Abstract
Context and results
The study examines the physical characteristics of Co2ZrZ compounds using the Wien2k code and the Anisimov and Gunnarsson approach. Results show metallic attributes in Co2ZrBi and Co2ZrAs, while Co2ZrPb exhibits semi-metallic tendencies. Energy gap evaluations reveal significant infrared transitions, indicating altered electron mobility compensated by increased ultraviolet absorption. These compounds have potential in space solar energy applications due to UV light absorption capabilities, especially in Co2ZrPb. The study also identifies optical phenomena like “super-luminescence” and plasmatic oscillations.
Computational and theoretical techniques
The study uses computational techniques like Wien2k calculation code and Hubbard parameter calculations to investigate Co2ZrPb, a compound with potential for space energy applications. Energy gap assessments are conducted using GGA and mBJ-GGA methods. The study also analyzes the optical behavior of the compounds, including infrared and ultraviolet absorption. The BoltzTraP code is used for thermoelectric investigations, revealing a P-type charge carrier predominance in Co2ZrPb. This comprehensive approach provides valuable insights into electrical conductivity and thermoelectric properties.
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Acknowledgements
The authors would like to express their deepest gratitude to the Deanship of Scientific Research and to the College of Engineering at the University of Hail for providing necessary support to conducting this research.
Funding
The research reported herein was funded by the Deanship of Scientific Research at the University of Hail, Saudi Arabia, through the project number RG-21 084.
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M.H and B.B write the manuscript; S.M and B.A and T.L do the calculation; S.H and A.K and A.A draw the figures;M.M and A.B and S.B chech the formating of the Manuscript
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Houari, M., Mesbah, S., Lantri, T. et al. Investigating the physical and optoelectronic characteristics of Co2ZrZ compounds: findings from computational analysis and thermoelectric evaluation. J Mol Model 30, 110 (2024). https://doi.org/10.1007/s00894-024-05903-6
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DOI: https://doi.org/10.1007/s00894-024-05903-6