On the physical nature of the source of ultraluminous X-ray pulsations

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• 作者：G. Ter-Kazarian
• 关键词：Black hole physics ; Accretion ; accretion discs ; X ; rays ; binaries ; X ; rays ; individual (NuSTAR J095551+6940.8)
• 刊名：Astrophysics and Space Science
• 出版年：2016
• 出版时间：January 2016
• 年：2016
• 卷：361
• 期：1
• 全文大小：1,415 KB
• 参考文献：Alexander, T., Natarajan, P.: Science 345, 1330 (2014) ADS
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• 作者单位：G. Ter-Kazarian (1)
  
  1. Ambartsumian Byurakan Astrophysical Observatory, Byurakan, 378433, Aragatsotn District, Armenia
  
• 刊物类别：Physics and Astronomy
• 刊物主题：Physics
  Astronomy
  
• 出版者：Springer Netherlands
• ISSN：1572-946X

文摘

To reconcile the observed unusual high luminosity of NuSTAR X-ray pulsations from M82X-2 with the most extreme violation of the Eddington limit, and in view that the persistent X-ray radiation from M82X-2 almost precludes the possibility of common pulsars, we tackle the problem by the implications of microscopic theory of black hole (MTBH). The preceding developments of MTBH are proved to be quite fruitful for the physics of ultra-high energy (UHE) cosmic-rays. Namely, replacing a central singularity by the infrastructures inside event horizon, subject to certain rules, MTBH explains the origin of ZeV-neutrinos which are of vital interest for the source of UHE-particles. The M82X-2 is assumed to be a spinning intermediate mass black hole resided in final stage of growth. Then, the thermal blackbody X-ray emission, arisen due to the rotational kinetic energy of black hole, escapes from event horizon through the vista to outside world, which is detected as ultraluminous X-ray pulsations. The M82X-2 indeed releases \(\sim99.6~\%\) of its pulsed radiative energy predominantly in the X-ray bandpass 0.3鈥?0 keV. We derive a pulse profile and give a quantitative account of energetics and orbital parameters of the semi-detached X-ray binary containing a primary accretor M82X-2 of inferred mass \(M\simeq138.5\mbox{--}226\,M_{\odot}\) and secondary massive, \(M_{2}> 48.3\mbox{--}64.9\,M_{\odot}\), O/B-type donor star with radius of \(R> 22.1\mbox{--} 25.7\,R_{\odot}\), respectively. We compute the torque added to M82X-2 per unit mass of accreted matter which yields the measured spin-up rate. Keywords Black hole physics Accretion: accretion discs X-rays: binaries X-rays: individual (NuSTAR J095551+6940.8)