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

593 citations

Showing 2010Show all

11 papers · 1 filter

cond-mat.mes-hall201080 cited

Nonlinear growth with the microwave intensity in radiation-induced magnetoresistance oscillations

R. G. Mani, C. Gerl, S. Schmult +2

We report the observation of inverse-magnetic-field-periodic, radiation-induced magnetoresistance oscillations in GaAs/AlGaAs heterostructures prepared in W. Wegscheider's group, c…

math.CV2010

On complex Banach manifolds similar to Stein manifolds

Imre Patyi

We give an abstract definition, similar to the axioms of a Stein manifold, of a class of complex Banach manifolds in such a way that a manifold belongs to the class if and only if…

astro-ph.SR2010131 cited

Discovery of a 1.6-year Magnetic Activity Cycle in the Exoplanet Host Star iota Horologii

T. S. Metcalfe, S. Basu, T. J. Henry +5

The Mount Wilson Ca HK survey revealed magnetic activity variations in a large sample of solar-type stars with timescales ranging from 2.5 to 25 years. This broad range of cycle pe…

hep-ex201035 cited

Event Structure and Double Helicity Asymmetry in Jet Production from Polarized p+p Collisions at sqrt(s) = 200 GeV

A. Adare, S. Afanasiev, C. Aidala +372

We report on event structure and double helicity asymmetry () of jet production in longitudinally polarized p+p collisions at =200 GeV. Photons and charged particle…

hep-ex201042 cited

Measurement of Transverse Single-Spin Asymmetries for J/psi Production in Polarized p+p Collisions at sqrt(s) = 200 GeV

A. Adare, S. Afanasiev, C. Aidala +444

We report the first measurement of transverse single-spin asymmetries in production from transversely polarized collisions at GeV with data taken by th…

astro-ph.HE201015 cited

H-alpha Emission Variability in the gamma-ray Binary LS I +61 303

M. Virginia McSwain, Erika D. Grundstrom, Douglas R. Gies +1

LS I +61 303 is an exceptionally rare example of a high mass X-ray binary (HMXB) that also exhibits MeV-TeV emission, making it one of only a handful of "gamma-ray binaries". Here…