Results 31 to 40 of about 4,470,820 (395)
THE SPECTRUM OF ISOTROPIC DIFFUSE GAMMA-RAY EMISSION BETWEEN 100 MeV AND 820 GeV [PDF]
The γ-ray sky can be decomposed into individually detected sources, diffuse emission attributed to the interactions of Galactic cosmic rays with gas and radiation fields, and a residual all-sky emission component commonly called the isotropic diffuse γ ...
T. A. C. M. Ackermann +143 more
semanticscholar +1 more source
InPBi Quantum Dots for Super-Luminescence Diodes
InPBi thin film has shown ultra-broad room temperature photoluminescence, which is promising for applications in super-luminescent diodes (SLDs) but met problems with low light emission efficiency.
Liyao Zhang +4 more
doaj +1 more source
We demonstrate InGaN/GaN superluminescent diodes with broadened emission spectra fabricated on surface-shaped bulk GaN (0001) substrates. The patterning changes the local vicinal angle linearly along the device waveguide, which results in an indium ...
A. Kafar +8 more
semanticscholar +1 more source
In an attempt to improve U II analysis, the lowest configurations of both parities have been interpreted by means of the Racah-Slater parametric method, using Cowan codes.
Ali Meftah +3 more
doaj +1 more source
On the Integrated Spectrum of the X-ray Binaries and the Origin of Soft X-ray Emission from the Bulge of M31 [PDF]
Using ROSAT PSPC data, we have performed several tests aimed at understanding the origin of the soft X-ray spectral component detected from the bulge of M31.
Aschenbach B. +4 more
core +4 more sources
Tailoring emission spectra by using microcavities
We present a theoretical model to describe emission spectrum of an emitter in a micro-cavity. Our model proposes that the spectrum in a metal micro-cavity depends on the product of the emission spectrum in free space and the local density of states (LDOS)
Muhammad Hanif Ahmed Khan Khushik +1 more
doaj +1 more source
Spectroscopic Identification of the Infrared Counterpart to GX5-1 [PDF]
Using CGS4 on UKIRT, we have obtained a 1.95-2.45 micron infrared spectrum of the primary candidate counterpart to the bright Z LMXB GX5-1. IR photometry by Naylor, Charles, & Longmore (1992) and the astrometry of Jonker et al.
Bandyopadhyay, R. M. +2 more
core +2 more sources
Quasiclassical approach to synergic synchrotron–Cherenkov radiation in polarized vacuum
Photon emission by an ultrarelativistic charged particle in extremely strong magnetic field is analyzed, with vacuum polarization and photon recoil taken into account. Vacuum polarization is treated phenomenologically via refractive index.
I I Artemenko +2 more
doaj +1 more source
Emission spectrum of the driven nonlinear oscillator [PDF]
Motivated by recent "circuit QED" experiments we investigate the noise properties of coherently driven nonlinear resonators. By using Josephson junctions in superconducting circuits, strong nonlinearities can be engineered, which lead to the appearance ...
St'ephane Andr'e +4 more
semanticscholar +1 more source
Observations of the post shock break-out emission of SN 2011dh with XMM-Newton [PDF]
After the occurrence of the type cIIb SN 2011dh in the nearby spiral galaxy M 51 numerous observations were performed with different telescopes in various bands ranging from radio to gamma-rays.
Ducci, Lorenzo, Sasaki, Manami
core +4 more sources

