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Spin Foam Gravity (SFG) has reached a stage of development where perhaps we could have a new abbreviation to distinguish it from previous Loop gravity formulations. I could be wrong about this, of course, but I want to see how things look from that angle. There seem to be some language/organization innovations in Wieland's thesis that preserve basic content but give the theory a different look. E.g. the use of spinors (which has become widespread in recent research), and see also the footnote on page 135.
==from page 6==
.. can show that spin foam gravity comes from the canonical quantisation of a classical theory. This is a version of first-order Regge calculus [64], with spinors as the fundamental configuration variables. I will present this result in chapters 3 and 4. It should be a convincing evidence that spinors provide a universal language to bring the two sides of the theory together.
==endquote==
http://tel.archives-ouvertes.fr/docs/00/95/24/98/PDF/diss.pdf
==from pages 134-135==
To canonically quantise gravity it is often thought that one first needs to start from a 3+1 split, study the ADM (Arnowitt–Deser–Miser) formulation in the “right” variables, identify the canonical structure and perform a Schrödinger quantisation. The results of this thesis question this idea.
The ADM formulation is very well adapted to a continuous spacetime, but in spinfoam gravity we are working with a discretisation of the manifold, hence lacking that assumption. Instead we have simplices glued together and should find a Hamiltonian formulation better adapted to the problem.
After the introductory chapters 1 and 2, we found such a Hamiltonian formalism for the discretised theory. The underlying Hamiltonian generates the time evolution along the edges of the spinfoam. The corresponding time variable parametrises the edges of the discretisation, it is nothing but a coordinate, and does not measure duration as given by a clock…
…
...
In summary, the classical part introduced a canonical formulation of spinfoam gravity adapted to a simplicial discretisation of spacetime. This framework should be of general interest, as it provides a solid foundation where different models could fruitfully be compared.
The last section was about quantum theory. With the Hamiltonian formulation of the spinfoam dynamics at hand, canonical quantisation was straight-forward. We used an auxiliary Hilbert space to define the operators. Physical states are in the kernel of the first-class constraints. The second-class constraints act as ladder operators. One of them (Fˆn) annihilates physical states, while the other one (Fˆn†) maps them to their orthogonal complement, i.e. into the spurious part of the auxiliary Hilbert space. This is exactly what happens in the Gupta–Bleuler formalism.
Dynamics is determined by the Schrödinger equation. We quantised the classical Hamiltonian and solved the Schrödinger equation that gives the evolution of the quantum states along the boundary of a spinfoam face. This boundary evolution matched the Schrödinger equation introduced by Bianchi in the thermodynamical analysis of spinfoam gravity [113]. Gluing the individual transition amplitudes together, we got the amplitude for a spinfoam face*, which was in exact agreement with the EPRL model.
…
..
__________________
*We can organise the EPRL amplitudes such that each spinfoam vertex contributes through its vertex amplitude to the total amplitude, while the contribution from the faces looks rather trivial. Here we do the opposite, and assign non-trivial amplitudes to the spinfoam faces. These are two different ways to write the same model. Reference [62] gives several equivalent definitions of the amplitudes, and explains the equivalence.
==endquote==
==from page 6==
.. can show that spin foam gravity comes from the canonical quantisation of a classical theory. This is a version of first-order Regge calculus [64], with spinors as the fundamental configuration variables. I will present this result in chapters 3 and 4. It should be a convincing evidence that spinors provide a universal language to bring the two sides of the theory together.
==endquote==
http://tel.archives-ouvertes.fr/docs/00/95/24/98/PDF/diss.pdf
==from pages 134-135==
To canonically quantise gravity it is often thought that one first needs to start from a 3+1 split, study the ADM (Arnowitt–Deser–Miser) formulation in the “right” variables, identify the canonical structure and perform a Schrödinger quantisation. The results of this thesis question this idea.
The ADM formulation is very well adapted to a continuous spacetime, but in spinfoam gravity we are working with a discretisation of the manifold, hence lacking that assumption. Instead we have simplices glued together and should find a Hamiltonian formulation better adapted to the problem.
After the introductory chapters 1 and 2, we found such a Hamiltonian formalism for the discretised theory. The underlying Hamiltonian generates the time evolution along the edges of the spinfoam. The corresponding time variable parametrises the edges of the discretisation, it is nothing but a coordinate, and does not measure duration as given by a clock…
…
...
In summary, the classical part introduced a canonical formulation of spinfoam gravity adapted to a simplicial discretisation of spacetime. This framework should be of general interest, as it provides a solid foundation where different models could fruitfully be compared.
The last section was about quantum theory. With the Hamiltonian formulation of the spinfoam dynamics at hand, canonical quantisation was straight-forward. We used an auxiliary Hilbert space to define the operators. Physical states are in the kernel of the first-class constraints. The second-class constraints act as ladder operators. One of them (Fˆn) annihilates physical states, while the other one (Fˆn†) maps them to their orthogonal complement, i.e. into the spurious part of the auxiliary Hilbert space. This is exactly what happens in the Gupta–Bleuler formalism.
Dynamics is determined by the Schrödinger equation. We quantised the classical Hamiltonian and solved the Schrödinger equation that gives the evolution of the quantum states along the boundary of a spinfoam face. This boundary evolution matched the Schrödinger equation introduced by Bianchi in the thermodynamical analysis of spinfoam gravity [113]. Gluing the individual transition amplitudes together, we got the amplitude for a spinfoam face*, which was in exact agreement with the EPRL model.
…
..
__________________
*We can organise the EPRL amplitudes such that each spinfoam vertex contributes through its vertex amplitude to the total amplitude, while the contribution from the faces looks rather trivial. Here we do the opposite, and assign non-trivial amplitudes to the spinfoam faces. These are two different ways to write the same model. Reference [62] gives several equivalent definitions of the amplitudes, and explains the equivalence.
==endquote==