KMS National Astronomical Observatories, CAS
| Magnetized Particle Motion around Black Holes in Conformal Gravity: Can Magnetic Interaction Mimic Spin of Black Holes? | |
| Haydarov, Kamoliddin1; Abdujabbarov, Ahmadjon1,2,3,4,5; Rayimbaev, Javlon3,5,6; Ahmedov, Bobomurat3,4,5 | |
| 2020-03-01 | |
| Source Publication | UNIVERSE
 |
| Volume | 6Issue:3Pages:20 |
| Abstract | Magnetized particle motion around black holes in conformal gravity immersed in asymptotically uniform magnetic field has been studied. We have also analyzed the behavior of magnetic fields near the horizon of the black hole in conformal gravity and shown that with the increase of conformal parameters L and N the value of angular component of magnetic field at the stellar surface decreases. The maximum value of the effective potential corresponding to circular motion of the magnetized particle increases with the increase of conformal parameters. It is shown that in all cases of neutral, charged and magnetized particle collisions in the black hole environment the center-of-mass energy decreases with the increase of conformal parameters L and N. In the case of the magnetized and negatively charged particle collisions, the innermost collision point with the maximum center-of-mass energy comes closer to the central object due to the effects of the parameters of the conformal gravity. We have applied the results to the real astrophysical scenario when a pulsar treated as a magnetized particle is orbiting the super massive black hole (SMBH) Sgr A* in the center of our galaxy in order to obtain the estimation of magnetized compact object's orbital parameter. The possible detection of pulsar in Sgr A* close environment can provide constraints on black hole parameters. Here we have shown that there is degeneracy between spin of SMBH and ambient magnetic field and consequently the interaction of magnetic field similar to 10(2) Gauss with magnetic moment of magnetized neutron star can in principle mimic spin of Kerr black holes up to 0.6. |
| Keyword | black hole magnetized particle motion magnetic field conformal gravity constraints on black hole parameters |
| Funding Organization | UzbekistanMinistry for Innovative Development ; UzbekistanMinistry for Innovative Development ; Abdus Salam International Centre for Theoretical Physics ; Abdus Salam International Centre for Theoretical Physics ; SU ; SU ; NUUz ; NUUz ; UzbekistanMinistry for Innovative Development ; UzbekistanMinistry for Innovative Development ; Abdus Salam International Centre for Theoretical Physics ; Abdus Salam International Centre for Theoretical Physics ; SU ; SU ; NUUz ; NUUz ; UzbekistanMinistry for Innovative Development ; UzbekistanMinistry for Innovative Development ; Abdus Salam International Centre for Theoretical Physics ; Abdus Salam International Centre for Theoretical Physics ; SU ; SU ; NUUz ; NUUz ; UzbekistanMinistry for Innovative Development ; UzbekistanMinistry for Innovative Development ; Abdus Salam International Centre for Theoretical Physics ; Abdus Salam International Centre for Theoretical Physics ; SU ; SU ; NUUz ; NUUz |
| DOI | 10.3390/universe6030044 |
| WOS Keyword | ENERGY-EXTRACTION PROCESSES ; ORBITS ; FIELD |
| Language | 英语 |
| Funding Project | UzbekistanMinistry for Innovative Development[VA-FA-F-2-008] ; UzbekistanMinistry for Innovative Development[MRB-AN-2019-29] ; UzbekistanMinistry for Innovative Development[YFA-Ftech-2018-8] ; Abdus Salam International Centre for Theoretical Physics[OEA-NT-01] ; SU ; NUUz |
| Funding Organization | UzbekistanMinistry for Innovative Development ; UzbekistanMinistry for Innovative Development ; Abdus Salam International Centre for Theoretical Physics ; Abdus Salam International Centre for Theoretical Physics ; SU ; SU ; NUUz ; NUUz ; UzbekistanMinistry for Innovative Development ; UzbekistanMinistry for Innovative Development ; Abdus Salam International Centre for Theoretical Physics ; Abdus Salam International Centre for Theoretical Physics ; SU ; SU ; NUUz ; NUUz ; UzbekistanMinistry for Innovative Development ; UzbekistanMinistry for Innovative Development ; Abdus Salam International Centre for Theoretical Physics ; Abdus Salam International Centre for Theoretical Physics ; SU ; SU ; NUUz ; NUUz ; UzbekistanMinistry for Innovative Development ; UzbekistanMinistry for Innovative Development ; Abdus Salam International Centre for Theoretical Physics ; Abdus Salam International Centre for Theoretical Physics ; SU ; SU ; NUUz ; NUUz |
| WOS Research Area | Astronomy & Astrophysics ; Physics |
| WOS Subject | Astronomy & Astrophysics ; Physics, Particles & Fields |
| WOS ID | WOS:000524323700008 |
| Publisher | MDPI |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.bao.ac.cn/handle/114a11/56089 |
| Collection | 中国科学院国家天文台 |
| Corresponding Author | Ahmedov, Bobomurat |
| Affiliation | 1.Tashkent Univ Informat Technol, Dept Phys, Amir Temur 108, Tashkent 100014, Uzbekistan 2.Shanghai Astron Observ, 80 Nandan Rd, Shanghai 200030, Peoples R China 3.Ulugh Beg Astron Inst, Astron Skaya 33, Tashkent 100052, Uzbekistan 4.Tashkent Inst Irrigat & Agr Mechanizat Engineers, Dept Phys & Chem, Kori Niyoziy 39, Tashkent 100000, Uzbekistan 5.Natl Univ Uzbekistan, Phys Fac, Univ 4, Tashkent 100174, Uzbekistan 6.Inst Nucl Phys, Lab Theoret Nucl Phys, Ulugbek 1, Tashkent 100214, Uzbekistan |
| Recommended Citation GB/T 7714 | Haydarov, Kamoliddin,Abdujabbarov, Ahmadjon,Rayimbaev, Javlon,et al. Magnetized Particle Motion around Black Holes in Conformal Gravity: Can Magnetic Interaction Mimic Spin of Black Holes?[J]. UNIVERSE,2020,6(3):20. |
| APA | Haydarov, Kamoliddin,Abdujabbarov, Ahmadjon,Rayimbaev, Javlon,&Ahmedov, Bobomurat.(2020).Magnetized Particle Motion around Black Holes in Conformal Gravity: Can Magnetic Interaction Mimic Spin of Black Holes?.UNIVERSE,6(3),20. |
| MLA | Haydarov, Kamoliddin,et al."Magnetized Particle Motion around Black Holes in Conformal Gravity: Can Magnetic Interaction Mimic Spin of Black Holes?".UNIVERSE 6.3(2020):20. |
| Files in This Item: | There are no files associated with this item. | |||||
Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.
Edit Comment