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Hamiltonian finite-temperature quantum field theory from its vacuum on partially compactified space | Hugo Reinhardt
; | Date: |
21 Apr 2016 | Abstract: | The partition function of a relativistic invariant quantum field theory is
expressed by its vacuum energy calculated on a spatial manifold with one
dimension compactified to a 1-sphere $S^1 (eta)$, whose circumference $eta$
represents the inverse temperature. Explicit expressions for the usual energy
density and pressure in terms of the energy density on the partially
compactified spatial manifold $mathbb{R}^2 imes S^1 (eta)$ are derived. To
make the resulting expressions mathematically well-defined a Poisson
resummation of the Matsubara sums as well as an analytic continuation in the
chemical potential are required. The new approach to finite-temperature quantum
field theories is advantageous in a Hamilton formulation since it does not
require the usual thermal averages with the density operator. Instead, the
whole finite-temperature behaviour is encoded in the vacuum wave functional on
the spatial manifold $mathbb{R}^2 imes S^1 (eta)$. We illustrate this
approach by calculating the pressure of a relativistic Bose and Fermi gas and
reproduce the known results obtained from the usual grand canonical ensemble.
As a first non-trivial application we calculate the pressure of Yang-Mills
theory as function of the temperature in a quasi-particle approximation
motivated by variational calculations in Coulomb gauge. | Source: | arXiv, 1604.6273 | Services: | Forum | Review | PDF | Favorites |
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