Ciencias,UNAM

SUPERSYMMETRIC PROPERTIES AND STABILITY OF THE DIRAC SEA

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dc.contributor.author ROMERO, RPM
dc.contributor.author MORENO, M
dc.contributor.author ZENTELLA, A
dc.date.accessioned 2011-01-22T10:28:51Z
dc.date.available 2011-01-22T10:28:51Z
dc.date.issued 1991
dc.identifier.issn 0556-2821
dc.identifier.uri http://hdl.handle.net/11154/3613
dc.description.abstract In this work we construct a superalgebra for potential problems in the Dirac equation. We show that this superalgebra is closed for the large class of interactions that leave the Dirac sea stable. In this case, we find that it is possible to perform an exact SU(2) transformation for the Dirac Hamiltonian of the problem. This procedure is formally equivalent to obtaining an exact form for the related Foldy-Wouthuysen Hamiltonian. The potential problems that can be exactly diagonalized include the Dirac oscillator, an arbitrary, time-independent magnetic field, and all the odd potentials, as well as its non-Abelian generalizations. We find that the internal group generators do not destroy the structure of the superalgebra. We work out explicitly the example of the Dirac oscillator. en_US
dc.language.iso en en_US
dc.title SUPERSYMMETRIC PROPERTIES AND STABILITY OF THE DIRAC SEA en_US
dc.type Article en_US
dc.identifier.idprometeo 3486
dc.source.novolpages 43(6):2036-2040
dc.subject.wos Astronomy & Astrophysics
dc.subject.wos Physics, Particles & Fields
dc.description.index WoS: SCI, SSCI o AHCI
dc.relation.journal Physical Review D

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