Moore–Gibson–Thompson model for thermal and rotational dynamics in microelongated semiconductor solids with gravitational field
Source abstract
Abstract
The propagation of plane harmonic waves in a semiconductor photothermal thermoelastic half-space is studied using the Moore–Gipson–Thompson heat conduction model. The medium is characterized by a microelongational structure and is influenced by rotation and gravity. A harmonic wave solution is utilized to derive the qualifier functions of the medium. The results are analyzed and illustrated for various rotation and gravity values. It is observed that both factors significantly affect the plasma effect and other field functions positively. Silicon is selected for the numerical scheme due to its relevance in manufacturing applications. The development of technologies in semiconducting media is widely used in modern engineering, such as smart materials and manufacturing processes.
Source: crossref · Quality: baseline
Research context
OpenAlex topics: Thermoelastic and Magnetoelastic Phenomena · Nonlocal and gradient elasticity in micro/nano structures · Thermal Radiation and Cooling Technologies
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Department of Basic Science, Faculty of Engineering, Sinai University 1 , Al-Arish,
Department of Mathematics, Faculty of Science, Zagazig University 2 , P.O. Box 44519, Zagazig,
Department of Basic Sciences, Common First Year, King Saud University 3 , Riyadh 11451,
Department of Mathematics, College of Science, King Saud University 4 , P.O. Box 2455, Riyadh 11451,
Department of Mathematics, Chandigarh University 5 , Gharuan, Punjab,
Funding
King Saud University
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