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2521
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2522por CMS Collaboration“…The following additional factors will be provided for use if desired by the analysis: dependence on the fraction of jet energy in the electromagnetic calorimeter; dependence on the flavor of the final state jet; removal of underlying event energy; and correction back to the parton level. …”
Publicado 2008
Enlace del recurso
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2523por CMS Collaboration“…Electronics noise in the CMS calorimeters, energy from additional $\mathrm{pp}$ interactions within the same bunch crossing, and energy integrated by the read-out electronics from preceding and subsequent bunch crossings, can lead to spurious energy contributions to reconstructed hadronic jets, which we call an ``offset''. …”
Publicado 2009
Enlace del recurso
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2524por CMS Collaboration“…CMS will correct the measured jet energy for instrumental effects. In addition, some measurements can benefit from further corrections which connect on average the $p_T$ of a jet to the $p_T$ of the associated parton in the hard scattering. …”
Publicado 2009
Enlace del recurso
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2525
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2526
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2527por Mount, Richard, Brooks, Travis, Le Diberder, Francois, Dubois-Felsmann, Gregory, Neal, Homer, Bellis, Matt, Boehnlein, Amber, Votava, Margaret, White, Vicky, Wolbers, Stephen, Konigsberg, Jacobo, Roser, Robert, Snider, Rick, Lucchesi, Donatella, Denisov, Dmitri, Soldner-Rembold, Stefan, Li, Qizhong, Varnes, Erich, Jonckheere, Alan, Gasthuber, Martin, Gulzow, Volker, Kemp, Yves, Ozerov, Dmitri, Diaconu, Cristinel, South, David, Lobodzinski, Bogdan, Olsson, Jan, Haas, Tobias, Wrona, Krzysztof, Szuba, Janusz, Schnell, Gunar, Sasaki, Takashi, Katayama, Nobu, Hernandez, Fabio, Mele, Salvatore, Holzner, Andre, Hemmer, Frederic, Schroeder, Matthias, Barring, Olof, Brun, Rene, Maggi, Marcello, Igo-Kemenes, Peter, Van Wezel, Jos, Heiss, Andreas, Chen, Gang, Wang, Yifang, Asner, David, Riley, Daniel, Corney, David, Gordon, John“…Data from high-energy physics (HEP) experiments are collected with significant financial and human effort and are mostly unique. …”
Publicado 2009
Enlace del recurso
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2528
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2529
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2530
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2531
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2532
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2533
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2534
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2535
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2536
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2537
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2538por Bustamante, M, Carrillo Montoya, G, de Paula, W, Duarte Chavez, J A, Gago, A M, Hakobyan, H, Jez, P, Monroy Montañez, J A, Ortiz Velasquez, A, Padilla Cabal, F, Pino Rozas, M, Rodriguez Patarroyo, D J, Romeo, G L, Saldaña-Salazar , U J, Velasquez, M, von Steinkirch, M“…We briefly review the basics of ultrahigh-energy cosmic-ray acceleration. The Hillas criterion is introduced as a geometrical criterion that must be fulfilled by potential acceleration sites, and energy losses are taken into account in order to obtain a more realistic scenario. …”
Publicado 2010
Enlace del recurso
Enlace del recurso
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2539
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2540por Allasia, D, Angelini, C, Argento, A, Baldo-Ceolin, Massimilla, Barlag, S, Bertanza, L, Bigi, A, Bini, V, Bloch, M, Bobisut, F, Bolognese, T, Calimani, E, Capiluppi, P, Casali, R, Ciampolillo, S, van Dam, P, Derkaoui, J E, Faccini-Turluer, M L, Fantechi, R, Flaminio, Vincenzo, Fridman, A, Gamba, D, Giacomelli, G, Hartjes, F G, Huzita, H, Jongejans, B, Van Leeuwen, W, Loreti, M, Louedeo, C, Mandrioli, G, Mattioli, F, Mazzanti, P, Marzari-Chiesa, A, Miari, G, Mosca, L, Nappi, A, Pazzi, R, Petri, C, Pierazzini, G M, Puglierin, G, Ramello, L, Ranzi-Minguzzi, A, Riccati, L, Romero, A, Rossi, A M, Saudraix, Jean, Sconza, A, Serra-Lugaresi, P, Tenner, A, Troncone, G, Vianello, A, Vignaud, D, Visser, C, Wigmans, R, De Wolf, EEnlace del recurso
Publicado 1980