activity
20032011
most citedTransverse momentum and collision energy dependence of high hadron suppression in Au+Au collisions at ultrarelativistic energies

717 citations · 5.3k across the 56 of their papers we have counts for

collaborators

56 papers

nucl-ex2011★ 130 cited

Strangeness Enhancement in Cu+Cu and Au+Au Collisions at \sqrt{s_{NN}} = 200 GeV

STAR Collaboration, H. Agakishiev, M. M. Aggarwal +369

We report new STAR measurements of mid-rapidity yields for the , , , , , , particles in Cu+Cu collisions at \sNN{200}, and…

nucl-ex2010★ 7 cited

Measurements of Dihadron Correlations Relative to the Event Plane in Au+Au Collisions at GeV

H. Agakishiev, M. M. Aggarwal, Z. Ahammed +366

Dihadron azimuthal correlations containing a high transverse momentum () trigger particle are sensitive to the properties of the nuclear medium created at RHIC through the str…

nucl-ex2010★ 54 cited

Scaling properties at freeze-out in relativistic heavy ion collisions

STAR Collaboration, M. M. Aggarwal

Identified charged pion, kaon, and proton spectra are used to explore the system size dependence of bulk freeze-out properties in Cu+Cu collisions at =200 and 62.4 G…

physics.ins-det2010★ 12 cited

ALICE EMCal Physics Performance Report

Rene Bellwied

The ALICE detector at the LHC (A Large Ion Collider Experiment) will carry out comprehensive measurements of high energy nucleus-nucleus collisions, in order to study QCD matter un…

nucl-ex2010★ 81 cited

Measurement of the Bottom contribution to non-photonic electron production in collisions at =200 GeV

STAR Collaboration, M. M. Aggarwal

The contribution of meson decays to non-photonic electrons, which are mainly produced by the semi-leptonic decays of heavy flavor mesons, in collisions at 20…

nucl-ex2010★ 84 cited

K*0 production in Cu+Cu and Au+Au collisions at \sqrt{s_NN} = 62.4 GeV and 200 GeV

M. M. Aggarwal, Z. Ahammed, A. V. Alakhverdyants +383

We report on K*0 production at mid-rapidity in Au+Au and Cu+Cu collisions at \sqrt{s_{NN}} = 62.4 and 200 GeV collected by the Solenoid Tracker at RHIC (STAR) detector. The K*0 is…