Dynamics of particles around a Schwarzschild-like black hole in the presence of quintessence and magnetic field

The European Physical Journal C

Saqib Hussain¹  Bushra Majeed¹  Mubasher Jamil¹ 

[1] School of Natural Sciences (SNS), National University of Sciences and Technology (NUST), H-12, Islamabad, Pakistan;

关键词: Magnetic Field;    Black Hole;    Angular Momentum;    Dark Energy;    Lyapunov Exponent;   

DOI  :  10.1140/epjc/s10052-014-3230-7

来源: Springer

【 摘 要 】

We have investigated the dynamics of a neutral and a charged particle around a static and spherically symmetric black hole in the presence of quintessence matter and external magnetic field. We explore the conditions under which the particle moving around the black hole could escape to infinity after colliding with another particle. The innermost stable circular orbit (ISCO) for the particles are studied in detail. Mainly the dependence of ISCO on dark energy and on the presence of external magnetic field in the vicinity of black hole is discussed. By using the Lyapunov exponent, we compare the stabilities of the orbits of the particles in the presence and absence of dark energy and magnetic field. The expressions for the center of mass energies of the colliding particles near the horizon of the black hole are derived. The effective force on the particle due to dark energy and magnetic field in the vicinity of black hole is also discussed.

【 授权许可】

CC BY