(2)输运丝产生环向磁场准直强流电子束;(3)外加磁场导引强流电子束提高耦合效率;(4)抑制束流不稳定性以降低随机磁场对电子束流的散射。 相似文献
2.
The characteristics of the space-charge oscillations of a long-pulse relativistic electron beam in magnetically insulated
diodes are determined for different geometries of the electron acceleration section and for explosive-emission cathodes of
different materials. The important role of the stream of electrons having high transverse velocities in the evolution of the
oscillations is demonstrated, and the laws governing the generation of this stream are determined. Possible mechanisms of
the space-charge oscillations are described, taking into account the interaction of the electron stream in the beam halo with
the main electron stream, the development of diocotron instability in the stream of electrons emitted by the outer lateral
surface of the plasma emitter, and the instability of the space charge of “long-lived” electrons in the beam transport channel.
Zh. Tekh. Fiz. 68, 102–106 (April 1998) 相似文献
3.
A theoretical model is given, along with a numerical analysis of the evolution of beam-plasma discharge in the propagation
of a long-pulse relativistic electron beam in a rarefied gas at medium pressure. It is shown that the self-stabilization of
beam-plasma discharge as a result of longitudinal inhomogeneity of the density of the discharge plasma makes it possible for
the beam to traverse the beam chamber with relatively low total energy losses, including ionization losses and energy losses
in the generation of oscillations. During the dissociative recombination of electrons and ions of the discharge-driven plasma,
heat is released and spent in raising the temperature of the gas. The investigated collective-discharge mechanism underlying
heating of the gas for a relativistic beam can be more efficient than the classical heating mechanism due to ionization losses
of the beam in pair collisions of its electrons with gas particles.
Zh. Tekh. Fiz. 67, 94–98 (May 1997) 相似文献
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In the field of fast ignition scheme, self-generated magnetic fields via beam resistive filamentation have a significant role in the angular divergence of the relativistic electron beam, which can be affected by the intensity of other self-generated magnetic fields. In this context, the effects of pressure gradient sources arising from temperature and density gradient of the pellet along the beam flow direction are investigated. The results showed that the resistive filamentation instability can be strongly amplified compared to the fully homogeneous plasma. In this respect, for the distance away from the critical surface, the instability is protected for a longer wave number. Also, the beam and plasma properties such as the beam relativistic factor, the beam number density, and the degree of the plasma temperature anisotropy might be effective. 相似文献
6.
《Waves in Random and Complex Media》2013,23(2):114-127
Abstract The excitation of surface plasma waves due to the interaction of an elliptical relativistic density modulated electron beam with the magnetized dusty plasma column with elliptical cross-section has been studied. The dispersion relation of surface plasma waves has been retrieved from the derived dispersion relation by considering that the beam is absent and there is no dust in the plasma elliptical cylinder. It is shown that the Cherenkov and fast cyclotron interactions appear between the beam and eigen-modes of plasma column. The growth rate of the instability increases with the beam density and modulation index as one-third power of the beam density in Cherenkov interaction and is proportional to the square root of beam density in fast cyclotron interaction. The numerical results and graphs are presented, too. 相似文献
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The nonlinear stage in the development of a resistive hose instability of a highcurrent relativistic electron beam in a finite-conductivity plasma has been studied in the rigid-beam model. The attenuation of the force of the interaction of the beam with the magnetic field of the total current for large beam displacements is shown to result in the stabilization of the instability. The stabilization time and the amplitudes of the oscillations in the saturation regime are determined as functions of the parameters of the beam in the plasma.Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Fiz., No. 10, pp. 78–81, October, 1987. 相似文献
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An equation describing the evolution of the transverse energy of a segment of a paraxial axisymmetric relativistic electron
beam (REB) propagating in a gas-plasma scattering medium along an external magnetic field is used to find the equation relating
the final equilibrium radius of the beam to its initial nonequilibrium value. An analytical expression for the increase in
the mean-square emittance of an REB during transport up to achievement of the equilibrium state is found for the case considered.
The dependence of the final equilibrium radius and the corresponding increase in the mean-square emittance on the density
of the scattering medium and the induction of the external magnetic field is investigated.
Pis’ma Zh. Tekh. Fiz. 67, 108–111 (July 1997) 相似文献
12.
The interaction of a relativistic classical electron with an inhomogeneous electromagnetic field is investigated. In second-order
perturbation theory the motion is separated into fast and slow motions, and the relativistic Newtonian equation is averaged
over the fast oscillations. The rate of change obtained for the slow component of the electron momentum is interpreted as
a relativistic ponderomotive force. The result is generalized to the relativistic case of the wellknown expression for the
Gaponov-Miller force acting on an electron at rest. The expressions obtained for the relativistic ponderomotive forces are
very complicated in the general case. They simplify in the limit of a stationary field (pulses of long duration) and a small
gradient. The most typical and simplest special case of an inhomogeneous field—a stationary plane-focused beam—is investigated.
The main difference between relativistic ponderomotive forces and their nonrelativistic limit is they have multiple components.
In addition to the usual force directed along the gradient of the field, the relativistic case is also characterized by force
components that do not have the form of the gradient of a potential and are parallel to the wave vector and the direction
of the field polarization. It is shown that when a relativistic electron travels in a direction close to the direction of
the wave vector of a focused laser beam, these components can greatly exceed the gradient force. A force directed along the
field polarization vector arises even when the gradient of the field in this direction is zero.
Zh. éksp. Teor. Fiz. 116, 1198–1209 (October 1999) 相似文献
13.
Vishnu M Bannur 《Pramana》2001,57(4):755-761
We derive relativistic fluid set of equations for neutrinos and electrons from relativistic Vlasov equations with Fermi weak
interaction force. Using these fluid equations, we obtain a dispersion relation describing neutrino beam plasma instability,
which is little different from normal dispersion relation of streaming instability. It contains new, nonelectromagnetic, neutrino-plasma
(or electroweak) stable and unstable modes also. The growth of the instability is weak for the highly relativistic neutrino
flux, but becomes stronger for weakly relativistic neutrino flux in the case of parameters appropriate to the early universe
and supernova explosions. However, this mode is dominant only for the beam velocity greater than 0.25c and in the other limit electroweak unstable mode takes over. 相似文献
14.
The filamentation instability is one of the basic beam-plasma instabilities that play a significant role in the energy deposition mechanism of the relativistic electrons generated by the laser-plasma interaction in the fast ignition scenario. In this paper, the effect of the density gradient into plasma on the filamentation instability was investigated in the Weibel unstable plasma, where the plasma temperature anisotropy can play an important role. Results indicated that the density gradient enhances the instability growth rate so that decreasing the density gradient from the critical surface to the core of fuel leads to instability for longer regions in k space. Also, investigations in the region close to the critical surface showed that for decreasing the beam number density nb ≤ 0.01n0, the instability occurs for while this can be different for higher values. Increasing the beam relativistic factor causes a decreasing peak of instability growth rate because of a reduction in beam current, whereas the initial thermal spread of plasma amplifies the filamentation instability. 相似文献
15.
We consider the effect of the multiple Coulomb scattering on the spatial dynamics of the relativistic hose instability of a relativistic electron beam propagating along an Ohmic plasma channel. It is shown that the enhancement of scattering noticeably suppresses this instability.
相似文献16.
A numerical simulation is made of the processes occurring in a plasma lens under conditions when the focusing of a relativistic
electron beam is strongly affected by the ionization of the residual gas in the lens region by the beam itself. The paraxial,
azimuthally symmetric, 1.5-dimensional, electrostatic kinetic model, taking account of plasma production, expansion of the
plasma electrons away from the beam region, and contraction of the ions toward the axis of the beam, was used for the calculation.
The dynamics of the formation of a focal spot is studied, and the size and position of the spot are determined as functions
of time for different values of the gas pressure, initial plasma density, and energy of the beam electrons.
Zh. Tekh. Fiz. 67, 90–94 (October 1997) 相似文献
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Liu C.S. Tripathi V.K. 《IEEE transactions on plasma science. IEEE Nuclear and Plasma Sciences Society》1993,21(1):191-193
A plasma filled backward wave oscillator supports Trivelpiece-Gould (TG) and TM modes. The former can be driven unstable by a relativistic electron beam via Cerenkov interaction or by the plasma return current as two stream instability. This unstable TG mode can parametrically couple to a TM mode via a negative energy beam mode giving rise to an explosive instability 相似文献
19.
S. L. Ginzburg V. F. D’yachenko V. V. Paleichik K. V. Khodataev 《Technical Physics》1999,44(2):212-217
A three-dimensional computer model, described by a system of Maxwell-Vlasov equations, for the interaction of a plasma with
the electromagnetic field was used to calculate the excitation of a field by a relativistic electron beam with a virtual cathode
oscillating in a resonance chamber. The characteristics of the generator radiation are investigated.
Zh. Tekh. Fiz. 69, 87–92 (February 1999) 相似文献
20.
The use of incoherent multiwave pump radiation or randomly varying magnetostatic fields (stochastic undulators) for improving
the energy conversion efficiency in free-electron lasers based on stimulated wave scattering and the stimulated undulator
emission of relativistic electron beams is proposed. It is shown within the quasilinear approximation that the electronic
efficiency increases in proportion to the width of the pump spectrum due to enrichment of the spectrum of combination waves
which are synchronous with the electron beam and realization of a mechanism of stochastic particle deceleration when the signal
wave is monochromatic. At the same time, the efficiency scarcely depends on the spread of the beam parameters, making the
use of the method promising for improving the efficiency of free-electron lasers powered by intense relativistic electron
beams.
Zh. Tekh. Fiz. 67, 77–81 (July 1997) 相似文献