Built on

M. Hansen, A. Lupo, and N. Tantalo, Phys. Rev. D 99
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1903
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C. Bonanno, G. Clemente, M. D’Elia, and F. Sanfilippo, JHEP 10
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N. Astrakhantsev, V. V. Braguta, M. D’Elia, A. Y. Kotov, A. A. Nikolaev, and F. Sanfilippo, Phys. Rev. D 102
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M. P. Lombardo and A. Trunin, Int. J. Mod. Phys. A 35
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2023

Sphaleron rate of $N_f=2+1$ QCD

Bonanno, Claudio, D'Angelo, Francesco, D'Elia, Massimo et al.

Understand

We compute the sphaleron rate of $N_f=2+1$ QCD at the physical point for a range of temperatures $200$ MeV $\lesssim T \lesssim 600$ MeV.

We adopt a strategy recently applied in the quenched case, based on the extraction of the rate via a modified version of the Backus-Gilbert method from finite-lattice-spacing and finite-smoothing-radius Euclidean topological charge density correlators.
The physical sphaleron rate is finally computed by performing a continuum limit at fixed physical smoothing radius, followed by a zero-smoothing extrapolation.
Dynamical fermions were discretized using the staggered formulation, which is known to yield large lattice artifacts for the topological susceptibility.

Built on

M. Hansen, A. Lupo, and N. Tantalo, Phys. Rev. D 99
Original
1903
Earlier work this paper cites.
C. Bonanno, G. Clemente, M. D’Elia, and F. Sanfilippo, JHEP 10
Original
1908
Earlier work this paper cites.
N. Astrakhantsev, V. V. Braguta, M. D’Elia, A. Y. Kotov, A. A. Nikolaev, and F. Sanfilippo, Phys. Rev. D 102
Original
1910
Earlier work this paper cites.
M. Berni, C. Bonanno, and M. D’Elia, Phys. Rev. D 100
Original
1911
Earlier work this paper cites.
G. Backus and F. Gilbert, Geophysical Journal International 16
1968
Earlier work this paper cites.
P. Di Vecchia, K. Fabricius, G. C. Rossi, and G. Veneziano, Nucl. Phys. B 192
1981
Earlier work this paper cites.
B. Berg, Phys. Lett. B 104
1981
Earlier work this paper cites.
Y. Iwasaki and T. Yoshie, Phys. Lett. B 131
1983
Earlier work this paper cites.
S. Itoh, Y. Iwasaki, and T. Yoshie, Phys. Lett. B 147
1984
Earlier work this paper cites.
M. Teper, Phys. Lett. B 162
1985
Earlier work this paper cites.
E.-M. Ilgenfritz, M. Laursen, G. Schierholz, M. Müller-Preussker, and H. Schiller, Nucl. Phys. B 268
1986
Earlier work this paper cites.
M. Albanese et al. (APE), Phys. Lett. B 192
1987
Earlier work this paper cites.
M. Campostrini, A. Di Giacomo, and H. Panagopoulos, Phys. Lett. B 212
1988
Earlier work this paper cites.
M. Campostrini, A. Di Giacomo, H. Panagopoulos, and E. Vicari, Nucl. Phys. B 329
1990
Earlier work this paper cites.
B. Alles, G. Boyd, M. D’Elia, A. Di Giacomo, and E. Vicari, Phys. Lett. B 389
1996
Earlier work this paper cites.
B. Alles, L. Cosmai, M. D’Elia, and A. Papa, Phys. Rev. D 62
2000
Earlier work this paper cites.
M. D’Elia, Nucl. Phys. B 661
2003
Earlier work this paper cites.
C. Morningstar and M. J. Peardon, Phys. Rev. D 69
2004
Earlier work this paper cites.
L. Del Debbio, G. M. Manca, and E. Vicari, Phys. Lett. B 594
2004
Earlier work this paper cites.
M. P. Lombardo and A. Trunin, Int. J. Mod. Phys. A 35
Original
2005
Earlier work this paper cites.