Phase dynamics of a relativistic electron driven by the potential field of a wave packet: Poincaré transformation dynamics

1998 ◽  
Vol 41 (6) ◽  
pp. 517-522
Author(s):  
A. C. Krotov ◽  
A. A. Tel'nikhin



2013 ◽  
Vol 88 (7) ◽  
Author(s):  
Lóránt Zs. Szabó ◽  
Mihály G. Benedict ◽  
Attila Czirják ◽  
Péter Földi


1946 ◽  
Vol 42 (3) ◽  
pp. 286-291 ◽  
Author(s):  
C. A. Coulson ◽  
G. S. Rushbrooke

The paper deals with the motion of a Gaussian wave-packet in a parabolic potential field, contrasting the quantum-mechanical behaviour of the packet with that which follows from pure classical mechanics.The behaviour is entirely classical only if the initial phase of the space-wave-function is linear in the space coordinate; in which case the wave-packet is initially a ‘best-possible’ packet according to Heisenberg's uncertainty relationship.The paper concludes with a brief reference to the similar problem for a free particle.Note added in Proof, 16 February 1946. Through the courtesy of Mr M. S. Bartlett, we have been privileged to see the manuscripts of some work by Mr J. E. Moyal and himself, in which the motion of a probability wave-packet is discussed in more general terms than our own: and in which it appears that the motion of our wave-packet, which we have described as non-classical, is indeed actually classical provided that a certain correlation exists between momentum and position in the p, q-distribution function. With this knowledge we now find that classical and quantal predictions agree precisely provided that the initial classical probability function is given bythis is a particular case of their more general results.



1966 ◽  
Vol 25 ◽  
pp. 93-97
Author(s):  
Richard Woolley

It is now possible to determine proper motions of high-velocity objects in such a way as to obtain with some accuracy the velocity vector relevant to the Sun. If a potential field of the Galaxy is assumed, one can compute an actual orbit. A determination of the velocity of the globular clusterωCentauri has recently been completed at Greenwich, and it is found that the orbit is strongly retrograde in the Galaxy. Similar calculations may be made, though with less certainty, in the case of RR Lyrae variable stars.



1989 ◽  
Vol 50 (20) ◽  
pp. 3075-3087 ◽  
Author(s):  
B. Caroli ◽  
C. Caroli ◽  
B. Roulet




2015 ◽  
Vol 135 (6) ◽  
pp. 355-356 ◽  
Author(s):  
Takahiro Kazetoh ◽  
Kazumasa Takahashi ◽  
Toru Sasaki ◽  
Takashi Kikuchi ◽  
Nob. Harada ◽  
...  




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