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Finite-temperature Field Theory - Theoretical Physics (TIFR)

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Basics of Statistical <strong>Physics</strong> and Thermodynamics<br />

Scalar fields at finite <strong>temperature</strong><br />

Interacting scalar fields<br />

Partition function for scalar field theory<br />

Non-interacting examples<br />

◮ Expand fields in terms of their Fourier modes<br />

◮<br />

ϕ(τ, x) = T ∑ ∫<br />

d 3 p<br />

ei(p·x+ωnτ)<br />

(2π) 3 ϕ n (p),<br />

n<br />

ω n = 2nπT , n ∈ Z<br />

Fourier series in τ direction due to compactness of<br />

temporal direction<br />

◮ Now, a short exercise produces (up to T -indep. constant)<br />

ln Z = − V ∑<br />

∫<br />

d 3 (<br />

p<br />

2 (2π) 3 ln n 2 + β2 (p 2 + m 2 )<br />

)<br />

(2π) 2 n<br />

∫ [√<br />

d 3 p p<br />

= −V<br />

2 + m 2<br />

(2π) 3 + ln<br />

(1 − e −β√ p 2 +m 2) ]<br />

2T<br />

◮ Reminiscent of point particle result for bosons!<br />

logo<br />

Aleksi Vuorinen, CERN<br />

<strong>Finite</strong>-<strong>temperature</strong> <strong>Field</strong> <strong>Theory</strong>

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