A comparison between different propagative schemes for the simulation of tapered step index slab waveguides

The performance and accuracy of a number of propagative algorithms are compared for the simulation of tapered high contrast step index slab waveguides. The considered methods include paraxial as well as nonparaxial formulations of optical field propagation. In particular attention is paid to the validity of the paraxial approximation. To test the internal consistency of the various methods the property of reciprocity is verified and it is shown that for the paraxial algorithms the reciprocity can only be fulfilled if the paraxial approximation of the power flux expression using the Poynting vector is considered. Finally, modeling results are compared with measured fiber coupling losses for an experimentally realized taper structure

All-sky search for long-duration gravitational wave transients with initial LIGO

We present the results of a search for long-duration gravitational wave transients in two sets of data collected by the LIGO Hanford and LIGO Livingston detectors between November 5, 2005 and September 30, 2007, and July 7, 2009 and October 20, 2010, with a total observational time of 283.0 days and 132.9 days, respectively. The search targets gravitational wave transients of duration 10-500 s in a frequency band of 40-1000 Hz, with minimal assumptions about the signal waveform, polarization, source direction, or time of occurrence. All candidate triggers were consistent with the expected background; as a result we set 90% confidence upper limits on the rate of long-duration gravitational wave transients for different types of gravitational wave signals. For signals from black hole accretion disk instabilities, we set upper limits on the source rate density between 3.4×10-5 and 9.4×10-4 Mpc-3 yr-1 at 90% confidence. These are the first results from an all-sky search for unmodeled long-duration transient gravitational waves. © 2016 American Physical Society

All-sky search for long-duration gravitational wave transients with initial LIGO

We present the results of a search for long-duration gravitational wave transients in two sets of data collected by the LIGO Hanford and LIGO Livingston detectors between November 5, 2005 and September 30, 2007, and July 7, 2009 and October 20, 2010, with a total observational time of 283.0 days and 132.9 days, respectively. The search targets gravitational wave transients of duration 10-500 s in a frequency band of 40-1000 Hz, with minimal assumptions about the signal waveform, polarization, source direction, or time of occurrence. All candidate triggers were consistent with the expected background; as a result we set 90% confidence upper limits on the rate of long-duration gravitational wave transients for different types of gravitational wave signals. For signals from black hole accretion disk instabilities, we set upper limits on the source rate density between 3.4×10-5 and 9.4×10-4 Mpc-3 yr-1 at 90% confidence. These are the first results from an all-sky search for unmodeled long-duration transient gravitational waves. © 2016 American Physical Society

Search for Tensor, Vector, and Scalar Polarizations in the Stochastic Gravitational-Wave Background

The detection of gravitational waves with Advanced LIGO and Advanced Virgo has enabled novel tests of general relativity, including direct study of the polarization of gravitational waves. While general relativity allows for only two tensor gravitational-wave polarizations, general metric theories can additionally predict two vector and two scalar polarizations. The polarization of gravitational waves is encoded in the spectral shape of the stochastic gravitational-wave background, formed by the superposition of cosmological and individually unresolved astrophysical sources. Using data recorded by Advanced LIGO during its first observing run, we search for a stochastic background of generically polarized gravitational waves. We find no evidence for a background of any polarization, and place the first direct bounds on the contributions of vector and scalar polarizations to the stochastic background. Under log-uniform priors for the energy in each polarization, we limit the energy densities of tensor, vector, and scalar modes at 95% credibility to Ω0T<5.58×10-8, Ω0V<6.35×10-8, and Ω0S<1.08×10-7 at a reference frequency f0=25 Hz. © 2018 American Physical Society

Bauelement der integrierten Optik

DE 3600458 A UPAB: 19930922 The integrated optical element consists of a monolithic electro-optical component with electrodes to generate a horizontal or vertical electric field. The element alters the phase and the polarisation direction of the light passing through it. The element may have a flat bottom surface and a stepped top surface. To generate a horizontal field, there are electrodes on either side of the raised stop in the top surface, one of them having a p+ doped area under it, the other having a n+ area. To generate a vertical field, electrodes are applied to the raised step on the top surface and to the flat bottom surface. There is a p+ doped area at the top electrode with a n' area underneath and the bottom portion over the bottom electrode is n+ doped. USE - Lasers, photodiodes, optical waveguides. 0/

Verfahren zum Herstellen strukturierter Epitaxieschichten

DE 2944118 A UPAB: 19930915 The method of forming structured epitaxial layers on semiconductor elements uses molecular radiation which is directed towards the substrate on which is formed a pattern of different crystal regions. Laser radiation is applied selectively to produce a pattern of light and shadow zones, by using a mask. This causes different rates of crystal growth, so that single crystal regions alternate with polycrystalline regions. This forms part of an epitaxial etching system, the wavelength and intensity of the laser radiation being modified selectively. The laser beam may be made up of two sets of radiation of two different wavelengths

Self-aligned waveguide mirrors for optical integration on InGaAsP/InP

Totally reflecting mirrors for monomode rib waveguides in InGaAsP/InP were fabricated by reactive ion etching using a self-aligning technique. For eight mirrors in series an average excess loss of 1.5 dB per mirror was observed. The loss mechanisms are discussed