New physics explanations of aμ in light of the FNAL muon g − 2 measurement
A bstract The Fermilab Muon g − 2 experiment recently reported its first measurement of the anomalous magnetic moment a μ FNAL , which is in full agreement with the previous BNL measurement and pushes the world average deviation ∆ a μ 2021 from the Standard Model to a significance of 4 . 2 σ . Here...
Saved in:
| Published in: | The journal of high energy physics Vol. 2021; no. 9; pp. 1 - 115 |
|---|---|
| Main Authors: | , , , , , |
| Format: | Journal Article |
| Language: | English |
| Published: |
Berlin/Heidelberg
Springer Berlin Heidelberg
14.09.2021
Springer Nature B.V SpringerOpen |
| Subjects: | |
| ISSN: | 1029-8479, 1029-8479 |
| Online Access: | Get full text |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
| Summary: | A
bstract
The Fermilab Muon
g −
2 experiment recently reported its first measurement of the anomalous magnetic moment
a
μ
FNAL
, which is in full agreement with the previous BNL measurement and pushes the world average deviation
∆
a
μ
2021
from the Standard Model to a significance of 4
.
2
σ
. Here we provide an extensive survey of its impact on beyond the Standard Model physics. We use state-of-the-art calculations and a sophisticated set of tools to make predictions for
a
μ
, dark matter and LHC searches in a wide range of simple models with up to three new fields, that represent some of the few ways that large ∆
a
μ
can be explained. In addition for the particularly well motivated Minimal Supersymmetric Standard Model, we exhaustively cover the scenarios where large ∆
a
μ
can be explained while simultaneously satisfying all relevant data from other experiments. Generally, the
a
μ
result can only be explained by rather small masses and/or large couplings and enhanced chirality flips, which can lead to conflicts with limits from LHC and dark matter experiments. Our results show that the new measurement excludes a large number of models and provides crucial constraints on others. Two-Higgs doublet and leptoquark models provide viable explanations of
a
μ
only in specific versions and in specific parameter ranges. Among all models with up to three fields, only models with chirality enhancements can accommodate
a
μ
and dark matter simultaneously. The MSSM can simultaneously explain
a
μ
and dark matter for Bino-like LSP in several coannihilation regions. Allowing under abundance of the dark matter relic density, the Higgsino- and particularly Wino-like LSP scenarios become promising explanations of the
a
μ
result. |
|---|---|
| Bibliography: | ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 14 |
| ISSN: | 1029-8479 1029-8479 |
| DOI: | 10.1007/JHEP09(2021)080 |