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The Photogravitational Elliptical Restricted Three Body Problem models the intricate motion of a small body under the combined influence of gravitational forces and solar radiation pressure from two larger, orbiting primary bodies, specifically considering their elliptical trajectories. This complex astrophysical scenario is vital for understanding spacecraft dynamics, solar sail missions, and orbital stability in systems where light pressure significantly impacts movement, offering critical insights into mission planning and celestial mechanics.

Explore the impact of pressure on the molecular dynamics of glassforming systems. This study investigates how varying pressure conditions influence the structural and dynamic properties of glass materials at a molecular level, providing insights into their behavior and potential applications in various fields. The research focuses on understanding the relationship between pressure, molecular mobility, and the glass transition phenomenon within these complex systems.