We give a brief description of the purpose of the LHCf experiment, detectors and their performance, and what has been done in the first year experiment. A short summary of results at root s = 900 GeV is given although the energy is not an "intrinsic" LHC energy. Since detailed results at root s = 7 TeV will appear soon elsewhere, here we limit ourselves to giving also a brief account of what will come in that paper.

First year results from LHCf / K. Kasahara, M. Nakai, Y. Shimizu, T. Suzuki, S. Torii, K. Yoshida, T. Tamura, K. Fukatsu, Y. Itow, K. Kawade, T. Mase, K. Masuda, Y. Matsubara, G. Mitsuka, T. Sako, K. Suzuki, K. Taki, H. Menjo, Y. Muraki, M. Haguenauer, et al.. - In: AIP CONFERENCE PROCEEDINGS. - ISSN 0094-243X. - STAMPA. - 1367:(2011), pp. 58-63. (International Symposium on the Recent Progress of Ultra-High Energy Cosmic Ray Observation, UHECR2010 ) [10.1063/1.3628716].

First year results from LHCf

ADRIANI, OSCAR;BONECHI, LORENZO;BONGI, MASSIMO;D'ALESSANDRO, RAFFAELLO;
2011

Abstract

We give a brief description of the purpose of the LHCf experiment, detectors and their performance, and what has been done in the first year experiment. A short summary of results at root s = 900 GeV is given although the energy is not an "intrinsic" LHC energy. Since detailed results at root s = 7 TeV will appear soon elsewhere, here we limit ourselves to giving also a brief account of what will come in that paper.
2011
Proceedings of International Symposium on the Recent Progress of Ultra-High Energy Cosmic Ray Observation, UHECR2010
International Symposium on the Recent Progress of Ultra-High Energy Cosmic Ray Observation, UHECR2010
K. Kasahara;M. Nakai;Y. Shimizu;T. Suzuki;S. Torii;K. Yoshida;T. Tamura;K. Fukatsu;Y. Itow;K. Kawade;T. Mase;K. Masuda;Y. Matsubara;G. M...espandi
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Utilizza questo identificatore per citare o creare un link a questa risorsa: https://hdl.handle.net/2158/645215
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