Abstract

Nowadays, one needs to consider seriously the possibility that a large separation between the scale of new physics and the electroweak scale exists. Nevertheless, there are still observables in this scenario, in particular the Higgs mass, which are sensitive to the properties of the UV theory. In order to obtain reliable predictions for a model which involves very heavy degrees of freedom, the precise matching to an effective theory is necessary. While this has been so far only studied for a few selected examples, we present an extension of the Mathematica package SARAH to perform automatically the matching between two scalar sectors at the full one-loop level for general models. We show that we can reproduce all important results for commonly studied models like split- or high-scale supersymmetry. One can now easily go beyond that and study new ideas involving very heavy states, where the effective model can either be just the standard model or an extension of it. Also scenarios with several matching scales can be easily considered. We provide model files for the MSSM with seven different mass hierarchies as well as two high-scale versions of the NMSSM. Moreover, it is explained how new models are implemented.

Highlights

  • Even if states beyond the Standard Model (SM) (BSM) are too heavy to be produced at current colliders, they often still have an in-print in experimental results, see e.g. Refs. [18,19]

  • In order to obtain reliable predictions for a model which involves very heavy degrees of freedom, the precise matching to an effective theory is necessary. While this has been so far only studied for a few selected examples, we present an extension of the Mathematica package SARAH to perform automatically the matching between two scalar sectors at the full one-loop level for general models

  • In terms of the effective field theory (EFT) ansatz this means that the full model involving heavy and light states must be matched to an effective theory at the scale at which the heavy degrees of freedom are integrated out

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Summary

Introduction

Even if states beyond the SM (BSM) are too heavy to be produced at current colliders, they often still have an in-print in experimental results, see e.g. Refs. [18,19]. C (2019) 79:163 a large uncertainty in the prediction of the numerical value of mh [23,24,25,26] This can be resolved either by the standard ansatz of an effective field theory (EFT) in which the heavy states are integrated out [27,28,29,30,31,32,33,34,35,36], or by a hybrid method in which the fixed-order calculation is combined with the higher-order leading logarithms extracted from an EFT [37,38,39,40].

General ansatz
Renormalisation scheme
Parametrisation of the results at the matching scale
General information about SARAH and SPheno
Available options to perform the matching
Analytical approach
Interactive mode: calculating individual matching conditions
Run SPheno
Matching at two scales
Numerical approach
One matching scale without RGE running above
Copy the files and compile SPheno
Running above the matching scale
Several matching scales
Included models and input files in SARAH
Low-energy limits of the MSSM
Split-SUSY
High-scale SUSY
High-scale NMSSM
Summary
A.1.1: Quartic couplings
A.1.3: Bilinear parameters
A.2.3: Wave-function corrections
B: IR-safe loop-functions
B.1: One- and two-point integrals The tadpole integral A0 is given by
B.4: Derivatives of the loop-functions
RealParameters
RenormalizationScale
Full Text
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