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1. MACRO results on atmospheric neutrinos

Author

Ambrosio M, Antolini R, Assiro R, Auriemma G, Bakari D, Baldini A, Barbarino GC, Barbarito E, Barish BC, Battistoni G, Becherini Y, Bellotti R, Bemporad C, Bernardini P, Bilokon H, Bisi V, Bloise C, Bottazzi E, Bower C, Brigida M, Cafagna F, Calicchio M, Campana D, Candela A, Carboni M, Cecchini S, Cei F, Ceres A, Chiarella V, Choudhary BC, Coutu S, Cozzi M, Creti P, De Cataldo G, Degli Esposti L, Dekhissi H, 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, G. GIACOMELLI, A.MARGIOTTA, Ambrosio, M, Antolini, R, Assiro, R, Auriemma, G, Bakari, D, Baldini, A, Barbarino, Gc, Barbarito, E, Barish, Bc, Battistoni, G, Becherini, Y, Bellotti, R, Bemporad, C, Bernardini, P, Bilokon, H, Bisi, V, Bloise, C, Bottazzi, E, Bower, C, Brigida, M, Bussino, Severino Angelo Maria, Cafagna, F, Calicchio, M, Campana, D, Candela, A, Carboni, M, Cecchini, S, Cei, F, Ceres, A, Chiarella, V, Choudhary, Bc, Coutu, S, Cozzi, M, Creti, P, De Cataldo, G, Degli Esposti, L, Dekhissi, H, 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, D, 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, and Zaccheo, N.

Subjects
Physics, Nuclear and High Energy Physics, Particle physics, Muon, NEUTRINO OSCILLATIONS, Astrophysics (astro-ph), Monte Carlo method, FOS: Physical sciences, MACRO, Solar neutrino problem, Lorentz covariance, Astrophysics, Atomic and Molecular Physics, and Optics, High Energy Physics - Experiment, Atmospheric Neutrino, atmospheric neutrino, High Energy Physics - Experiment (hep-ex), Measurements of neutrino speed, High Energy Physics::Experiment, Neutrino, Neutrino oscillation, Underground detector, Event (particle physics)
Abstract

We discuss the final results of the MACRO experiment on atmospheric neutrino oscillations. The data concern event topologies with average neutrino energies of ~3 and ~50 GeV. Multiple Coulomb Scattering of the high energy muons was used to estimate the neutrino energy event by event. The angular distributions, the L/E_nu distribution, the particle ratios and the absolute fluxes all favor nu_mu --> nu_tau oscillations with maximal mixing and Delta m^2 ~0.0023 eV^2. Emphasis is given to measured ratios which are not affected by Monte Carlo (MC) absolute normalization; a discussion is made on MC uncertainties. A preliminary search for possible Lorentz invariance violation contributions to atmospheric neutrino oscillations is presented and discussed., 4 pages, 6 figures. Paper presented at the NOW 2004 Workshop, Conca Specchiulla, Otranto, Italy, September 2004

Published
2005

2. Atmospheric neutrino oscillations in the macro experiment

Author

Ambrosio M, Antolini R, Assiro R, Auriemma G, Bakari D, Baldini A, Barbarino GC, Barbarito E, Barish BC, Battistoni G, Becherini Y, Bellotti R, Bemporad C, Bernardini P, Bilokon H, Bisi V, Bloise C, Bottazzi E, Bower C, Brigida M, Cafagna F, Calicchio M, Campana D, Candela A, Carboni M, Cecchini S, Cei F, Ceres A, Chiarella V, Choudhary BC, Coutu S, Cozzi M, Creti P, De Cataldo G, Degli Esposti L, Dekhissi H, 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, Ambrosio, M, Antolini, R, Assiro, R, Auriemma, G, Bakari, D, Baldini, A, Barbarino, Gc, Barbarito, E, Barish, Bc, Battistoni, G, Becherini, Y, Bellotti, R, Bemporad, C, Bernardini, P, Bilokon, H, Bisi, V, Bloise, C, Bottazzi, E, Bower, C, Brigida, M, Bussino, Severino Angelo Maria, Cafagna, F, Calicchio, M, Campana, D, Candela, A, Carboni, M, Cecchini, S, Cei, F, Ceres, A, Chiarella, V, Choudhary, Bc, Coutu, S, Cozzi, M, Creti, P, De Cataldo, G, Degli Esposti, L, Dekhissi, H, 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, D, 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, and Zaccheo, N.

Subjects
Physics, Particle physics, Nuclear and High Energy Physics, Muon, Neutrino oscillation, Oscillation, Physics::Instrumentation and Detectors, Solar neutrino, Astrophysics::High Energy Astrophysical Phenomena, High Energy Physics::Phenomenology, Atmospheric neutrino, MACRO, Solar neutrino problem, Atomic and Molecular Physics, and Optics, Nuclear physics, Neutrino detector, Measurements of neutrino speed, High Energy Physics::Experiment, Neutrino
Abstract

In the MACRO experiment the flux of atmospheric muon neutrinos has been studied through the detection of upward-going muons generated in the rock below the detector and also through neutrino interactions inside the apparatus. Several topologies of neutrino events have been detected, which correspond to different neutrino parent energies. The measured flux in the different data sets shows a deficit with respect to the Monte Carlo predictions. Moreover, the upward-throughgoing muon sample (median neutrino energy ∼ 50 GeV ) also shows a distortion in the angular distribution shape. Interpreted in terms of neutrino oscillation, these results favor a ν μ into ν τ oscillation scenario, while the ν μ into ν sterile channel is disfavared at 99% C.L.

Published
2002

3. Atmospheric neutrino induced muons in the MACRO detector

Author

Ronga F, Ambrosio M, Antolini R, Aramo C, Auriemma G, Baldini A, Barbarino GC, Barish BC, Battistoni G, Bellotti R, Bemporad C, Bernardini P, Bilokon H, Bisi V, Bloise C, Bower C, Cafagna F, Calicchio M, Campana D, Carboni M, Castellano M, Cecchini S, Cei F, Chiarella V, Choudhary BC, Coutu S, De Benedictis L, De Cataldo G, Dekhissi H, De Marzo C, De Mitri I, Derkaoui J, De Vincenzi M, Di Credico Alessandra, Erriquez O, Favuzzi C, Forti C, Fusco P, Giacomelli G, Giannini G, Giglietto N, Giorgini M, Grassi M, Gray L, Grillo A, Guarino F, Guarnaccia P, Gustavino C, Habig Alec, Hanson K, Hawthorne A, Heinz R, Huang Y, Iarocci E, Katsavounidis E, Katsavounidis I, Kearns E, Kim H, Kyriazopoulou S, Lamanna E, Lane Charles E, Levin DS, Lipari P, Longley NP, Longo MJ, Maaroufi F, Mancarella G, Mandrioli G, Manzoor S, Margiotta Neri A, Marini A, Martello D, Marzari Chiesa A, Mazziotta MN, Mazzotta C, Michael DG, Mikheyev S, Miller L, Monacelli Piero, Montaruli T, Monteno M, Mufson Stuart L, Musser J, Nicolo D, Nolty R, Okada C, Orth C, Osteria G, Ouchrif M, Palamara O, Patera V, Patrizii L, Pazzi R, Peck CW, Petrera S, Pistilli P, Popa V, Pugliese V, Raino A, Reynoldson J, Rubizzo U, Sanzgiri A, Satriano C, Satta L, Scapparone E, Scholberg K, Sciubba A, Serra Lugaresi P, Severi M, Sioli M, Sitta M, Spinelli P, Spinetti M, Spurio M, Steinberg R, Stone JL, Sulak LR, Surdo A, Tarle G, Togo V, Ugolotti D, Vakili M., BUSSINO, Severino Angelo Maria, Ronga, F, Ambrosio, M, Antolini, R, Aramo, C, Auriemma, G, Baldini, A, Barbarino, Gc, Barish, Bc, Battistoni, G, Bellotti, R, Bemporad, C, Bernardini, P, Bilokon, H, Bisi, V, Bloise, C, Bower, C, Bussino, Severino Angelo Maria, Cafagna, F, Calicchio, M, Campana, D, Carboni, M, Castellano, M, Cecchini, S, Cei, F, Chiarella, V, Choudhary, Bc, Coutu, S, De Benedictis, L, De Cataldo, G, Dekhissi, H, De Marzo, C, De Mitri, I, Derkaoui, J, De Vincenzi, M, Di Credico, Alessandra, Erriquez, O, Favuzzi, C, Forti, C, Fusco, P, Giacomelli, G, Giannini, G, Giglietto, N, Giorgini, M, Grassi, M, Gray, L, Grillo, A, Guarino, F, Guarnaccia, P, Gustavino, C, Habig, Alec, Hanson, K, Hawthorne, A, Heinz, R, Huang, Y, Iarocci, E, Katsavounidis, E, Katsavounidis, I, Kearns, E, Kim, H, Kyriazopoulou, S, Lamanna, E, Lane Charles, E, Levin, D, Lipari, P, Longley, Np, Longo, Mj, Maaroufi, F, Mancarella, G, Mandrioli, G, Manzoor, S, Margiotta Neri, A, Marini, A, Martello, D, Marzari Chiesa, A, Mazziotta, Mn, Mazzotta, C, Michael, Dg, Mikheyev, S, Miller, L, Monacelli, Piero, Montaruli, T, Monteno, M, Mufson Stuart, L, Musser, J, Nicolo, D, Nolty, R, Okada, C, Orth, C, Osteria, G, Ouchrif, M, Palamara, O, Patera, V, Patrizii, L, Pazzi, R, Peck, Cw, Petrera, S, Pistilli, P, Popa, V, Pugliese, V, Raino, A, Reynoldson, J, Rubizzo, U, Sanzgiri, A, Satriano, C, Satta, L, Scapparone, E, Scholberg, K, Sciubba, A, Serra Lugaresi, P, Severi, M, Sioli, M, Sitta, M, Spinelli, P, Spinetti, M, Spurio, M, Steinberg, R, Stone, Jl, Sulak, Lr, Surdo, A, Tarle, G, Togo, V, Ugolotti, D, Vakili, M., F., Ronga, Guarino, Fausto, Barbarino, Giancarlo, and The MACRO, Collaboration

Subjects
Physics, Nuclear and High Energy Physics, Particle physics, cosmic radiation [neutrino], Muon, Physics::Instrumentation and Detectors, Detector, FOS: Physical sciences, Flux, interaction [neutrino nucleon], Atomic and Molecular Physics, and Optics, Bin, High Energy Physics - Experiment, charged current, High Energy Physics - Experiment (hep-ex), High Energy Physics::Experiment, Neutrino, Neutrino oscillation, Event (particle physics), Particle Physics - Experiment, Zenith
Abstract

A measurement of the flux of neutrino-induced muons using the MACRO detector is presented. Different event topologies, corresponding to different neutrino parent energies can be detected. The upward throughgoing muon sample is the larger event sample. The observed upward-throughgoing muons are 26% fewer than expected and the zenith angle distribution does not fit with the expected one. Assuming neutrino oscillations, both measurements suggest maximum mixing and Dm2 of a few times 10-3 eV2. The other samples are due to the internally produced events and to upward-going stopping muons. These data show a regular deficit of observed events in each angular bin, as expected assuming neutrino oscillations with maximum mixing, in agreement with the analysis of the upward-throughgoing muon sample., Comment: 7 pages 6 figures to appear in the proceedings of XVIII International Conference on Neutrino Physics and Astrophysics (Neutrino'98), Takayama, Japan 4-9 June, 1998

Published
1999

4. Neutrino Astronomy with MACRO

Author

Ambrosio M, Antolini R, Assiro R, Auriemma G, Bakari D, Baldini A, Barbarino GC, Barbarito E, Barish BC, Battistoni G, Becherini Y, Bellotti R, Bemporad C, Bernardini P, Bilokon H, Bisi V, Bloise C, Bottazzi E, Bower C, Brigida M, Cafagna F, Calicchio M, Campana D, Candela A, Carboni M, Cecchini S, Cei F, Ceres A, Chiarella V, Choudhary BC, Coutu S, Cozzi M, Creti P, De Cataldo G, Degli Esposti L, Dekhissi H, 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, Perrone, Lorenzo, ON BEHALF OF THE MACRO, Collaboration, Ambrosio, M, Antolini, R, Assiro, R, Auriemma, G, Bakari, D, Baldini, A, Barbarino, Gc, Barbarito, E, Barish, Bc, Battistoni, G, Becherini, Y, Bellotti, R, Bemporad, C, Bernardini, P, Bilokon, H, Bisi, V, Bloise, C, Bottazzi, E, Bower, C, Brigida, M, Bussino, Severino Angelo Maria, Cafagna, F, Calicchio, M, Campana, D, Candela, A, Carboni, M, Cecchini, S, Cei, F, Ceres, A, Chiarella, V, Choudhary, Bc, Coutu, S, Cozzi, M, Creti, P, De Cataldo, G, Degli Esposti, L, Dekhissi, H, 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, D, 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, and Zaccheo, N.

Subjects
Physics, Nuclear and High Energy Physics, Muon, Physics::Instrumentation and Detectors, High-energy astronomy, Astrophysics::High Energy Astrophysical Phenomena, Solar neutrino, Astrophysics, Solar neutrino problem, Atomic and Molecular Physics, and Optics, Neutrino detector, Measurements of neutrino speed, High Energy Physics::Experiment, Neutrino, Neutrino astronomy
Abstract

High energy neutrinos from astrophysical sources can be detected as upward-going muons produced in charged-current interactions with the matter surrounding the detector. We present the results of a search for either a diffuse astrophysical neutrino flux or a point-like source of neutrinos in the sample of upward-going muons gathered by MACRO. We find no evidence for both signals. The muon flux upper limit for the diffuse signal has been set at the level of 1.7 × 10^-14cm^-2 s^-1 sr^-1.

Published
2002

5. Cosmic Ray composition around the knee from EAS electromagnetic and muon data

Author

Ambrosio M, Antolini R, Assiro R, Auriemma G, Bakari D, Baldini A, Barbarino GC, Barbarito E, Barish BC, Battistoni G, Becherini Y, Bellotti R, Bemporad C, Bernardini P, Bilokon H, Bisi V, Bloise C, Bottazzi E, Bower C, Brigida M, Cafagna F, Calicchio M, Campana D, Candela A, Carboni M, Cecchini S, Cei F, Ceres A, Chiarella V, Choudhary BC, Coutu S, Cozzi M, Creti P, De Cataldo G, Degli Esposti L, Dekhissi H, 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, Ambrosio, M, Antolini, R, Assiro, R, Auriemma, G, Bakari, D, Baldini, A, Barbarino, Gc, Barbarito, E, Barish, Bc, Battistoni, G, Becherini, Y, Bellotti, R, Bemporad, C, Bernardini, P, Bilokon, H, Bisi, V, Bloise, C, Bottazzi, E, Bower, C, Brigida, M, Bussino, Severino Angelo Maria, Cafagna, F, Calicchio, M, Campana, D, Candela, A, Carboni, M, Cecchini, S, Cei, F, Ceres, A, Chiarella, V, Choudhary, Bc, Coutu, S, Cozzi, M, Creti, P, De Cataldo, G, Degli Esposti, L, Dekhissi, H, 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, D, 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, and Zaccheo, N.

Subjects
Nuclear physics, Physics, Nuclear and High Energy Physics, Muon, Coincident, EAS-TOP, Cosmic ray, MACRO, Composition (combinatorics), Atomic and Molecular Physics, and Optics
Abstract

We report the analysis of the N ϵ - N μ coincident events collected by the MACRO/EAS-TOP collaboration at the Gran Sasso Laboratories. The result points to a primary composition becoming heavier around the knee of the primary spectrum (in the energy region 10 15 – 10 16 eV). The result is in very good agreement with the measurements of EAS-TOP alone at the surface, wich detects muons with energy E μ > 1 GeV and uses the same (QGSJET) interaction model.

Published
2002

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