Energy extraction and particle acceleration around a rotating black hole in quintessence

被引:30
作者
Oteev, Tursinbay [1 ,2 ]
Abdujabbarov, Ahmadjon [1 ,2 ,3 ,4 ]
Stuchlik, Zdenek [1 ,2 ]
Ahmedov, Bobomurat [3 ,4 ]
机构
[1] Silesian Univ Opava, Fac Philosophy & Sci, Inst Phys, Bezrucovo Namesti 13, Opava 74601, Czech Republic
[2] Silesian Univ Opava, Fac Philosophy & Sci, Res Ctr Theoret Phys & Astrophys, Bezrucovo Namesti 13, Opava 74601, Czech Republic
[3] Ulugh Begh Astron Inst, Astron Skaya 33, Tashkent 100052, Uzbekistan
[4] Natl Univ Uzbekistan, Tashkent 100174, Uzbekistan
关键词
Black hole; Particle acceleration; Energy extraction; Quintessence; THICK DISCS; SITTER; KERR; DYNAMICS; KERR-(ANTI); ORBITS;
D O I
10.1007/s10509-016-2850-9
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study motion and collision of particles in the gravitational field of rotating black hole immersed in quintessential dark energy characterized with the quintessential parameter omega(q) is an element of (-1;-1/3) governing the equation of state of the dark energy, and the dimensionless quintessential field parameter (c) over tilde. We focus on the acceleration of particles due to collisional processes and show how the center of mass energy depends on the quintessential field parameter (c) over tilde. We also make comparison of the obtained results to the collisional energetics of quintessential static black holes demonstrating the crucial role of the rotation parameter a in the particle acceleration. Finally we study the dependence of the maximal value of the efficiency of energy extraction through Penrose process for rotating black hole with quintessential field parameter (c) over tilde. It is found that quintessence field decreases the energy extraction efficiency through Penrose process and when the parameter (c) over tilde vanishes one can get the standard value of the efficiency coefficient for the Kerr black hole as eta similar to 21 %.
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页数:8
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