Partial Hamiltonian formalism, multi-time dynamics and singular theories

Abstract

We formulate singular classical theories without involving constraints. Applying the action principle for the action (27) we develop a partial (in the sense that not all velocities are transformed to momenta) Hamiltonian formalism in the initially reduced phase space (with the canonical coordinates qi,pi, where the number np of momenta pi, i=1,\...,np (17) is arbitrary np≤ n, where n is the dimension of the configuration space), in terms of the partial Hamiltonian H0 (18) and (n-np) additional Hamiltonians Hα, α=np+1,\...,n (20). We obtain (n-np+1) Hamilton-Jacobi equations (25)-(26). The equations of motion are first order differential equations (33)-(34) with respect to qi,pi and second order differential equations (35) for qα. If H0, Hα do not depend on qα (42), then the second order differential equations (35) become algebraic equations (43) with respect to qα. We interpret qα as additional times by (45), and arrive at a multi-time dynamics. The above independence is satisfied in singular theories and rW≤ np (58), where rW is the Hessian rank. If np=rW, then there are no constraints. A classification of the singular theories is given by analyzing system (62) in terms of Fαβ (63). If its rank is full, then we can solve the system (62); if not, some of qα remain arbitrary (sign of a gauge theory). We define new antisymmetric brackets (69) and (80) and present the equations of motion in the Hamilton-like form, (67)-(68) and (81)-(82) respectively. The origin of the Dirac constraints in our framework is shown: if we define extra momenta pα by (86), then we obtain the standard primary constraints (87), and the new brackets transform to the Dirac bracket. Quantization is discussed.

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