Abstract
Polarization of phonons in a magnetic field has been analyzed in terms of the isotropic model. It has been demonstrated that, in the presence of spin-phonon interaction, phonons possess circular polarization, which is responsible for the appearance of the heat flux component perpendicular to the temperature gradient and the magnetic field.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
