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Feb 1 – 3, 2017
Mezzanine level
US/Eastern timezone

Sivers program at STAR

Feb 3, 2017, 2:00 PM
25m
Hoover (Mezzanine level)

Hoover

Mezzanine level

Marriott Wardman Park, 2660 Woodley Rd. NW, Washington, DC 20008

Speaker

Dr Salvatore Fazio (Brookhaven National Laboratory)

Description

Accessing the Sivers TMD function in proton+proton collisions through the measurement of transverse single spin asymmetries (TSSAs) in weak boson production is an effective path to test the fundamental QCD prediction of the non-universality of the Sivers function. Furthermore, it provides data to study the spin-flavor structure of valence and sea quarks inside the proton and to test the evolution of parton distributions. The TSSA amplitude, $A_N$, has been measured at STAR in proton+proton collisions at $\sqrt{s}= 500$~GeV, with a recorded integrated luminosity of 25~pb$^{-1}$. Within relatively large statistical uncertainties, the current data favor theoretical models that include change of sign for the Sivers function relative to observations in SIDIS measurements, if TMD evolution effects are small. RHIC plans to run proton+proton collisions of transversely polarized beams at $\sqrt{s}= 510$~GeV in 2017, delivering an integrated luminosity of 400~pb$^{-1}$. This will allow STAR to perform a precise measurement of TSSAs in both weak boson and Drell-Yan production as well as other observables sensitive to the non-universality of the Sivers function via Twist-3, e.g. the TSSA of direct photons.

Primary author

Dr Salvatore Fazio (Brookhaven National Laboratory)

Presentation materials