Imperial College London

Morgan O. Wascko

Faculty of Natural SciencesDepartment of Physics

Academic Visitor
 
 
 
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Contact

 

+44 (0)20 7594 3465m.wascko Website CV

 
 
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Assistant

 

Ms Paula Brown +44 (0)20 7594 7823

 
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Location

 

522Blackett LaboratorySouth Kensington Campus

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Summary

 

Publications

Citation

BibTex format

@article{Li:2018:10.1103/PhysRevD.98.052006,
author = {Li, Z and Abe, K and Bronner, C and Hayato, Y and Ikeda, M and Iyogi, K and Kameda, J and Kato, Y and Kishimoto, Y and Marti, L and Miura, M and Moriyama, S and Nakahata, M and Nakajima, Y and Nakano, Y and Nakayama, S and Orii, A and Pronost, G and Sekiya, H and Shiozawa, M and Sonoda, Y and Takeda, A and Takenaka, A and Tanaka, H and Tasaka, S and Tomura, T and Akutsu, R and Kajita, T and Nishimura, Y and Okumura, K and Tsui, KM and Fernandez, P and Labarga, L and Blaszczyk, FDM and Gustafson, J and Kachulis, C and Kearns, E and Raaf, JL and Stone, JL and Sulak, LR and Berkman, S and Tobayama, S and Elnimr, M and Kropp, WR and Locke, S and Mine, S and Weatherly, P and Smy, MB and Sobel, HW and Takhistov, V and Ganezer, KS and Hill, J and Kim, JY and Lim, IT and Park, RG and Himmel, A and O'Sullivan, E and Scholberg, K and Walter, CW and Ishizuka, T and Nakamura, T and Jang, JS and Choi, K and Learned, JG and Matsuno, S and Smith, SN and Amey, J and Litchfield, RP and Ma, WY and Uchid},
doi = {10.1103/PhysRevD.98.052006},
journal = {PHYSICAL REVIEW D},
title = {Measurement of the tau neutrino cross section in atmospheric neutrino oscillations with Super-Kamiokande},
url = {http://dx.doi.org/10.1103/PhysRevD.98.052006},
volume = {98},
year = {2018}
}

RIS format (EndNote, RefMan)

TY  - JOUR
AB - Using 5326 days of atmospheric neutrino data, a search for atmospheric tau neutrino appearance has been performed in the Super-Kamiokande experiment. Super-Kamiokande measures the tau normalization to be 1.47±0.32 under the assumption of normal neutrino hierarchy, relative to the expectation of unity with neutrino oscillation. The result excludes the hypothesis of no-tau appearance with a significance level of 4.6σ. The inclusive charged-current tau neutrino cross section averaged by the tau neutrino flux at Super-Kamiokande is measured to be (0.94±0.20)×10−38  cm2. The measurement is consistent with the Standard Model prediction, agreeing to within 1.5σ.
AU - Li,Z
AU - Abe,K
AU - Bronner,C
AU - Hayato,Y
AU - Ikeda,M
AU - Iyogi,K
AU - Kameda,J
AU - Kato,Y
AU - Kishimoto,Y
AU - Marti,L
AU - Miura,M
AU - Moriyama,S
AU - Nakahata,M
AU - Nakajima,Y
AU - Nakano,Y
AU - Nakayama,S
AU - Orii,A
AU - Pronost,G
AU - Sekiya,H
AU - Shiozawa,M
AU - Sonoda,Y
AU - Takeda,A
AU - Takenaka,A
AU - Tanaka,H
AU - Tasaka,S
AU - Tomura,T
AU - Akutsu,R
AU - Kajita,T
AU - Nishimura,Y
AU - Okumura,K
AU - Tsui,KM
AU - Fernandez,P
AU - Labarga,L
AU - Blaszczyk,FDM
AU - Gustafson,J
AU - Kachulis,C
AU - Kearns,E
AU - Raaf,JL
AU - Stone,JL
AU - Sulak,LR
AU - Berkman,S
AU - Tobayama,S
AU - Elnimr,M
AU - Kropp,WR
AU - Locke,S
AU - Mine,S
AU - Weatherly,P
AU - Smy,MB
AU - Sobel,HW
AU - Takhistov,V
AU - Ganezer,KS
AU - Hill,J
AU - Kim,JY
AU - Lim,IT
AU - Park,RG
AU - Himmel,A
AU - O'Sullivan,E
AU - Scholberg,K
AU - Walter,CW
AU - Ishizuka,T
AU - Nakamura,T
AU - Jang,JS
AU - Choi,K
AU - Learned,JG
AU - Matsuno,S
AU - Smith,SN
AU - Amey,J
AU - Litchfield,RP
AU - Ma,WY
AU - Uchida,Y
AU - Wascko,MO
AU - Cao,S
AU - Friend,M
AU - Hasegawa,T
AU - Ishida,T
AU - Ishii,T
AU - Kobayashi,T
AU - Nakadaira,T
AU - Nakamura,K
AU - Oyama,Y
AU - Sakashita,K
AU - Sekiguchi,T
AU - Tsukamoto,T
AU - Abe,KE
AU - Hasegawa,M
AU - Suzuki,AT
AU - Takeuchi,Y
AU - Yano,T
AU - Hayashino,T
AU - Hiraki,T
AU - Hirota,S
AU - Huang,K
AU - Jiang,M
AU - Mori,M
AU - Nakamura,KE
AU - Nakaya,T
AU - Patel,ND
AU - Wendell,RA
AU - Anthony,LHV
AU - McCauley,N
AU - Pritchard,A
AU - Fukuda,Y
AU - Itow,Y
AU - Murase,M
AU - Muto,F
AU - Mijakowski,P
AU - Frankiewicz,K
AU - Jung,CK
AU - Li,X
AU - Palomino,JL
AU - Santucci,G
AU - Vilela,C
AU - Wilking,MJ
AU - Yanagisawa,C
AU - Yang,G
AU - Ito,S
AU - Fukuda,D
AU - Ishino,H
AU - Kibayashi,A
AU - Koshio,Y
AU - Nagata,H
AU - Sakuda,M
AU - Xu,C
AU - Kuno,Y
AU - Wark,D
AU - Di,Lodovico F
AU - Richards,B
AU - Sedgwick,SM
AU - Tacik,R
AU - Kim,SB
AU - Cole,A
AU - Thompson,L
AU - Okazawa,H
AU - Choi,Y
AU - Ito,K
AU - Nishijima,K
AU - Koshiba,M
AU - Suda,Y
AU - Yokoyama,M
AU - Calland,RG
AU - Hartz,M
AU - Martens,K
AU - Murdoch,M
AU - Quilain,B
AU - Simpson,C
AU - Suzuki,Y
AU - Vagins,MR
AU - Hamabe,D
AU - Kuze,M
AU - Okajima,Y
AU - Yoshida,T
AU - Ishitsuka,M
AU - Martin,JF
AU - Nantais,CM
AU - Tanaka,HA
AU - Towstego,T
AU - Konaka,A
AU - Chen,S
AU - Wan,L
AU - Zhang,Y
AU - Minamino,A
AU - Wilkes,RJ
DO - 10.1103/PhysRevD.98.052006
PY - 2018///
SN - 2470-0010
TI - Measurement of the tau neutrino cross section in atmospheric neutrino oscillations with Super-Kamiokande
T2 - PHYSICAL REVIEW D
UR - http://dx.doi.org/10.1103/PhysRevD.98.052006
UR - http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000444599100001&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=1ba7043ffcc86c417c072aa74d649202
UR - http://hdl.handle.net/10044/1/62752
VL - 98
ER -