Partial Hamiltonian formalism, multi-time dynamics and singular theories

preprint2013arXivOpen access

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,piq_{i},p_{i}, where the number npn_{p} of momenta pip_{i}, i=1,.˙.,npi=1,\...,n_{p} (17) is arbitrary np≤nn_{p}\leq n, where nn is the dimension of the configuration space), in terms of the partial Hamiltonian H0H_{0} (18) and (n−np)(n-n_{p}) additional Hamiltonians HαH_α, α=np+1,.˙.,nα=n_{p}+1,\...,n (20). We obtain (n−np+1)(n-n_{p}+1) Hamilton-Jacobi equations (25)-(26). The equations of motion are first order differential equations (33)-(34) with respect to qi,piq_{i},p_{i} and second order differential equations (35) for qαq_α. If H0H_{0}, HαH_α do not depend on q˙α\dot{q}_α (42), then the second order differential equations (35) become algebraic equations (43) with respect to q˙α\dot{q}_α. We interpret qαq_α as additional times by (45), and arrive at a multi-time dynamics. The above independence is satisfied in singular theories and rW≤npr_{W}\leq n_{p} (58), where rWr_{W} is the Hessian rank. If np=rWn_{p}=r_{W}, then there are no constraints. A classification of the singular theories is given by analyzing system (62) in terms of FαβF_{αβ} (63). If its rank is full, then we can solve the system (62); if not, some of q˙α\dot{q}_α 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 pαp_α 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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