activity
20122016
most citedObservation of meson nuclear modifications in Au+Au collisions at = 200 GeV

221 citations · 512 across the 7 of their papers we have counts for

collaborators

7 papers

nucl-ex201627 cited

Charge-dependent directed flow in Cu+Au collisions at = 200 GeV

STAR Collaboration, L. Adamczyk, J. K. Adkins +337

We present the first measurement of charge-dependent directed flow in Cu+Au collisions at = 200 GeV. The results are presented as a function of the particle tran…

hep-ph201437 cited

Reviving quark nuggets as a candidate for dark matter

Abhishek Atreya, Anjishnu Sarkar, Ajit M. Srivastava

We discuss a novel mechanism for segregation of baryons and anti-baryons in the quark-gluon plasma phase which can lead to formation of quark and antiquark nuggets in the early uni…

nucl-ex2014221 cited

Observation of meson nuclear modifications in Au+Au collisions at = 200 GeV

L. Adamczyk, J. K. Adkins, G. Agakishiev +352

We report the first measurement of charmed-hadron () production via the hadronic decay channel () in Au+Au collisions at

nucl-ex2014211 cited

Beam-energy dependence of charge separation along the magnetic field in Au+Au collisions at RHIC

STAR Collaboration, L. Adamczyk, J. K. Adkins +353

Local parity-odd domains are theorized to form inside a Quark-Gluon-Plasma (QGP) which has been produced in high-energy heavy-ion collisions. The local parity-odd domains manifest…

nucl-ex20145 cited

Beam energy dependent two-pion interferometry and the freeze-out eccentricity of pions in heavy ion collisions at STAR

STAR Collaboration, L. Adamczyk, J. K. Adkins +353

We present results of analyses of two-pion interferometry in Au+Au collisions at = 7.7, 11.5, 19.6, 27, 39, 62.4 and 200 GeV measured in the STAR detector as part o…

astro-ph.CO2012

Flat directions and gravitino production in SUSY models

Raghavan Rangarajan, Anjishnu Sarkar

Flat directions in supersymmetric models can get large vacuum expectation values in the early Universe which leads to a large mass for gauge bosons and gauginos. We point out that…