scholarly journals Stability of particle orbits

1987 ◽  
Vol 43 (1-4) ◽  
pp. 163-176
Author(s):  
E. Keil
Keyword(s):  
Particle Orbits

scholarly journals The relation between wave asymmetry and particle orbits analysed by Slepian models

2021 ◽  
Vol 924 ◽  
Author(s):  
Georg Lindgren ◽  
Marc Prevosto
Keyword(s):  
Particle Orbits

Abstract

Cosmic censorship, black holes, and particle orbits

1979 ◽  
Vol 10 (2) ◽  
pp. 99-103 ◽  
Author(s):  
William A. Hiscock
Keyword(s):  
Black Holes ◽  
Cosmic Censorship ◽  
Particle Orbits

scholarly journals Shallow water gravity waves: A note on the particle orbits

1996 ◽  
Vol 52 (3) ◽  
pp. 353-357 ◽  
Author(s):  
Kern E. Kenyon
Keyword(s):  
Shallow Water ◽  
Gravity Waves ◽  
Particle Orbits

COLLECTIVE BANDS IN 68Se

2002 ◽  
Vol 11 (06) ◽  
pp. 531-538 ◽  
Author(s):  
K. C. TRIPATHY ◽  
R. SAHU
Keyword(s):  
Configuration Space ◽  
Single Particle ◽  
Fock States ◽  
Hartree Fock ◽  
Ground Band ◽  
Prolate Shape ◽  
Particle Orbits ◽  
Excited Band ◽  
Inert Core ◽  
Configuration Mixing

The collective bands of the N = Z nucleus 68 Se are studied within our deformed configuration mixing shell model based on Hartree–Fock states. The configuration space consists of the spherical single particle orbits 1p3/2, 0f5/2, 1p1/2 and 0g9/2 with 56 Ni as the inert core. A modified Kuo interaction for this basis space has been used in our calculation. The calculated ground band, K = 2+ excited band and the K = 5- excited band agree reasonably well with the experiment. Our calculation shows that the ground band is essentially of oblate shape and the excited K = 2+ band is of prolate shape. This is in agreement with the conclusions drawn from the recent experimental analysis.

scholarly journals Particle Orbits, Trapping, and Acceleration in a Filamentary Current Sheet Model

1994 ◽  
Vol 142 ◽  
pp. 719-728
Author(s):  
Bernhard Kliem
Keyword(s):  
Particle Acceleration ◽  
Electric Field ◽  
Test Particle ◽  
Solar Flares ◽  
Acceleration Of Particles ◽  
Acceleration Process ◽  
Two Dimensional ◽  
Magnetic Island ◽  
Particle Orbits ◽  
Island Dynamics

AbstractTest particle orbits in the two-dimensional Fadeev equilibrium with a perpendicular electric field added are analyzed to show that impulsive bursty reconnection, which has been proposed as a model for fragmentary energy release in solar flares, may account also for particle acceleration to (near) relativistic energies within a fraction of a second. The convective electric field connected with magnetic island dynamics can play an important role in the acceleration process.Subject headings: acceleration of particles — MHD — plasmas — Sun: corona — Sun: flares

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