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Measurement of the charged-current electron (anti-)neutrino inclusive cross-sections at the T2K off-axis near detector ND280

Journal of High Energy Physics. 2020;2020(10):1-43 DOI 10.1007/JHEP10(2020)114

 

Journal Homepage

Journal Title: Journal of High Energy Physics

ISSN: 1029-8479 (Online)

Publisher: SpringerOpen

Society/Institution: International School for Advanced Studies (SISSA)

LCC Subject Category: Science: Physics: Nuclear and particle physics. Atomic energy. Radioactivity

Country of publisher: Germany

Language of fulltext: English

Full-text formats available: PDF

 

AUTHORS


The T2K collaboration

K. Abe (University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory)

N. Akhlaq (Queen Mary University of London, School of Physics and Astronomy)

R. Akutsu (University of Tokyo, Institute for Cosmic Ray Research, Research Center for Cosmic Neutrinos)

A. Ali (Kyoto University, Department of Physics)

C. Alt (ETH Zurich, Institute for Particle Physics and Astrophysics)

C. Andreopoulos (University of Liverpool, Department of Physics)

L. Anthony (Imperial College London, Department of Physics)

M. Antonova (IFIC (CSIC & University of Valencia))

S. Aoki (Kobe University)

A. Ariga (University of Bern, Albert Einstein Center for Fundamental Physics, Laboratory for High Energy Physics (LHEP))

T. Arihara (Tokyo Metropolitan University, Department of Physics)

Y. Asada (Yokohama National University, Faculty of Engineering)

Y. Ashida (Kyoto University, Department of Physics)

E. T. Atkin (Imperial College London, Department of Physics)

Y. Awataguchi (Tokyo Metropolitan University, Department of Physics)

S. Ban (Kyoto University, Department of Physics)

M. Barbi (University of Regina, Department of Physics)

G. J. Barker (University of Warwick, Department of Physics)

G. Barr (Oxford University, Department of Physics)

D. Barrow (Oxford University, Department of Physics)

C. Barry (University of Liverpool, Department of Physics)

M. Batkiewicz-Kwasniak (H. Niewodniczanski Institute of Nuclear Physics PAN)

A. Beloshapkin (Institute for Nuclear Research of the Russian Academy of Sciences)

F. Bench (University of Liverpool, Department of Physics)

V. Berardi (INFN Sezione di Bari and Università e Politecnico di Bari, Dipartimento Interuniversitario di Fisica)

L. Berns (Tokyo Institute of Technology, Department of Physics)

S. Bhadra (York University, Department of Physics and Astronomy)

S. Bienstock (Sorbonne Université, Université Paris Diderot, CNRS/IN2P3, Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE))

A. Blondel (University of Geneva, section de Physique, DPNC)

S. Bolognesi (IRFU, CEA Saclay)

T. Bonus (Wroclaw University, Faculty of Physics and Astronomy)

B. Bourguille (Institut de Fisica d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB)

S. B. Boyd (University of Warwick, Department of Physics)

D. Brailsford (Lancaster University, Physics Department)

A. Bravar (University of Geneva, section de Physique, DPNC)

D. Bravo Berguño (University Autonoma Madrid, Department of Theoretical Physics)

C. Bronner (University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory)

S. Bron (University of Geneva, section de Physique, DPNC)

A. Bubak (University of Silesia, Institute of Physics)

M. Buizza Avanzini (Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet)

J. Calcutt (Michigan State University, Department of Physics and Astronomy)

T. Campbell (University of Colorado at Boulder, Department of Physics)

S. Cao (High Energy Accelerator Research Organization (KEK))

S. L. Cartwright (University of Sheffield, Department of Physics and Astronomy)

M. G. Catanesi (INFN Sezione di Bari and Università e Politecnico di Bari, Dipartimento Interuniversitario di Fisica)

A. Cervera (IFIC (CSIC & University of Valencia))

A. Chappell (University of Warwick, Department of Physics)

C. Checchia (INFN Sezione di Padova and Università di Padova, Dipartimento di Fisica)

D. Cherdack (University of Houston, Department of Physics)

N. Chikuma (University of Tokyo, Department of Physics)

G. Christodoulou (CERN European Organization for Nuclear Research)

M. Cicerchia (INFN Sezione di Padova and Università di Padova, Dipartimento di Fisica)

J. Coleman (University of Liverpool, Department of Physics)

G. Collazuol (INFN Sezione di Padova and Università di Padova, Dipartimento di Fisica)

L. Cook (Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo)

D. Coplowe (Oxford University, Department of Physics)

A. Cudd (University of Colorado at Boulder, Department of Physics)

A. Dabrowska (H. Niewodniczanski Institute of Nuclear Physics PAN)

G. De Rosa (INFN Sezione di Napoli and Università di Napoli, Dipartimento di Fisica)

T. Dealtry (Lancaster University, Physics Department)

P. F. Denner (University of Warwick, Department of Physics)

S. R. Dennis (University of Liverpool, Department of Physics)

C. Densham (STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory)

F. Di Lodovico (King’s College London, Department of Physics)

N. Dokania (State University of New York at Stony Brook, Department of Physics and Astronomy)

S. Dolan (CERN European Organization for Nuclear Research)

T. A. Doyle (Lancaster University, Physics Department)

O. Drapier (Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet)

J. Dumarchez (Sorbonne Université, Université Paris Diderot, CNRS/IN2P3, Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE))

P. Dunne (Imperial College London, Department of Physics)

A. Eguchi (University of Tokyo, Department of Physics)

L. Eklund (University of Glasgow, School of Physics and Astronomy)

S. Emery-Schrenk (IRFU, CEA Saclay)

A. Ereditato (University of Bern, Albert Einstein Center for Fundamental Physics, Laboratory for High Energy Physics (LHEP))

P. Fernandez (IFIC (CSIC & University of Valencia))

T. Feusels (University of British Columbia, Department of Physics and Astronomy)

A. J. Finch (Lancaster University, Physics Department)

G. A. Fiorentini (York University, Department of Physics and Astronomy)

G. Fiorillo (INFN Sezione di Napoli and Università di Napoli, Dipartimento di Fisica)

C. Francois (University of Bern, Albert Einstein Center for Fundamental Physics, Laboratory for High Energy Physics (LHEP))

M. Friend (High Energy Accelerator Research Organization (KEK))

Y. Fujii (High Energy Accelerator Research Organization (KEK))

R. Fujita (University of Tokyo, Department of Physics)

D. Fukuda (Okayama University, Department of Physics)

R. Fukuda (Tokyo University of Science, Faculty of Science and Technology, Department of Physics)

Y. Fukuda (Miyagi University of Education, Department of Physics)

K. Fusshoeller (ETH Zurich, Institute for Particle Physics and Astrophysics)

C. Giganti (Sorbonne Université, Université Paris Diderot, CNRS/IN2P3, Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE))

T. Golan (Wroclaw University, Faculty of Physics and Astronomy)

M. Gonin (Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet)

A. Gorin (Institute for Nuclear Research of the Russian Academy of Sciences)

M. Guigue (Sorbonne Université, Université Paris Diderot, CNRS/IN2P3, Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE))

D. R. Hadley (University of Warwick, Department of Physics)

J. T. Haigh (University of Warwick, Department of Physics)

P. Hamacher-Baumann (RWTH Aachen University, III. Physikalisches Institut)

M. Hartz (Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo)

T. Hasegawa (High Energy Accelerator Research Organization (KEK))

S. Hassani (IRFU, CEA Saclay)

N. C. Hastings (High Energy Accelerator Research Organization (KEK))

T. Hayashino (Kyoto University, Department of Physics)

Y. Hayato (Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo)

A. Hiramoto (Kyoto University, Department of Physics)

M. Hogan (Colorado State University, Department of Physics)

J. Holeczek (University of Silesia, Institute of Physics)

N. T. Hong Van (Institute For Interdisciplinary Research in Science and Education (IFIRSE), ICISE)

T. Honjo (Osaka City University, Department of Physics)

F. Iacob (INFN Sezione di Padova and Università di Padova, Dipartimento di Fisica)

A. K. Ichikawa (Kyoto University, Department of Physics)

M. Ikeda (University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory)

T. Ishida (High Energy Accelerator Research Organization (KEK))

T. Ishii (High Energy Accelerator Research Organization (KEK))

M. Ishitsuka (Tokyo University of Science, Faculty of Science and Technology, Department of Physics)

K. Iwamoto (University of Tokyo, Department of Physics)

A. Izmaylov (Institute for Nuclear Research of the Russian Academy of Sciences)

N. Izumi (Tokyo University of Science, Faculty of Science and Technology, Department of Physics)

M. Jakkapu (High Energy Accelerator Research Organization (KEK))

B. Jamieson (University of Winnipeg, Department of Physics)

S. J. Jenkins (University of Sheffield, Department of Physics and Astronomy)

C. Jesús-Valls (Institut de Fisica d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB)

M. Jiang (Kyoto University, Department of Physics)

S. Johnson (University of Colorado at Boulder, Department of Physics)

P. Jonsson (Imperial College London, Department of Physics)

C. K. Jung (State University of New York at Stony Brook, Department of Physics and Astronomy)

X. Junjie (University of Tokyo, Institute for Cosmic Ray Research, Research Center for Cosmic Neutrinos)

P. B. Jurj (Imperial College London, Department of Physics)

M. Kabirnezhad (Oxford University, Department of Physics)

A. C. Kaboth (Royal Holloway University of London, Department of Physics)

T. Kajita (University of Tokyo, Institute for Cosmic Ray Research, Research Center for Cosmic Neutrinos)

H. Kakuno (Tokyo Metropolitan University, Department of Physics)

J. Kameda (University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory)

D. Karlen (TRIUMF)

S. P. Kasetti (Louisiana State University, Department of Physics and Astronomy)

Y. Kataoka (University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory)

Y. Katayama (Yokohama National University, Faculty of Engineering)

T. Katori (King’s College London, Department of Physics)

Y. Kato (University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory)

E. Kearns (Boston University, Department of Physics)

M. Khabibullin (Institute for Nuclear Research of the Russian Academy of Sciences)

A. Khotjantsev (Institute for Nuclear Research of the Russian Academy of Sciences)

T. Kikawa (Kyoto University, Department of Physics)

H. Kikutani (University of Tokyo, Department of Physics)

H. Kim (Osaka City University, Department of Physics)

S. King (King’s College London, Department of Physics)

J. Kisiel (University of Silesia, Institute of Physics)

A. Knight (University of Warwick, Department of Physics)

A. Knox (Lancaster University, Physics Department)

T. Kobata (Osaka City University, Department of Physics)

T. Kobayashi (High Energy Accelerator Research Organization (KEK))

L. Koch (Oxford University, Department of Physics)

T. Koga (University of Tokyo, Department of Physics)

A. Konaka (TRIUMF)

L. L. Kormos (Lancaster University, Physics Department)

Y. Koshio (Okayama University, Department of Physics)

A. Kostin (Institute for Nuclear Research of the Russian Academy of Sciences)

K. Kowalik (National Centre for Nuclear Research)

H. Kubo (Kyoto University, Department of Physics)

Y. Kudenko (Institute for Nuclear Research of the Russian Academy of Sciences)

N. Kukita (Osaka City University, Department of Physics)

S. Kuribayashi (Kyoto University, Department of Physics)

R. Kurjata (Warsaw University of Technology, Institute of Radioelectronics and Multimedia Technology)

T. Kutter (Louisiana State University, Department of Physics and Astronomy)

M. Kuze (Tokyo Institute of Technology, Department of Physics)

L. Labarga (University Autonoma Madrid, Department of Theoretical Physics)

J. Lagoda (National Centre for Nuclear Research)

M. Lamoureux (INFN Sezione di Padova and Università di Padova, Dipartimento di Fisica)

D. Last (University of Pennsylvania, Department of Physics and Astronomy)

M. Laveder (INFN Sezione di Padova and Università di Padova, Dipartimento di Fisica)

M. Lawe (Lancaster University, Physics Department)

M. Licciardi (Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet)

T. Lindner (TRIUMF)

R. P. Litchfield (University of Glasgow, School of Physics and Astronomy)

S. L. Liu (State University of New York at Stony Brook, Department of Physics and Astronomy)

X. Li (State University of New York at Stony Brook, Department of Physics and Astronomy)

A. Longhin (INFN Sezione di Padova and Università di Padova, Dipartimento di Fisica)

L. Ludovici (INFN Sezione di Roma and Università di Roma “La Sapienza”)

X. Lu (Oxford University, Department of Physics)

T. Lux (Institut de Fisica d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB)

L. N. Machado (INFN Sezione di Napoli and Università di Napoli, Dipartimento di Fisica)

L. Magaletti (INFN Sezione di Bari and Università e Politecnico di Bari, Dipartimento Interuniversitario di Fisica)

K. Mahn (Michigan State University, Department of Physics and Astronomy)

M. Malek (University of Sheffield, Department of Physics and Astronomy)

S. Manly (University of Rochester, Department of Physics and Astronomy)

L. Maret (University of Geneva, section de Physique, DPNC)

A. D. Marino (University of Colorado at Boulder, Department of Physics)

L. Marti-Magro (Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo)

J. F. Martin (University of Toronto, Department of Physics)

T. Maruyama (High Energy Accelerator Research Organization (KEK))

T. Matsubara (High Energy Accelerator Research Organization (KEK))

K. Matsushita (University of Tokyo, Department of Physics)

V. Matveev (Institute for Nuclear Research of the Russian Academy of Sciences)

C. Mauger (University of Pennsylvania, Department of Physics and Astronomy)

K. Mavrokoridis (University of Liverpool, Department of Physics)

E. Mazzucato (IRFU, CEA Saclay)

M. McCarthy (York University, Department of Physics and Astronomy)

N. McCauley (University of Liverpool, Department of Physics)

J. McElwee (University of Sheffield, Department of Physics and Astronomy)

K. S. McFarland (University of Rochester, Department of Physics and Astronomy)

C. McGrew (State University of New York at Stony Brook, Department of Physics and Astronomy)

A. Mefodiev (Institute for Nuclear Research of the Russian Academy of Sciences)

C. Metelko (University of Liverpool, Department of Physics)

M. Mezzetto (INFN Sezione di Padova and Università di Padova, Dipartimento di Fisica)

A. Minamino (Yokohama National University, Faculty of Engineering)

O. Mineev (Institute for Nuclear Research of the Russian Academy of Sciences)

S. Mine (University of California, Irvine, Department of Physics and Astronomy)

M. Miura (University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory)

L. Molina Bueno (ETH Zurich, Institute for Particle Physics and Astrophysics)

S. Moriyama (University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory)

J. Morrison (Michigan State University, Department of Physics and Astronomy)

Th. A. Mueller (Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet)

L. Munteanu (IRFU, CEA Saclay)

S. Murphy (ETH Zurich, Institute for Particle Physics and Astrophysics)

Y. Nagai (University of Colorado at Boulder, Department of Physics)

T. Nakadaira (High Energy Accelerator Research Organization (KEK))

M. Nakahata (Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo)

Y. Nakajima (University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory)

A. Nakamura (Okayama University, Department of Physics)

K. G. Nakamura (Kyoto University, Department of Physics)

K. Nakamura (High Energy Accelerator Research Organization (KEK))

Y. Nakano (Kobe University)

S. Nakayama (Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo)

T. Nakaya (Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo)

K. Nakayoshi (High Energy Accelerator Research Organization (KEK))

C. Nantais (University of Toronto, Department of Physics)

C. E. R. Naseby (Imperial College London, Department of Physics)

T. V. Ngoc (Institute For Interdisciplinary Research in Science and Education (IFIRSE), ICISE)

K. Niewczas (Wroclaw University, Faculty of Physics and Astronomy)

K. Nishikawa (High Energy Accelerator Research Organization (KEK))

Y. Nishimura (Keio University, Department of Physics)

E. Noah (University of Geneva, section de Physique, DPNC)

T. S. Nonnenmacher (Imperial College London, Department of Physics)

F. Nova (STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory)

P. Novella (IFIC (CSIC & University of Valencia))

J. Nowak (Lancaster University, Physics Department)

J. C. Nugent (University of Glasgow, School of Physics and Astronomy)

H. M. O’Keeffe (Lancaster University, Physics Department)

L. O’Sullivan (University of Sheffield, Department of Physics and Astronomy)

T. Odagawa (Kyoto University, Department of Physics)

T. Ogawa (High Energy Accelerator Research Organization (KEK))

R. Okada (Okayama University, Department of Physics)

K. Okumura (Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo)

T. Okusawa (Osaka City University, Department of Physics)

S. M. Oser (University of British Columbia, Department of Physics and Astronomy)

R. A. Owen (Queen Mary University of London, School of Physics and Astronomy)

Y. Oyama (High Energy Accelerator Research Organization (KEK))

V. Palladino (INFN Sezione di Napoli and Università di Napoli, Dipartimento di Fisica)

J. L. Palomino (State University of New York at Stony Brook, Department of Physics and Astronomy)

V. Paolone (University of Pittsburgh, Department of Physics and Astronomy)

M. Pari (INFN Sezione di Padova and Università di Padova, Dipartimento di Fisica)

W. C. Parker (Royal Holloway University of London, Department of Physics)

S. Parsa (University of Geneva, section de Physique, DPNC)

J. Pasternak (Imperial College London, Department of Physics)

P. Paudyal (University of Liverpool, Department of Physics)

M. Pavin (TRIUMF)

D. Payne (University of Liverpool, Department of Physics)

G. C. Penn (University of Liverpool, Department of Physics)

L. Pickering (Michigan State University, Department of Physics and Astronomy)

C. Pidcott (University of Sheffield, Department of Physics and Astronomy)

G. Pintaudi (Yokohama National University, Faculty of Engineering)

E. S. Pinzon Guerra (York University, Department of Physics and Astronomy)

C. Pistillo (University of Bern, Albert Einstein Center for Fundamental Physics, Laboratory for High Energy Physics (LHEP))

B. Popov (Sorbonne Université, Université Paris Diderot, CNRS/IN2P3, Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE))

K. Porwit (University of Silesia, Institute of Physics)

M. Posiadala-Zezula (University of Warsaw, Faculty of Physics)

A. Pritchard (University of Liverpool, Department of Physics)

B. Quilain (Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet)

T. Radermacher (RWTH Aachen University, III. Physikalisches Institut)

E. Radicioni (INFN Sezione di Bari and Università e Politecnico di Bari, Dipartimento Interuniversitario di Fisica)

B. Radics (ETH Zurich, Institute for Particle Physics and Astrophysics)

P. N. Ratoff (Lancaster University, Physics Department)

E. Reinherz-Aronis (Colorado State University, Department of Physics)

C. Riccio (State University of New York at Stony Brook, Department of Physics and Astronomy)

E. Rondio (National Centre for Nuclear Research)

S. Roth (RWTH Aachen University, III. Physikalisches Institut)

A. Rubbia (ETH Zurich, Institute for Particle Physics and Astrophysics)

A. C. Ruggeri (INFN Sezione di Napoli and Università di Napoli, Dipartimento di Fisica)

C. A. Ruggles (University of Glasgow, School of Physics and Astronomy)

A. Rychter (Warsaw University of Technology, Institute of Radioelectronics and Multimedia Technology)

K. Sakashita (High Energy Accelerator Research Organization (KEK))

F. Sánchez (University of Geneva, section de Physique, DPNC)

G. Santucci (York University, Department of Physics and Astronomy)

C. M. Schloesser (ETH Zurich, Institute for Particle Physics and Astrophysics)

K. Scholberg (Duke University, Department of Physics)

J. Schwehr (Colorado State University, Department of Physics)

M. Scott (Imperial College London, Department of Physics)

Y. Seiya (Osaka City University, Department of Physics)

T. Sekiguchi (High Energy Accelerator Research Organization (KEK))

H. Sekiya (Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo)

D. Sgalaberna (ETH Zurich, Institute for Particle Physics and Astrophysics)

R. Shah (Oxford University, Department of Physics)

A. Shaikhiev (Institute for Nuclear Research of the Russian Academy of Sciences)

F. Shaker (University of Winnipeg, Department of Physics)

A. Shaykina (Institute for Nuclear Research of the Russian Academy of Sciences)

M. Shiozawa (Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo)

W. Shorrock (Imperial College London, Department of Physics)

A. Shvartsman (Institute for Nuclear Research of the Russian Academy of Sciences)

A. Smirnov (Institute for Nuclear Research of the Russian Academy of Sciences)

M. Smy (University of California, Irvine, Department of Physics and Astronomy)

J. T. Sobczyk (Wroclaw University, Faculty of Physics and Astronomy)

H. Sobel (University of California, Irvine, Department of Physics and Astronomy)

F. J. P. Soler (University of Glasgow, School of Physics and Astronomy)

Y. Sonoda (University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory)

J. Steinmann (RWTH Aachen University, III. Physikalisches Institut)

S. Suvorov (IRFU, CEA Saclay)

A. Suzuki (Kobe University)

S. Y. Suzuki (High Energy Accelerator Research Organization (KEK))

Y. Suzuki (Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo)

A. A. Sztuc (Imperial College London, Department of Physics)

M. Tada (High Energy Accelerator Research Organization (KEK))

M. Tajima (Kyoto University, Department of Physics)

A. Takeda (University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory)

Y. Takeuchi (Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo)

H. K. Tanaka (University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory)

H. A. Tanaka (SLAC National Accelerator Laboratory, Stanford University)

S. Tanaka (Osaka City University, Department of Physics)

Y. Tanihara (Yokohama National University, Faculty of Engineering)

M. Tani (Kyoto University, Department of Physics)

N. Teshima (Osaka City University, Department of Physics)

L. F. Thompson (University of Sheffield, Department of Physics and Astronomy)

W. Toki (Colorado State University, Department of Physics)

C. Touramanis (University of Liverpool, Department of Physics)

T. Towstego (University of Toronto, Department of Physics)

K. M. Tsui (University of Liverpool, Department of Physics)

T. Tsukamoto (High Energy Accelerator Research Organization (KEK))

M. Tzanov (Louisiana State University, Department of Physics and Astronomy)

Y. Uchida (Imperial College London, Department of Physics)

M. Vagins (University of California, Irvine, Department of Physics and Astronomy)

S. Valder (University of Warwick, Department of Physics)

Z. Vallari (State University of New York at Stony Brook, Department of Physics and Astronomy)

D. Vargas (Institut de Fisica d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB)

G. Vasseur (IRFU, CEA Saclay)

C. Vilela (State University of New York at Stony Brook, Department of Physics and Astronomy)

W. G. S. Vinning (University of Warwick, Department of Physics)

T. Vladisavljevic (STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory)

V. V. Volkov (Institute for Nuclear Research of the Russian Academy of Sciences)

T. Wachala (H. Niewodniczanski Institute of Nuclear Physics PAN)

J. Walker (University of Winnipeg, Department of Physics)

J. G. Walsh (Lancaster University, Physics Department)

Y. Wang (State University of New York at Stony Brook, Department of Physics and Astronomy)

D. Wark (Oxford University, Department of Physics)

M. O. Wascko (Imperial College London, Department of Physics)

A. Weber (Oxford University, Department of Physics)

R. Wendell (Kyoto University, Department of Physics)

M. J. Wilking (State University of New York at Stony Brook, Department of Physics and Astronomy)

C. Wilkinson (University of Bern, Albert Einstein Center for Fundamental Physics, Laboratory for High Energy Physics (LHEP))

J. R. Wilson (King’s College London, Department of Physics)

R. J. Wilson (Colorado State University, Department of Physics)

K. Wood (State University of New York at Stony Brook, Department of Physics and Astronomy)

C. Wret (University of Rochester, Department of Physics and Astronomy)

Y. Yamada (High Energy Accelerator Research Organization (KEK))

K. Yamamoto (Osaka City University, Department of Physics)

C. Yanagisawa (State University of New York at Stony Brook, Department of Physics and Astronomy)

G. Yang (State University of New York at Stony Brook, Department of Physics and Astronomy)

T. Yano (University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory)

K. Yasutome (Kyoto University, Department of Physics)

S. Yen (TRIUMF)

N. Yershov (Institute for Nuclear Research of the Russian Academy of Sciences)

M. Yokoyama (University of Tokyo, Department of Physics)

T. Yoshida (Tokyo Institute of Technology, Department of Physics)

M. Yu (York University, Department of Physics and Astronomy)

A. Zalewska (H. Niewodniczanski Institute of Nuclear Physics PAN)

J. Zalipska (National Centre for Nuclear Research)

K. Zaremba (Warsaw University of Technology, Institute of Radioelectronics and Multimedia Technology)

G. Zarnecki (National Centre for Nuclear Research)

M. Ziembicki (Warsaw University of Technology, Institute of Radioelectronics and Multimedia Technology)

E. D. Zimmerman (University of Colorado at Boulder, Department of Physics)

M. Zito (Sorbonne Université, Université Paris Diderot, CNRS/IN2P3, Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE))

S. Zsoldos (King’s College London, Department of Physics)

A. Zykova (Institute for Nuclear Research of the Russian Academy of Sciences)

EDITORIAL INFORMATION

Blind peer review

Editorial Board

Instructions for authors

Time From Submission to Publication: 12 weeks

 

Abstract | Full Text

Abstract The electron (anti-)neutrino component of the T2K neutrino beam constitutes the largest background in the measurement of electron (anti-)neutrino appearance at the far detector. The electron neutrino scattering is measured directly with the T2K off-axis near detector, ND280. The selection of the electron (anti-)neutrino events in the plastic scintillator target from both neutrino and anti-neutrino mode beams is discussed in this paper. The flux integrated single differential charged-current inclusive electron (anti-)neutrino cross-sections, dσ/dp and dσ/d cos(θ), and the total cross-sections in a limited phase-space in momentum and scattering angle (p > 300 MeV/c and θ ≤ 45°) are measured using a binned maximum likelihood fit and compared to the neutrino Monte Carlo generator predictions, resulting in good agreement.