Theoretical and Natural Science

- The Open Access Proceedings Series for Conferences


Theoretical and Natural Science

Vol. 13, 30 November 2023


Open Access | Article

Exploring black hole-neutron star binary merger by detecting gravitational waves

Jiahao Zhang * 1
1 ACS International Singapore City

* Author to whom correspondence should be addressed.

Theoretical and Natural Science, Vol. 13, 59-64
Published 30 November 2023. © 2023 The Author(s). Published by EWA Publishing
This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
Citation Jiahao Zhang. Exploring black hole-neutron star binary merger by detecting gravitational waves. TNS (2023) Vol. 13: 59-64. DOI: 10.54254/2753-8818/13/20240790.

Abstract

Unlike black hole binary merger, the merger between a neutron star and a black hole will produce an abundant number of gravitational waves and electromagnetic waves. Using this information, scientists can easily find many properties of the universe and test the general relativity and some other gravitational theories. The detection of the gravitational wave from source is essential to develop the current knowledge of the gravitational force. From last century, scientists were trying to detect the gravitational waves, and as the time passes, the method of detection has already developed from on land detector to space detector in order to take more precise readings. This paper provides some basic information of the neutron star and the black hole, together with the formation of the binary neutron star-black hole system. The relationship between the neutron star and black hole is explained in this paper. The knowledge of the current methods of detecting gravitational waves is also provided and the paper specifically elaborated the space laser interferometry.

Keywords

Gravitational Wave, Black Hole, Neutron Star, Space Laser Interferometry

References

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3. Sedda, Manuel Arca. (2020). Dissecting the Properties of Neutron Star–black Hole Mergers Originating in Dense Star Clusters. Communications Physics, 3, 43.

4. Lu, Youjun, & Guo, Xiao. (2022). The first detection of neutron star-black hole binary mergers. Science China Press, 67(22): 2610-2615

5. Zhou, Enping, (2019). Numerical relativity and binary neutron star merges. Physics, 48(9): 573-580.

6. Xu, Renxin. (2018). The ideal tool to measure the expansion of the universe-neutron star-black hole binary merger. Physics, 47(9), 591

7. Vincentelli, F. M., Neilsen, J., Tetarenko, A.J. et al. (2023). A shared accretion instability for black holes and neutron stars. Nature, 615, 45–49.

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Data Availability

The datasets used and/or analyzed during the current study will be available from the authors upon reasonable request.

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Volume Title
Proceedings of the 3rd International Conference on Computing Innovation and Applied Physics
ISBN (Print)
978-1-83558-189-6
ISBN (Online)
978-1-83558-190-2
Published Date
30 November 2023
Series
Theoretical and Natural Science
ISSN (Print)
2753-8818
ISSN (Online)
2753-8826
DOI
10.54254/2753-8818/13/20240790
Copyright
30 November 2023
Open Access
This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited

Copyright © 2023 EWA Publishing. Unless Otherwise Stated