Measurement of the Transverse Single-Spin Asymmetries for $\pi^{0}$ and Jet-like Events at Forward Rapidities at STAR in $p+p$ Collisions at $\sqrt{s}$ = 500 GeV

TL;DR

This paper reports measurements of transverse single-spin asymmetries for neutral pions and jet-like events at forward rapidities in proton-proton collisions at 500 GeV, aiming to disentangle different spin-momentum correlation contributions.

Contribution

It presents the first measurement of $A_N$ for $b0$ and jet-like events at forward rapidities at STAR, exploring asymmetries across different event classes and jet correlations.

Findings

$A_N$ varies with the number of photons in the event

Forward jet asymmetries are studied in relation to midrapidity jets

Results provide insights into spin-momentum correlations in proton structure

Abstract

Large transverse single-spin asymmetries ($A_N$) have been observed for forward inclusive hadron production in $p+p$ collisions at various experiments. In the collinear perturbative scattering picture, twist-3 multi-parton correlations can give rise to such an asymmetry. A transversely polarized quark can also give rise to a spin-dependent distribution of its hadron fragments via the higher twist effects or the Collins fragmentation function. The observed $A_N$ may involve contributions from both processes. These can be disentangled by studying asymmetries for jets, direct photons and jet-fragments. The STAR Forward Meson Spectrometer (FMS), a Pb-glass electromagnetic calorimeter covering the pseudo-rapidity ($\eta$) range 2.6-4.2 and full azimuth, can detect photons, neutral pions and eta mesons. We are measuring $A_N$ for $\pi^{0}$ and jet-like events reconstructed from photons in the FMS in $p+p$ collisions at $\sqrt{s}$ = 500 GeV that were recorded during the 2011 RHIC run. We study $A_N$ as a function of the number of observed photons in the FMS, thereby exploring asymmetries for a range of event classes. We further study $A_N$ for forward jets and its dependency on forward-midrapidity jet correlation. The current status of the analysis will be discussed.