Fetching the paper…

Reading the bibliography…

2011

Explaining jet quenching with perturbative QCD alone

Zapp, Korinna C., Krauss, Frank, Wiedemann, Urs A.

Original
PDF
Post on X

Understand

We present a new formulation of jet quenching in perturbative QCD beyond the eikonal approximation.

Multiple scattering in the medium is modelled through infra-red-continued (2 -> 2) scattering matrix elements in QCD and the parton shower describing further emissions.
The interplay between these processes is arranged in terms of a formation time constraint such that coherent emissions can be treated consistently.
Emerging partons are hadronised by the Lund string model, tuned to describe LEP data in conjunction with the parton shower.

Explaining jet quenching with perturbative QCD alone · Around

Built on

B. Andersson, G. Gustafson, G. Ingelman, and T. Sjostrand, Phys. Rept. 97
1983
Earlier work this paper cites.
T. Sjostrand, Nucl. Phys. B248
1984
Earlier work this paper cites.
R. Baier, Y. L. Dokshitzer, A. H. Mueller, S. Peigne, and D. Schiff, Nucl. Phys. B484
1997
Earlier work this paper cites.
B. G. Zakharov, JETP Lett. 65
1997
Earlier work this paper cites.
U. A. Wiedemann, Nucl. Phys. B588
2000
Earlier work this paper cites.
X.-N. Wang and X.-f. Guo, Nucl. Phys. A696
2001
Earlier work this paper cites.
M. Gyulassy, P. Levai, and I. Vitev, Nucl. Phys. B594
2001
Earlier work this paper cites.
P. B. Arnold, G. D. Moore, and L. G. Yaffe, JHEP 0206
2002
Earlier work this paper cites.
J. Pumplin et al. , JHEP 07
2002
Earlier work this paper cites.

Similar

M. Whalley, D. Bourilkov, and R. Group(2005), arXiv:hep-ph/0508110 [hep-ph]
2005
Cited alongside, same era.
T. Sjostrand, S. Mrenna, and P. Skands, JHEP 05
2006
Cited alongside, same era.
K. Zapp, G. Ingelman, J. Rathsman, and J. Stachel, Phys. Lett. B637
2006
Cited alongside, same era.
A. Adare et al. (PHENIX), Phys. Rev. D76
Original
2007
Cited alongside, same era.
A. Adare et al. (PHENIX Collaboration), Phys.Rev.Lett. 101
Original
2008
Cited alongside, same era.
K. Zapp, J. Stachel, and U. A. Wiedemann, Phys. Rev. Lett. 103
Original

Then

W. Horowitz and M. Gyulassy, Nucl.Phys. A872
Original
2011
Closest in time.
T. Renk, H. Holopainen, R. Paatelainen, and K. J. Eskola, Phys.Rev. C84
Original
2011
Closest in time.
X.-F. Chen, T. Hirano, E. Wang, X.-N. Wang, and H. Zhang, Phys.Rev. C84
Original
2011
Closest in time.
A. Majumder and C. Shen(2011), arXiv:1103.0809 [hep-ph]
Original
2011
Closest in time.
N. Armesto, B. Cole, C. Gale, W. A. Horowitz, P. Jacobs, et al. (2011), arXiv:1106.1106 [hep-ph]
Original
2011
Closest in time.

Beyond the bibliography

alphaXiv searches the wider corpus for related work and actual follow-ups.

Open on alphaXiv

alphaXiv is searching for related work…

2009

Cited alongside, same era.

K. Zapp, G. Ingelman, J. Rathsman, J. Stachel, and U. A. Wiedemann, Eur.Phys.J. C60

2009

Cited alongside, same era.

K. J. Eskola, H. Paukkunen, and C. A. Salgado, JHEP 04

2009

Cited alongside, same era.

A. Buckley et al. (2010), arXiv:1003.0694 [hep-ph]

2010

Cited alongside, same era.

This approximation can easily be improved numerically

Cited in the paper.

Although the present code goes far beyond the eikonal kinematics, it is clear how to recover this limit of the full emission pattern encoded here

Cited in the paper.

K. C. Zapp, J. Stachel, and U. A. Wiedemann, JHEP 07

2011

Closest in time.

Y.-J. Lee, J. Phys. G38

2011

Closest in time.

H. Appelshauser (ALICE), J. Phys. G38

2011

Closest in time.

K. C. Zapp and U. A. Wiedemann(2012), arXiv:1202.1192 [hep-ph]

2012

Closest in time.