Magnetic traversable wormhole as accelerator of charged particles

2020 ◽  
Vol 35 (02n03) ◽  
pp. 2040026
Author(s):  
A. A. Kirillov ◽  
E. P. Savelova

We show that the scattering of radiation on a traversable wormhole forms a vortex in the radiation energy flux. Then, if the wormhole possesses also a magnetic fields, the vortex accelerates charged particles along the magnetic lines and such a system works as an accelerator. If the vortex is small, the system reaches the stationary state, when the income of the kinetic energy reradiates completely in the form of the synchrotron radiation. Such a mechanism allows us to relate a part of observed sources of the synchrotron radiation to magnetic wormholes.

2010 ◽  
Vol 19 (9) ◽  
pp. 090402
Author(s):  
Meng Qing-Miao ◽  
Jiang Ji-Jian ◽  
Li Zhong-Rang ◽  
Wang Shuai

2016 ◽  
Vol 52 (3-4) ◽  
pp. 212-216 ◽  
Author(s):  
E. M. Abutalipova ◽  
D. E. Bugai ◽  
A. N. Avrenyuk ◽  
O. B. Strel’tsov ◽  
I. R. Sungatullin

2010 ◽  
Vol 49 (8) ◽  
pp. 1739-1745 ◽  
Author(s):  
Qing-Miao Meng ◽  
Ji-Jian Jiang ◽  
Jing-Lun Liu ◽  
Zhong-Rang Li

2016 ◽  
Vol 31 (03) ◽  
pp. 1650008
Author(s):  
Tangmei He ◽  
Jingyi Zhang ◽  
Jinbo Yang ◽  
Hongwei Tan

In this paper, the lifespan under the generalized uncertainty principle (GUP) of rotating black hole is derived through the corrected radiation energy flux and the first law of the thermodynamics of black hole. The radiation energy flux indicates that there exist the highest temperature and the minimum mass both of which are relevant to the initial mass of the black hole in the final stage of the radiation. The lifespan of rotating black hole includes three terms: the dominant term is just the lifespan in the flat spacetime; the other two terms are individually induced by the rotation and the GUP.


2011 ◽  
Vol 20 (supp02) ◽  
pp. 50-56
Author(s):  
◽  
PETER SCHIFFER

The Pierre Auger Observatory is the world's largest experiment for the measurement of ultra-high energy cosmic rays (UHECRs). These UHECRs are assumed to be to be charged particles, and thus are deflected in cosmic magnetic fields. Recent results of the Pierre Auger Observatory addressing the complex of energy ordering of the UHECRs arrival directions are reviewed in this contribution. So far no significant energy ordering has been observed.


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