magnetic field transverse
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2016 ◽  
Vol 14 (3) ◽  
pp. 319-335
Author(s):  
Yu.A. Sitenko ◽  
V.M. Gorkavenko

An influence of a classical magnetic field on the vacuum of the quantized charged spinor matter field confined between two parallel material plates is studied. In the case of the uniform magnetic field transverse to the plates, the Casimir effect is shown to be repulsive, independently of a choice of boundary conditions and of a distance between the plates.


2010 ◽  
Vol 3 (2) ◽  
pp. 76-79
Author(s):  
Andrey V. Ivanov ◽  
Mikhail A. Tiunov

The technique of adiabatic invariant calculation in cross-section of magnetized intensive relativistic beam with consideration of drift motion of beam particles centers of rotation is suggested. Example of adiabatic invariant calculation of electrons of intensive beam in electrostatic accelerating system with longitudinal magnetic field is presented. It was shown that in strong enough magnetic field transverse energy of electrons preserves even at abrupt alteration of electric field.


2010 ◽  
Vol 76 (2) ◽  
pp. 129-134
Author(s):  
D. S. SPICER ◽  
ROBERT BINGHAM ◽  
S. O'SULLIVAN

AbstractIn this letter, we propose a model to explain the disintegration of extragalactic jets and to predict the associated timescale. The model assumes that a jet is current and charge neutral as well as collimated at its source; however, the forward electron current gradually decays producing a magnetic field transverse to the direction of jet propagation. This growing transverse magnetic field eventually causes the jet to disintegrate.


2006 ◽  
Vol 18 (13) ◽  
pp. 3401-3408 ◽  
Author(s):  
Raúl C Munoz ◽  
Ricardo Henríquez ◽  
Juan Pablo García ◽  
Ana María Moncada ◽  
Andrés Espinosa ◽  
...  

2004 ◽  
Vol 7 (3) ◽  
pp. 175-175 ◽  
Author(s):  
T. Franklin ◽  
C. Rinaldi ◽  
J. W. M. Bush ◽  
M. Zahn

1996 ◽  
Vol 175 ◽  
pp. 51-52
Author(s):  
D.C. Gabuzda ◽  
A.B. Pushkarev ◽  
T.V. Cawthorne

The major distinguishing features of BL Lacertae Objects are weak or absent line emission and strong and variable optical, infrared, and radio polarization (Angel and Stockman 1980; Kollgaard 1994). The radio emission and much of the optical emission is believed to be synchrotron radiation. There are now some 20 BL Lacertae objects for which VLBI polarization (VLBP) images have been made at λ = 6 cm (Gabuzda et al. 1994 and references therein). In nearly every BL Lacertae object in which polarization structure has been detected, the polarization position angles in knots in the jets are nearly parallel to the VLBI structural axis. Assuming the jet components to be optically thin, the magnetic fields inferred by this orientation are nearly perpendicular to the direction of the jet; perhaps the most natural interpretation of this is that the knots are associated with shocks that compress an initially tangled magnetic field as they propagate down the VLBI jet, enhancing the magnetic field transverse to the compression (Laing 1980; Hughes, Aller, & Aller 1989).


1994 ◽  
Vol 12 (3) ◽  
pp. 371-377 ◽  
Author(s):  
S.Yu. Gus'kov ◽  
V.B. Rozanov ◽  
T. Pisarczyk

The idea of controlling the plasma flows in laser targets by action of a strong external magnetic field (H ≥ 1 MG) is presented. The magnetic control of plasma flows for the keeping of a transparency of entrance holes of indirect-compression targets and other type targets operating at an introduction of the laser beams into the interior of the target is suggested. It is shown that the magnetic field, transverse versus the direction of the propagation of the plasma flow with an intensity of 2–4 MG, causes a decrease (1.5–3 times) of the closing speed of holes for the laser beam introduction into the hohlraum target.


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