The boundary data is an N-dimensional row vector of quaternion entries. ..... expansion with a simple pole, which was sufficient to visualize the monopole energy ...
Nov 11, 2005 - ficient Vm of râmâ1 will be proportional to (âi)m Tr ( ...... I would like to thank my supervisor Pierre van Baal for his scientific guidance, encour-.
Feb 5, 2012 - Specialists in quantum field theory on curved space are engaged in a similar debate ......  http://www.rssd.esa.int/index.php?project=Planck.
May 20, 2012 - However, infrared divergences break de Sitter invariance ... Although this propagator breaks de Sitter invariance because of its gauge fix-.
Mar 8, 2016 - in a tight-binding model hosting Weyl nodes and see that this vector electron-phonon coupling is chiral, providing an example of axial ... best examples so far arose in one spacial dimension (Lut- tinger liquids)  or in two ... tice
Jan 19, 2011 - features will be general relativistic-like and this, in turn, opens the doors to speculate whether .....  J. K. Pachos, M. Stone, K. Temme, Phys.
We explore the 1/4 BPS configurations of the supersymmetric gauge theories on R1+3 Ã S1. The BPS bound for energy and the BPS equations are obtained and the characteristics of the BPS solutions are studied. These BPS configurations describe electric
with recovering the boundary conditions for the caloron and calculating its instanton charge. The caloron constructed from a set of Nahm data is defined using a ...
Mar 9, 2004 - the corresponding symmetric monopoles and symmetric instantons occur as limit- ... only the N = 1 case admits the relevant symmetry. So one ...
Mar 4, 2015 - Brooklyn College, City University of New York. Brooklyn, New York 11210, USA ... Thus it follows that the existence of an arbitrary-charge hyperbolic caloron  is obtained. In the next section, ... we know that the solution remains bo
Sep 30, 2014 - Its Lie algebra is generated by the operators Pa, Mab and D as- .... RabMab. (16) we find. Fa = dea + Ïa b < eb + Ï < ea. Rab = dÏab + Ïa.
Sep 26, 2014 - Woodhouse, have shown3, 4 that one is able to consider a more general geometry. 1 .... that plays the same role as the metric in GR,c which we will call effective metric. Therefore, it is just a matter of ...... ourselves to the interm
dyonic structures, obtained by cooling in order to understand their variety and signature. An analysis of the zero modes of the lattice Dirac .... pendence for any zero mode might be an excel- lent, simple and stable tool to highlight the pres- .....
Oct 9, 2018 - family of Harrington-Shepard calorons , which are (1, 1) calorons with Âµ = 0. These calorons are often referred to as having trivial holonomy.
Jul 26, 2016 - of matter can also arise in fermionic lattices preserving both T and P. We .... The definition of their physical sym- ..... of the form Oss = ei Î± Ï.
May 16, 2007 - In Section 2, we summarise the work of Nye and Singer towards showing that the Nahm transform is an equivalence between calorons and appropriate solutions to Nahm's equations. In Section 3, following in large part on work of Garland an
Sep 10, 2008 - first constructed on Euclidean space by Harrington and Shepard  using the ansatz (2), with. Ï =1+ ÏÎ½2 Î²r sinh(2Ïr/Î²) cosh(2Ïr/Î²) â cos(2Ït/Î²).
Apr 13, 2005 - Thus, hvac defines a map from the compactified spatial manifold,. S2 comp, into S2 internal, and the winding number is the degree of this map.
k d Ï = and. /. 1. z h. k d Ï = Â± planes in Fig. 4(b) carry net topological charges of 2+ and 2- respectively. Thus for arbitrary fixed z k lying between these two planes, the net Berry flux through the reduced 2D BZ is 2Ï and the Chern number is
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Jan 18, 1996 - symmetry . Here, matters are more involved due to the quite different manifestation of this symmetry on the light cone. The paper is organised as follows ..... Ïâ+aâ. +. 1. 2LÏG(â¥)ââiji+aâ jââ. 1. 2. jiG(â¥)[0
Aug 28, 2017 - In this work, we describe a toolbox to realize and probe synthetic axial gauge fields in engineered. Weyl semimetals. These synthetic electromagnetic fields, which are sensitive to the chirality associ- ated with Weyl nodes, emerge due
Sep 10, 2008 - in the action (9) and verifying that their integrals converge. .... one might expect the hyperbolic caloron gauge field to converge to a hyper-.
Calorons in Weyl Gauge Gerald V. Dunne Department of Physics, University of Connecticut, Storrs, CT 06269-3046, USA
Bayram Tekin Theoretical Physics, University of Oxford, 1 Keble Rd., Oxford, OX1 3NP, UK
arXiv:hep-th/0011169v3 13 Feb 2001
We demonstrate by explicit construction that while the untwisted Harrington-Shepard caloron Aµ is manifestly periodic in Euclidean time, with period β = T1 , when transformed to the Weyl (A0 = 0) gauge, the caloron gauge field Ai is periodic only up to a large gauge transformation, with winding number equal to the caloron’s topological charge. This helps clarify the tunneling interpretation of these solutions, and their relation to Chern-Simons numbers and winding numbers.
PACS: 11.15.-q, 11.10.Wx, 11.27.+d Instantons have many important applications in particle physics [1–6]. They may be defined as classical solutions to the Euclidean Yang-Mills equations that minimize the Yang-Mills action within a given topological charge sector. Explicit instanton solutions  can be found by solving the first-order self-duality equation Fµν =
1 ǫµνρσ Fρσ 2
At zero temperature, instantons provide a semiclassical description of tunneling between classical minima of the Yang-Mills potential that are connected by large gauge transformations [8,9]. At finite temperature, the simplest instanton solutions are the untwisted ’calorons’ of Harrington and Shepard . These calorons are solutions to the self-duality equation (1) that are periodic in Euclidean time, with period β = T1 equal to the inverse temperature. At first sight, it may seem puzzling that a periodic solution, with Aµ (~x, t = − β2 ) = Aµ (~x, t = + β2 ), could describe tunneling from one sector to another since the gauge field Aµ is the same at either end. The answer is very simple but illustrative, and does not appear to have been spelled out in detail before. In the Weyl (A0 = 0) gauge, which is most convenient for describing Hamiltonian processes such as tunneling, the coordinate gauge field Ai is not periodic; rather, Ai (~x, t = + β2 ) is related to Ai (~x, t = − β2 ) by a fixed-time large gauge transformation whose winding number is equal to the integer topological charge of the caloron solution. Here we present a simple explicit construction of this gauge transformation, yielding the Weyl gauge form of the caloron. We conclude with some comments concerning the distinction between the caloron solutions and the so-called “periodic instantons” studied in [11–14]. For simplicity, we concentrate in this paper on untwisted calorons , which are related to tunneling between sectors of different Chern-Simons charge; we will not address twisted calorons [15–17], which involve tunneling between different flux sectors. Twisted calorons are important for Yang-Mills-Higgs theory with symmetry breaking, and especially for understanding the monopole content of the theory. The calorons have nontrivial holonomy, characterized by R twisted β a nontrivial Polyakov loop at spatial infinity: P exp 0 dtA0 , and the expectation value of A0 at infinity plays the role of a Higgs expectation value [15–17]. Thus, it is simpler to discuss first the Weyl gauge for untwisted calorons which have a trivial holonomy. In discussing SU(2) instantons, it is convenient to use a radially symmetric ansatz form . Here, we adopt the a conventions of  for the symmetric ansatz for the SU(2) instanton field Aµ = σ2i Aaµ : xi xa xi xa φ1 φ2 − 1 δ − + A1 2 ǫ x + Aai = ia iak k 2 2 r r r r xa Aa0 = A0 (2) r √ where A0 , A1 , φ1 , and φ2 are functions of r = ~x2 and t only. The charge 1 instanton for SU(2) can then be expressed in terms of a single function ρ(r, t), with the ansatz functions in (2) given by: A0 = ∂r ln ρ A1 = −∂0 ln ρ
φ1 = −r ∂0 ln ρ φ2 = 1 + r∂r ln ρ 1
Then the gauge field described by (2,3) satisfies the instanton equation (1) if ρ satisfies the linear equation: ✷ρ = 0. For the zero temperature, charge 1, instanton in SU(2), the function ρ(r, t) can be chosen : ρ=1+
λ2 r 2 + t2
This form corresponds to a single instanton located at the origin in R4 , and with scale parameter λ. This choice is known as the ‘singular gauge’. To facilitate the transformation of the gauge field in (2) into the Weyl (A0 = 0) gauge, we use the fact  that the ansatz fields A0 , A1 , φ1 and φ2 , which appear in (2) and (3), transform in an abelian-like manner under a particular a type of SU(2) gauge transformation on the non-abelian gauge field Aµ = σ2i Aaµ . Namely, if the gauge transformation matrix U has the special form f f i x · ~σ ) sin( ) U (~x, t) = e− 2 f (r,t)ˆx·~σ = cos( ) − i(ˆ 2 2
then the SU(2) gauge transformation, Aµ → A˜µ = U −1 Aµ U +U −1 ∂µ U , has the following effect on the ansatz functions A0 , A1 , φ1 and φ2 : A0 → A˜0 = A0 + ∂0 f A1 → A˜1 = A1 + ∂r f φ1 → φ˜1 = cos f φ1 + sin f φ2
φ2 → φ˜2 = − sin f φ1 + cos f φ2
Thus, to achieve the Weyl gauge, A˜a0 = 0, we simply need a gauge transformation U (~x, t) of the form in (5) where the function f (r, t) satisfies ∂0 f = −∂r ln ρ
For the zero temperature, charge 1, instanton with ρ given by (4), this leads to r t t −√ π + 2 arctan √ f (r, t) = π + 2 arctan r r2 + λ2 r2 + λ2
where we have chosen the constant of integration so that f (r, t = −∞) = 0. The arctan function is understood to take values in the [− π2 , π2 ] branch. The gauge field, A˜ai , in Weyl gauge has the ansatz form (2), with ansatz functions φ˜1 , φ˜2 , A˜1 , (and A˜0 ≡ 0) given by (6). The tunneling interpretation of the instanton solution becomes evident by noting that A˜i is pure gauge at t = ±∞. At t = −∞, A˜ai (~x, t = −∞) = 0
while at t = +∞, A˜ai (~x, t = +∞) =
√ 2πr r 2 +λ2 r2
sin ǫiak xk −
√ 2πr r 2 +λ2
xi xa 2πλ2 xi xa δia − 2 − 2 r (r + λ2 )3/2 r2
where the static gauge function W (~x) is W (~x) = e
− 2i f (r,t=+∞)ˆ x·~ σ
πr xˆ · ~σ = − exp i √ 2 r + λ2
Thus, as t goes from t = −∞ to t = +∞, the instanton gauge field A˜i in Weyl gauge interpolates between the pure gauge A˜i = 0 in (9), and the pure gauge A˜i = W −1 ∂i W in (10). These fields A˜i are neighboring minima (in fact, zeros) of the classical Yang-Mills potential Z 1 V = d3 x Bia Bia (12) 2 2
¿From (9) and (10) we see that these two minima are related by the large gauge transformation W (~x) in (11). Furthermore, the fixed-time gauge transformation in (11) is W (~x) = U (~x, t = +∞), where U (~x, t) is the (timedependent) gauge transformation used to transform to the Weyl gauge. To evaluate the winding number of the i fixed-time gauge transformation W , we note that if a gauge transformation has the form W (~x) = e− 2 g(r)ˆx·~σ , then the winding number N is determined  by the values of g(r) at r = 0 and r = ∞ : Z 1 1 r=∞ [g(r) − sin g(r) ]r=0 (13) N≡ d3 x ǫijk tr W −1 ∂i W W −1 ∂j W W −1 ∂k W = − 2 24π 2π
Thus, for the gauge transformation in (11), we find N = 1. Having reviewed this familiar tunneling interpretation of zero temperature instantons, we now turn to finite temperature instantons, or ‘calorons’. At finite T, the Euclidean time direction is compactified onto the finite interval t ∈ [− β2 , + β2 ], where β = T1 is the inverse temperature. The manifold is now R3 × S 1 , rather than R4 . Instantons are solutions to the same self-duality equation (1), but the gauge fields, being bosonic, satisfy periodic boundary conditions [20,3] on the Euclidean time interval [− β2 , + β2 ]. The untwisted Harrington-Shepard (HS) caloron solution is consistent with the ansatz form described in (2) and (3). The only change is that the function ρ(r, t) becomes  2πr 2 sinh β β 1 2πλ ρ(r, t) = 1 + 2 β 2πr cosh 2πr − cos 2πt β
¯2 1λ sinh r¯ ≡1+ 2 r¯ cosh r¯ − cos t¯
where we have defined the convenient short-hand: r¯ = 2πr β , etc. Note that ρ in (14) satisfies ✷ρ = 0. The caloron solution given by (2), (3) and (14) corresponds to an infinite line of zero temperature instantons, each of scale λ and each at spatial position ~x = 0, lined up along the t axis, with period β. It is straightforward to check that in the zero temperature limit (β → ∞), the expression for ρ(r, t) in (14) reduces smoothly to that in (4), and we recover the zero temperature instanton. At finite T, the caloron solution (2)-(3) is manifestly periodic in t, Aµ (~x, t + β) = Aµ (~x, t), since ρ(r, t) in (14) has period β. To explore the tunneling interpretation of this caloron solution, we transform it to the Weyl gauge. Once again, the Weyl gauge can be attained most easily by using the abelian-like transformation properties (6) of the ansatz functions in (2). The required SU(2) transformation matrix has the form in (5), with f (r, t) satisfying (7), and ρ is now given by (14). The solution to (7) in this case is r¯ t¯ f (r, t) = π + 2 arctan coth( ) tan( ) + 2 2 " #! 2 2 2 ¯2 sinh r¯ + 2¯ ¯ ¯ t¯ λ r(1 + cosh r¯) (λ − 2¯ r ) sinh r¯ − λ r¯ cosh r¯ p π + 2 arctan tan( ) p (15) ¯ 2 r¯ cosh r¯ + (λ ¯ 4 + 4¯ ¯ 2 r¯ cosh r¯ + (λ ¯ 4 + 4¯ 2 r¯ sinh r¯(4λ r2 ) sinh r¯) sinh r¯(4λ r2 ) sinh r¯) where the constant of integration has been chosen so that f (r, t = − β2 ) = 0. Note that this function f (r, t), and hence the gauge transformation U (~x, t) = exp(− 2i f (r, t) x ˆ · ~σ ) that transforms the HS caloron to the Weyl gauge, is manifestly periodic in t, with period β. It is straightforward to check that f (r, t) in (15) reduces smoothly, as β → ∞, to the zero temperature function in (8). Given the function f (r, t) in (15), the caloron fields A˜ai in the Weyl gauge are obtained simply from (2) and (6). To investigate the relation of this caloron solution to quantum tunneling, we evaluate A˜ai at t = ± β2 . At t = − β2 , the ¯2 ansatz fields satisfy A˜1 = φ˜1 = 0, while φ˜2 = [1 + r∂r ln ρ(r, t = − β2 )], where ρ(r, t = − β2 ) = 1 + λ2¯r tanh( r2¯ ). Thus, 2 πr πr πr 2 λ π tanh( ) − sech ( ) β β β β A˜ai (~x, t = − ) = − ǫiak xk (16) λ2 π πr 2 3 βr 1 + tanh( ) rβ
For low temperatures,
2 β A˜ai (~x, t = − ) ∼ − λ2 π 4 T 4 ǫiak xk 2 3 3
which is nonzero, but which vanishes at zero temperature, as in (9). At t = + β2 , the expression for A˜ai (~x, t = + β2 ) is more cumbersome to write out, but it is completely specified by the ansatz form (2) with β β β φ˜1 (r, t = + ) = sin f (r, t = + ) φ2 (r, t = + ) 2 2 2 β β β φ˜2 (r, t = + ) = cos f (r, t = + ) φ2 (r, t = + ) 2 2 2 β β ˜ A1 (r, t = + ) = ∂r f (r, t = + ) 2 2
and where f is given by (15), and φ2 is as in (3). We now ask how A˜ai (~x, t = + β2 ) is related to A˜ai (~x, t = − β2 ). Since the ansatz functions satisfy A˜1 (r, t = − β2 ) = 0, and φ2 (r, t = + β2 ) = φ˜2 (r, t = − β2 ), this shows that A˜ai (~x, t = + β2 ) and A˜ai (~x, t = − β2 ) are related by a gauge transformation β β A˜i (~x, t = + ) = W −1 A˜i (~x, t = − ) W + W −1 ∂i W 2 2
where the static large gauge transformation W (~x) is i
W (~x) = e− 2 f (r,t=+ 2 )ˆx·~σ "
# ¯ 2 − 2¯ ¯2 r¯ cosh r¯ (λ r2 ) sinh r¯ − λ (ˆ x · ~σ ) = − exp iπ p ¯ 2 r¯ cosh r¯ + (λ ¯ 4 + 4¯ r¯ sinh r¯(4λ r2 ) sinh r¯)
Using (13), the winding number of this gauge transformation is r=∞ β 1 β f (r, t = + ) − sin f (r, t = + ) N =− 2π 2 2 r=0 =1
for all inverse temperatures β and scales λ. Notice that (19) shows that in the Weyl gauge the gauge fields A˜i are not strictly periodic. Rather, A˜i is periodic up to a large gauge transformation. This fixed-time gauge transformation is W (~x) = U (~x, t = + β2 ), where U (~x, t) is the time-dependent gauge transformation used to transform to the Weyl gauge. So, just as in the T = 0 case, the initial and final gauge fields, A˜i (~x, t = ∓ β2 ), are related by a static large gauge transformation of unit winding number. But at finite T, these initial and final gauge fields A˜i (~x, t = ∓ β2 ) are not pure gauge. This means that the tunneling at finite T is not between minima of the classical Yang-Mills potential (12), but between fields of higher potential energy. With the ansatz (2), the corresponding magnetic field strength is (and since the instanton solution is self-dual, this also gives the electric field strength) 1 − φ21 − φ22 (∂r φ1 − A1 φ2 ) (∂r φ2 + A1 φ1 ) xi xa a Bi = − ǫiak xk + xi xa (22) δia − 2 + r2 r r r4
˜ a (~x, t) is nonvanishing at t = ∓ β . The magnetic potential energy (12) can be It is straightforward to verify that B i 2 expressed in terms of the ansatz functions in (2) and (3) [since V is gauge invariant, it doesn’t matter whether we use the original gauge or the Weyl gauge] : Z ∞ 1 (23) dr 2(∂r φ1 − A1 φ2 )2 + 2(∂r φ2 + A1 φ1 )2 + 2 (1 − φ21 − φ22 )2 V = 2π r 0 At zero temperature, V (t = ∓∞) = 0, since the zero temperature instanton is a pure gauge at t = ∓∞. But at finite temperature, V (t = ∓ β2 ) is nonzero, even though it approaches zero as β → ∞. It is straightforward to evaluate numerically V in (23) for the zero and finite temperature instantons discussed above. In Figure 1 we plot the potential energy as a function of Euclidean time for the zero temperature instanton for which ρ(r, t) is given by (4), and in Figure 2 for the finite temperature caloron for which ρ(r, t) is given by (14).
FIG. 1. The potential energy (23) as a function of t, at zero temperature. The dashed line is for instanton scale parameter λ = 1, while the solid line has λ = 2. Note that V → 0 at t = ±∞, as the Weyl gauge solutions are pure gauge at t = ±∞.
FIG. 2. The potential energy (23) as a function of t¯ = 2πt , at finite temperature. The dashed line is for scale parameter β ¯ ¯ λ = 1, while the solid line is for λ = 2. Note that V does not vanish at t¯ = ±π, as the Weyl gauge solutions are not pure gauge at t = ± β2 .
We now consider the instanton’s topological charge and its relation with Chern-Simons numbers and winding numbers. Recall that the instanton charge may be expressed as Z 1 Q=− d4 x ǫµνρσ tr (Fµν Fρσ ) 32π 2 Z 2 1 4 (24) ≡ d x ∂µ Kµ , where Kµ = − 2 ǫµνρσ tr Aν ∂ρ Aσ + Aν Aρ Aσ 8π 3 This leads to a natural separation of Q as Z
d CS(t) + dt
d K(r) dr 0 R In terms of the ansatz fields in (2), the Chern-Simons term, CS ≡ d3 xK0 , is Z ∞ 1 dr φ1 φ′2 − φ2 φ′1 − A1 (1 − φ21 − φ22 ) + φ′1 CS(t) = 2π 0 Q=
i h dt −φ1 φ˙2 + φ2 φ˙1 + A0 (1 − φ21 − φ22 ) − φ˙1
Here φ′ and φ˙ denote derivative with respect to r and t respectively. At zero temperature, the t integration in (27) is from −∞ to +∞, while at finite temperature it is over [− β2 , + β2 ]. Note that both CS(t) and K(r) are gauge 5
dependent, while Q itself is gauge invariant. Also note that the last terms in each of CS(t) and K(r) cancel one another in the decomposition (25), but are required for the correct transformation properties of the respective terms. For example, under a gauge transformation of the form (5), the Chern-Simons term changes as Z Z 1 1 3 −1 g d3 x ǫijk tr U −1 ∂i U U −1 ∂j U U −1 ∂k U CS = CS + 2 d x ǫijk ∂i tr ∂j U U Ak + 8π 24π 2 Z ∞ Z ∞ 1 1 d d = CS + (28) dr [(φ2 − 1) sin f + φ1 (cos f − 1)] − dr [f − sin f ] 2π 0 dr 2π 0 dr It is a simple but instructive exercise to check that this nonabelian transformation law agrees with the transformation of (26) under the abelian-like transformations (6) of the ansatz functions, provided one includes the φ′1 term in CS(t) . For the instanton solutions studied in this paper, one can evaluate numerically the functions CS(t) and K(r) in (26) and (27), in the original gauge (3), and in the Weyl gauge A˜i where A˜0 = 0. At zero temperature, with the scalar function ρ(r, t) given by (4), the functions CS(t) and K(r) are plotted in Figures 3 and 4. In this gauge, CS(t = +∞) − CS(t = −∞) = 0, and K(r = ∞) − K(r = 0) = 1. Thus, in this gauge the entire contribution to the instanton charge Q comes from the K(r) term in the decomposition (25). On the other hand, in the Weyl gauge, the g and K(r) ˜ functions CS(t) are plotted in Figures 5 and 6. In the Weyl gauge, the entire contribution to Q comes from the change in the Chern-Simons number. Also note that in the Weyl gauge the Chern-Simons number is an integer at t = ±∞; this is because at t = ±∞ the Weyl gauge field is pure gauge [see (9) and (10)], and for a pure gauge field the Chern-Simons term is equal to the winding number of the corresponding group element. The time-dependent ˆ · ~σ ), with f (r, t) in (8), that transforms from the original singular gauge gauge transformation U = exp(− 2i f (r, t) x to the Weyl gauge can be considered to have a t-dependent winding number N (t) that, from (13) and (8), is a step function in time: N (t) =
1 (1 + sign(t)) 2
This is consistent with the plots in Figures 3 and 5, since the middle term in (28) vanishes in this case. Thus, in the Weyl gauge, the Chern-Simons number provides a meaningful label for the distinct classical wells of the Yang-Mills potential. At t = 0, the Weyl gauge Chern-Simons number is 21 , corresponding to the sphaleron at the peak of the barrier between neighboring wells. The winding number of the gauge transformation U (~x, t) is also 12 when t = 0.
CS 0.5 0.25
-0.25 -0.5 FIG. 3. Plot of the Chern-Simons function CS(t) in (26), in the singular gauge at zero temperature, as a function of t. The instanton scale factor λ has been scaled to 1.
-0.2 -0.4 -0.6 -0.8 -1 FIG. 4. Plot of the function K(r) in (27), in the singular gauge at zero temperature, as a function of r. The instanton scale factor λ has been scaled to 1.
CS 1 0.8 0.6 0.4 0.2 -4
FIG. 5. Plot of the Chern-Simons function CS(t) in (26), in the Weyl gauge at zero temperature, as a function of t. The instanton scale factor λ has been scaled to 1.
-0.05 -0.1 -0.15 -0.2 -0.25 FIG. 6. Plot of the function K(r) in (27), in the Weyl gauge at zero temperature, as a function of r. The instanton scale factor λ has been scaled to 1.
At finite temperature, the situation is similar. The only change is that the scalar function ρ(r, t) is now given by (14), and the t integration in (27) is over the finite interval [− β2 , + β2 ]. In the Harrington-Shepard gauge (3,14), the functions CS(t) and K(r) are plotted in Figures 7 and 8. (These plots, and those in Figs. 9 and 10, are for scale ¯ = 1. For different λ, ¯ the plots have the same form.) Once again, in this gauge, the entire contribution parameter λ to the instanton charge comes from the change in K(r). The corresponding plots for the Weyl gauge are in Figures 9 and 10, and we see that the entire contribution to Q comes from the change CS(t). From the fact (19) that in the Weyl gauge A˜i (t = + β2 ) is related to A˜i (t = − β2 ) by a static gauge transformation of winding number 1, we know g = + β ) − CS(t g = − β ) = 1. But it is interesting to note further that in the Weyl gauge the that the difference CS(t 2 2 7
Chern-Simons number is an integer at t = ± β2 , even though the gauge field is not a pure gauge [see (16) and (19)]. At t = 0, the Weyl gauge Chern-Simons number is 12 , as is the winding number of the gauge transformation U (~x, t) that connects the HS gauge to the Weyl gauge.
CS 0.5 0.25
-0.25 -0.5 FIG. 7. Plot of the Chern-Simons function CS(t) in (26), in the Harrington-Shepard gauge at finite temperature, as a ¯ = 1. function of t¯ = 2πt . The scale factor has been chosen λ β
-0.2 -0.4 -0.6 -0.8 -1 FIG. 8. Plot of the function K(r) in (27), in the Harrington-Shepard gauge at finite temperature, as a function of r¯ = ¯ = 1. The scale factor has been chosen λ
2πr . β
CS 1 0.8 0.6 0.4 0.2 -3
FIG. 9. Plot of the Chern-Simons function CS(t) in (26), in the Weyl gauge at finite temperature, as a function of t¯ = ¯ = 1. The scale factor has been chosen λ
2πt . β
-0.05 -0.1 -0.15 -0.2 -0.25 FIG. 10. Plot of the function K(r) in (27), in the Weyl gauge at finite temperature, as a function of r¯ = ¯ = 1. factor has been chosen λ
2πr . β
In conclusion, we have demonstrated explicitly that while the HS caloron solution is manifestly periodic, so that Aµ (~x, t = + β2 ) = Aµ (~x, t = − β2 ), when transformed to the Weyl (A0 = 0) gauge, the gauge field is periodic up to a large gauge transformation, A˜i (~x, t = + β2 ) = W −1 A˜i (~x, t = − β2 )W + W −1 ∂i W , where W is a fixed-time gauge transformation with integer winding number equal to the caloron’s topological charge. This gauge transformation W connects different Chern-Simons-number sectors of the classical Yang-Mills potential energy, just as is familiar from zero temperature. However, the caloron solution in Weyl gauge interpolates, as t goes from − β2 to + β2 , not between classical minima but between classical gauge fields of nonzero potential energy. Having understood the tunneling interpretation of the HS calorons in Weyl gauge, we conclude with some brief comments concerning the difference between these calorons and the ”periodic instantons” studied in [11–14]. These are very different objects, but the names can be somewhat confusing since calorons are themselves instantons that are periodic in Euclidean time. This distinction, and some of its physical consequences, have been stated clearly in , but we re-iterate these distinctions here in the light of our Weyl gauge calorons. The ”periodic instantons” are most easily introduced in the simple context of a quantum mechanical model; for example, a double well potential V = (q 2 − 1)2 /4. This captures most of the essential physics. This potential model has well-known instanton solutions  that are periodic in Euclidean time t: r t 2ν sn √ − K ;ν , (30) q(t) = 1+ν 1+ν where sn(x; ν) is a Jacobi elliptic function , and the modulus parameter 0 ≤ ν ≤ 1 is related to the energy by E = (ν − 1)2 /(4(ν + 1)2 ). These solutions are manifestly periodic: q(t = − β2 ) = q(t = + β2 ), where the period √ β = 4 1 + ν K(ν), and K(ν) is the elliptic quarter-period . Physically, these periodic instantons correspond to tunneling from one well to the next, and then back again to the original starting position (since they are periodic!). By contrast, the Weyl gauge calorons describe tunneling from one classical well (characterized by Chern-Simons number 0) to the next well (with CS=1); they do not tunnel back again, since the Weyl gauge field A˜i (t = + β2 ) differs from A˜i (t = − β2 ) by a large gauge transformation, as we have demonstrated explicitly in (19,20). This difference between calorons and periodic instantons also manifests itself through the fact that the calorons have nonzero topological charge per period (the explicit ones studied here have Q=1), while the ”periodic instantons” have zero net topological charge per period. For low temperatures, the periodic instantons can be approximated by an infinite chain of alternating zero temperature instantons and anti-instantons. Indeed, this is particularly easy to see in the quantum mechanical double-well potential case (30), owing to the remarkable elliptic function identity: sn
t √ ;ν 1+ν
π = √ ′ 2 νK
π β √ (t − n ) 2 2 1 + νK ′
Here K ′ (ν) ≡ K(1−ν). This leads to the simple interpretation of the periodic instanton in (30) as a series of alternating instantons and anti-instantons. The zero temperature limit corresponds to ν → 1, in which case the period β → ∞, and E → 0, and we approach the usual zero temperature kink-like instantons. But, on the full period [− β2 , β2 ], the sn function reduces to a pair of an anti-kink and a kink. This explains why the net topological charge per period√is zero. It is only on the half-period [0, β2 ] that q(t) approaches the familiar zero temperature instanton: q = tanh(t/ 2). By 9
contrast, the HS caloron is a periodic sum of instantons (and an HS anti-caloron is a periodic sum of anti-instantons), not a periodic sum of alternating instantons and anti-instantons. Indeed, in Yang-Mills theory there is no known exact ”periodic instanton” that is an exact alternating chain of instantons and anti-instantons, although approximate chains of this form have been extensively studied [11,5]. This difference between calorons and periodic instantons can be reconciled because even though the caloron solutions are manifestly periodic, Aµ (t + β) = Aµ (t), since this is a gauge theory, the Aµ are not all independent physical fields; when we transform the caloron to the Weyl gauge we see that the coordinate fields A˜i are periodic only up to a large gauge tranformation. We hope that our explicit construction of the Weyl gauge caloron fields helps to clarify this important distinction between calorons and ”periodic instantons”. Acknowledgments: GD is supported by the U.S. DOE grant DE-FG02-92ER40716.00. GD also thanks Balliol College, Oxford, the Theoretical Physics Department at Oxford, and the CSSM at Adelaide University, where this work was begun. BT is supported by PPARC.
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