Dirac equation with a magnetic field in 3D non-commutative phase space
For a spin-l/2 particle moving in a background magnetic field in noncommutative phase space, the Dirac equation is solved when the particle is allowed to move off the plane that the magnetic field is perpendicular to. It is shown that the motion of the charged particle along the magnetic field has t...
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          | Published in | Chinese physics C Vol. 37; no. 6; pp. 42 - 46 | 
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| Main Author | |
| Format | Journal Article | 
| Language | English | 
| Published | 
          
        01.06.2013
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| Subjects | |
| Online Access | Get full text | 
| ISSN | 1674-1137 0254-3052  | 
| DOI | 10.1088/1674-1137/37/6/063106 | 
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| Summary: | For a spin-l/2 particle moving in a background magnetic field in noncommutative phase space, the Dirac equation is solved when the particle is allowed to move off the plane that the magnetic field is perpendicular to. It is shown that the motion of the charged particle along the magnetic field has the effect of increasing the magnetic field. In the classical limit, matrix elements of the velocity operator related to the probability give a clear physical picture. Along an effective magnetic field, the mechanical momentum is conserved and the motion perpendicular to the effective magnetic field follows a round orbit. If using the velocity operator defined by the coordinate operators, the motion becomes complicated. | 
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| Bibliography: | 11-5641/O4 non-commutative phase space, Dirac equation, velocity operator, magnetic field For a spin-l/2 particle moving in a background magnetic field in noncommutative phase space, the Dirac equation is solved when the particle is allowed to move off the plane that the magnetic field is perpendicular to. It is shown that the motion of the charged particle along the magnetic field has the effect of increasing the magnetic field. In the classical limit, matrix elements of the velocity operator related to the probability give a clear physical picture. Along an effective magnetic field, the mechanical momentum is conserved and the motion perpendicular to the effective magnetic field follows a round orbit. If using the velocity operator defined by the coordinate operators, the motion becomes complicated. LIANG Mai-Lin ZHANG Ya-Bin YANG Rui-Lin ZHANG Fu-Lin( Physics Department, School of Science, Tianjin University, Tianjin 300072, China) ObjectType-Article-2 SourceType-Scholarly Journals-1 ObjectType-Feature-1 content type line 23  | 
| ISSN: | 1674-1137 0254-3052  | 
| DOI: | 10.1088/1674-1137/37/6/063106 |