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Advances in perturbative thermal field theory - Ultra-relativistic ...

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394 U Kraemmer and A Rebhan<br />

Orig<strong>in</strong>ally, the Debye mass (squared) has been def<strong>in</strong>ed as the IR limit 00 (ω = 0,k → 0),<br />

which <strong>in</strong>deed is correct at the HTL level (cf (5.17)).<br />

In QED, this def<strong>in</strong>ition has the advantage of be<strong>in</strong>g directly related to the electric<br />

susceptibility, i.e. the second derivative of the thermodynamic pressure with respect to the<br />

chemical potential, µ, so that the higher-order terms available for the latter also determ<strong>in</strong>e<br />

those of QED<br />

00<br />

(ω = 0,k → 0) through [215, 8]<br />

∣ ( √ ···)<br />

00 (0,k → 0)| µ=0 = e 2 ∂2 P ∣∣∣µ=0<br />

= e2 T 2<br />

1 − 3e2 3e<br />

3<br />

∂µ 2 3 8π + 2 4π + . (7.3)<br />

3<br />

This result is gauge-<strong>in</strong>dependent because <strong>in</strong> QED all of µν is.<br />

In the case of QCD, there is no such relation. Moreover, δm 2 D / ˆm2 D ∼ g rather than g3<br />

because of gluonic self-<strong>in</strong>teractions and Bose enhancement. The calculation of this quantity<br />

should be much easier than the dynamic ones considered earlier because <strong>in</strong> the static limit the<br />

HTL effective action collapses to just the local, bil<strong>in</strong>ear HTL Debye mass term,<br />

HTL static<br />

L −→ − 1 2 ˆm2 D trA2 0 . (7.4)<br />

This is also gauge-<strong>in</strong>variant because A 0 behaves like an adjo<strong>in</strong>t scalar under time-<strong>in</strong>dependent<br />

gauge transformations. Resummed perturbation <strong>theory</strong> for static quantities thus reduces to a<br />

resummation of the HTL Debye mass <strong>in</strong> the electrostatic propagator [310, 114, 8].<br />

However, <strong>in</strong> QCD this simple (‘r<strong>in</strong>g’) resummation leads to the gauge-dependent<br />

result [345]<br />

√<br />

00 (0, 0)<br />

ˆm 2 = 1+α N 6<br />

g, (7.5)<br />

D<br />

4π 2N + N f<br />

where α is the gauge parameter of general covariant gauge (which co<strong>in</strong>cides with general<br />

Coulomb gauge <strong>in</strong> the static limit).<br />

This result was <strong>in</strong>itially <strong>in</strong>terpreted as mean<strong>in</strong>g either that the non-Abelian Debye mass<br />

could not be obta<strong>in</strong>ed <strong>in</strong> resummed perturbation <strong>theory</strong> [346] or that one should use a<br />

physical gauge <strong>in</strong>stead [196, 8]. In particular, the temporal axial gauge was put forward<br />

because <strong>in</strong> this gauge there is, as <strong>in</strong> QED, a l<strong>in</strong>ear relationship between electric <strong>field</strong> strength<br />

correlators and the gauge propagator. However, because static r<strong>in</strong>g resummation clashes with<br />

the temporal gauge, <strong>in</strong>conclusive and contradict<strong>in</strong>g results were obta<strong>in</strong>ed by different authors<br />

[347, 348, 196]. A consistent calculation <strong>in</strong> fact requires vertex resummations [349, 350],<br />

but this does not resolve the gauge-dependence issue because the non-Abelian <strong>field</strong> strength<br />

correlator is gauge-variant [351].<br />

On the other hand, <strong>in</strong> view of the gauge-dependence identities discussed <strong>in</strong> section 5.1.1,<br />

the gauge-dependence of (7.5) is no longer surpris<strong>in</strong>g. Gauge-<strong>in</strong>dependence can only be<br />

expected ‘on-shell’, which here means ω = 0butk 2 →−ˆm 2 D .<br />

Indeed, the exponential fall-off of the electrostatic propagator is determ<strong>in</strong>ed by the position<br />

of the s<strong>in</strong>gularity of B (0,k), and not simply by its IR limit. This implies <strong>in</strong> particular that<br />

one should use a different def<strong>in</strong>ition of the Debye mass already <strong>in</strong> QED, despite the gauge<strong>in</strong>dependence<br />

of (7.3), namely [352]<br />

m 2 D = 00(0,k)| k 2 →−m . (7.6)<br />

2 D<br />

For QED (with massless electrons), the Debye mass is thus not given by (7.3) but rather<br />

as [352]<br />

m 2 D = 00(0,k → 0) +[ 00 (0,k)| k 2 =−m 2 − 00(0,k → 0)]<br />

D<br />

√<br />

= e2 T 2 (1 − 3e2 3e<br />

3<br />

[<br />

3 8π + e2<br />

+ ···− ln ˜µ<br />

2 4π 3 6π 2 πT + γ E − 4 ] )<br />

+ ··· , (7.7)<br />

3

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