Abstract
In this article an introduction to the thermal field theory within imaginary time vis-a-vis Matsubara formalism has been discussed in detail. The imaginary time formalism has been introduced through both the operatorial and the functional integration method. The prescription to perform frequency sum for boson and fermion has been discussed in detail. Green’s function both in Minkowski time as well as in Euclidean time has been derived. The tadpole diagram in \(\lambda \phi ^4\) theory and the self-energy in \(\lambda \phi ^3\) theory have been computed and their consequences have also been discussed. The basic features of general two point functions, such as self-energy and propagator, for both fermions and bosons in presence of a heat bath have been discussed. The imaginary time has also been introduced from the relation between the functional integral and the partition function. Then the free partition functions and thermodynamic quantities for scalar, fermion and gauge field, and interacting scalar field have been obtained from first principle calculation. The quantum electrodynamics (QED) and gauge fixing have been discussed in details. The one-loop self-energy for electron and photon in QED have been obtained in hard thermal loop (HTL) approximation. The dispersion properties and collective excitations of both electron and photon in a material medium in presence of a heat bath have been presented. The spectral representation of fermion and gauge boson propagators have been obtained. In HTL approximation, the generalisation of QED results of two point functions to quantum chromodynamics (QCD) have been outlined that mostly involve group theoretical factors. Therefore, one learns about the collective excitations in a QCD plasma from the acquired knowledge of QED plasma excitations. Then, some subtleties of finite temperature field theory have been outlined. As an effective field theory approach the HTL resummation and the HTL perturbation theory (HTLpt) have been introduced. The leading order (LO), next-to-leading order (NLO) and next-to-next-leading order (NNLO) free energy and pressure for deconfined QCD medium created in heavy-ion collisions have been computed within HTLpt. The general features of the deconfined QCD medium have also been outlined with non-perturbative effects like gluon condensate and Gribov–Zwanziger action. The dilepton production rates from quark–gluon plasma with these non-perturbative effects have been computed and discussed in details.
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Notes
One can also get it as a solution of Klein Gordon equation with a unit source term.
We note that the Lorentz invariance is broken at \(T\ne 0\) which we will discuss later in detail. However, E can be written in the rest frame of the medium (heat bath) as \(E=u_\mu K^\mu = u\cdot K\), where u is four velocity of the medium (heat bath) in its rest frame with \(u_\mu =(1,0,0,0)\).
A meromorphic function is a ratio of two well-behaved (holomorphic) functions in complex plane as \(f(z)=g(z)/h(z)\) with \(h(z)\ne 0\). However such a function will still be well-behaved if it has finite order, isolated poles and zeros and no essential singularities or branch cuts in its domain.
At \(m=0\) and \(|k| \rightarrow 0 \, \Rightarrow n_{\rm B}(\omega _k=0) =1/(1-1)\rightarrow \infty\) there is an infrared divergence due to zero bosonic mode caused by \(\omega _n=2\pi n T\) for \(n=0\). We will come back later how can this infrared divergence be regulated.
This identity is a generalisation of the one dimensional Gaussian integral \(\int \nolimits _{-\infty }^\infty \text{d}x \ \ \exp (-\frac{1}{2} a y^2) =\sqrt{2\pi /a}\) and can be shown by expressing the bilinear \({{\textbf{y}}}\cdot {{\widehat{A}}} {{\textbf{y}}}\) in terms of eigenvalues of \({\widehat{A}}\).
The details of HTL approximation will be discussed in Sect. 12.
Singularities from both electric and magnetic sectors.
Equation (13.25) is a one-loop result. In the vacuum, the two-loop result has been computed [160] and the form of Gribov propagator in (13.27) remains unaffected. Only \(\gamma _G\) itself is changed to take into account the two-loop correction. It is expected that this would be valid also at finite temperature.
This procedure only constrains the longitudinal part of the vertex function.
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Acknowledgements
I would like to thank Aritra Bandyopadhyay, Aritra Das, Bithika Karmakar, Chowdhury Aminul Islam, Najmul Haque and Ritesh Ghosh for various discussions and help received during the preparation of this article. It is also a great pleasure to acknowledge the support received from Sanjay Ghosh and Rajarshi Ray who were tutors of my lectures given at SERC Advanced School on Theoretical High Energy Physics, November 16-December 5, 2015 at Birla institute of Technology, Pilani, India. Finally, I would like to thank Department of Atomic Energy, Government of India for the project TPAES in Theory division of Saha Institute of Nuclear Physics.
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A Appendix
A Appendix
1.1 A.1 One-loop fermionic sum integrals
The dimensionally regularized fermionic sum-integrals are defined as,
where \(d-2\epsilon\) is the spatial dimension, P is the fermion loop momentum, \(\Lambda\) is the \(\overline{\text {MS}}\) renormalization scale that introduces the factor \(\left( \frac{e^{\gamma _E}}{4\pi }\right) ^\epsilon\) along with it, where \(\gamma _E\) being the Euler–Mascheroni constant.
The result of various fermionic sum-integrals are listed below:
where the angular integrations are given as
with
1.2 A.2 One-loop bosonic sum integrals
The dimensionally regularized bosonic sum-integrals are defined as,
where \(d-2\epsilon\) is the spatial dimension, P is the boson loop momentum, \(\Lambda\) is the \(\overline{\text {MS}}\) renormalization scale that introduces the factor \(\left( \frac{e^{\gamma _E}}{4\pi }\right) ^\epsilon\) along with it, where \(\gamma _E\) being the Euler–Mascheroni constant.
Below we list various bosonic sum-integrals:
1.3 A.3 Braaten–Pisarski–Yuan (BPY) prescription
Lets consider a complex function f(z) having branch cut
considering \(\xi =x+i\epsilon\), one can write
where the discontinuity is related to the imaginary part of a complex function as
Combining (A.8) and (A.9) one can write
where the spectral density \(\rho\) is defined as
The spectral density \(\rho _1 (\omega _1)\) is related to the any complex function \(F_1(k_0)\) as given in (A.10)
We note that \(K\equiv (k_0,\vec{\varvec{k}})\) is the fermionic momentum with \(k_0 =(2m+1) i\pi T\).
Lets have,
where T is the temperature. Now, considering \(x=(\omega _1-k_0-i\epsilon _1)\) one can write (A.13) as
Combining (A.14) with (A.12), one gets
Now, using \(e^{k_0/T} = e^{(2m+1)i\pi } = -1\), one can write as
Similarly, one can write another complex function \(F_2(q_0)\) as
where \(q_0=(p_0-k_0)\) and P is the bosonic momentum with \(p_0=2mi\pi T\).
We would like to compute the imaginary part of the product of two complex functions \(T\sum _{k_0} F_1(k_0)F_2(q_0)\):
Performing \(\tau _2\)-integration using \(\delta\)-function, one can write
where \(\epsilon =\epsilon _1+\epsilon _2\). Now performing the \(\tau _1\)-integration, one gets
Now using
one gets
where \(\beta =1/T\).
We finally obtain following (A.9) and (A.22), the discontinuity or the imaginary part of a product of two complex functions [81] as
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Mustafa, M.G. An introduction to thermal field theory and some of its application. Eur. Phys. J. Spec. Top. 232, 1369–1457 (2023). https://doi.org/10.1140/epjs/s11734-023-00868-8
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DOI: https://doi.org/10.1140/epjs/s11734-023-00868-8