SU(N) caloron with non-trivial holonomy and its fermionic determinant. Sergey Slizovskiy, Nikolay Gromov Petersburg INP Outline of the talk Finite temperature QCD Non-trivial holonomy Caloron with non-trivial holonomy, Nc>2. Monopole constituents Why and when to expect calorons with nontrivial holonomy Partition function, role of zero modes ADHMN construction The fermionic determinant. 2 Finite temperature QCD The finite-temperature behavior of any theory is specified by the partition function For QCD one finds (Abers and Lee, 1973; Faddeev, 1976) The functional integral is restricted to fields satisfying the periodicity conditions 3 Non-trivial holonomy All fields with finite energy can be classified by the behavior of the Polyakov line = holonomy at spatial infinity topological charge and magnetic charges 4 Calorons with non-trivial holonomy Exact solutions with topological charge 1 Constructed in 1998 by Kraan, van Baal, Lee, Lu. Composed of Nc monopole constituents Reduce to the periodical instanton at trivial holonomy. Action density of SU(3) caloron 5 BPS Dyon • Static SU(2) field configuration with unit electric and magnetic charges. It is embedded in the SU(n) along the simple roots. • A4 plays the role of the Higgs field and assumed to be Abelian (lies in the Cartan cubalgebra). 6 Dyon embedding M dyons Becomes time dependent! 7 Field near dyon The field near the embedded dyon is composed of Constant part – orthogonal to the root And the dyon part along t1 , t2 , t3 8 Far field – simple formula. Dyon sizes are calculated to be The asymptotic gauge field is 9 Why could we expect the nontrivial holonomy? 1-loop quantum corrections (non-zero modes) prefer trivial holonomy, but at non-trivial holonomy the moduli space is richer, which could overwhelm the non-zero mode determinant. Some lattice simulations confirm these expectations. 10 Partition function with fermions. The contribution of one caloron configuration is zero, since it has an exact zero mode. Only caloron – anticaloron ensembles with zero topological charge could contribute. The would be zero modes are localized on only one dyon in the caloron. (M.Chernodub, P.van Baal et al. ) It leads to attraction between certain types of constituent dyons from different calorons and anticalorons. Non-zero modes are accounted for by the functional determinant in the fundamental representation 11 Calculation of the determinant Calculate the variation of the determinant in the far-field limit: In the dyon core In the rest space Find the integration constant. Reduce the configuration to the SU(N-1) ! …! SU(2) by moving the parameters. Find the variation of determinant during this reduction. Add the known SU(2) result. 12 Periodicity issues There are N different calorons with the same action density. They are related by the nonperiodical gauge transformation e2 i t k/N for integer k. It is equivalent to twisting the periodic propagator: Adding a matrix proportional to the unit matrix to the gauge field is also equivalent to the additional twist of the propagator. We have found a simple exact universal recipe to account for these twists. 13 The variation: general formulas 14 Currents We separate the current J=Jsingular+Jregular according to n=0 and n 0 terms in the propagator and use the standard regularization for the singular current. With exponential precision the result is just J(x) = P’(A4(x)) It suggests the need of unified treatment without separation, which is still missing. 15 Atiyah-Drinfeld-Hitchin-Manin-Nahm (ADHMN) construction of SU(N) caloron 16 ADHM expression for the gauge field 17 ADHMN Green’s function 18 ADHM expressions for the currents. The singular current is The regular current is We have proved that the regular current is a total derivative and so can be calculated exactly from the exponential precision limit of ADHMN construction 19 Results for the currents We have calculated the total current far from the monopoles. We proved explicitly that the dyon core regions are the same as in the SU(2) case plus constant field part, equivalent to the twist. So we easily extract the core currents from our previous work.* Since the twist changes only the regular current, only the P(v) terms are simply changed to P(v+twist) * 20 Finding a constant To find a constant in the determinant we reduce the SU(N) configuration to SU(N-1) We found explicitly the SU(N-1) ADHMN construction when i ! i+1 and the i-th dyon is situated on the line connecting the (i-1) with (i+1) dyons! We have proved that the blowed up i-th dyon does not contribute to the constant. 21 The result = for anti-periodic boundary conditions and is a Pauli-Villars mass. 22 Thak you! Спасибо! Merci! Danke! Tack! 23
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