Multimodal Analysis of Gravitational Wave Signals and Gamma-Ray Bursts from Binary Neutron Star Mergers

被引:5
|
作者
Cuoco, Elena [1 ,2 ,3 ]
Patricelli, Barbara [1 ,3 ]
Iess, Alberto [4 ]
Morawski, Filip [5 ]
机构
[1] European Gravitat Observ EGO, Via E Amaldi 5, I-56021 Cascina, Italy
[2] Scuola Normale Super SNS, Piazza Cavalieri 7, I-56126 Pisa, Italy
[3] INFN, Sez Pisa, Largo Bruno Pontecorvo 3, I-56127 Pisa, Italy
[4] INFN, Sez Roma Tor Vergata, Via Ric Sci 1, I-00133 Rome, Italy
[5] Polish Acad Sci, Nicolaus Copernicus Astron Ctr, Bartycka 18, PL-00716 Warsaw, Poland
关键词
gravitational waves; gamma-ray bursts; neutron stars; multi-messenger astronomy; multimodal analysis; EQUATION-OF-STATE; EXTENDED EMISSION; IDENTIFICATION; COUNTERPART; CONSTRAINTS;
D O I
10.3390/universe7110394
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A major boost in the understanding of the universe was given by the revelation of the first coalescence event of two neutron stars (GW170817) and the observation of the same event across the entire electromagnetic spectrum. With third-generation gravitational wave detectors and the new astronomical facilities, we expect many multi-messenger events of the same type. We anticipate the need to analyse the data provided to us by such events not only to fulfil the requirements of real-time analysis, but also in order to decipher the event in its entirety through the information emitted in the different messengers using machine learning. We propose a change in the paradigm in the way we do multi-messenger astronomy, simultaneously using the complete information generated by violent phenomena in the Universe. What we propose is the application of a multimodal machine learning approach to characterize these events.
引用
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页数:11
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