In the context of a gauge theory for the translation group, a conserved energy-momentum gauge current for the gravitational field is obtained. It is a true spacetime and gauge tensor, and transforms covariantly under global Lorentz transformations. By rewriting the gauge gravitational field equation in a purely spacetime form, it becomes the teleparallel equivalent of Einstein's equation, and the gauge current reduces to the M{\o}ller's canonical energy-momentum density of the gravitational field
Quantum mechanics in the presence of $\delta$-function potentials is known to be plagued by UV diver...
We consider toy cosmological models in which a classical, homogeneous, spinor field provides a domin...
We introduce a method to obtain deformed defects starting from a given scalar field theory which pos...
A measurement strategy is developed for a new kind of hypothesis testing. It assigns, with minimum p...
We show that the existence of appropriate spatial homothetic Killing vectors is directly related to ...
We consider general relativistic Cauchy data representing two nonspinning, equal-mass black holes bo...
From two different modifications of the Gell-Mann-Okubo mass relation for (1/2)^+ baryons: the first...
We reconsider the phenomenon of mass generation via coordinate-dependent compactifications of higher...
Strong, fast pulses, called ``bang-bang'' controls can be used to eliminate the effects of system-en...
We consider static axially symmetric Einstein-Yang-Mills black holes in the isolated horizon formali...
We present Cu and Ba abundances for 7 G-K dwarf stars, members of the solar-metallicity, 0.3 Gyr old...
This is the third of a series of papers treating light baryon resonances up to 3 GeV within a relati...
In order to obtain stable and accurate general relativistic simulations, re-formulations of the Eins...
Several numerical relativity groups are using a modified ADM formulation for their simulations which...
The entanglement of excitonic states in a system of $N$ spatially separated semiconductor microcryst...
Quantum mechanics in the presence of $\delta$-function potentials is known to be plagued by UV diver...
We consider toy cosmological models in which a classical, homogeneous, spinor field provides a domin...
We introduce a method to obtain deformed defects starting from a given scalar field theory which pos...
A measurement strategy is developed for a new kind of hypothesis testing. It assigns, with minimum p...
We show that the existence of appropriate spatial homothetic Killing vectors is directly related to ...
We consider general relativistic Cauchy data representing two nonspinning, equal-mass black holes bo...
From two different modifications of the Gell-Mann-Okubo mass relation for (1/2)^+ baryons: the first...
We reconsider the phenomenon of mass generation via coordinate-dependent compactifications of higher...
Strong, fast pulses, called ``bang-bang'' controls can be used to eliminate the effects of system-en...
We consider static axially symmetric Einstein-Yang-Mills black holes in the isolated horizon formali...
We present Cu and Ba abundances for 7 G-K dwarf stars, members of the solar-metallicity, 0.3 Gyr old...
This is the third of a series of papers treating light baryon resonances up to 3 GeV within a relati...
In order to obtain stable and accurate general relativistic simulations, re-formulations of the Eins...
Several numerical relativity groups are using a modified ADM formulation for their simulations which...
The entanglement of excitonic states in a system of $N$ spatially separated semiconductor microcryst...
Quantum mechanics in the presence of $\delta$-function potentials is known to be plagued by UV diver...
We consider toy cosmological models in which a classical, homogeneous, spinor field provides a domin...
We introduce a method to obtain deformed defects starting from a given scalar field theory which pos...