Electromagnetic counterpart to gravitational waves from coalescence of binary black hole with magnetic monopole charge

Author:

Win Aung Naing1,Chu Yu-Ming23,Shah Hasrat Hussain4ORCID,Abbas Syed Zaheer15,Shah Munawar6

Affiliation:

1. School of Mathematics and Statistics, Beijing Institute of Technology, Beijing, 100081, P. R. China

2. Department of Mathematics, Huzhou University, Huzhou 313000, P. R. China

3. Hunan Provincial Key Laboratory of Mathematical Modelling and Analysis in Engineering, Changsha University of Science & Technology, Changsha 410114, P. R. China

4. Department of Mathematical Sciences, Baluchistan University of Information Technology, Engineering and Management Sciences, Quetta 87300, Pakistan

5. Department of Mathematics and Statistics, Hazara University Mansehra, KPK, Pakistan

6. Department of GNSS, Institute of Space Technology, Islamabad, Pakistan

Abstract

A Satellite Fermi GBM detected recent putative short Gamma Ray Bursts (GRBs) in coincident with the gravitational wave signal GW 150914 produced by the merger of binary black hole (BH). If at least one BH possess magnetic monopole charge in the binary BH system then the short-duration GRBs may produce during the final phase of a binary BH merger. The detection of gravitational waves GW 150914, GW 151226 and LVT 151012 by LIGO gave the evidence that merging of the compact object like binary BH often happens in our universe. In this paper, we report the qualitative model to discuss the generation of electromagnetic radiation from the merging of two BHs with equal masses and at least one BH carrying the magnetic monopole charge in the binary system. In this model, BH possess a magnetic monopole charge that may not be neutralized before the coalescence. During the inspiralling process, the magnetic monopole charge on the BH would produced the electric dipole moment. Short duration GRB would produce by the rapidly evolution of the electric dipole moment which may detectable on Earth. We predict that this model would be beneficial in the future to explain the generation of gravitational wave (GW) plus a electromagnetic signal of multi-wavelength from mergers of magnetically charged BHs.

Funder

China National Funds for Distinguished Young Scientists

Publisher

World Scientific Pub Co Pte Lt

Subject

Astronomy and Astrophysics,Nuclear and High Energy Physics,Atomic and Molecular Physics, and Optics

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