Abstract

The present study investigates the positions and stability of C70 fullerenes. Numerically, the positions and stability have been computed C70 fullerene at the nanoscale to show the effects of the parameters involved with the help of software MATHEMATICA. The total molecular energy evidenced refers to the total pairwise molecular interactions between two C 70 fullerenes, which is an approximation of a continuous approach. The attractive Vand der Waals forces between only molecules provide the centripetal forces between three fullerenes. The total pairwise molecular interactions between two C 70 fullerenes, which is an approximation of a continuous approach, is termed the total molecular energy evidenced. The attractive Vand der Waals forces between single molecules create the centripetal forces between three fullerenes. We have predicted the collective potential function, mutual force and angular velocity. The stationary points are collinearly lying on the ξ−axis which are symmetric about the η−axis as the molecules of the carbon atoms in the nucleus are evenly distributed. There is at least one complex root with the positive real part for each set of values, it has been discovered. The stationary points are thus unstable in the Lyapunov sense.

Highlights

  • The present study investigates the positions and stability of C70 fullerenes

  • In like manner, when we observe on a large scale the configuration of our solar system and other exoplanets, we discover a high correlation in their dynamic behaviour with occurrences at the nanoscale sub-atomic level

  • The analytical works are calculated based on the positions and stability natures of the research in question

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Summary

Introduction

The present study investigates the positions and stability of C70 fullerenes. Numerically, the positions and stability have been computed C70 fullerene at the nanoscale to show the effects of the parameters involved with the help of software MATHEMATICA. The restricted three-body problem (R3BP) is a problem that has continues to be of great theoretical, practical, historical and educational importance The study of this problem has had important implications in various scientific fields, some of which includes; celestial mechanics chaos theory, galactic dynamics, molecular physics and many others. Suraj et al [4] considered the out-of-plane equilibrium points in the planar Restricted Three-body Problem with heterogeneous oblate primaries and three layers of different densities. They confirmed that the points are unstable for all mass ratios and other parameters. It is well known that nature possesses certain phenomena that establish similarity and order in their co-existence These observed phenomena have direct links to models that are found in science and technology. It implies that the orbital motion is a common phenomenon of dynamics at mega and nanoscale levels

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