In the manuscript, we study the efficiency of pair creation by means of the centrifugal mechanism. The strong magnetic field and the effects of rotation, which always take place in Kerr-type black holes, guarantee the frozen-in condition, leading to the generation of an exponentially amplifying electrostatic field. This field, when reaching the Schwinger threshold, leads to efficient pair production. The process has been studied for a wide range of AGN luminosities and black hole masses, and it was found that the mechanism is very efficient, indicating that for AGNs where centrifugal effects are significant, the annihilation lines in the MeV range will be very strong.Comment: 15 pages, 5 figure
According to the Banados-Silk-West (BSW) process, rotating black holes can act as particle colliders...
Recent advances in general relativistic magnetohydrodynamic modeling of jets offer unprecedented ins...
We study a rotating black hole with anisotropic matter and electromagnetic fields. We show that the ...
In this paper we study the possibility of efficient pair production in a pulsar’s magnetosphere. It ...
Magnetic reconnection is ubiquitous in astrophysical systems, and in many such systems, the plasma s...
It has been recently shown that magnetic reconnection can provide us a novel mechanism to extract bl...
We present general relativistic magneto-hydrodynamical simulations of equal-mass spinning black hole...
We describe global, 3D, time‐dependent, non‐radiative, general‐relativistic, magnetohydrodynamic sim...
In this paper, we study the magnetic reconnection process of energy extraction from a rapidly rotati...
By solving the quantum field theoretical version of the Klein-Gordon equation numerically, we study ...
In this paper, we investigate the pair creation of charged and rotating black hole pairs in a backgr...
Large-scale magnetic fields in the nuclear regions of protogalaxies can promote the formation and ea...
We compute pair production rate of charged black holes in de Sitter space in four dimensional Einste...
The production of electron-positron pairs by single photons in magnetic fields 10 to the twelth pow...
We explore the hypothesis that the abundant presence of relativistic antimatter (positrons) in the p...
According to the Banados-Silk-West (BSW) process, rotating black holes can act as particle colliders...
Recent advances in general relativistic magnetohydrodynamic modeling of jets offer unprecedented ins...
We study a rotating black hole with anisotropic matter and electromagnetic fields. We show that the ...
In this paper we study the possibility of efficient pair production in a pulsar’s magnetosphere. It ...
Magnetic reconnection is ubiquitous in astrophysical systems, and in many such systems, the plasma s...
It has been recently shown that magnetic reconnection can provide us a novel mechanism to extract bl...
We present general relativistic magneto-hydrodynamical simulations of equal-mass spinning black hole...
We describe global, 3D, time‐dependent, non‐radiative, general‐relativistic, magnetohydrodynamic sim...
In this paper, we study the magnetic reconnection process of energy extraction from a rapidly rotati...
By solving the quantum field theoretical version of the Klein-Gordon equation numerically, we study ...
In this paper, we investigate the pair creation of charged and rotating black hole pairs in a backgr...
Large-scale magnetic fields in the nuclear regions of protogalaxies can promote the formation and ea...
We compute pair production rate of charged black holes in de Sitter space in four dimensional Einste...
The production of electron-positron pairs by single photons in magnetic fields 10 to the twelth pow...
We explore the hypothesis that the abundant presence of relativistic antimatter (positrons) in the p...
According to the Banados-Silk-West (BSW) process, rotating black holes can act as particle colliders...
Recent advances in general relativistic magnetohydrodynamic modeling of jets offer unprecedented ins...
We study a rotating black hole with anisotropic matter and electromagnetic fields. We show that the ...