Published August 17, 2020 | Version v1
Journal article Open

Relative material parameters αE, αH, ϑG, ϑF, ξE, ξF, βH, βG, ζE, ζG, λH, and λF for magnetoelectroelastics to model acoustic wave propagation incorporating gravitational phenomena

  • 1. International Institute of Zakharenko Waves (IIZWs)

Description

Regarding solid materials of symmetry class 6 mm, it is natural to deal with mechanical, electrical, magnetic, gravitational, and cogravitational properties. In addition to the electromagnetic α and gravitocogravitic ϑ constants, the incorporation of gravitational phenomena for these smart magnetoelectroelastics adds the gravitoelectric ζ, cogravitoelectric ξ, gravitomagnetic β, and cogravitomagnetic λ constants. All of them contribute to the value of the coefficient of the electromagnetogravitocogravitomechanical coupling (CEMGCMC). The CEMGCMC represents one of very important material characteristics because the dynamic characteristics such as the bulk and surface acoustic wave speeds depend on it. Therefore, it requires experimental determinations of the α, ϑ, ζ, ξ, β, and λ. In addition to the well-known relative parameters αE and αH, this report introduces the relative material parameters ϑG, ϑF, ξE, ξF, βH, βG, ζE, ζG, λH, and λF, where the subscripts “E”, “H”, “G”, “F” relate to the electrical, magnetic, gravitational, and cogravitational subsystems, respectively. It is expected that their measurements can be preferable due to the successful measurements of αE and αM during the last six decades. The knowledge of the complete set of the material parameters for different magnetoelectroelastics can provide a class of commercially fitting materials to constitute various technical devices with suitable characteristics. This can actually contribute to the development of infrastructure for signal processing based on the new fast waves that can propagate in the solids at the speeds Λ1 = (ζλ)–1/2 → ~ 1013CL and Λ2 = (ξβ)–1/2 → ~ 1013CL, where CL is the light speed in a vacuum. Also, the new fast waves can propagate in a vacuum at the speeds Λ01 = (ζ0λ0)–1/2 → ~ 1013CL and Λ02 = (ξ0β0)–1/2 → ~ 1013CL. These speeds Λ01 and Λ02 are already apt for development of the instant interplanetary communication.

Files

HJ43(2)171_186(2020)_aaz.pdf

Files (11.3 MB)

Name Size Download all
md5:dd20a0717eef811b0018ae4d31eed07c
11.3 MB Preview Download