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The most commonly employed formalisms of radiative energy loss have been derived in the high- energy approximation.
C. A. Salgado and U. A. Wiedemann, Phys. Rev. Lett. 93
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F. Carminati et al
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J. Putschke [STAR Collaboration], Eur. Phys. J. C 61
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S. Salur [STAR Collaboration], Eur. Phys. J. C 61
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N. Armesto, M. Cacciari, T. Hirano, J. L. Nagle and C. A. Salgado, arXiv:0907.0667 [hep-ph]
Cited in the paper.
http://igfae.usc.es/QatMC
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N. Armesto, L. Cunqueiro and C. A. Salgado, Eur. Phys. J. C 61
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R. Baier, D. Schiff and B. G. Zakharov, Ann. Rev. Nucl. Part. Sci. 50
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