Open AccessNon-Radial Pulsations of Distorted Stellar Structures: Effect of Mass Variation
Author(s) -
Seema Saini,
Sunil Kumar,
Vineet Bhatt,
Pradeep Bedi
Publication year - 2021
Publication title -
international journal of mathematical, engineering and management sciences
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.228
H-Index - 10
ISSN - 2455-7749
DOI - 10.33889/ijmems.2021.6.5.084
Subject(s) - equipotential , physics , radial velocity , variation (astronomy) , astrophysics , reflection (computer programming) , equipotential surface , star (game theory) , stars , quantum mechanics , computer science , programming language
Eigen-frequencies (EF) of non–radial modes (NRM) of pulsations of differentially rotating (D R) and tidally distorted (T D) stellar models by considering the effect of mass variation (MV) on its equi-potentials surfaces inside a star. The method utilizes an averaging proposal of Kippenhahn and Thomas (K and T) with conjunction of the concept of Roche-equipotential. The study accolades and corrects earlier studies of non-radial (NR) pulsations of DR and TD stellar structures of different natures such as radial and non-radial oscillations, X-ray, gamma ray and other electromagnetic disturbances. The reflection of the work comes from the requirements of the inclusion of non-uniform densities that yield Lane-Emden equation to have reliable results up to second order disturbances.