Geometry of Mechanics
Miguel C. Muñoz-Lecanda, Narciso Román-Roy
TL;DR
This work provides a comprehensive geometric tour of mechanics, detailing autonomous and nonautonomous, as well as dissipative systems, through symplectic, cosymplectic, and contact formalisms. It builds from foundational symplectic geometry to Lagrangian and canonical Hamiltonian descriptions, then unifies them via Skinner–Rusk’s framework, all while addressing symmetries, conserved quantities, and reduction. Central to the exposition are momentum maps, Noether’s theorem, and Hamilton–Jacobi theory, which together yield a cohesive toolbox for analyzing regular and, when possible, singular dynamics. The treatment emphasizes both local (coordinate) expressions and global geometric structures, enabling rigorous analysis of classical problems and laying groundwork for extensions to more general and dissipative contexts. Overall, the geometry of mechanics emerges as a versatile, unifying language for describing the dynamics of physical systems through canonical forms, variational principles, and symmetry-driven reductions.
Abstract
The aim of this work is to study the geometry underlying mechanics and its application to describe autonomous and nonautonomous conservative dynamical systems of different types; as well as dissipative dynamical systems. We use different geometric descriptions to study the main properties and characteristics of these systems; such as their Lagrangian, Hamiltonian and unified formalisms, their symmetries, the variational principles, and others. The study is done mainly for the regular case, although some comments and explanations about singular systems are also included.
