Nettet17. mar. 2024 · The linewidth is roughly determined by the average slope in the fluctuation range of the parameter X. At the EP, the linewidth is about 100 times … Nettet2 dager siden · These studies demand a re-evaluation of the role of the turbulence in massive star formation. Aims. We aim to study the turbulence in a typical massive star-forming region G35.20-0.74 N with a sufficient spatial resolution to resolve the thermal Jeans length, and a spectral resolution to resolve the thermal linewidth. Methods.
7.3.6 Homogeneous and Inhomogeneous Broadening - MIT …
NettetHomogeneous Broadening Definition: the increase in the linewidth of an atomic transition caused by effects which affect different radiating or absorbing atoms in the same way German: homogene Verbreiterung Category: physical foundations How to cite the article; suggest additional literature Author: Dr. Rüdiger Paschotta NettetThe obtained linewidth of the transition spectra is about 10 MHz, which is are some greater than the natural linewidth and limited by the broadening from the probe and lattice light. Our experiment that measures the frequencies of the 3 P 0,2-3 S 1 transitions of 171 Yb atoms in an optical lattice differs from all previous work [33], [34]. trudel banoffee
Linewidth Broadening in Short-Wavelength Quantum Cascade …
Nettet6. jul. 2024 · It is predicted that the linewidth (Δ λQC) is mainly contributed by the two opposing effects: (i) the linewidth broadening due to the repulsive kinetic energy of … NettetThere are a couple of reasons for the absorption line to get broader, such as pressure, Doppler effect, and more - but as said earlier, even a single atom in vacuum has a … Nettet8. aug. 2014 · Abstract. A review of the models used for the calculation of the Stark broadening spectrum for plasmas is presented. The aim is to provide an overview of the related theories using a simple formalism, useful for an introduction to the study of this phenomenon, which is encountered in plasma diagnostics. trudence hicks