Abstract
In this study, we discuss the central force problem by using the nonlocal-in-time kinetic energy approach. At low length scales, the system is dominated by the generalized 4th-order extended Fisher-Kolmogorov stationary equation and by the 4th-order stationary Swift-Hohenberg differential equation under explicit conditions. The energy is a conserved quantity along orbits of the extended Fisher-Kolmogorov stationary equation. The system is quantized, the system is stable, and the ground energy problem is solved.
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11 February 2022
A Correction to this paper has been published: https://doi.org/10.1007/s42064-022-0136-2
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I would like to thank the group of anonymous referees for their useful comments and valuable suggestions.
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Rami Ahmad El-Nabulsi holds a Ph.D. degree in particle physics, mathematical physics and modeling from Provence University, France, and a diploma of advanced studies in plasma physics and radiation astrophysics from the same institution. He worked with different worldwide research departments in UK, Republic of Korea, China, Greece and he is actually affiliated to ATINER-Athens, Mathematics and Physics Departments. He is the author of more than 190 peer-reviewed papers in peer-refereed journals and a reviewer for more than 65 scientific journals where he has reviewed more than 750 manuscripts till the present moment. His research ranges from applied mathematics to theoretical physics including nonlinear dynamical systems, space physics, celestial dynamics, high-energy astrophysics and cosmology, geophysical flows, physics and chemistry of solids, magnetic materials, quantum mechanics, and physics at nanoscales among others.
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El-Nabulsi, R.A. Orbital dynamics satisfying the 4th-order stationary extended Fisher-Kolmogorov equation. Astrodyn 4, 31–39 (2020). https://doi.org/10.1007/s42064-019-0058-9
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DOI: https://doi.org/10.1007/s42064-019-0058-9