The measurement of upward going muons using the MACRO detector

✍ Scribed by T. Montaruli; M. Ambrosio; R. Antolini; C. Aramo; G. Auriemma; A. Baldini; G.C. Barbarino; B.C. Barish; G. Battistoni; R. Bellotti; C. Bemporad; P. Bernardini; H. Bilokon; V. Bisi; C. Bloise; C. Bower; S. Bussino; F. Cafagna; M. Calicchio; D. Campana; M. Carboni; M. Castellano; S. Cecchini; F. Cei; V. Chiarella; S. Coutu; G. Cunti; L. De Benedictis; G. De Cataldo; H. Dekhissi; C. De Marzo; I. De Mitri; M. De Vincenzi; A. Di Credico; O. Erriquez; C. Favuzzi; C. Forti; P. Fusco; G. Giacomelli; G. Giannini; N. Giglietto; M. Grassi; L. Gray; A. Grillo; F. Guarino; P. Guarnaccia; C. Gustavino; A. Habig; K. Hanson; A. Hawthorne; R. Heinz; E. Iarocci; E. Katsavounidis; E. Kearns; S. Kyriazopoulou; E. Lamanna; C. Lane; D.S. Levin; P. Lipari; N.P. Longley; M.J. Longo; F. Maaroufi; G. Mancarella; G. Mandrioli; S. Manzoor; A. Margiotta Neri; A. Marini; D. Martello; A. Marzari-Chiesa; M.N. Mazziotta; C. Mazzotta; D.G. Michael; S. Mikheyev; L. Miller; P. Monacelli; T. Montaruli; M. Monteno; S. Mufson; J. Musser; D. Nicoló; R. Nolty; C. Okada; C. Orth; G. Osteria; O. Palamara; V. Patera; L. Patrizii; R. Pazzi; C.W. Peck; S. Petrera; P. Pistilli; V. Popa; V. Pugliese; A. Rainó; J. Reynoldson; F. Ronga; U. Rubizzo; A. Sanzgiri; C. Satriano; L. Satta; E. Scapparone; K. Scholberg; A. Sciubba; P. Serra-Lugaresi; M. Severi; M. Sioli; M. Sitta; P. Spinelli; M. Spinetti; M. Spurio; R. Steinberg; J.L. Stone; L.R. Sulak; A. Surdo; G. Tarlé; V. Togo; C.W. Walter; R. Webb

• Publisher: Elsevier Science
• Year: 1999
• Tongue: English
• Weight: 409 KB
• Volume: 70
• Category: Article
• ISSN: 0920-5632
• DOI: 10.1016/s0920-5632(98)00454-x

✦ Synopsis

The upward-going muon flux (Ep > 1 GeV) has been measured with the underground detector MACRO at LNGS. The total number of measured events is compatible at the 8% c.1. with the expected one. Moreover, the zenith angular distribution of the measured flux does not match the expectation showing a deficit in the vertical direction where the apparatus performance is best known. Assuming an oscillation hyphotesis with parameters in the range recently suggested to solve the atmospheric neutrino problem, the agreement increases, but not significantly. The results of an indirect dark matter search for a signal of WIMPS from the core of the Sun and of the Earth are given. Neutrino astronomy with MACRO is giving interesting results regarding possible high energy neutrino emission from pointlike sources and coincidences of neutrino events with -y-ray bursts.