# GLV-WMC

Radiative energy loss results using the **Wicks Monte Carlo** evaluation of **(D)GLV**.

## Summary

Based on numerical work given in:

Up to and beyond ninth order in opacity: Radiative energy loss with GLV

Simon Wicks

This uses the radiative energy loss formulae from GLV [1] and DGLV [2]. The parameters (temperature, Debye mass, gluon mean free path etc) are set in the same manner as in WHDG. The n=1 version including a (small) jet and gluon mass should be identical to the inelastic only curves in WHDG (up to small variations due to eg possible q integral limits, to be investigated).

## Results

Using DGLV (ie including a small mass for the jet and emitted gluon): Q=up, p=10GeV, L=5fm, T=300 MeV, α=.3

## References

[1] Heavy quark radiative energy loss in QCD matter.

Magdalena Djordjevic, Miklos Gyulassy (Columbia U.) . Oct 2003. 31pp.

Published in Nucl.Phys.A733:265-298,2004.

e-Print: nucl-th/0310076

[2] Reaction operator approach to nonAbelian energy loss.

M. Gyulassy (Columbia U.) , P. Levai (Columbia U. & Budapest, RMKI) , I. Vitev (Columbia U.) . CU-TP-979, Jun 2000. 39pp.

Published in Nucl.Phys.B594:371-419,2001.

e-Print: nucl-th/0006010