Gravitational Wave Detection and Its Applications in Multi-Messenger Astronomy

Haoyu Wang

doi:10.54097/z2jex339

Authors

Haoyu Wang

DOI:

https://doi.org/10.54097/z2jex339

Keywords:

Gravitational Waves, Interferometers, Binary Black Hole, Binary Neutron Star.

Abstract

It ushered in a new era of astronomy with the direct detection of gravitational waves in 2015. A whole new way of stepping into the dark, scary world that Einstein predicted. This paper reviews the theoretical background of gravitational waves and provides an overview of four main categories of primary astrophysical sources, with a particular emphasis on the transient chirp signal. Explanations of principles of detection through laser interferometry, both for those on the ground, LIGO/Virgo, and proposed plans for a space-based version known as the Laser Interferometer Space Antenna (LISA). The gist of this paper is that the first binary black holes, GW150914 in 2015, and the first binary neutron star, GW170817 in 2017, were found. Verifying that the primary origin of heavy elements like gold as well as platinum was the connection between GW and its equivalent EM wave. This was the beginning of multi-messenger astronomy. A brief explanation of astronomical statistics is also provided.

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References

[1] Einstein, A. Näherungsweise integration der feldgleichungen der gravitation. Sitzungsberichte der Königlich Preußischen Akademie der Wissenschaften, 1916, 688-696.

[2] Hulse, R. A., & Taylor, J. H. Discovery of a pulsar in a binary system. Astrophysical Journal, 1975, 195: L51-L53.

[3] Abbott, B. P., Abbott, R., Abbott, T. D., Abernathy, M. R., Acernese, F., Ackley, K., ... & Cavalieri, R. Observation of gravitational waves from a binary black hole merger. Physical Review Letters, 2016, 116(6): 061102.

[4] Abbott, B. P., Abbott, R., Abbott, T. D., Acernese, F., Ackley, K., Adams, C., ... & Cahillane, C. GW170817: observation of gravitational waves from a binary neutron star inspiral. Physical Review Letters, 2017, 119(16): 161101.

[5] Flanagan, E. E., & Hughes, S. A. The basics of gravitational wave theory. New Journal of Physics, 2005, 7(1): 204.

[6] Pitkin, M., Reid, S., Rowan, S., & Hough, J. Gravitational wave detection by interferometry (ground and space). Living Reviews in Relativity, 2011, 14(1): 5.

[7] Miller, M. C., & Yunes, N. The new frontier of gravitational waves. Nature, 2019, 568(7753): 469-476.

[8] Acernese, F., Agathos, M., Agatsuma, K., Aisa, D., Allemandou, N., Allocca, A., ... & Meidam, J. Advanced Virgo: a second-generation interferometric gravitational wave detector. Classical and Quantum Gravity, 2014, 32(2): 024001.

[9] Amaro-Seoane, P., Audley, H., Babak, S., Baker, J., Barausse, E., Bender, P., ... & Zweifel, P. Laser Interferometer Space Antenna. arXiv preprint, 2017, arXiv:1702.00786.

[10] Abbott, B. P., Abbott, R., & Abbott, T. D. Tests of General Relativity with GW150914. Physical Review Letters, 2016, 31 May: 2016.

[11] Goldstein, A., Veres, P., Burns, E., Briggs, M. S., Hamburg, R., Kocevski, D., ... & Stanbro, M. An ordinary short gamma-ray burst with extraordinary implications: Fermi-GBM detection of GRB 170817A. The Astrophysical Journal Letters, 2017, 848(2): L14.

[12] Cowan, J. J., Sneden, C., Lawler, J. E., Aprahamian, A., Wiescher, M., Langanke, K., ... & Thielemann, F. K. Origin of the heaviest elements: The rapid neutron-capture process. Reviews of Modern Physics, 2021, 93(1): 015002.

[13] Pian, E., D’Avanzo, P., Benetti, S., Branchesi, M., Brocato, E., Campana, S., ... & Vergani, D. Spectroscopic identification of r-process nucleosynthesis in a double neutron-star merger. Nature, 2017, 551(7678): 67-70.

[14] Bailes, M., Berger, B. K., Brady, P. R., Branchesi, M., Danzmann, K., Evans, M., ... & Vitale, S. Gravitational-wave physics and astronomy in the 2020s and 2030s. Nature Reviews Physics, 2021, 3(5): 344-366.

[15] Abbott, R., Abe, H., Acernese, F., Ackley, K., Adhikari, N., Adhikari, R. X., ... & Boër, M. Tests of general relativity with GWTC-3. arXiv preprint, 2021, arXiv:2112.06861.