Abstract

The present paper is the first in a series that addresses the calculation of the full one-loop corrections of dark matter (DM) annihilation cross sections in the low mass region of the inert doublet model (IDM). This series is a sequel to our recent publication concerning these corrections in the high mass region. We first review the renormalization of the model both in a fully on shell (OS) scheme as well as in a mixed scheme that combines on shell (for the masses) and a $\overline{\mathrm{MS}}$ approach when the partial invisible width is closed and does not allow the use of a full OS scheme. The scale dependence introduced by the mixed scheme is shown to be tracked through an analysis of a parametrization of the tree-level cross section and the $\ensuremath{\beta}$ constant of a specific coupling; this analysis could be followed in theories. We discuss how to minimize the scale dependence. The theoretical uncertainty brought by the scale dependence leads us to introduce a new criterion on the perturbativity of the IDM. This criterion further delimits the allowed parameter space, which we investigate carefully by including a host of constraints, both theoretical and experimental, including in particular, new data from the LHC. We come up with a set of benchmark points that cover three different mechanisms for a viable relic density of DM: (i) a dominance of coannihilation into a fermion pair, (ii) annihilation into two vector bosons of which one is off shell that requires the calculation of a $2\ensuremath{\rightarrow}3$ process, (iii) annihilation that proceeds through the very narrow standard model Higgs resonance. Since the $2\ensuremath{\rightarrow}3$ vector boson channel features in all three channels and is essentially a buildup on the simpler annihilation to OS vector bosons, we study the latter in detail in the present paper. We confirm again that the corrected cross sections involve a parameter that can be considered as rescattering in the dark sector, which a tree-level computation is not sensitive to. The setup of the renormalization detailed in the present paper will be the backbone of the accompanying papers where each mechanism requires, calculationally, a specific treatment. One-loop corrections to $2\ensuremath{\rightarrow}3$ processes for DM annihilation are technically challenging and have not been attempted before. We dedicate one of the accompanying papers to such a computation. The one-loop correction in the presence of a resonance will be presented separately since we need to supplement our general schemes with a complex scheme. For the coannihilation into fermions, our study will show that the annihilation cross sections can be excellently parametrized through simple effective couplings.

Highlights

  • Cosmology has entered the era of precision measurements

  • As will be shown in this series, the parameter dependence for the one-loop improved analyses of the relic density is larger than that based on tree-level calculations; a crucial parameter of the inert doublet model (IDM) model only appears at one-loop

  • We show the values of the Higgs boson to diphoton signal strength that includes the IDM contribution, should this observable be better constrained in future LHC analyses

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Summary

INTRODUCTION

Cosmology has entered the era of precision measurements. One such measurement is the inferred relic density of dark matter (DM) that is determined at the percent level [1]. Next-to-leading order (NLO) corrections to DM direct detection have been calculated in some cases [41,42,43,44,45,46,47,48,49,50,51] In this series of papers, we will tackle the computation of many annihilation rates that occur in different viable scenarios of the inert double model (IDM) [52,53,54], in particular the low mass DM region in this model, beyond the tree-level approximation. As will be shown in this series, the parameter dependence for the one-loop improved analyses of the relic density is larger than that based on tree-level calculations; a crucial parameter of the IDM model only appears at one-loop This indirect effect is akin to the indirect dependence of LEP observables on the top and Higgs masses.

THE MODEL AND THE PARAMETERS
Automation of the calculation
The SM parameters
Gauge fixing
On shell renormalization for the masses of the IDM scalars
The β constant for βλL
PRESENT CONSTRAINTS ON THE PARAMETER SPACE OF THE IDM
Dark matter direct detection
Stability of the potential
Tree-level unitarity
Direct searches at LEP
Characteristics of the benchmarks points
Cross sections and velocity dependence
THE DIFFERENT STEPS IN THE CALCULATION OF THE RELIC DENSITY
Findings
VIII. CONCLUSIONS
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