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The Hamilton-Jacobi treatment for an abelian Chern-Simons system
Mathematical Physics · Submitted 19 Jan 2001
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim It is shown that their simultaneous solutions with the constraints lead to obtain canonical phase space coordinates and the reduced phase space Hamiltonian with out introducing Lagrange multipliers and with out any additional gauge fixing condition.
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The abstract, sentence by sentence
The abelian Chern-Simons system is treated as a constrained system using the Hamilton-Jacobi approach. The equations of motion are obtained as total differential equations in many variables. It is shown that their simultaneous solutions with the constraints lead to obtain canonical phase space coordinates and the reduced phase space Hamiltonian with out introducing Lagrange multipliers and with out any additional gauge fixing condition.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | The abelian Chern-Simons system is treated as a constrained system using the Hamilton-Jacobi approach. | method 0.52 | 0.87 | 0.11 | asserted 1.00 |
| s1 | The equations of motion are obtained as total differential equations in many variables. | result 0.56 | 0.87 | 0.07 | asserted 1.00 |
| s2 | It is shown that their simultaneous solutions with the constraints lead to obtain canonical phase space coordinates and the reduced phase space Hamiltonian with out introducing Lagrange multipliers and with out any additional gauge fixing condition. | result 0.92 | 0.93 | 0.78 | asserted 1.00 |
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Original abstract
The abelian Chern-Simons system is treated as a constrained system using the Hamilton-Jacobi approach. The equations of motion are obtained as total differential equations in many variables. It is shown that their simultaneous solutions with the constraints lead to obtain canonical phase space coordinates and the reduced phase space Hamiltonian with out introducing Lagrange multipliers and with out any additional gauge fixing condition.
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