A perceptive overview of nucleus-acoustic waves in degenerate quantum astroplasmas

We present a theoretic model formalism perspectively developed to explore the stability behavioral dynamics of the nucleus-acoustic waves (NAWs) in diversified gyrogravitating degenerate quantum astroplasmas. It evolves under the joint influence of the Bohm potential, Coriolis rotation, electrostatic confinement pressure (ECP), viscoelasticity, etc. Application of a standard normal spherical mode analysis yields a generalized linear septic dispersion law. It is interestingly found that the Coriolis rotation enhancement suppresses the NAW growth features. The adopted system is more sensitive to the rotational force than the viscoelasticity, and so forth. It is useful to study the NAWs and stability features excitable in compact astrophysical objects, like white dwarfs (WDs), brown dwarfs, neutron stars, etc.

Automated summary

In this study, a theoretical model is presented to explore the stability dynamics of nucleus-acoustic waves in gyrogravitating degenerate quantum astroplasmas. The analysis reveals that the enhancement of Coriolis rotation suppresses the growth features of the nucleus-acoustic waves, and the system is more sensitive to rotational forces than viscoelasticity.