A theoretical investigation is carried out into the impact of incoherent pumping fields and quantum interference induced by incoherent pumping fields on the Kerr nonlinearity in a three-level asymmetric semiconductor quantum well system. It is found that Kerr nonlinearity is so sensitive to the rate of incoherent pumping fields, but insensitive to the quantum interference induced by incoherent ...

We find an exact solution of Kerr-Newman-de Sitter type on the braneworld(4D) of the DGP model. When a constant 4D Ricci scalar is assumed, only zero(flat) and a positive(deSitter) values satisfy the Hamiltonian constraint equation coming from the extra dimension. With a Z2-symmetry across the brane and a stationary and axisymmetric metric ansatz on the brane, we solve the constraint equation e...

The standard approach to initial data for both analytic and numerical computations of black hole collisions has been to use conformally-flat initial geometry. Among other advantages, this choice allows the simple superposition of holes with arbitrary mass, location and spin. The conformally flat restriction, however, is inappropriate to the study of Kerr holes, for which the standard constant-t...

We discuss a simple and experimentally realizable model for creation of enhanced Kerr nonlinearities accompanied by vanishing absorption. The model involves a V -type atom subjected to a strong drive laser, a weak probe laser and coupled to a single-mode cavity field. Working in the bad-cavity limit, we find that the simultaneous coupling of the cavity field to both atomic transitions creates a...

We formulate conditions on the geometry of a non-expanding horizon ∆ which are sufficient for the space-time metric to coincide on ∆ with the Kerr metric. We introduce an invariant which can be used as a measure of how different the geometry of a given non-expanding horizon is from the geometry of the Kerr horizon. Directly, our results concern the space-time metric at ∆ at the zeroth and the f...

Replace this text with the abstract of your paper. ENERGY OF KERR-NEWMAN BLACK-HOLES AND GRAVITOMAGNETISM Marcelo Samuel Berman Editora Albert Einstein R. Candido Hartman, 575, #17, Ed. Renoir 80730-440 Curitiba PR Brazil eMail: [email protected] Abstract New formulae are obtained for the energy of K.N. b.h.’s that point out a gravitomagnetic energy effect. The results are valid for slowly or ...

We consider the electromagnetic response of a topological Weyl semimetal (TWS) with a pair of Weyl nodes in the bulk and corresponding Fermi arcs in the surface Brillouin zone. We compute the frequency-dependent complex conductivities σαβ(ω) and also take into account the modification of Maxwell equations by the topological θ-term to obtain the Kerr and Faraday rotations in a variety of geometr...

This is a review paper of basic knowledge and recent advances in the area of spatial solitons in Kerr and Kerr-like media. We consider spatial bright and dark solitons, sol-itons in waveguide geometries, optical bullets, vortex solitons and, brie¯y, dissipative cases. In our treatment, we use a Hamiltonian approach when considering stability issues.

The importance of Dr. Robert Kerr in Canadian history is not large, but he played a significant role in the early years of what is now Ontario. Though his Canadian years were spent largely in active military service and, after his discharge, at Kingston and in the Niagara peninsula, nevertheless, in the compact and sparse settlements and posts of the times he was widely known and influential. M...