BibTex format
@article{Abubakar:2025:10.1038/s41586-025-09599-3,
author = {Abubakar, S and Acero, MA and Acharya, B and Adamson, P and Anfimov, N and Antoshkin, A and Arrieta-Diaz, E and Asquith, L and Aurisano, A and Azevedo, D and Back, A and Balashov, N and Baldi, P and Bambah, BA and Bannister, EF and Barros, A and Bat, A and Bays, K and Bernstein, R and Bezerra, TJC and Bhatnagar, V and Bhuyan, B and Bian, J and Booth, AC and Bowles, R and Brahma, B and Bromberg, C and Buchanan, N and Butkevich, A and Calvez, S and Carceller, JM and Carroll, TJ and Catano-Mur, E and Cesar, JP and Chirco, R and Choudhary, BC and Christensen, A and Cicala, MF and Coan, TE and Contreras, T and Cooleybeck, A and Coveyou, D and Cremonesi, L and Davies, GS and Derwent, PF and Ding, P and Djurcic, Z and Dobbs, K and Dolce, M and Dueñas, Tonguino D and Dukes, EC and Dye, A and Ehrlich, R and Ewart, E and Filip, P and Frank, MJ and Gallagher, HR and Giri, A and Gomes, RA and Goodman, MC and Group, R and Habig, A and Hakl, F and Hartnell, J and Hatcher, R and Hays, JM and He, M an},
doi = {10.1038/s41586-025-09599-3},
journal = {Nature},
pages = {818--824},
title = {Joint neutrino oscillation analysis from the T2K and NOvA experiments},
url = {http://dx.doi.org/10.1038/s41586-025-09599-3},
volume = {646},
year = {2025}
}
RIS format (EndNote, RefMan)
TY - JOUR
AB - The landmark discovery that neutrinos have mass and can change type (or flavour) as they propagate—a process called neutrino oscillation1,2,3,4,5,6—has opened up a rich array of theoretical and experimental questions being actively pursued today. Neutrino oscillation remains the most powerful experimental tool for addressing many of these questions, including whether neutrinos violate charge-parity (CP) symmetry, which has possible connections to the unexplained preponderance of matter over antimatter in the Universe7,8,9,10,11. Oscillation measurements also probe the mass-squared differences between the different neutrino mass states (Δm2), whether there are two light states and a heavier one (normal ordering) or vice versa (inverted ordering), and the structure of neutrino mass and flavour mixing12. Here we carry out the first joint analysis of datasets from NOvA13 and T2K14, the two currently operating long-baseline neutrino oscillation experiments (hundreds of kilometres of neutrino travel distance), taking advantage of our complementary experimental designs and setting new constraints on several neutrino sector parameters. This analysis provides new precision on the
AU - Abubakar,S
AU - Acero,MA
AU - Acharya,B
AU - Adamson,P
AU - Anfimov,N
AU - Antoshkin,A
AU - Arrieta-Diaz,E
AU - Asquith,L
AU - Aurisano,A
AU - Azevedo,D
AU - Back,A
AU - Balashov,N
AU - Baldi,P
AU - Bambah,BA
AU - Bannister,EF
AU - Barros,A
AU - Bat,A
AU - Bays,K
AU - Bernstein,R
AU - Bezerra,TJC
AU - Bhatnagar,V
AU - Bhuyan,B
AU - Bian,J
AU - Booth,AC
AU - Bowles,R
AU - Brahma,B
AU - Bromberg,C
AU - Buchanan,N
AU - Butkevich,A
AU - Calvez,S
AU - Carceller,JM
AU - Carroll,TJ
AU - Catano-Mur,E
AU - Cesar,JP
AU - Chirco,R
AU - Choudhary,BC
AU - Christensen,A
AU - Cicala,MF
AU - Coan,TE
AU - Contreras,T
AU - Cooleybeck,A
AU - Coveyou,D
AU - Cremonesi,L
AU - Davies,GS
AU - Derwent,PF
AU - Ding,P
AU - Djurcic,Z
AU - Dobbs,K
AU - Dolce,M
AU - Dueñas,Tonguino D
AU - Dukes,EC
AU - Dye,A
AU - Ehrlich,R
AU - Ewart,E
AU - Filip,P
AU - Frank,MJ
AU - Gallagher,HR
AU - Giri,A
AU - Gomes,RA
AU - Goodman,MC
AU - Group,R
AU - Habig,A
AU - Hakl,F
AU - Hartnell,J
AU - Hatcher,R
AU - Hays,JM
AU - He,M
AU - Heller,K
AU - Hewes,V
AU - Himmel,A
AU - Horoho,T
AU - Ivanova,A
AU - Jargowsky,B
AU - Kakorin,I
AU - Kalitkina,A
AU - Kaplan,DM
AU - Khanam,A
AU - Kirezli,B
AU - Kleykamp,J
AU - Klimov,O
AU - Koerner,LW
AU - Kolupaeva,L
AU - Kralik,R
AU - Kumar,A
AU - Kuruppu,CD
AU - Kus,V
AU - Lackey,T
AU - Lang,K
AU - Lasorak,P
AU - Lesmeister,J
AU - Lister,A
AU - Liu,J
AU - Lock,JA
AU - MacMahon,M
AU - Magill,S
AU - Mann,WA
AU - Manoharan,MT
AU - Manrique,Plata M
AU - Marshak,ML
AU - Martinez-Casales,M
AU - Matveev,V
AU - Mehta,B
AU - Messier,MD
AU - Meyer,H
AU - Miao,T
AU - Miller,WH
AU - Mishra,SR
AU - Mohanta,R
AU - Moren,A
AU - Morozova,A
AU - Mu,W
AU - Mualem,L
AU - Muether,M
AU - Mulder,K
AU - Myers,D
AU - Naples,D
AU - Nelleri,S
AU - Nelson,JK
AU - Nichol,R
AU - Niner,E
AU - Norman,A
AU - Norrick,A
AU - Oh,H
AU - Olshevskiy,A
AU - Olson,T
AU - Ozkaynak,M
AU - Pal,A
AU - Paley,J
AU - Panda,L
AU - Patterson,RB
AU - Pawloski,G
AU - Petti,R
AU - Plunkett,RK
AU - Porter,JCC
AU - Prais,LR
AU - Rafique,A
AU - Raj,V
AU - Rajaoalisoa,M
AU - Ramson,B
AU - Rebel,B
AU - Robles,E
AU - Roy,P
AU - Samoylov,O
AU - Sanchez,MC
AU - Sánchez,Falero S
AU - Shanahan,P
AU - Sharma,P
AU - Sheshukov,A
AU - Shivam
AU - Shmakov,A
AU - Shorrock,W
AU - Shukla,S
AU - Singh,I
AU - Singh,P
AU - Singh,V
AU - Singh,Chhibra S
AU - Singha,DK
AU - Smith,A
AU - Smolik,J
AU - Snopok,P
AU - Solomey,N
AU - Sousa,A
AU - Soustruznik,K
AU - Strait,M
AU - Suter,L
AU - Sutton,A
AU - Swain,S
AU - Sweeney,C
AU - Sztuc,A
AU - Talukdar,N
AU - Tas,P
AU - Thakore,T
AU - Thomas,J
AU - Tiras,E
AU - Titus,M
AU - Torun,Y
AU - Tran,D
AU - Trokan-Tenorio,J
AU - Urheim,J
AU - Vahle,P
AU - Vallari,Z
AU - Vockerodt,KJ
AU - Waldron,AV
AU - Wallbank,M
AU - Warburton,TK W
DO - 10.1038/s41586-025-09599-3
EP - 824
PY - 2025///
SN - 0028-0836
SP - 818
TI - Joint neutrino oscillation analysis from the T2K and NOvA experiments
T2 - Nature
UR - http://dx.doi.org/10.1038/s41586-025-09599-3
UR - https://doi.org/10.1038/s41586-025-09599-3
VL - 646
ER -