ar X iv : h ep - e x / 98 07 00 6 v 1 7 J ul 1 99 8 Observation of the Shadowing of Cosmic Rays by the Moon using a Deep Underground Detector
نویسندگان
چکیده
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, B. C. Choudhary, S. Coutu , L. De Benedictis, G. De Cataldo, H. Dekhissi , C. De Marzo, I. De Mitri, J. Derkaoui , M. De Vincenzi, A. Di Credico , O. Erriquez, C. Favuzzi, C. Forti, P. Fusco, G. Giacomelli , G. Giannini , N. Giglietto, M. Giorgini , M. Grassi , L. Gray , A. Grillo , F. Guarino , P. Guarnaccia, C. Gustavino , A. Habig , K. Hanson , R. Heinz , Y. Huang, E. Iarocci 6,g , E. Katsavounidis, E. Kearns , H. Kim, 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, C. Orth , G. Osteria , M. Ouchrif , O. Palamara , V. Patera 6,g , L. Patrizii , R. Pazzi , C. W. Peck, S. Petrera , P. Pistilli , V. Popa , V. Pugliese , A. Rainò, J. Reynoldson , F. Ronga , U. Rubizzo , C. Satriano , L. Satta , E. Scapparone , K. Scholberg , A. Sciubba 6,g , 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. Tarlè, V. Togo , D. Ugolotti , M. Vakili , C. W. Walter , and R. Webb .
منابع مشابه
ar X iv : h ep - p h / 98 07 21 1 v 3 8 J ul 1 99 8 Challenges of Nuclear Shadowing in DIS
Nuclear shadowing in DIS at moderately small x is suppressed by the nuclear formfactor and depends on the effective mass of a hadronic fluctuation of the virtual photon. We propose a solution to the problems (i) of how to combine a definite transverse size of the fluctuation with a definite effective mass, and (ii) of how to include the nuclear formfactor in the higher multiple scattering terms...
متن کاملar X iv : h ep - p h / 98 07 21 1 v 1 1 J ul 1 99 8 Challenges of Nuclear Shadowing in DIS
Nuclear shadowing in DIS at moderately small x is suppressed by the nuclear formfactor and depends on the effective mass of a hadronic fluctuation of the virtual photon. We propose a solution to the problems (i) of how to combine a definite transverse size of the fluctuation with a definite effective mass, and (ii) of how to include the nuclear formfactor in the higher multiple scattering terms...
متن کاملar X iv : h ep - p h / 98 07 21 1 v 2 3 J ul 1 99 8 Challenges of Nuclear Shadowing in DIS
Nuclear shadowing in DIS at moderately small x is suppressed by the nuclear formfactor and depends on the effective mass of a hadronic fluctuation of the virtual photon. We propose a solution to the problems (i) of how to combine a definite transverse size of the fluctuation with a definite effective mass, and (ii) of how to include the nuclear formfactor in the higher multiple scattering terms...
متن کاملar X iv : h ep - p h / 98 07 25 2 v 1 6 J ul 1 99 8 Studying thermodynamics in heavy ion collisions
We discuss the possibility to measure entropy of the system created in heavy ion collisions using the Ma coincidence method.
متن کاملar X iv : h ep - e x / 99 05 01 8 v 1 1 3 M ay 1 99 9 HE . 3 . 2 . 13 Transition Radiation Detector in MACRO
The MACRO detector is located in the Gran Sasso Laboratory. MACRO's overburden varies from 3150 to 7000 hg/cm 2. A transition radiation detector (TRD) has been added to the MACRO detector in order to measure the residual energy of muons entering MACRO, i.e. the energy they have after passing through the Gran Sasso's rock overburden. The TRD consists of three identical modules with a total horiz...
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تاریخ انتشار 2013