Some time ago it was conjectured that the coefficients of an expansion of the Jones polynomial in terms of the cosmological constant could provide an infinite string of knot invariants that are solutions of the vacuum Hamiltonian constraint of quantum gravity in the loop representation. Here we discuss the status of this conjecture at third order in the cosmological constant. The calculation is performed in the extended loop representation, a generalization of the loop representation. It is shown that the the Hamiltonian does not annihilate the third coefficient of the Jones polynomal (J_3) for general extended loops. For ordinary loops the result acquires an interesting geometrical meaning and new possibilities appear for J_3 to represent ...
We apply the ideas of Alvarez and Labastida to the invariant of spin networks defined by Witten and ...
We show that Vassiliev invariants of knots, appropriately generalized to the spin network context, a...
We show that the Hamiltonian of four-dimensional Lorentzian gravity, defined on a space of real, SU(...
Solutions to both the diffeomorphism and the hamiltonian constraint of quantum gravity have been fou...
We find a consistent formulation of the constraints of quantum gravity with a cosmological constant ...
In this paper we review the status of several solutions to all the constraints of quantum gravity th...
In the loop representation the quantum constraints of gravity can be solved. This fact allowed signi...
These notes summarize the lectures delivered in the V Mexican School of Particle Physics, at the Uni...
We propose a new representation for gauge theories and quantum gravity. Alternatively, it can be vie...
We propose to interpret the action of the quantum Hamiltonian constraint of general relativity in th...
We study three-dimensional Chern-Simons theory with complex gauge group SL(2,ℂ), which has many inte...
We present an implementation of the loop representation of quantum gravity on a square lattice. Inst...
The loop-space representation based on Ashtekars new variables has allowed for the first time the co...
We show that the second coefficient of the Conway knot polynomial is annihilated by the Hamiltonian ...
We describe a deformation of the observable algebra of quantum gravity in which the loop algebra is ...
We apply the ideas of Alvarez and Labastida to the invariant of spin networks defined by Witten and ...
We show that Vassiliev invariants of knots, appropriately generalized to the spin network context, a...
We show that the Hamiltonian of four-dimensional Lorentzian gravity, defined on a space of real, SU(...
Solutions to both the diffeomorphism and the hamiltonian constraint of quantum gravity have been fou...
We find a consistent formulation of the constraints of quantum gravity with a cosmological constant ...
In this paper we review the status of several solutions to all the constraints of quantum gravity th...
In the loop representation the quantum constraints of gravity can be solved. This fact allowed signi...
These notes summarize the lectures delivered in the V Mexican School of Particle Physics, at the Uni...
We propose a new representation for gauge theories and quantum gravity. Alternatively, it can be vie...
We propose to interpret the action of the quantum Hamiltonian constraint of general relativity in th...
We study three-dimensional Chern-Simons theory with complex gauge group SL(2,ℂ), which has many inte...
We present an implementation of the loop representation of quantum gravity on a square lattice. Inst...
The loop-space representation based on Ashtekars new variables has allowed for the first time the co...
We show that the second coefficient of the Conway knot polynomial is annihilated by the Hamiltonian ...
We describe a deformation of the observable algebra of quantum gravity in which the loop algebra is ...
We apply the ideas of Alvarez and Labastida to the invariant of spin networks defined by Witten and ...
We show that Vassiliev invariants of knots, appropriately generalized to the spin network context, a...
We show that the Hamiltonian of four-dimensional Lorentzian gravity, defined on a space of real, SU(...