# Measurement of $\hat{q}$ in Relativistic Heavy Ion Collisions using   di-hadron correlations

**Authors:** M. J. Tannenbaum

arXiv: 1702.00840 · 2017-07-27

## TL;DR

This paper measures the transport coefficient  in relativistic heavy ion collisions using di-hadron correlations, accounting for energy loss effects, and compares results with theoretical predictions and previous experimental findings.

## Contribution

It introduces a method to correct the measured  for energy loss effects in di-hadron correlations, providing a more precise estimate of  in Au+Au collisions.

## Key findings

-  in Au+Au collisions estimated as 0.30 1.09 GeV^2/fm.
- Results are consistent with previous theoretical calculations.
- The method improves the precision of  measurements in heavy ion collisions.

## Abstract

The azimuthal width of the di-hadron correlations in p$+$p collisons, beyond the fragmentation transverse momentum, $j_T$, is dominated by $k_T$, the so-called intrinsic transverse momentum of a parton in a nucleon, which can be measured. The predicted azimuthal broadening in A$+$A collisions should produce a larger $k_T$ than in p$+$p collisions. The present work introduces the observation that the $k_T$ measured in p$+$p collisions for di-hadrons with $p_{Tt}$ and $p_{Ta}$ must be reduced to compensate for the energy loss of both the trigger and away parent partons when comparing to the $k_T$ measured with the same di-hadron $p_{Tt}$ and $p_{Ta}$ in Au$+$Au collisions. This idea is applied to a recent STAR di-hadron measurement, with result $\langle{\hat{q}L}\rangle=2.1\pm 0.6$ GeV$^2$. This is more precise but in agreement with a theoretical calulation of $\langle{\hat{q}L}\rangle=14^{+42}_{-14}$ GeV$^2$ using the same data. Assuming a length $\langle{L}\rangle\approx 7$ fm for central Au$+$Au collisions the present result gives $\hat{q}=0.30\pm 0.09$ GeV$^2$/fm, in fair agreement with the JET collaboration result of $\hat{q}\approx 1.2\pm 0.3$ GeV$^2$/fm at initial time $\tau_0=0.6$ fm/c in Au+Au collisions at $\sqrt{s_{NN}}=200$ GeV.

## Full text

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## Figures

10 figures with captions in the complete paper: https://tomesphere.com/paper/1702.00840/full.md

## References

26 references — full list in the complete paper: https://tomesphere.com/paper/1702.00840/full.md

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