Abstract The absolute muon flux between 20 and 3000 GeV is measured with the L3 magnetic muon spectrometer for zenith angles ranging from 0? to 58?. Due to the large exposure of about 150 m2 sr d, and the excellent momentum resolution of the L3 muon chambers, a precision of 2.3% at 150 GeV in the vertical direction is achieved. The ratio of positive to negative muons is studied between 20 and 500 GeV, and the average vertical muon charge ratio is found to be 1.285 ± 0.003(stat.)± 0.019(syst.). ? 2004 Elsevier B.V. All rights reserved.
Measurement of the atmospheric muon spectrum from 20 to 3000 GeV / Achard, P; Adriani, O; AGUILAR BENITEZ, M; VAN DEN AKKER, M; Alcaraz, J; Alemanni, G; Allaby, J; Aloisio, A; Alviggi, Mg; Anderhub, H; Andreev, Vp; Anselmo, F; Arefiev, A; Azemoon, T; Aziz, T; Bagnaia, Paolo; Bajo, A; Baksay, G; Baksay, L; Bahr, J; Baldew, Sv; Banerjee, S; Banerjee, S; Barczyk, A; Barillere, R; Bartalini, P; Batalova, N; Battiston, R; Bay, A; Becattini, F; Becker, U; Behner, F; Bellucci, L; Berbeco, R; Berdugo, J; Berges, P; Bertucci, B; Betev, Bl; Biasini, M; Biglietti, M; Biland, A; Blaising, Jj; Blyth, Sc; Bobbink, Gj; Bohm, A; Boldizsar, L; Borgia, Bruno; Bottai, S; Bourilkov, D; Bourquin, M; Braccini, S; Branson, Jg; Brochu, F; Burger, Jd; Burger, Wj; Cai, Xd; Capell, M; Romeo, Gc; Carlino, G; Cartacci, A; Casaus, J; Cavallari, F; Cavallo, N; Cecchi, C; Cerrada, M; Chamizo, M; Chiarusi, T; Chang, Yh; Chemarin, M; Chen, A; Chen, G; Chen, Gm; Chen, Hf; Chen, Hs; Chiefari, G; Cifarelli, L; Cindolo, F; Clare, I; Clare, R; Coignet, G; Colino, N; Costantini, S; DE LA CRUZ, B; Cucciarelli, S; VAN DALEN, Ja; DE ASMUNDIS, R; Deglon, P; Debreczeni, J; Degre, A; Dehmelt, K; Deiters, K; DELLA VOLPE, D; Delmeire, E; Denes, P; Denotaristefani, F; DE SALVO, A; Diemoz, M; Dierckxsens, M; Ding, Lk; Dionisi, Carlo; Dittmar, M; Doria, A; Dova, Mt; Duchesneau, D; Duda, M; Duran, I; Echenard, B; Eline, A; EL HAGE, A; EL MAMOUNI, H; Engler, A; Eppling, Fj; Extermann, P; Faber, G; Falagan, Ma; Falciano, S; Favara, A; Fay, J; Fedin, O; Felcini, M; Ferguson, T; Fesefeldt, H; Fiandrini, E; Field, Jh; Filthaut, F; Fisher, W; Fisk, I; Forconi, G; Freudenreich, K; Furetta, C; Galaktionov, Y; Ganguli, Sn; GARCIA ABIA, P; Gataullin, M; Gentile, Simonetta; Giagu, Stefano; Gong, Zf; Grabosch, Hj; Grenier, G; Grimm, O; Groenstege, H; Gruenewald, Mw; Guida, M; Guo, Yn; Gupta, S; Gupta, Vk; Gurtu, A; Gutay, Lj; Haas, D; Haller, C; Hatzifotiadou, D; He, Z; Hebbeker, T; Herve, A; Hirschfelder, J; Hofer, H; Hofer, H; Hohlmann, M; Holzner, G; Hou, Sr; Huo, Ax; Hu, Y; Ito, N; Jin, Bn; Jing, Cl; Jones, Lw; DE JONG, P; JOSA MUTUBERRIA, I; Kantserov, V; Kaur, M; Kawakami, S; KIENZLE FOCACCI, Mn; Kim, Jk; Kirkby, J; Kittel, W; Klimentov, A; Konig, Ac; Kok, E; Korn, A; Kopal, M; Koutsenko, V; Kraber, M; Kuang, Hh; Kraemer, Rw; Kruger, A; Kuijpers, J; Kunin, A; DE GUEVARA, Pl; Laktineh, I; Landi, G; Lebeau, M; Lebedev, A; Lebrun, P; Lecomte, P; Lecoq, P; LE COULTRE, P; LE GOFF, Jm; Lei, Y; Leich, H; Leiste, R; Levtchenko, M; Levtchenko, P; Li, C; Li, L; Li, Zc; Likhoded, S; Lin, Ch; Lin, Wt; Linde, Fl; Lista, L; Liu, Za; Lohmann, W; Longo, Egidio; Lu, Y; Luci, Claudio; Luminari, L; Lustermann, W; Ma, Wg; Ma, Xh; Ma, Yq; Malgeri, L; Malinin, A; Mana, C; Mans, J; Martin, Jp; Marzano, F; Mazumdar, K; Mcneil, Rr; Mele, S; Meng, Xw; Merola, L; Meschini, M; Metzger, Wj; Mihul, A; VAN MIL, A; Milcent, H; Mirabelli, G; Mnich, J; Mohanty, Gb; Monteleoni, B; Muanza, Gs; Muijs, Ajm; Musicar, B; Musy, M; Nagy, S; Nahnhauer, R; Naumov, Va; Natale, S; Napolitano, M; NESSI TEDALDI, F; Newman, H; Nisati, A; Novak, T; Nowak, H; Ofierzynski, R; Organtini, Giovanni; Pal, I; Palomares, C; Paolucci, P; Paramatti, Riccardo; Parriaud, Jf; Passaleva, G; Patricelli, S; Paul, T; Pauluzzi, M; Paus, C; Pauss, F; Pedace, M; Pensotti, S; PERRET GALLIX, D; Petersen, B; Piccolo, D; Pierella, F; Pieri, M; Pioppi, M; Piroue, Pa; Pistolesi, E; Plyaskin, V; Pohl, M; Pojidaev, V; Pothier, J; Prokofiev, D; Quartieri, J; Qing, Cr; RAHAL CALLOT, G; Rahaman, Ma; Raics, P; Raja, N; Ramelli, R; Rancoita, Pg; Ranieri, R; Raspereza, A; Ravindran, Kc; Razis, P; Ren, D; Rescigno, M; Reucroft, S; Rewiersma, P; Riemann, S; Riles, K; Roe, Bp; Rojkov, A; Romero, L; Rosca, A; Rosemann, C; Rosenbleck, C; ROSIER LEES, S; Roth, S; Rubio, Ja; Ruggiero, G; Rykaczewski, H; Saidi, R; Sakharova, A; Saremi, S; Sarkar, S; Salicio, J; Sanchez, E; Schafer, C; Schegelsky, V; Schmitt, V; Schoeneich, B; Schopper, H; Schotanus, Dj; Sciacca, C; Servoli, L; Shen, Cq; Shevchenko, S; Shivarov, N; Shoutko, V; Shumilov, E; Shvorob, A; Son, D; Souga, C; Spillantini, P; Steuer, M; Stickland, Dp; Stoyanov, B; Straessner, A; Sudhakar, K; Sulanke, H; Sultanov, G; Sun, Lz; Sushkov, S; Suter, H; Swain, Jd; Szillasi, Z; Tang, Xw; Tarjan, P; Tauscher, L; Taylor, L; Tellili, B; Teyssier, D; Timmermans, C; Ting, Scc; Ting, Sm; Tonwar, Sc; Toth, J; Trowitzsch, G; Tully, C; Tung, Kl; Ulbricht, J; Unger, M; Valente, E; Verkooijen, H; VAN DE WALLE, Rt; Vasquez, R; Veszpremi, V; Vesztergombi, G; Vetlitsky, I; Vicinanza, D; Viertel, G; Villa, S; Vivargent, M; Vlachos, S; Vodopianov, I; Vogel, H; Vogt, H; Vorobiev, I; Vorobyov, Aa; Wadhwa, M; Wang, Rg; Wang, Q; Wang, Xl; Wang, Xw; Wang, Zm; Weber, M; VAN WIJK, R; Wijnen, Tam; Wilkens, H; Wynhoff, S; Xia, L; Xu, Yp; Xu, Js; Xu, Zz; Yamamoto, J; Yang, Bz; Yang, Cg; Yang, Hj; Yang, M; Yang, Xe; Yao, Zg; Yeh, Sc; Yu, Zq; Zalite, A; Zalite, Y; Zhang, C; Zhang, F; Zhang, J; Zhang, S; Zhang, Zp; Zhao, J; Zhou, Sj; Zhu, Gy; Zhu, Ry; Zhuang, Hl; Zhu, Qq; Zichichi, A; Zimmermann, B; Zoller, M; Zwart, Anm. - In: PHYSICS LETTERS. SECTION B. - ISSN 0370-2693. - 598:(2004), pp. 15-32. [10.1016/j.physletb.2004.08.003]
Measurement of the atmospheric muon spectrum from 20 to 3000 GeV
ACHARD P; ADRIANI O; AGUILAR BENITEZ M; VAN DEN AKKER M; ALCARAZ J; ALEMANNI G; ALLABY J; ALOISIO A; ALVIGGI MG; ANDERHUB H; ANDREEV VP; ANSELMO F; AREFIEV A; AZEMOON T; AZIZ T; BAGNAIA, Paolo ;BAJO A; BAKSAY G; BAKSAY L; BAHR J; BALDEW SV; BANERJEE S; BANERJEE S; BARCZYK A; BARILLERE R; BARTALINI P; BATALOVA N; BATTISTON R; BAY A; BECATTINI F; BECKER U; BEHNER F; BELLUCCI L; BERBECO R; BERDUGO J; BERGES P; BERTUCCI B; BETEV BL; BIASINI M; BIGLIETTI M; BILAND A; BLAISING JJ; BLYTH SC; BOBBINK GJ; BOHM A; BOLDIZSAR L; BORGIA, BRUNO ;BOTTAI S; BOURILKOV D; BOURQUIN M; BRACCINI S; BRANSON JG; BROCHU F; BURGER JD; BURGER WJ; CAI XD; CAPELL M; ROMEO GC; CARLINO G; CARTACCI A; CASAUS J; CAVALLARI F; CAVALLO N; CECCHI C; CERRADA M; CHAMIZO M; CHIARUSI T; CHANG YH; CHEMARIN M; CHEN A; CHEN G; CHEN GM; CHEN HF; CHEN HS; CHIEFARI G; CIFARELLI L; CINDOLO F; CLARE I; CLARE R; COIGNET G; COLINO N; COSTANTINI S; DE LA CRUZ B; CUCCIARELLI S; VAN DALEN JA; DE ASMUNDIS R; DEGLON P; DEBRECZENI J; DEGRE A; DEHMELT K; DEITERS K; DELLA VOLPE D; DELMEIRE E; DENES P; DENOTARISTEFANI F; DE SALVO A; DIEMOZ M; DIERCKXSENS M; DING LK; DIONISI, Carlo ;DITTMAR M; DORIA A; DOVA MT; DUCHESNEAU D; DUDA M; DURAN I; ECHENARD B; ELINE A; EL HAGE A; EL MAMOUNI H; ENGLER A; EPPLING FJ; EXTERMANN P; FABER G; FALAGAN MA; FALCIANO S; FAVARA A; FAY J; FEDIN O; FELCINI M; FERGUSON T; FESEFELDT H; FIANDRINI E; FIELD JH; FILTHAUT F; FISHER W; FISK I; FORCONI G; FREUDENREICH K; FURETTA C; GALAKTIONOV Y; GANGULI SN; GARCIA ABIA P; GATAULLIN M; GENTILE, Simonetta ;GIAGU, Stefano ;GONG ZF; GRABOSCH HJ; GRENIER G; GRIMM O; GROENSTEGE H; GRUENEWALD MW; GUIDA M; GUO YN; GUPTA S; GUPTA VK; GURTU A; GUTAY LJ; HAAS D; HALLER C; HATZIFOTIADOU D; HE Z; HEBBEKER T; HERVE A; HIRSCHFELDER J; HOFER H; HOFER H; HOHLMANN M; HOLZNER G; HOU SR; HUO AX; HU Y; ITO N; JIN BN; JING CL; JONES LW; DE JONG P; JOSA MUTUBERRIA I; KANTSEROV V; KAUR M; KAWAKAMI S; KIENZLE FOCACCI MN; KIM JK; KIRKBY J; KITTEL W; KLIMENTOV A; KONIG AC; KOK E; KORN A; KOPAL M; KOUTSENKO V; KRABER M; KUANG HH; KRAEMER RW; KRUGER A; KUIJPERS J; KUNIN A; DE GUEVARA PL; LAKTINEH I; LANDI G; LEBEAU M; LEBEDEV A; LEBRUN P; LECOMTE P; LECOQ P; LE COULTRE P; LE GOFF JM; LEI Y; LEICH H; LEISTE R; LEVTCHENKO M; LEVTCHENKO P; LI C; LI L; LI ZC; LIKHODED S; LIN CH; LIN WT; LINDE FL; LISTA L; LIU ZA; LOHMANN W; LONGO, Egidio ;LU Y; LUCI, Claudio ;LUMINARI L; LUSTERMANN W; MA WG; MA XH; MA YQ; MALGERI L; MALININ A; MANA C; MANS J; MARTIN JP; MARZANO F; MAZUMDAR K; MCNEIL RR; MELE S; MENG XW; MEROLA L; MESCHINI M; METZGER WJ; MIHUL A; VAN MIL A; MILCENT H; MIRABELLI G; MNICH J; MOHANTY GB; MONTELEONI B; MUANZA GS; MUIJS AJM; MUSICAR B; MUSY M; NAGY S; NAHNHAUER R; NAUMOV VA; NATALE S; NAPOLITANO M; NESSI TEDALDI F; NEWMAN H; NISATI A; NOVAK T; NOWAK H; OFIERZYNSKI R; ORGANTINI, Giovanni ;PAL I; PALOMARES C; PAOLUCCI P; PARAMATTI, Riccardo ;PARRIAUD JF; PASSALEVA G; PATRICELLI S; PAUL T; PAULUZZI M; PAUS C; PAUSS F; PEDACE M; PENSOTTI S; PERRET GALLIX D; PETERSEN B; PICCOLO D; PIERELLA F; PIERI M; PIOPPI M; PIROUE PA; PISTOLESI E; PLYASKIN V; POHL M; POJIDAEV V; POTHIER J; PROKOFIEV D; QUARTIERI J; QING CR; RAHAL CALLOT G; RAHAMAN MA; RAICS P; RAJA N; RAMELLI R; RANCOITA PG; RANIERI R; RASPEREZA A; RAVINDRAN KC; RAZIS P; REN D; RESCIGNO M; REUCROFT S; REWIERSMA P; RIEMANN S; RILES K; ROE BP; ROJKOV A; ROMERO L; ROSCA A; ROSEMANN C; ROSENBLECK C; ROSIER LEES S; ROTH S; RUBIO JA; RUGGIERO G; RYKACZEWSKI H; SAIDI R; SAKHAROVA A; SAREMI S; SARKAR S; SALICIO J; SANCHEZ E; SCHAFER C; SCHEGELSKY V; SCHMITT V; SCHOENEICH B; SCHOPPER H; SCHOTANUS DJ; SCIACCA C; SERVOLI L; SHEN CQ; SHEVCHENKO S; SHIVAROV N; SHOUTKO V; SHUMILOV E; SHVOROB A; SON D; SOUGA C; SPILLANTINI P; STEUER M; STICKLAND DP; STOYANOV B; STRAESSNER A; SUDHAKAR K; SULANKE H; SULTANOV G; SUN LZ; SUSHKOV S; SUTER H; SWAIN JD; SZILLASI Z; TANG XW; TARJAN P; TAUSCHER L; TAYLOR L; TELLILI B; TEYSSIER D; TIMMERMANS C; TING SCC; TING SM; TONWAR SC; TOTH J; TROWITZSCH G; TULLY C; TUNG KL; ULBRICHT J; UNGER M; VALENTE E; VERKOOIJEN H; VAN DE WALLE RT; VASQUEZ R; VESZPREMI V; VESZTERGOMBI G; VETLITSKY I; VICINANZA D; VIERTEL G; VILLA S; VIVARGENT M; VLACHOS S; VODOPIANOV I; VOGEL H; VOGT H; VOROBIEV I; VOROBYOV AA; WADHWA M; WANG RG; WANG Q; WANG XL; WANG XW; WANG ZM; WEBER M; VAN WIJK R; WIJNEN TAM; WILKENS H; WYNHOFF S; XIA L; XU YP; XU JS; XU ZZ; YAMAMOTO J; YANG BZ; YANG CG; YANG HJ; YANG M; YANG XE; YAO ZG; YEH SC; YU ZQ; ZALITE A; ZALITE Y; ZHANG C; ZHANG F; ZHANG J; ZHANG S; ZHANG ZP; ZHAO J; ZHOU SJ; ZHU GY; ZHU RY; ZHUANG HL; ZHU QQ; ZICHICHI A; ZIMMERMANN B; ZOLLER M; ZWART ANM
2004
Abstract
Abstract The absolute muon flux between 20 and 3000 GeV is measured with the L3 magnetic muon spectrometer for zenith angles ranging from 0? to 58?. Due to the large exposure of about 150 m2 sr d, and the excellent momentum resolution of the L3 muon chambers, a precision of 2.3% at 150 GeV in the vertical direction is achieved. The ratio of positive to negative muons is studied between 20 and 500 GeV, and the average vertical muon charge ratio is found to be 1.285 ± 0.003(stat.)± 0.019(syst.). ? 2004 Elsevier B.V. All rights reserved.
Citazione
Measurement of the atmospheric muon spectrum from 20 to 3000 GeV / Achard, P; Adriani, O; AGUILAR BENITEZ, M; VAN DEN AKKER, M; Alcaraz, J; Alemanni, G; Allaby, J; Aloisio, A; Alviggi, Mg; Anderhub, H; Andreev, Vp; Anselmo, F; Arefiev, A; Azemoon, T; Aziz, T; Bagnaia, Paolo; Bajo, A; Baksay, G; Baksay, L; Bahr, J; Baldew, Sv; Banerjee, S; Banerjee, S; Barczyk, A; Barillere, R; Bartalini, P; Batalova, N; Battiston, R; Bay, A; Becattini, F; Becker, U; Behner, F; Bellucci, L; Berbeco, R; Berdugo, J; Berges, P; Bertucci, B; Betev, Bl; Biasini, M; Biglietti, M; Biland, A; Blaising, Jj; Blyth, Sc; Bobbink, Gj; Bohm, A; Boldizsar, L; Borgia, Bruno; Bottai, S; Bourilkov, D; Bourquin, M; Braccini, S; Branson, Jg; Brochu, F; Burger, Jd; Burger, Wj; Cai, Xd; Capell, M; Romeo, Gc; Carlino, G; Cartacci, A; Casaus, J; Cavallari, F; Cavallo, N; Cecchi, C; Cerrada, M; Chamizo, M; Chiarusi, T; Chang, Yh; Chemarin, M; Chen, A; Chen, G; Chen, Gm; Chen, Hf; Chen, Hs; Chiefari, G; Cifarelli, L; Cindolo, F; Clare, I; Clare, R; Coignet, G; Colino, N; Costantini, S; DE LA CRUZ, B; Cucciarelli, S; VAN DALEN, Ja; DE ASMUNDIS, R; Deglon, P; Debreczeni, J; Degre, A; Dehmelt, K; Deiters, K; DELLA VOLPE, D; Delmeire, E; Denes, P; Denotaristefani, F; DE SALVO, A; Diemoz, M; Dierckxsens, M; Ding, Lk; Dionisi, Carlo; Dittmar, M; Doria, A; Dova, Mt; Duchesneau, D; Duda, M; Duran, I; Echenard, B; Eline, A; EL HAGE, A; EL MAMOUNI, H; Engler, A; Eppling, Fj; Extermann, P; Faber, G; Falagan, Ma; Falciano, S; Favara, A; Fay, J; Fedin, O; Felcini, M; Ferguson, T; Fesefeldt, H; Fiandrini, E; Field, Jh; Filthaut, F; Fisher, W; Fisk, I; Forconi, G; Freudenreich, K; Furetta, C; Galaktionov, Y; Ganguli, Sn; GARCIA ABIA, P; Gataullin, M; Gentile, Simonetta; Giagu, Stefano; Gong, Zf; Grabosch, Hj; Grenier, G; Grimm, O; Groenstege, H; Gruenewald, Mw; Guida, M; Guo, Yn; Gupta, S; Gupta, Vk; Gurtu, A; Gutay, Lj; Haas, D; Haller, C; Hatzifotiadou, D; He, Z; Hebbeker, T; Herve, A; Hirschfelder, J; Hofer, H; Hofer, H; Hohlmann, M; Holzner, G; Hou, Sr; Huo, Ax; Hu, Y; Ito, N; Jin, Bn; Jing, Cl; Jones, Lw; DE JONG, P; JOSA MUTUBERRIA, I; Kantserov, V; Kaur, M; Kawakami, S; KIENZLE FOCACCI, Mn; Kim, Jk; Kirkby, J; Kittel, W; Klimentov, A; Konig, Ac; Kok, E; Korn, A; Kopal, M; Koutsenko, V; Kraber, M; Kuang, Hh; Kraemer, Rw; Kruger, A; Kuijpers, J; Kunin, A; DE GUEVARA, Pl; Laktineh, I; Landi, G; Lebeau, M; Lebedev, A; Lebrun, P; Lecomte, P; Lecoq, P; LE COULTRE, P; LE GOFF, Jm; Lei, Y; Leich, H; Leiste, R; Levtchenko, M; Levtchenko, P; Li, C; Li, L; Li, Zc; Likhoded, S; Lin, Ch; Lin, Wt; Linde, Fl; Lista, L; Liu, Za; Lohmann, W; Longo, Egidio; Lu, Y; Luci, Claudio; Luminari, L; Lustermann, W; Ma, Wg; Ma, Xh; Ma, Yq; Malgeri, L; Malinin, A; Mana, C; Mans, J; Martin, Jp; Marzano, F; Mazumdar, K; Mcneil, Rr; Mele, S; Meng, Xw; Merola, L; Meschini, M; Metzger, Wj; Mihul, A; VAN MIL, A; Milcent, H; Mirabelli, G; Mnich, J; Mohanty, Gb; Monteleoni, B; Muanza, Gs; Muijs, Ajm; Musicar, B; Musy, M; Nagy, S; Nahnhauer, R; Naumov, Va; Natale, S; Napolitano, M; NESSI TEDALDI, F; Newman, H; Nisati, A; Novak, T; Nowak, H; Ofierzynski, R; Organtini, Giovanni; Pal, I; Palomares, C; Paolucci, P; Paramatti, Riccardo; Parriaud, Jf; Passaleva, G; Patricelli, S; Paul, T; Pauluzzi, M; Paus, C; Pauss, F; Pedace, M; Pensotti, S; PERRET GALLIX, D; Petersen, B; Piccolo, D; Pierella, F; Pieri, M; Pioppi, M; Piroue, Pa; Pistolesi, E; Plyaskin, V; Pohl, M; Pojidaev, V; Pothier, J; Prokofiev, D; Quartieri, J; Qing, Cr; RAHAL CALLOT, G; Rahaman, Ma; Raics, P; Raja, N; Ramelli, R; Rancoita, Pg; Ranieri, R; Raspereza, A; Ravindran, Kc; Razis, P; Ren, D; Rescigno, M; Reucroft, S; Rewiersma, P; Riemann, S; Riles, K; Roe, Bp; Rojkov, A; Romero, L; Rosca, A; Rosemann, C; Rosenbleck, C; ROSIER LEES, S; Roth, S; Rubio, Ja; Ruggiero, G; Rykaczewski, H; Saidi, R; Sakharova, A; Saremi, S; Sarkar, S; Salicio, J; Sanchez, E; Schafer, C; Schegelsky, V; Schmitt, V; Schoeneich, B; Schopper, H; Schotanus, Dj; Sciacca, C; Servoli, L; Shen, Cq; Shevchenko, S; Shivarov, N; Shoutko, V; Shumilov, E; Shvorob, A; Son, D; Souga, C; Spillantini, P; Steuer, M; Stickland, Dp; Stoyanov, B; Straessner, A; Sudhakar, K; Sulanke, H; Sultanov, G; Sun, Lz; Sushkov, S; Suter, H; Swain, Jd; Szillasi, Z; Tang, Xw; Tarjan, P; Tauscher, L; Taylor, L; Tellili, B; Teyssier, D; Timmermans, C; Ting, Scc; Ting, Sm; Tonwar, Sc; Toth, J; Trowitzsch, G; Tully, C; Tung, Kl; Ulbricht, J; Unger, M; Valente, E; Verkooijen, H; VAN DE WALLE, Rt; Vasquez, R; Veszpremi, V; Vesztergombi, G; Vetlitsky, I; Vicinanza, D; Viertel, G; Villa, S; Vivargent, M; Vlachos, S; Vodopianov, I; Vogel, H; Vogt, H; Vorobiev, I; Vorobyov, Aa; Wadhwa, M; Wang, Rg; Wang, Q; Wang, Xl; Wang, Xw; Wang, Zm; Weber, M; VAN WIJK, R; Wijnen, Tam; Wilkens, H; Wynhoff, S; Xia, L; Xu, Yp; Xu, Js; Xu, Zz; Yamamoto, J; Yang, Bz; Yang, Cg; Yang, Hj; Yang, M; Yang, Xe; Yao, Zg; Yeh, Sc; Yu, Zq; Zalite, A; Zalite, Y; Zhang, C; Zhang, F; Zhang, J; Zhang, S; Zhang, Zp; Zhao, J; Zhou, Sj; Zhu, Gy; Zhu, Ry; Zhuang, Hl; Zhu, Qq; Zichichi, A; Zimmermann, B; Zoller, M; Zwart, Anm. - In: PHYSICS LETTERS. SECTION B. - ISSN 0370-2693. - 598:(2004), pp. 15-32. [10.1016/j.physletb.2004.08.003]
Non ci sono file associati a questo prodotto.
I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
Sei sicuro che questo prodotto debba essere cancellato?
Il report seguente simula gli indicatori relativi alla propria produzione scientifica in relazione alle soglie ASN 2023-2025 del proprio SC/SSD. Si ricorda che il superamento dei valori soglia (almeno 2 su 3) è requisito necessario ma non sufficiente al conseguimento dell'abilitazione.
