English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

The multi-dissipative photogravitational triaxial elliptic restricted threebody problem is treated. The perturbed locations of triangular points arecomputed. The stability of the triangular points under changing one or moreperturbing parameter is investigated. The results revealed that at certainvalues of the considered perturbing parameters, we haven't triangularequilibrium points, or at least there exists but very far from the origin. Thechange in the stability/instability regions with eccentricity seems to benonlinear. It seems that increasing the eccentricity the enlarge the stabilityregions and vice versa. It is revealed that we have two disjoint stabilityregions. The stability/instability regions for a new set of eccentricities aremerged to one region. Consider a very high eccentricity stability region forthe whole domain of the mass ratio except in the neighborhood of 0.3 isobtained. stability/asymptotic stability/instability regions due to certainphotogravitational effects correspond are revealed.

Perturbed locations and stability of the Triangular equilibrium points in the multi-dissipative photogravitational triaxial elliptic RTBP