- Access by Xinjiang University
Just how different are the and Landau-gauge propagators in the infrared regime?
Phys. Rev. D 76, 114507 – Published 18 December, 2007
DOI: https://doi.org/10.1103/PhysRevD.76.114507
Abstract
The infrared behavior of gluon and ghost propagators in Yang-Mills theories is of central importance for understanding quark and gluon confinement in QCD. While simulations of pure gauge theory correspond to the physical case in the limit of infinite quark mass, the case (i.e. pure two-color QCD) is usually employed as a simplification, in the hope that qualitative features be the same as for the case. Here we carry out the first comparative study of lattice (Landau) propagators for these two gauge groups. Our data were especially produced with equivalent lattice parameters in order to allow a careful comparison of the two cases. We find very good agreement between and propagators, showing that in the IR limit the equivalence of the two cases is quantitative, at least down to about 1 GeV. Our results suggest that the infrared behavior of these propagators is independent of the gauge group , as predicted by Schwinger-Dyson equations.
Article Text
References (61)
- V. N. Gribov, Nucl. Phys. B139, 1 (1978).
- D. Zwanziger, Phys. Lett. B 257, 168 (1991); Nucl. Phys. B364, 127 (1991); B412, 657 (1994).
- T. Kugo and I. Ojima, Prog. Theor. Phys. Suppl. 66, 1 (1979); 71, 1121(E) (1984).
- R. Alkofer and L. von Smekal, Phys. Rep. 353, 281 (2001).
- P. Maris and C. D. Roberts, Int. J. Mod. Phys. E 12, 297 (2003).
- L. von Smekal, A. Hauck, and R. Alkofer, Ann. Phys. (N.Y.) 267, 1 (1998).
- C. Lerche and L. von Smekal, Phys. Rev. D 65, 125006 (2002).
- D. Zwanziger, Phys. Rev. D 65, 094039 (2002).
- A. C. Aguilar, A. A. Natale, and P. S. Rodrigues da Silva, Phys. Rev. Lett. 90, 152001 (2003).
- A. C. Aguilar and A. A. Natale, J. High Energy Phys. 08 (2004) 57.
- G. t’Hooft, Nucl. Phys. B72, 461 (1974).
- J. E. Mandula and M. Ogilvie, Phys. Lett. B 185, 127 (1987).
- C. W. Bernard, C. Parrinello, and A. Soni, Phys. Rev. D 49, 1585 (1994).
- P. Marenzoni, G. Martinelli, and N. Stella, Nucl. Phys. B455, 339 (1995).
- D. B. Leinweber, J. I. Skullerud, A. G. Williams, and C. Parrinello, Phys. Rev. D 58, 031501 (1998); 60, 094507 (1999).
- J. P. Ma, Mod. Phys. Lett. A 15, 229 (2000).
- D. Becirevic et al., Phys. Rev. D 61, 114508 (2000).
- H. Nakajima and S. Furui, Nucl. Phys. A680, 151 (2001).
- F. D. R. Bonnet, P. O. Bowman, D. B. Leinweber, and A. G. Williams, Phys. Rev. D 62, 051501 (2000).
- F. D. R. Bonnet, P. O. Bowman, D. B. Leinweber, A. G. Williams, and J. M. Zanotti, Phys. Rev. D 64, 034501 (2001).
- P. J. Silva and O. Oliveira, Nucl. Phys. B690, 177 (2004).
- S. Furui and H. Nakajima, Phys. Rev. D 69, 074505 (2004).
- O. Oliveira and P. J. Silva, AIP Conf. Proc. 756, 290 (2005).
- O. Oliveira and P. J. Silva, Proc. Sci., LAT2005 (2005) 287.
- A. Sternbeck, E.-M. Ilgenfritz, M. Müller-Preussker, and A. Schiller, Phys. Rev. D 72, 014507 (2005).
- P. J. Silva and O. Oliveira, Phys. Rev. D 74, 034513 (2006).
- A. Sternbeck, E.-M. Ilgenfritz, M. Müller-Preussker, A. Schiller, and I. L. Bogolubsky, Proc. Sci., LAT2006 (2006) 076.
- P. J. Silva and O. Oliveira, Proc. Sci., LAT2006 (2006) 075.
- O. Oliveira and P. J. Silva, Braz. J. Phys. 37, 201 (2007).
- O. Oliveira and P. J. Silva, arXiv:0705.0964.
- A. Cucchieri, Nucl. Phys. B508, 353 (1997).
- A. Cucchieri, Phys. Lett. B 422, 233 (1998).
- K. Langfeld, H. Reinhardt, and J. Gattnar, Nucl. Phys. B621, 131 (2002).
- A. Cucchieri, T. Mendes, and A. R. Taurines, Phys. Rev. D 67, 091502 (2003).
- J. C. R. Bloch, A. Cucchieri, K. Langfeld, and T. Mendes, Nucl. Phys. B687, 76 (2004).
- A. Cucchieri, T. Mendes, and A. R. Taurines, Phys. Rev. D 71, 051902 (2005).
- A. Cucchieri and T. Mendes, Braz. J. Phys. 37, 484 (2007).
- A. Cucchieri and T. Mendes, Phys. Rev. D 73, 071502 (2006).
- A. Cucchieri, A. Maas, and T. Mendes, Phys. Rev. D 74, 014503 (2006).
- A. Maas, A. Cucchieri, and T. Mendes, Braz. J. Phys. 37, 219 (2007).
- A. Maas, Phys. Rev. D 75, 116004 (2007).
- P. O. Bowman, U. M. Heller, D. B. Leinweber, M. B. Parappilly, and A. G. Williams, Phys. Rev. D 70, 034509 (2004).
- E.-M. Ilgenfritz, M. Müller-Preussker, A. Sternbeck, A. Schiller, and I. L. Bogolubsky, Braz. J. Phys. 37, 193 (2007).
- S. Furui and H. Nakajima, Phys. Rev. D 73, 094506 (2006).
- P. O. Bowman et al., Phys. Rev. D 76, 094505 (2007).
- C. S. Fischer, A. Maas, J. M. Pawlowski, and L. von Smekal, arXiv:hep-ph/0701050 [Ann. Phys. (N.Y.) (to be published)].
- H. Suman and K. Schilling, Phys. Lett. B 373, 314 (1996).
- Ph. Boucaud et al., Phys. Rev. D 72, 114503 (2005).
- Ph. Boucaud et al., J. High Energy Phys. 01 (2006) 37.
- A. Cucchieri, T. Mendes, A. Mihara, Phys. Rev. D 72, 094505 (2005).
- I. L. Bogolubsky, G. Burgio, V. K. Mitrjushkin, and M. Müeller-Preussker, Phys. Rev. D 74, 034503 (2006).
- A. Cucchieri and T. Mendes, Phys. Rev. D 73, 071502 (2006).
- O. Oliveira and P. J. Silva, Eur. Phys. J. A 31, 790 (2007).
- G. S. Bali and K. Schilling, Phys. Rev. D 47, 661 (1993).
- The configurations were generated with the MILC code http://physics.indiana.edu/~sg/milc.html
- F. de Soto and C. Roiesnel, J. High Energy Phys. 09 (2007) 007.
- A. Sternbeck, L. von Smekal, D. B. Leinweber, and A. G. Williams, Proc. Sci., LAT2007 (2007) 340.
- G. Damm, W. Kerler, and V. K. Mitrjushkin, Phys. Lett. B 433, 88 (1998).
- A. Cucchieri, Phys. Rev. D 60, 034508 (1999).
- I. L. Bogolubsky et al., arXiv:0707.3611.
- I. L. Bogolubsky et al., Proc. Sci., LAT2007 (2007) 318.