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Mixed Models: Combining Incompatible Scalar Models in Any Spacetime Dimension

High Energy Physics - Theory 2017-02-01 v2 Mathematical Physics math.MP Quantum Physics

Abstract

Traditionally, covariant scalar field theory models are either super renormalizable, strictly renormalizable, or nonrenormalizable. The goal of `Mixed Models' is to make sense of sums of these distinct examples, e.g., gφ34+gφ36+gφ38g\varphi^4_3+g'\varphi^6_3+g''\varphi^8_3, which includes an example of each kind for spacetime dimension n=3n=3. We show how the several interactions such mixed models have may be turned on and off in any order without any difficulties. Analogous results are shown for gφn4+gφn138g\varphi^4_n+g'\varphi^{138}_n, etc., for all n3n\ge3. Different categories hold for n=2n=2 such as, e.g., gP(φ)2+gN ⁣P(φ)2{g P(\varphi)_2+g' N\!P}(\varphi)_2, that involve polynomial (PP) and suitable nonpolynomial (N ⁣PN\!P) interactions, etc. Analogous situations for n=1n=1 (time alone) offer simple `toy' examples of how such mixed models may be constructed.

Keywords

Cite

@article{arxiv.1605.06725,
  title  = {Mixed Models: Combining Incompatible Scalar Models in Any Spacetime Dimension},
  author = {John R. Klauder},
  journal= {arXiv preprint arXiv:1605.06725},
  year   = {2017}
}

Comments

14 pages

R2 v1 2026-06-22T14:06:32.539Z