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20022008
most citedObservational Constraints on the Nature of the Dark Energy: First Cosmological Results from the ESSENCE Supernova Survey

927 citations

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7 papers · 1 filter

nucl-ex200810 cited

Gamow-Teller strengths in 24Na using the 24Mg(t,3He) reaction at 115 AMeV

M. E. Howard, R. G. T. Zegers, Sam M. Austin +16

Gamow-Teller transitions from 24Mg to 24Na were studied via the (t,3He) reaction at 115 AMeV using a secondary triton beam produced via fast fragmentation of 150 AMeV 16O ions. Com…

nucl-ex2008267 cited

Centrality dependence of charged hadron and strange hadron elliptic flow from sqrt(s_NN) = 200 GeV Au+Au collisions

STAR Collaboration, B. I. Abelev

We present STAR results on the elliptic flow v_2 of charged hadrons, strange and multi-strange particles from sqrt(s_NN) = 200 GeV Au+Au collisions at RHIC. The detailed study of t…

nucl-ex200877 cited

Hadronic resonance production in +Au collisions at = 200 GeV at RHIC

B. I. Abelev

We present the first measurements of the , (892), (1232), (1385), and (1520) resonances in +Au collisions at = 200 GeV, reconst…

nucl-ex200777 cited

On the extraction of weak transition strengths via the (3He,t) reaction at 420 MeV

R. G. T Zegers, T. Adachi, H. Akimune +32

Differential cross sections for transitions of known weak strength were measured with the (3He,t) reaction at 420 MeV on targets of 12C, 13C, 18O, 26Mg, 58Ni, 60Ni, 90Zr, 118Sn, 12…

nucl-ex20074 cited

Forward Lambda Production and Nuclear Stopping Power in d + Au Collisions at sqrt(s_NN) = 200 GeV

STAR Collaboration, B. I. Abelev

We report the measurement of Lamda and Anti-Lamda yields and inverse slope parameters in d + Au collisions at sqrt(s_NN) = 200 GeV at forward and backward rapidities (y = +- 2.75),…

nucl-ex2007129 cited

Enhanced strange baryon production in Au+Au collisions compared to p+p at sqrts = 200 GeV

STAR Collaboration, B. I. Abelev

We report on the observed differences in production rates of strange and multi-strange baryons in Au+Au collisions at sqrts = 200 GeV compared to pp interactions at the same energy…