Buffer Gas Cooling in Molecular Spectroscopy
ISEF · 2016
Overview
To improve the molecular spectral resolution, the gas of interest must be cooled to reduce thermal noise. A method of buffer gas cooling is used, where a noble gas (buffer gas) cooled by a cryogenic pump is flowed in with the gas of focus. This is an efficient and simple way of cooling a gas down to a few-Kelvin temperatures. We have studied which buffer gas provides the best spectral resolution comparing Helium to Neon. We find that despite the expected enhanced clustering advantages of Neon, Helium provides the least Doppler broadening, resulting in best spectral resolution.
Competition history
- ISEF 2016
Resources
Related projects
ISEF · 2024
Design of Active Magnetic Field Stabilization for Quantum Gas Experiments
ISEF · 2026
Computations Fluid Dynamics Based Evaluation of Cryogenic Heat Transfer in Helical Tube Heat Exchangers
ISEF · 2019
Applications of Helium-4 Doubly Forbidden Singlet-Triplet Transition Lines in Astronomical Spectroscopy
ISEF · 2019
High-Accuracy Measurements of Gas Velocities in Regions of Star Formation
Closest projects by meaning, across every fair and year in the corpus.
Source: Regeneron International Science and Engineering Fair