In terms of two-spinors a chiral formulation of general relativity with the Ashtekar Lagrangian and its Hamiltonian formalism in which the basic dynamic variables are the dyad spinors are presented. The extended Witten identities are derived. A new expression of the Hamiltonian boundary term is obtained. Using this expression and the extended Witten identities the proof of the positive energy theorem is extended to a case including momentum and angular momentum
We show that the Einstein-Hilbert, the Einstein-Palatini, and the Holst actions can be derived from ...
An overview of the field of Chiral Lagrangians is given. This includes Chiral Perturbation Theory an...
DescriptionContentsResourcesCoursesAbout the Authors This monograph describes the different formulat...
We calculate the energy momentum tensor to orderE 4 in chiral perturbation theory. New terms not pre...
We calculate the energy momentum tensor to order E4 in chiral perturbation theory. New terms not pre...
The canonical transformation of the phase space of general relativity introduced by Ashtekar is exte...
In this letter we apply an alternative approach, recently developed, to the description of massless ...
Killing-Yano tensors are natural generalizations of Killing vectors to arbitrary rank antisymmetric ...
Classical gravity has sufficient supersymmetric extension that its Hamiltonian is expressible as a P...
We first describe a class of spinor-curvature identities (SCI) which have gravitational applications...
AbstractFollowing the Witten–Nester formalism, we present a useful prescription using Weyl spinors t...
Abstract We develop a new embedding-space formalism for AdS4 a...
To understand the coupling behavior of the spinor with spacetime, the explicit form of the energy-mo...
International audienceWe consider non-chiral, full Lorentz group-based Plebanski formulation of gene...
The improvement terms in the generalised energy-momentum tensor of Callan, Coleman and Jackiw can be...
We show that the Einstein-Hilbert, the Einstein-Palatini, and the Holst actions can be derived from ...
An overview of the field of Chiral Lagrangians is given. This includes Chiral Perturbation Theory an...
DescriptionContentsResourcesCoursesAbout the Authors This monograph describes the different formulat...
We calculate the energy momentum tensor to orderE 4 in chiral perturbation theory. New terms not pre...
We calculate the energy momentum tensor to order E4 in chiral perturbation theory. New terms not pre...
The canonical transformation of the phase space of general relativity introduced by Ashtekar is exte...
In this letter we apply an alternative approach, recently developed, to the description of massless ...
Killing-Yano tensors are natural generalizations of Killing vectors to arbitrary rank antisymmetric ...
Classical gravity has sufficient supersymmetric extension that its Hamiltonian is expressible as a P...
We first describe a class of spinor-curvature identities (SCI) which have gravitational applications...
AbstractFollowing the Witten–Nester formalism, we present a useful prescription using Weyl spinors t...
Abstract We develop a new embedding-space formalism for AdS4 a...
To understand the coupling behavior of the spinor with spacetime, the explicit form of the energy-mo...
International audienceWe consider non-chiral, full Lorentz group-based Plebanski formulation of gene...
The improvement terms in the generalised energy-momentum tensor of Callan, Coleman and Jackiw can be...
We show that the Einstein-Hilbert, the Einstein-Palatini, and the Holst actions can be derived from ...
An overview of the field of Chiral Lagrangians is given. This includes Chiral Perturbation Theory an...
DescriptionContentsResourcesCoursesAbout the Authors This monograph describes the different formulat...