2006
DOI: 10.1140/epjc/s2006-02622-7
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The reduced phase space of an open string in the background B-field

Abstract: The problem of an open string in background B-field is discussed. Using the discretized model in details we show that the system is influenced by infinite number of second class constraints. We interpret the allowed Fourier modes as the coordinates of the reduced phase space. This enables us to compute the Dirac brackets more easily. We prove that the coordinates of the string are non-commutative at the boundaries. We argue that in order to find the Dirac bracket or commutator algebra of the physical variables… Show more

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Cited by 8 publications
(15 citation statements)
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References 31 publications
(64 reference statements)
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“…The possibility (22) corresponds to zero mode solutions with sinh k 0 σ and cosh k 0 σ. Traditionally the zero mode solution is denoted as the zero frequency (infinite wave length) limiting term in the Fourier expansions, as shown for example for the massless case of the current problem in [11]. Here, however, we interpret the zero mode solution as a solution which satisfies the boundary conditions not only at the end-points but also throughout all the medium.…”
Section: Consider the Boundary Conditions As Primary Constraint φmentioning
confidence: 99%
“…The possibility (22) corresponds to zero mode solutions with sinh k 0 σ and cosh k 0 σ. Traditionally the zero mode solution is denoted as the zero frequency (infinite wave length) limiting term in the Fourier expansions, as shown for example for the massless case of the current problem in [11]. Here, however, we interpret the zero mode solution as a solution which satisfies the boundary conditions not only at the end-points but also throughout all the medium.…”
Section: Consider the Boundary Conditions As Primary Constraint φmentioning
confidence: 99%
“…The idea of considering boundary conditions as constraints of a physical system was proposed [27,28,29] by the late 1990s. In fact, boundary conditions in the background magnetic field are first order equations of time variable, whereas the Euler-Lagrange equation is a second order one, which means that the acceleration determines the dynamics of the motion.…”
Section: Introductionmentioning
confidence: 99%
“…In fact, boundary conditions in the background magnetic field are first order equations of time variable, whereas the Euler-Lagrange equation is a second order one, which means that the acceleration determines the dynamics of the motion. Hence, boundary conditions in Lagrangian equations are called acceleration-free equations [23,24,25,26,29]. So, these objects do not play any role in the dynamics of the system.…”
Section: Introductionmentioning
confidence: 99%
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“…consistently in the whole space because on the boundaries those BCs are inconsistent with the usual canonical commutation relations [1][2][3][4][5].…”
mentioning
confidence: 99%