Premerger detection of massive black hole binaries using deep learning
被引:3
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作者:
Ruan, Wen-Hong
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Univ Chinese Acad Sci, Hangzhou Inst Adv Study, Sch Fundamental Phys & Math Sci, Hangzhou 310024, Peoples R China
Univ Chinese Acad Sci, Sch Phys Sci, 19A Yuquan Rd, Beijing 100049, Peoples R ChinaUniv Chinese Acad Sci, Hangzhou Inst Adv Study, Sch Fundamental Phys & Math Sci, Hangzhou 310024, Peoples R China
Ruan, Wen-Hong
[1
,2
]
Guo, Zong-Kuan
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Univ Chinese Acad Sci, Hangzhou Inst Adv Study, Sch Fundamental Phys & Math Sci, Hangzhou 310024, Peoples R China
Univ Chinese Acad Sci, Sch Phys Sci, 19A Yuquan Rd, Beijing 100049, Peoples R China
Chinese Acad Sci, CAS Key Lab Theoret Phys, Inst Theoret Phys, Beijing 100190, Peoples R ChinaUniv Chinese Acad Sci, Hangzhou Inst Adv Study, Sch Fundamental Phys & Math Sci, Hangzhou 310024, Peoples R China
Guo, Zong-Kuan
[1
,2
,3
]
机构:
[1] Univ Chinese Acad Sci, Hangzhou Inst Adv Study, Sch Fundamental Phys & Math Sci, Hangzhou 310024, Peoples R China
[2] Univ Chinese Acad Sci, Sch Phys Sci, 19A Yuquan Rd, Beijing 100049, Peoples R China
[3] Chinese Acad Sci, CAS Key Lab Theoret Phys, Inst Theoret Phys, Beijing 100190, Peoples R China
Coalescing massive black hole binaries (MBHBs) are one of primary sources for space -based gravitational wave (GW) observations. The mergers of these binaries are expected to give rise to detectable electromagnetic (EM) emissions with a narrow time window. The premerger detection of GW signals is vital for follow-up EM observations. The conventional approach for searching GW signals involves high computational costs. In this study, we present a deep learning model to search for GW signals from MBHBs. Our model is able to process 4.7 days of simulated data within 0.01 seconds and detect GW signals several hours to days before the final merger. The model provides the possibility of the coincident GW and EM detection of MBHBs.
机构:
Eotvos Lorand Univ, Inst Phys, Pazmany P S 1-A, H-1117 Budapest, HungaryUniv Milano Bicocca, Dipartimento Fis G Occhialini, Piazza Sci 3, I-20126 Milan, Italy
Rasskazov, Alexander
Sesana, Alberto
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Univ Milano Bicocca, Dipartimento Fis G Occhialini, Piazza Sci 3, I-20126 Milan, Italy
Ist Nazl Fis Nucl, Sez Milano Bicocca, Piazza Sci 3, I-20126 Milan, ItalyUniv Milano Bicocca, Dipartimento Fis G Occhialini, Piazza Sci 3, I-20126 Milan, Italy
Sesana, Alberto
Dotti, Massimo
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Univ Milano Bicocca, Dipartimento Fis G Occhialini, Piazza Sci 3, I-20126 Milan, Italy
Ist Nazl Fis Nucl, Sez Milano Bicocca, Piazza Sci 3, I-20126 Milan, ItalyUniv Milano Bicocca, Dipartimento Fis G Occhialini, Piazza Sci 3, I-20126 Milan, Italy
Dotti, Massimo
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Haardt, Francesco
Leigh, Nathan W. C.
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Univ Concepcion, Fac Ciencias Fis & Matemat, Dept Astron, Concepcion, Chile
Amer Museum Nat Hist, Dept Astrophys, Cent Pk West & 79th St, New York, NY 10024 USAUniv Milano Bicocca, Dipartimento Fis G Occhialini, Piazza Sci 3, I-20126 Milan, Italy
Leigh, Nathan W. C.
Sedda, Manuel Arca
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Heidelberg Univ, Astronom Rechen Inst, Zentrum Astron, Monchhofstr 12-14, D-69120 Heidelberg, GermanyUniv Milano Bicocca, Dipartimento Fis G Occhialini, Piazza Sci 3, I-20126 Milan, Italy
Sedda, Manuel Arca
Fragione, Giacomo
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Northwestern Univ, Dept Phys & Astron, Evanston, IL 60202 USA
CIERA, Evanston, IL 60202 USAUniv Milano Bicocca, Dipartimento Fis G Occhialini, Piazza Sci 3, I-20126 Milan, Italy
Fragione, Giacomo
Rossi, Elena
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Leiden Univ, Leiden Observ, POB 9513, NL-2300 RA Leiden, NetherlandsUniv Milano Bicocca, Dipartimento Fis G Occhialini, Piazza Sci 3, I-20126 Milan, Italy
机构:
Univ Milano Bicocca, Dipartimento Fis G Occhialini, I-20126 Milan, ItalyUniv Milano Bicocca, Dipartimento Fis G Occhialini, I-20126 Milan, Italy
Dotti, M.
Sesana, A.
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Max Planck Inst Gravitat Phys, Albert Einstein Inst, Galaxy & Cosmol Dept, D-14476 Golm, GermanyUniv Milano Bicocca, Dipartimento Fis G Occhialini, I-20126 Milan, Italy
Sesana, A.
Decarli, R.
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Max Planck Inst Astron, D-69117 Heidelberg, GermanyUniv Milano Bicocca, Dipartimento Fis G Occhialini, I-20126 Milan, Italy