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MERLIN, a RT-LTE software supporting the LIBS diagnostic : application to H-isotopes measurements

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HAL Id: hal-03011810

https://hal.archives-ouvertes.fr/hal-03011810

Submitted on 18 Nov 2020

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MERLIN, a RT-LTE software supporting the LIBS diagnostic : application to H-isotopes measurements

Aurélien Favre, Morgan Lesage, Vincent Morel, Arnaud Bultel, Pascal Boubert

To cite this version:

Aurélien Favre, Morgan Lesage, Vincent Morel, Arnaud Bultel, Pascal Boubert. MERLIN, a RT- LTE software supporting the LIBS diagnostic : application to H-isotopes measurements. International Workshop on LIBS, Dec 2020, Szeged, Hungary. �hal-03011810�

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International Workshop on LIBS , Szeged , Hungary , 1 2 nd December 2020

CONTEXT & OBJECTIVES

LIBS (Laser-Induced Breakdown Spectroscopy) enables the determination of targets composition using Optical Emission Spectroscopy (OES). An efficient way to derive an accurate composition is to iterate the computation of the emission spectrum with respect to the best fit of experimental observations.

MERLIN, a RT-LTE software supporting the LIBS diagnostic:

application to H-isotopes measurements

CORIA, UMR CNRS 6614, Normandie Université, 76801 Saint-Étienne du Rouvray, F RANCE

aurelien.favre@coria.fr

A URÉLIEN FAVRE , Morgan LESAGE, V INCENT MOREL, A RNAUD BULTEL, P ASCAL BOUBERT

H, D & T stoichiometric mixture: isotopic resolution power

W Ai r

At t

= 4 ns

50 µm r 01

NECESSARY TOOL TO ANALYZE LIBS EXPERIMENTS Many upgrades are planned: potential lowering, resonant broadening, Zeeman broadening, non-homogenous media, multi-T support, etc...

MERLIN (MultiE lemental R adiative equi LibrI um emissio N ) has been developped to ensure a computational support OES experiments. This suit is based on Radiative Transfer (RT) Local Thermal Equilibrium (LTE) solving for homogeneous emitting media.

Ionizations and dissociations equations are dynamically generated and solved from elemental mole fractions. Spectral data are online requested to generate the emission spectrum of the mixture.

E x a m p l e o f e q u i l i b r i u m composition of a (0.25 Ar - 0.75 H 2 ) mixture versus temperature.

MERLIN shows a satisfactory agreement with published results

Upper levels population density driven by a Boltzmann statistic then allow a computation of emission spectrum.

= 13.598 X X = 15.759 X

Balmer-α HDT LTE emission spectra for a 1 mm wide emitting plasma with the following broadening parameters :

X Gyre ö = yX

X yG X GG = yX

X Gyre = . X G yX

X Gyre− rX y

= X. X y

G

X yX

• Higher pressure leads to a significant Stark broadening which is n e dependant.

• A competition between apparatus and Stark broadenings rules the resolution power.

• Element A ki ratios verifies equilibrium verifies at low densities.

Stark largely dominating

DECONVOLUTION

requiered to dissociate each isotope emission

( − ) ≈ . X yX

X > X(D − T )

X < X(H − D )

rX yX Gyre

>> 

X Gyre

( −  ) ≈ . XX yX

Fine structure emission

H mole fraction in Ar-H 2 mixture

Ar I and Ar II emission

multiplet emission

Temperature in zeolite-like structure H/D mole ratio in bulk W

~X G. GX

~X X. X y

~XGG. X X

~XGX. X

~XXX. X y

~XXX. X

~XXX. X X

~X X. X y

• H 2 dilution leads to significative H emission

• For every non-H lines : 

rX yX Gyre

= G X yr X GyXrXXy

• Since H ionization potential is lower than the one of Ar, diluting leads to greater X values.

• Since the ArH dissociation potention is very weak, dilution does not induce strong n Ar / n Ar+ variations at T and P constant.

• Argon and Hydrogen diagnostic appears to be appart one from the other with dilution.

Ionic lines with T increase H line broadened

with T increase

XGX. X ö

( −  ) ≈ . XX yX X < X(H − D )

= 13.598 X = 15.759 X

• Zeolite = porous structure with high hydrogen retention potential.

COMPOSITION :

0.087H / 0.087Al / 0.217Si / 0.609O

• For every non-H lines : 

rX yX Gyre

= G X yr X GyXrXXy

• Temperature increase heads to ionization degree growth (ionic lines, strong increase in n e and significative n H decrease).

• H and S I lines interfer : direct diagnostic appears to be tricky:

necessity to probe other Balmer lines.

• Light element probing in bulk heavy metallic matrix such as W.

COMPOSITION :

Constant 0.99W / 0.01(H-D) with variable x H-D ratio

• For every non-H lines :

rX yX Gyre

= G X yr X GyXrXXy

• W I 656.32 nm is (ö − ) ≈ . X yX from H which perturbs direct H probing : Al matrix alternative.

• Weak emission due to very low (H-D) charge : necessity to probe in low pressure plasma to reduce Stark as possible.

CONCLUSION & PERSPECTIVES

J. Liu et al. J. Chem. Phys 130 (2009) 174306

A. W. Mizolek et al., Fund. and Appl., Cambridge Univ. Press (2006) R. Fantoni et al., Spectrochimica Acta Part B 129 (2017) 8-13

Z. Mijatovic et al., Spectrochimica Acta Part B 166 (2020) 105821 A. Gigosos et al., Spectrochimica Acta Part B 58 (2003) 1489-1504

REFERENCES

P. Stancil et al. The Astrophysical Journal 430 (1994) 360-370 R. W. Patch et al., J. Chem. Phys 49 (1968) 961

M. A. Maltsev et al., TVT 53 (2019) 367-370

M. Capitelli et al., Springer (2012) ISBN: 978-1-4419-8181-3 P. Fauchais et al., Springer (1994) ISBN: 978-1-4899-1339-5

rX yX Gyre

>

X Gyre

rX yX Gyre

<

X Gyre

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