Nonholonomic stability aspects of piecewise holonomic systems (Q1289585)
From MaRDI portal
| This is the item page for this Wikibase entity, intended for internal use and editing purposes. Please use this page instead for the normal view: Nonholonomic stability aspects of piecewise holonomic systems |
scientific article; zbMATH DE number 1293236
| Language | Label | Description | Also known as |
|---|---|---|---|
| English | Nonholonomic stability aspects of piecewise holonomic systems |
scientific article; zbMATH DE number 1293236 |
Statements
Nonholonomic stability aspects of piecewise holonomic systems (English)
0 references
3 August 2000
0 references
It is known that Hamiltonian systems cannot have exponentially stable steady motions. Exponential stability for some of the variables (i.e. some eigenvalues of the linearized system having negative real parts, while the others have zero real parts) becomes possible in the presence of non-holonomic constraints. Non-holonomic mechanical systems can often be linked to a ``sister system'' which is piecewise holonomic and exhibits collisional contacts resulting in energy dissipation. An example is a rimless spoked wheel replacing a rolling disk. Here the author investigates the question whether the source of exponential stability is the above dissipation or it can be attributed to the non-holonomic nature of intermittent contact. He argues by way of the example of Chaplygin sleigh that the latter can be the case.
0 references
Hamiltonian systems
0 references
piecewise holonomic systems
0 references
non-holonomic systems
0 references
energy dissipation
0 references
exponential stability
0 references
intermittent contact
0 references
Chaplygin sleigh
0 references