Experimental methods for primary thermometry, after Kelvin unit redefinition on May 2019, become based on a known value of the Boltzmann constant rather than by measuring temperature with respect to a reference point. In this frame, we propose linestrength ratio thermometry (LRT) as a candidate method for primary thermometry in the 9?700 K temperature range. Temperature accuracies at the ppm level are prospected for LRT applied to optical transitions of the CO molecule in the range 80?700 K and of a rare-earth-doped crystal in the 9?100 K one. Future implementations of this technique can contribute to measure the calibration-discrepancies in the ITS-90 metrological scale of thermodynamic temperature which can have a measurable impact in applications ranging from fundamental-physics to meteorology and climatology.

Linestrength ratio spectroscopy as a new primary thermometer for redefined Kelvin dissemination

2019

Abstract

Experimental methods for primary thermometry, after Kelvin unit redefinition on May 2019, become based on a known value of the Boltzmann constant rather than by measuring temperature with respect to a reference point. In this frame, we propose linestrength ratio thermometry (LRT) as a candidate method for primary thermometry in the 9?700 K temperature range. Temperature accuracies at the ppm level are prospected for LRT applied to optical transitions of the CO molecule in the range 80?700 K and of a rare-earth-doped crystal in the 9?100 K one. Future implementations of this technique can contribute to measure the calibration-discrepancies in the ITS-90 metrological scale of thermodynamic temperature which can have a measurable impact in applications ranging from fundamental-physics to meteorology and climatology.
2019
Istituto Nazionale di Ottica - INO
Inglese
21
11
113008
113008
10
http://www.scopus.com/inward/record.url?eid=2-s2.0-85075156468&partnerID=q2rCbXpz
Sì, ma tipo non specificato
molecular spectroscopy
primary thermometry
laser spectroscopy
carbon monoxide
rare earth doped crystal
Kelvin dissemination
The authors acknowledge partially financial support by: Project MOST funded by Agenzia Spaziale Italiana, project WhiTech funded by Agenzia Spaziale Italiana and Progetti di Ricerca di Interesse Nazionale (PRIN), Project No. 20152MRAKH of the Italian Ministry of University and Research. We acknowledged I Galli for experimental support and discussions regarding N<INF>2</INF>O experimental test.
5
info:eu-repo/semantics/article
262
Amato Luigi Santamaria, ; de Cumis Mario Siciliani, ; Giuseppe, Bianco; Raffaele, Pastore; Pastor Pablo Cancio,
01 Contributo su Rivista::01.01 Articolo in rivista
none
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.14243/382630
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