Imperial College London
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Professor Yoshi Uchida

Faculty of Natural Sciences, Department of Physics

Professor of Physics
 
 
 
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Contact

 

+44 (0)20 7594 7821yoshi.uchida Website

 
 
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Location

 

524Blackett LaboratorySouth Kensington Campus

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Summary

 

Publications

Citation

BibTex format

@inproceedings{Abe:2022,
author = {Abe, K and Bronner, C and Hayato, Y and Hiraide, K and Ikeda, M and Kameda, J and Kanemura, Y and Kataoka, Y and Miki, S and Miura, M and Moriyama, S and Nagao, Y and Nakahata, M and Nakayama, S and Okamoto, K and Pronost, G and Sekiya, H and Shiozawa, M and Sonoda, Y and Suzuki, Y and Takeda, A and Takemoto, Y and Takenaka, A and Tanaka, H and Watanabe, S and Yano, T and Han, S and Kajita, T and Okumura, K and Tashiro, T and Xia, J and Megias, GD and Labarga, L and Marti, L and Zaldivar, B and Pointon, BW and Kearns, E and Raaf, JL and Wan, L and Wester, T and Bian, J and Griskevich, NJ and Kropp, WR and Locke, S and Mine, S and Smy, MB and Sobel, HW and Takhistov, V and Hill, J and Kim, JY and Lim, IT and Park, RG and Bodur, B and Scholberg, K and Walter, CW and Bernard, L and Coffani, A and Drapier, O and El, Hedri S and Giampaolo, A and Gonin, M and Mueller, TA and Paganini, P and Quilain, B and Ishizuka, T and Nakamura, T and Jang, JS and Learned, JG and Cao, S and Anthony, LHV an},
title = {Follow-up of GWTC-2 gravitational wave events with neutrinos from the Super-Kamiokande detector},
year = {2022}
}
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RIS format (EndNote, RefMan)

TY  - CPAPER
AB  - Super-Kamiokande (SK) is a 50-kt water Cherenkov detector, instrumented with ∼ 13k photo-multipliers and running since 1996. It is sensitive to neutrinos with energies ranging from 4.5 MeV to several TeV. A new framework has been developed for the follow-up of gravitational wave (GW) alerts issued by the LIGO-Virgo collaboration (LVC). Neutrinos are searched for, using a 1000-second time window centered on the alert time and in both SK low-energy and high-energy samples. Such observation can then be used to constrain the neutrino emission from the GW source. The significance of potential signals has been obtained by comparing neutrino direction with the localization of the GW. The computation of limits on incoming neutrino flux and on the total energy emitted in neutrinos by the source has been performed for the different neutrino flavors. The results using the LVC GWTC-2 catalog (covering O3a period) are presented, as well as the outlooks for the future real-time public release of follow-ups for the O4 period (in 2022) and beyond.
AU  - Abe,K
AU  - Bronner,C
AU  - Hayato,Y
AU  - Hiraide,K
AU  - Ikeda,M
AU  - Kameda,J
AU  - Kanemura,Y
AU  - Kataoka,Y
AU  - Miki,S
AU  - Miura,M
AU  - Moriyama,S
AU  - Nagao,Y
AU  - Nakahata,M
AU  - Nakayama,S
AU  - Okamoto,K
AU  - Pronost,G
AU  - Sekiya,H
AU  - Shiozawa,M
AU  - Sonoda,Y
AU  - Suzuki,Y
AU  - Takeda,A
AU  - Takemoto,Y
AU  - Takenaka,A
AU  - Tanaka,H
AU  - Watanabe,S
AU  - Yano,T
AU  - Han,S
AU  - Kajita,T
AU  - Okumura,K
AU  - Tashiro,T
AU  - Xia,J
AU  - Megias,GD
AU  - Labarga,L
AU  - Marti,L
AU  - Zaldivar,B
AU  - Pointon,BW
AU  - Kearns,E
AU  - Raaf,JL
AU  - Wan,L
AU  - Wester,T
AU  - Bian,J
AU  - Griskevich,NJ
AU  - Kropp,WR
AU  - Locke,S
AU  - Mine,S
AU  - Smy,MB
AU  - Sobel,HW
AU  - Takhistov,V
AU  - Hill,J
AU  - Kim,JY
AU  - Lim,IT
AU  - Park,RG
AU  - Bodur,B
AU  - Scholberg,K
AU  - Walter,CW
AU  - Bernard,L
AU  - Coffani,A
AU  - Drapier,O
AU  - El,Hedri S
AU  - Giampaolo,A
AU  - Gonin,M
AU  - Mueller,TA
AU  - Paganini,P
AU  - Quilain,B
AU  - Ishizuka,T
AU  - Nakamura,T
AU  - Jang,JS
AU  - Learned,JG
AU  - Cao,S
AU  - Anthony,LHV
AU  - Martin,D
AU  - Scott,M
AU  - Sztuc,AA
AU  - Uchida,Y
AU  - Berardi,V
AU  - Catanesi,MG
AU  - Radicioni,E
AU  - Calabria,NF
AU  - Machado,LN
AU  - De,Rosa G
AU  - Collazuol,G
AU  - Iacob,F
AU  - Lamoureux,M
AU  - Mattiazzi,M
AU  - Ospina,N
AU  - Ludovici,L
AU  - Maekawa,Y
AU  - Nishimura,Y
AU  - Friend,M
AU  - Hasegawa,T
AU  - Ishida,T
AU  - Kobayashi,T
AU  - Jakkapu,M
AU  - Matsubara,T
AU  - Nakadaira,T
AU  - Nakamura,K
AU  - Oyama,Y
AU  - Sakashita,K
AU  - Sekiguchi,T
AU  - Tsukamoto,T
PY  - 2022///
TI  - Follow-up of GWTC-2 gravitational wave events with neutrinos from the Super-Kamiokande detector
ER  -
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