Chromoelectric flux tubes in QCD

Cardaci MS, Cea P, Cosmai L, Falcone R, Papa A (2011)
Physical Review D 83(1): 014502.

Zeitschriftenaufsatz | Veröffentlicht | Englisch
 
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Autor*in
Cardaci, Mario Salvatore; Cea, Paolo; Cosmai, Leonardo; Falcone, RossellaUniBi; Papa, Alessandro
Abstract / Bemerkung
We analyze the distribution of the chromoelectric field generated by a static quark-antiquark pair in the SU(3) vacuum and revisit previous results for SU(2). We find that the transverse profile of the flux tube resembles the dual version of the Abrikosov vortex field distribution. We give an estimate of the London penetration length of the chromoelectric field in the confined vacuum. We also speculate on the value of the ratio between the penetration lengths for SU(2) and SU(3) gauge theories.
Erscheinungsjahr
2011
Zeitschriftentitel
Physical Review D
Band
83
Ausgabe
1
Art.-Nr.
014502
ISSN
1550-7998
eISSN
1550-2368
Page URI
https://pub.uni-bielefeld.de/record/2003303

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Cardaci MS, Cea P, Cosmai L, Falcone R, Papa A. Chromoelectric flux tubes in QCD. Physical Review D. 2011;83(1): 014502.
Cardaci, M. S., Cea, P., Cosmai, L., Falcone, R., & Papa, A. (2011). Chromoelectric flux tubes in QCD. Physical Review D, 83(1), 014502. https://doi.org/10.1103/PhysRevD.83.014502
Cardaci, Mario Salvatore, Cea, Paolo, Cosmai, Leonardo, Falcone, Rossella, and Papa, Alessandro. 2011. “Chromoelectric flux tubes in QCD”. Physical Review D 83 (1): 014502.
Cardaci, M. S., Cea, P., Cosmai, L., Falcone, R., and Papa, A. (2011). Chromoelectric flux tubes in QCD. Physical Review D 83:014502.
Cardaci, M.S., et al., 2011. Chromoelectric flux tubes in QCD. Physical Review D, 83(1): 014502.
M.S. Cardaci, et al., “Chromoelectric flux tubes in QCD”, Physical Review D, vol. 83, 2011, : 014502.
Cardaci, M.S., Cea, P., Cosmai, L., Falcone, R., Papa, A.: Chromoelectric flux tubes in QCD. Physical Review D. 83, : 014502 (2011).
Cardaci, Mario Salvatore, Cea, Paolo, Cosmai, Leonardo, Falcone, Rossella, and Papa, Alessandro. “Chromoelectric flux tubes in QCD”. Physical Review D 83.1 (2011): 014502.
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arXiv: 1011.5803

Inspire: 879086

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