“…These last two components constitute the so-called Poynting-Robertson (P-R) effect, which causes small particles of the solar system to spiral into the sun at a cosmically rapid rate. Knowing the importance of the P-R drag effect, many researchers like Stanley (1950), Chernikov (1970), Ragos and Zafiropoulos (1995), Lhotka and Celletti (2015), Singh and Amuda (2017), Pal and Kushvah (2015), Vincent and Perdiou (2021a, b), Vincent and Kalantonis (2023), Taura and Leke (2022), Tyokyaa and Atsue (2020), Vincent and Singh (2022) among others, devoted their work to study this problem with various characterizations. All these works have arrived at the conclusion that the P-R effect renders unstable those equilibrium points, which are conditionally stable in the classical case.…”