STAR Collaboration2015-05-152015-05-152014STAR Collaboration. "Beam-Energy Dependence of the Directed Flow of Protons, Antiprotons, and Pions in Au+Au Collisions." <i>Physical Review Letters,</i> 112, no. 16 (2014) American Physical Society: 162301. http://dx.doi.org/10.1103/PhysRevLett.112.162301.https://hdl.handle.net/1911/80238Rapidity-odd directed flow (v1) measurements for charged pions, protons, and antiprotons near midrapidity (y=0) are reported in √sNN=7.7, 11.5, 19.6, 27, 39, 62.4, and 200 GeV Au+Au collisions as recorded by the STAR detector at the Relativistic Heavy Ion Collider. At intermediate impact parameters, the proton and net-proton slope parameter dv1/dy|y=0 shows a minimum between 11.5 and 19.6 GeV. In addition, the net-proton dv1/dy|y=0 changes sign twice between 7.7 and 39 GeV. The proton and net-proton results qualitatively resemble predictions of a hydrodynamic model with a first-order phase transition from hadronic matter to deconfined matter, and differ from hadronic transport calculations.engArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.Beam-Energy Dependence of the Directed Flow of Protons, Antiprotons, and Pions in Au+Au CollisionsJournal articlehttp://dx.doi.org/10.1103/PhysRevLett.112.162301