|
Speaker |
Blixt, Daniel |
|
Coauthors |
Hohmann, Manuel; Pfeifer, Christian; Krššák, Martin |
| Talk Title |
Hamiltonian Analysis In New General Relativity |
|
Abstract |
It is known that one can formulate an action in teleparallel gravity which is equivalent to general relativity, up to a boundary term. In this geometry we have vanishing curvature, and non-vanishing torsion. The action is constructed by three different contractions of torsion with specific coefficients. By allowing these coefficients to be arbitrary we get the theory which is called "new general relativity". The Lagrangian for new general relativity is is written down in ADM-variables. In order to write down the Hamiltonian we need to invert the velocities to canonical variables. However, the inversion depends on the specific combination of constraints satisfied by the theory (which depends on the coefficients in the Lagrangian). It is found that one can combine these constraints in 9 different ways to obtain non-trivial theories, each with a different inversion formula. The teleparallel equivalent to general relativity gives 2 degrees of freedom. However, this number does not hold for arbitrary coefficients. |
|
Talk view |
|
|
|
|