Spectroscopic detection of radiocarbon dioxide at parts-per-quadrillion sensitivity
Year: 2016
Authors: Galli I., Bartalini S., Ballerini R., Barucci M., Cancio P., De Pas M., Giusfredi G., Mazzotti D., Akikusa N., De Natale P.
Autors Affiliation: CNR, INO, Via Carrara 1, I-50019 Sesto Fiorentino, FI, Italy; European Lab Nonlinear Spect LENS, Via Carrara 1, I-50019 Sesto Fiorentino, FI, Italy; CNR, INO, Largo Fermi 6, I-50125 Florence, FI, Italy; Hamamatsu Photon KK, Dev Bur Laser Device R&D Grp, Shizuoka 4348601, Japan.
Abstract: High-sensitivity radiocarbon detection has been, until now, a prerogative of accelerator mass spectrometry (AMS). Here we present a compact and simple spectroscopic apparatus, based on saturated-absorption cavity ring-down, approaching the ultimate AMS sensitivity. We measure radiocarbon dioxide concentration down to a few parts per quadrillion by use of a heterodyne-spectroscopy system with two quantum cascade lasers at 4.5 mu m, a reference cell, and a high-finesse cavity with the sample gas cooled down to 170 K. Our results pave the way to a paradigm change in radiocarbon measurement, with a number of significant applications in areas such as environment, nuclear security, pharmacology, and cultural heritage. (C) 2016 Optical Society of America
Journal/Review: OPTICA
Volume: 3 (4) Pages from: 385 to: 388
More Information: Programma Nazionale di Ricerche in Antartide (PNRA) (project 2013/AC4.01); ESFRI Roadmap Project “Extreme Light Infrastructure (ELI); EU 7th Framework Program 284464.KeyWords: Light measurement; Mass spectrometry; Quantum cascade lasers, Accelerator mass spectrometry; Cultural heritages; Heterodyne spectroscopy; High sensitivity; High-finesse cavity; Nuclear security; Saturated absorptions; Spectroscopic detection, Absorption spectroscopyDOI: 10.1364/OPTICA.3.000385ImpactFactor: 7.727Citations: 104data from “WEB OF SCIENCE” (of Thomson Reuters) are update at: 2024-12-08References taken from IsiWeb of Knowledge: (subscribers only)Connecting to view paper tab on IsiWeb: Click hereConnecting to view citations from IsiWeb: Click here