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S.Verzocchi, M.Villeneuve-Seguier, F.Vlimant, JRVon Toerne, E.Vreeswijk, M.Vu Anh, T.Wahl, H. D.Wang, L.Warchol, J.Watts, G.Wayne, M.Weber, M.Weerts, H.Wegner, M.Wermes, N.White, A.White, VWicke, D.Wijngaarden, D. A.Wilson, G. W.Wimpenny, S. J.Wittlin, J.Wobisch, M.Womersley, J.Wood, D. R.Wyatt, T. R.Xu, Q.Xuan, N.Yacoob, S.Yamada, R.Yan, M.Yasuda, T.Yatsunenko, Y. A.Yen, Y.Yip, K.Yoo, H. D.Youn, S. W.Yu, J.Yurkewicz, A.Zabi, A.Zatserklyaniy, A.Zdrazil, M.Zeitnitz, C.Zhang, D.Zhang, XZhao, T.Zhao, Z.Zhou, B.Zhu, J.Zielinski, M.Zieminska, D.Zieminski, A.Zitoun, R.Zutshi, VZverev, E. G.2014-05-202014-05-202005-08-26Physical Review Letters. College Pk: Amer Physical Soc, v. 95, n. 9, 7 p., 2005.0031-9007http://hdl.handle.net/11449/23285We report the first direct search for the Kaluza-Klein (KK) modes of Randall-Sundrum gravitons using dielectron, dimuon, and diphoton events observed with the D0 detector operating at the Fermilab Tevatron p (p) over bar Collider at root s = 1: 96 TeV. No evidence for resonant production of gravitons has been found in the data corresponding to an integrated luminosity of approximate to 260 pb(-1). Lower limits on the mass of the first KK mode at the 95% C. L. have been set between 250 and 785 GeV, depending on its coupling to standard model particles.7engArtigo10.1103/PhysRevLett.95.091801WOS:000231503600019Acesso restritoWOS000231503600019.pdf