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Nature of Roberge-Weiss transition end points for heavy quarks in $N_f=2$ lattice QCD with Wilson fermions

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arxiv 1405.2425 v2 pith:4H6TB4TA submitted 2014-05-10 hep-lat

classification hep-lat
keywords pointstransitionchemicalimaginarynaturepotentialsimulationsfermions
verification ladder T0 review T1 audit T2 compute T3 formal

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abstract

The phase structure of QCD with imaginary chemical potential provides information on the phase diagram of QCD with real chemical potential. With imaginary chemical potential $i\mu_I=i\pi T$, previous studies show that the Roberge-Weiss (RW) transition end points are triple points at both large and small quark masses, and second order transition points at intermediate quark masses. The triple and second order end points are separated by two tricritical ones. We present simulations with $ N_f=2 $ Wilson fermions to investigate the nature of RW transition end points. The simulations are carried out at 8 values of the hopping parameter $\kappa$ ranging from 0.020 to 0.140 on different lattice volumes. The Binder cumulant, susceptibility and reweighted distribution of the imaginary part of Polyakov loop are employed to determine the nature of RW transition end points. The simulations show that the two tricritical points are within the range $0.070-0.080$ and $0.120-0.140$, respectively.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Topological properties around the Roberge-Weiss transition in $N_f = 2 + 1 + 1$ QCD

    hep-lat 2026-08 conditional novelty 6.0 of 10

    Along the Roberge-Weiss line in 2+1+1 flavor QCD, the topological charge cumulant b2 becomes compatible with the dilute instanton gas value as soon as T exceeds T_RW, like in pure gauge theory.

  2. The Roberge-Weiss endpoint in $(2+1)$-flavor QCD with background magnetic fields

    hep-lat 2024-12 conditional novelty 6.0 of 10

    A background magnetic field lowers the Roberge-Weiss temperature in (2+1)-flavor QCD and turns the transition from second to first order between eB=1.0 and 2.5 GeV^2.

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