| Published Articles | |
| Title | Latest LHCf physics results |
| Author(s) | Adriani, O (INFN, Florence ; Florence U.) ; Berti, E (INFN, Florence ; Florence U.) ; Bonechi, L (INFN, Florence) ; Bongi, M (INFN, Florence ; Florence U.) ; Castellini, G (INFN, Florence ; IFAC, Florence) ; D'Alessandro, R (INFN, Florence ; Florence U.) ; Del Prete, M (INFN, Florence ; Florence U.) ; Haguenauer, M (Unlisted, FR) ; Itow, Y (Nagoya U., Solar-Terrestrial Environ. Lab. ; KMI, Nagoya) ; Kasahara, K (Waseda U., RISE) ; Kawade, K (Nagoya U., Solar-Terrestrial Environ. Lab.) ; Makino, Y (Nagoya U., Solar-Terrestrial Environ. Lab.) ; Masuda, K (Nagoya U., Solar-Terrestrial Environ. Lab.) ; Matsubayashi, E (Nagoya U., Solar-Terrestrial Environ. Lab.) ; Menjo, H (Nagoya U.) ; Mitsuka, G (Florence U. ; Nagoya U., Solar-Terrestrial Environ. Lab.) ; Muraki, Y (Nagoya U., Solar-Terrestrial Environ. Lab.) ; Papini, P (INFN, Florence) ; Perrot, A -L (CERN) ; Pfeiffer, D (CERN) ; Ricciarini, S (INFN, Florence ; IFAC, Florence) ; Sako, T (Nagoya U., Solar-Terrestrial Environ. Lab. ; KMI, Nagoya) ; Sakurai, N (KMI, Nagoya) ; Suzuki, T (Waseda U., RISE) ; Tamura, T (Senshu U., Kanagawa) ; Tiberio, A (INFN, Florence ; Florence U.) ; Torii, S (Waseda U., RISE) ; Tricomi, A (INFN, Catania ; Catania U.) ; Turner, W C (LBNL, Berkeley) |
| Publication | 2016 |
| Number of pages | 5 |
| In: | Nucl. Part. Phys. Proc. 273-275 (2016) 2073-2077 |
| In: | 37th International Conference on High Energy Physics, Valencia, Spain, 2 - 9 Jul 2014, pp.2073-2077 |
| DOI | 10.1016/j.nuclphysbps.2015.09.335 |
| Subject category | Particle Physics - Experiment |
| Accelerator/Facility, Experiment | CERN LHC ; LHCf |
| Abstract | The LHCf experiment is dedicated to the measurement of very forward particle production in the high energy hadron-hadron collisions at LHC, with the aim of improving the cosmic-ray air shower developments models. The detector has taken data in p-p collisions at different center of mass energies, from 900 GeV up to 7 TeV, and in p-Pb collisions at s=5.02 TeV . The results of forward production spectra of neutrons in p-p collisions and π0 in p-Pb collisions, compared with the models most widely used in the High Energy Cosmic Ray physics, are presented in this paper. |
| Copyright/License | Elsevier B.V. (License: CC-BY-4.0) |
Corresponding record in: Inspire
Rekord stworzony 2017-05-10, ostatnia modyfikacja 2021-05-04
