output
20022013
most citedEnergy Loss and Flow of Heavy Quarks in Au+Au Collisions at sqrt(s_NN) = 200 GeV

593 citations

Showing 2012Show all

7 papers · 1 filter

astro-ph.SR2012101 cited

Magnetic Activity Cycles in the Exoplanet Host Star epsilon Eridani

T. S. Metcalfe, A. P. Buccino, B. P. Brown +7

The active K2 dwarf epsilon Eri has been extensively characterized, both as a young solar analog and more recently as an exoplanet host star. As one of the nearest and brightest st…

cond-mat.mes-hall201277 cited

Observation of Resistively Detected Hole Spin Resonance and Zero-field Pseudo-spin Splitting in Epitaxial Graphene

R. G. Mani, J. Hankinson, C. Berger +1

Electronic carriers in graphene show a high carrier mobility at room temperature. Thus, this system is widely viewed as a potential future charge-based high-speed electronic-materi…

math.CO2012

The inverse inertia problem for the complements of partial -trees

Hein van der Holst

Let be an infinite field with characteristic different from two. For a graph with , let be the set of all symmetric $n\times n…

cond-mat.mes-hall201277 cited

Observation of linear-polarization-sensitivity in the microwave-radiation-induced magnetoresistance oscillations

R. G. Mani, A. N. Ramanayaka, W. Wegscheider

In the quasi two-dimensional GaAs/AlGaAs system, we investigate the effect of rotating \textit{in-situ} the electric field of linearly polarized microwaves relative to the current,…

astro-ph.CO201253 cited

The Stellar and Gas Kinematics of the LITTLE THINGS Dwarf Irregular Galaxy NGC 1569

Megan Johnson, Deidre A. Hunter, Se-Heon Oh +5

In order to understand the formation and evolution of dIm galaxies, one needs to understand their three-dimensional structure. We present measurements of the stellar velocity dispe…

math.CO20121 cited

The inertia set of a signed graph

Marina Arav, Frank J. Hall, Zhongshan Li +1

A signed graph is a pair , where is a graph (in which parallel edges are permitted, but loops are not) with and . By we denote…