Here, we explore the dynamics of particle near the horizon of charged Mandal-Sengupta-Wadia (MSW) black hole in 2+1 dimensions. It results analysis of angular momentum and potential energy for null and time-like geodesics. We also appraise the high center-of-mass energy of coming particles from rest at infinity near the horizon of the charged MSW black hole in 2+1 dimension for the extremal case. Finally, we study the ISCO and MBCO radii for this type of black hole.
Introduction:Recently, "Two particle collision at the neighborhood of horizons of the black hole" becomes fascinated window in Astrophysics. This method, known as BSW effect, has been firstly achieved by Banados, Silk and West [1] in 2009 for the Kerr black hole to get large center-of-mass (CM) energy if one of particles has critical angular momentum. To get this process, the black hole should be extremal. The CM energy for non-extremal black hole has been demonstrated by Jacobson and Sotiriou [2] where they have pointed out the drawback of this process. So, there must exist astrophysical limitations for extremal Kerr black hole. Lake [3] has found divergent CM energy at inner horizon for rotating Kerr black hole. Liu et al. [4] have studied BSW effect of the Kerr-Taub-NUT space-time for extremal case. Grib and Pavlov [5] have established disbursement of acceleration of the particles to produce high amount of CM energy for a rotating black hole in the case of extremal and non extremal both. Kerr-de Sitter black hole for non extremal case [6] acts as a particle accelerator with unbounded CM energy for two particle collisions. Wei et al. [7] have studied the same thing for the Sen black hole. For non rotating black hole, Zaslavskill [8] has studied particle acceleration. Extension of the BSW effect on particle acceleration on various type of black holes such as charged, non charged, rotating and non rotating black holes have been investigated in [9][10][11][12].Some attractions have been occurred on a new type of black hole, named as Regular black hole with non-singular curvature. Bardeen [13] has introduced First Regular black hole. Then slowly many authors have worked on this type of various black holes in [14][15][16]. Next Amir and Ghosh [17] have studied the rotating Hayward black hole as particle accelerator. Harada [18] has given an excellent review work on particle collision. Several authors have discussed particle collision in [19][20][21]. Now, the lower dimensional setting becomes more sharper than 3+1 dimensional case to get conceptual focus. To solve Einstein gravity equations, 2+1 dimensional black hole is exact solution than 3+1 dimensional black hole. Both 2+ 1 black hole and 3+ 1 black hole contribute same physical *