Abstract
The motion of a magnetized particle orbiting around non-Schwarzschild black hole immersed in an external uniform magnetic field is considered. The influence of deformation parameter \(h\) to effective potential of the radial motion of the magnetized particle around non-Schwarzschild black hole using Hamilton-Jacobi formalism is studied. We have obtained numerical values of area \(\Delta \rho \) where magnetized particles can move which is expanding (narrowing) due to the effect of the negative (positive) deformation. Finally, we have studied the collision of two particles (magnetized-neutral, magnetized-magnetized, magnetized-charged) in non-Schwarzschild spacetime and got the center-of-mass energy \((E_{c.m})\) for the particles. Moreover, we have found the capture radius (\(r_{cap}\)) – the distance from the central object to the point where particles collide and fall down to the central compact object. It is shown that non-Schwarzschild black holes could also act as particle accelerators with arbitrarily high center-of-mass energy.
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Acknowledgements
Author thanks Polat Tadjimuratov, Ahmadjon Abdujabbarov and Bobomurat Ahmedov for useful discussions and Atamuratov Farruh for assistance in making numerical calculations and graphs. Author is grateful to the IUCAA for the warm hospitality during his stay in Pune, India. This research is supported in part by Projects No. F2-FAF113, No. EF2-FA-0-12477, and No. F2-FA-F029 of the UzAS and by the ICTP through the OEA-PRJ-29 and the OEA-NET-76 projects and by the Volkswagen Stiftung (Grant No. 86 866).
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Rayimbaev, J.R. Magnetized particle motion around non-Schwarzschild black hole immersed in an external uniform magnetic field. Astrophys Space Sci 361, 288 (2016). https://doi.org/10.1007/s10509-016-2879-9
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DOI: https://doi.org/10.1007/s10509-016-2879-9