Mingling of the infrared and ultraviolet and the "cosmological constant" for interacting QFT in 2d
arXiv:2301.09019 · doi:10.1007/JHEP05(2023)222
Abstract
We propose a proper definition of the vacuum expectation value of the stress energy tensor for integrable quantum field theories in two spacetime dimensions, which is the analog of the cosmological constant in 4d. For a wide variety of models, massive or massless, we show exactly, where is a generalized coupling which we compute and is a basic mass scale. The kinds of models we consider are the massive sinh-Gordon and sine-Gordon theories and perturbations of the Yang-Lee and 3-state Potts models, pure perturbations of infra-red QFT's, and UV completions of the latter which are massless flows between UV and IR fixed points. In the massive case is the mass of the lightest particle and is related to parameters in the 2-body S-matrix. In some examples due to an unbroken fractional supersymmetry. For massless cases, can be a scale of spontaneous symmetry breaking. The "cosmological constant problem" generically arises in the free field limit , thus interactions can potentially resolve the problem at least for most cases considered in this paper. We speculate on extensions of these results to 4 spacetime dimensions and propose ,however without integrability we cannot yet propose a precise manner in which to calculate . Nevertheless, based on cosmological data on , if then the lightest mass particle is on the order of experimental values of proposed neutrino masses.
arXiv comment10 pages; version 2: The only change is our convention for the sign of the vacuum energy , which is now more in line with standard 4d cosmology literature version3: We included the example of the sine-Gordon model which is very illustrative. Previous results didn't change. Version 4: published version in JHEP, primary change is added references
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