scholarly journals Magnetic-field symmetry of pump currents of adiabatically driven mesoscopic structures

2005 ◽  
Vol 72 (3) ◽  
Author(s):  
M. Moskalets ◽  
M. Büttiker
1975 ◽  
Vol 53 (19) ◽  
pp. 2210-2220 ◽  
Author(s):  
James K. G. Watson

The structures of the symmetry groups for the rovibronic levels of a molecule in a homogeneous electric or magnetic field are derived, and the symmetry classification of the levels in terms of the representations and corepresentations of these groups is discussed. Specific results are given for molecules of the point groups C3, C2v, C3v, D2d, and Td in an electric field. Symmetry in combined electric and magnetic fields and the inclusion of nuclear spins are considered briefly.


2006 ◽  
Vol 96 (12) ◽  
Author(s):  
R. Leturcq ◽  
D. Sánchez ◽  
G. Götz ◽  
T. Ihn ◽  
K. Ensslin ◽  
...  

1997 ◽  
Vol 55 (4) ◽  
pp. R1946-R1949 ◽  
Author(s):  
T. Christen ◽  
M. Büttiker

2007 ◽  
Author(s):  
R. Leturcq ◽  
R. Bianchetti ◽  
G. Götz ◽  
T. Ihn ◽  
K. Ensslin ◽  
...  

1969 ◽  
Vol 9 (3) ◽  
pp. 233-238
Author(s):  
F. Hartz ◽  
J. Junker ◽  
F. Pohl ◽  
G.H. Wolf

1967 ◽  
Vol 31 ◽  
pp. 381-383
Author(s):  
J. M. Greenberg

Van de Hulst (Paper 64, Table 1) has marked optical polarization as a questionable or marginal source of information concerning magnetic field strengths. Rather than arguing about this–I should rate this method asq+-, or quarrelling about the term ‘model-sensitive results’, I wish to stress the historical point that as recently as two years ago there were still some who questioned that optical polarization was definitely due to magnetically-oriented interstellar particles.


1967 ◽  
Vol 31 ◽  
pp. 375-380
Author(s):  
H. C. van de Hulst

Various methods of observing the galactic magnetic field are reviewed, and their results summarized. There is fair agreement about the direction of the magnetic field in the solar neighbourhood:l= 50° to 80°; the strength of the field in the disk is of the order of 10-5gauss.


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