Add to ORKGWe define conserved gravitational charges in cosmologically extended topologically massive gravity, exhibit them in surface integral form about their de Sitter or flat vacua and verify their correctness in terms of two basic types of solution
The Green’s function of the Schr¨odinger equation with the Coulomb potential in the space of constan...
Strong, surprising, and multifaceted effects of the width of the external surface layer Δξ and inter...
We compute the energy and angular momenta of recent D-dimensional Kerr–AdS solutions to cosmological...
We define conserved gravitational charges in cosmologically extended topologically massive gravity, ...
The Parametrized Post-Newtonian expansion of gravitational theories with a scalar field coupled to t...
The antisymmetric sector of the nonsymmetric gravitational theory (NGT) does not possess a rigorous ...
We consider the coupling to gravity in 4+delta dimensions of a non linear electroweak symmetry break...
We consider a supersymmetric extension of the algebra associated with three and four dimensional Ant...
We present a model where a non-conventional scalar field may act like dark energy leading to cosmic ...
AbstractA dynamical symmetry, as well as special diffeomorphism algebras generalizing the Witt–Viras...
The tensor self energy is computed at one loop order in a model in which a vector and tensor interac...
A definition of the gravitational flow and a short description of the recipe of its calculation are ...
In our previous paper, we constructed bounds on the effective bulk modulus of isotropic multicompone...
When an open string ends with charges on a D2-brane, which involves constant background magnetic fie...
In this comment we show that the statement in Ahluwalia et al. that the existence of Elko spinor fie...
The Green’s function of the Schr¨odinger equation with the Coulomb potential in the space of constan...
Strong, surprising, and multifaceted effects of the width of the external surface layer Δξ and inter...
We compute the energy and angular momenta of recent D-dimensional Kerr–AdS solutions to cosmological...
We define conserved gravitational charges in cosmologically extended topologically massive gravity, ...
The Parametrized Post-Newtonian expansion of gravitational theories with a scalar field coupled to t...
The antisymmetric sector of the nonsymmetric gravitational theory (NGT) does not possess a rigorous ...
We consider the coupling to gravity in 4+delta dimensions of a non linear electroweak symmetry break...
We consider a supersymmetric extension of the algebra associated with three and four dimensional Ant...
We present a model where a non-conventional scalar field may act like dark energy leading to cosmic ...
AbstractA dynamical symmetry, as well as special diffeomorphism algebras generalizing the Witt–Viras...
The tensor self energy is computed at one loop order in a model in which a vector and tensor interac...
A definition of the gravitational flow and a short description of the recipe of its calculation are ...
In our previous paper, we constructed bounds on the effective bulk modulus of isotropic multicompone...
When an open string ends with charges on a D2-brane, which involves constant background magnetic fie...
In this comment we show that the statement in Ahluwalia et al. that the existence of Elko spinor fie...
The Green’s function of the Schr¨odinger equation with the Coulomb potential in the space of constan...
Strong, surprising, and multifaceted effects of the width of the external surface layer Δξ and inter...
We compute the energy and angular momenta of recent D-dimensional Kerr–AdS solutions to cosmological...