Beltrami identity
Let be a function , , and . Begin with the time-relative Euler-Lagrange condition
| (1) |
If , then the Euler-Lagrange condition reduces to
| (2) |
which is the Beltrami identity![]()
. In the calculus of variations
![]()
, the ability to use the Beltrami identity can vastly simplify problems, and as it happens, many physical problems have .
In space-relative terms, with , we have
| (3) |
If , then the Euler-Lagrange condition reduces to
| (4) |
To derive the Beltrami identity, note that
| (5) |
Multiplying (1) by , we have
| (6) |
Now, rearranging (5) and substituting in for the rightmost term of (6), we obtain
| (7) |
Now consider the total derivative
| (8) |
If , then we can substitute in the left-hand side of (8) for the leading portion of (7) to get
| (9) |
Integrating with respect to , we arrive at
| (10) |
which is the Beltrami identity.
| Title | Beltrami identity |
|---|---|
| Canonical name | BeltramiIdentity |
| Date of creation | 2013-03-22 12:21:08 |
| Last modified on | 2013-03-22 12:21:08 |
| Owner | PrimeFan (13766) |
| Last modified by | PrimeFan (13766) |
| Numerical id | 8 |
| Author | PrimeFan (13766) |
| Entry type | Definition |
| Classification | msc 47A60 |
| Related topic | CalculusOfVariations |
| Related topic | EulerLagrangeDifferentialEquation |