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F.Gallas, E.Galyaev, E.Garcia, C.Garcia-Bellido, A.Gavrilov, V.Gay, P.Geist, W.Gelé, D.Gerber, C. E.Gershtein, Y.Gillberg, D.Ginther, G.Gollub, N.Gómez, B.Goussiou, A.Grannis, P. D.Greenlee, H.Greenwood, Z. D.Gregores, E. M. [UNESP]Grenier, G.Gris, PhGrivaz, J. F.Grohsjean, A.Grünendahl, S.Grünewald, M. W.Guo, F.Guo, J.Gutierrez, G.Gutierrez, P.Haas, A.Hadley, N. J.Haefner, P.Hagopian, S.Haley, J.Hall, I.Hall, R. E.Han, L.Hanagaki, K.Hansson, P.Harder, K.Harel, A.Harrington, R.Hauptman, J. M.Hauser, R.Hays, J.Hebbeker, T.Hedin, D.Hegeman, J. G.Heinmiller, J. M.Heinson, A. P.Heintz, U.Hensel, C.Herner, K.Hesketh, G.Hildreth, M. D.Hirosky, R.Hobbs, J. D.Hoeneisen, B.Hoeth, H.Hohlfeld, M.Hong, S. J.Hooper, R.Hossain, S.Houben, P.Hu, Y.Hubacek, Z.Hynek, V.Iashvili, I.Illingworth, R.Ito, A. S.Jabeen, S.Jaffré, M.Jain, S.Jakobs, K.Jarvis, C.Jesik, R.Johns, K.Johnson, C.Johnson, M.Jonckheere, A.Jonsson, P.Juste, A.Käfer, D.Kahn, S.Kajfasz, E.Kalinin, A. M.Kalk, J. M.Kalk, J. 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M.Unalan, R.Uvarov, L.Uvarov, S.Uzunyan, S.Vachon, B.Van Den Berg, P. J.Van Eijk, B.Van Kooten, R.Van Leeuwen, W. M.Varelas, N.Varnes, E. W.Vartapetian, A.Vasilyev, I. A.Vaupel, M.Verdier, P.Vertogradov, L. S.Verzocchi, M.Villeneuve-Seguier, F.Vint, P.Von Toerne, E.Voutilainen, M.Vreeswijk, M.Wagner, R.Wahl, H. D.Wang, L.Wang, M. H.L.S.Warchol, J.Watts, G.Wayne, M.Weber, G.Weber, M.Weerts, H.Wenger, A.Wermes, N.Wetstein, M.White, A.Wicke, D.Wilson, G. W.Wimpenny, S. J.Wobisch, M.Wood, D. R.Wyatt, T. R.Xie, Y.Yacoob, S.Yamada, R.Yan, M.Yasuda, T.Yatsunenko, Y. A.Yip, K.Yoo, H. D.Youn, S. W.Yu, C.Yu, J.Yurkewicz, A.Zatserklyaniy, A.Zeitnitz, C.Zhang, D.Zhao, T.Zhou, B.Zhu, J.Zielinski, M.Zieminska, D.Zieminski, A.Zivkovic, L.Zutshi, V.Zverev, E. G.2022-04-282022-04-282007-08-06Physical Review Letters, v. 99, n. 6, 2007.0031-90071079-7114http://hdl.handle.net/11449/224952We report on a search for charge-1/3 third-generation leptoquarks (LQ) produced in pp̄ collisions at s=1.96TeV using the D0 detector at Fermilab. Third-generation leptoquarks are assumed to be produced in pairs and to decay to a tau neutrino and a b quark with branching fraction B. We place upper limits on σ(pp̄→LQLQ̄)B2 as a function of the leptoquark mass MLQ. Assuming B=1, we exclude at the 95% confidence level third-generation scalar leptoquarks with MLQ<229GeV. © 2007 The American Physical Society.engArtigo10.1103/PhysRevLett.99.0618012-s2.0-34547786729