Study of atmospheric neutrinos with the MACRO detector
- Ambrosio M
- Antolini R
- Assiro R
- Auriemma G
- Bakari D
- Baldini A
- Barbarino GC
- Barbarito E
- Barish BC
- Battistoni G
- Becherini Y
- Bellotti R
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- Bernardini P
- Bilokon H
- Bisi V
- Bloise C
- Bottazzi E
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- Brigida M
- Cafagna F
- Calicchio M
- Campana D
- Candela A
- Carboni M
- Cecchini S
- Cei F
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- Chiarella V
- Choudhary BC
- Coutu S
- Cozzi M
- Creti P
- De Cataldo G
- Degli Esposti L
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- De Marzo C
- De Mitri I
- Derkaoui J
- De Vincenzi M
- Di Credico A
- Di Ferdinando D
- Diotallevi R
- Erriquez O
- Favuzzi C
- Forti C
- Fusco P
- Gebhard M
- Giacomelli G
- Giacomelli R
- Giannini G
- Giglietto N
- Giorgini M
- Giuliani R
- Goretti M
- Grassi M
- Grau H
- Gray L
- Grillo A
- Guarino F
- Gustavino C
- Habig A
- Hanson J
- Hanson K
- Hawthorne A
- Heinz R
- Hong JT
- Iarocci E
- Katsavounidis E
- Katsavounidis I
- Kearns E
- Kim H
- Kyriazopoulou S
- Lamanna E
- Lane C
- Leone A
- Levin DS
- Lipari P
- Liu G
- Liu R
- Longley NP
- Longo MJ
- Loparco F
- Maaroufi F
- Mancarella G
- Mandrioli G
- Manzoor S
- Marrelli V
- Margiotta A
- Marini A
- Martello D
- Marzari Chiesa A
- Mazziotta MN
- Michael DG
- Mikheyev S
- Miller L
- Monacelli P
- Mongelli M
- Montaruli T
- Monteno M
- Mossbarger L
- Mufson S
- Musser J
- Nicolo D
- Nolty R
- Okada C
- Orsini M
- Orth C
- Osteria G
- Ouchrif M
- Palamara O
- Parlati S
- Patera V
- Patrizii L
- Pazzi R
- Peck CW
- Pellizzoni G
- Perchiazzi M
- Perrone L
- Petrakis J
- Petrera S
- Pignatano N
- Pinto C
- Pistilli P
- Popa V
- Raino A
- Reynoldson J
- Ronga F
- Rrhioua A
- Sacchetti A
- Saggese P
- Satriano C
- Satta L
- Scapparone E
- Scholberg K
- Sciubba A
- Serra P
- Sioli M
- Sirri G
- Sitta M
- Sondergaard S
- Spinelli P
- Spinetti M
- Spurio M
- Stalio S
- Steinberg R
- Stone JL
- Sulak LR
- Surdo A
- Tarle G
- Togo V
- Vakili M
- Valieri C
- Walter CW
- Webb R
- Zaccheo N.
- BUSSINO, Severino Angelo Maria
DOIAbstract
The MACRO experiment detected different categories of atmospheric muon neutrinos. We describe in this paper the energy estimate of upward throughgoing muons by using the multiple coulomb scattering. Combining the results of such analysis with the upgoing muon angular distribution, both not using the absolute ν flux normalization informations, an evidence above 4σ for atmospheric neutrino oscillation is found
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