Expectations for the muon g − 2 in simplified models with dark matter

Abstract We investigate simplified models of new physics that can accommodate the measured value of the anomalous magnetic moment of the muon and the relic density of dark matter. We define a set of renormalizable, SU(2)×U(1) invariant extensions of the Standard Model, each comprising an inert ℤ 2-o...

Full description

Bibliographic Details
Main Authors: Kamila Kowalska, Enrico Maria Sessolo
Format: Article
Language:English
Published: SpringerOpen 2017-09-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP09(2017)112
id doaj-20477faf94864e43852a94a04d69a7bb
record_format Article
spelling doaj-20477faf94864e43852a94a04d69a7bb2020-11-24T21:41:42ZengSpringerOpenJournal of High Energy Physics1029-84792017-09-012017913710.1007/JHEP09(2017)112Expectations for the muon g − 2 in simplified models with dark matterKamila Kowalska0Enrico Maria Sessolo1Institut für Physik, Technische Universität DortmundInstitut für Physik, Technische Universität DortmundAbstract We investigate simplified models of new physics that can accommodate the measured value of the anomalous magnetic moment of the muon and the relic density of dark matter. We define a set of renormalizable, SU(2)×U(1) invariant extensions of the Standard Model, each comprising an inert ℤ 2-odd scalar field and one or more vector-like pairs of colorless fermions that communicate to the muons through Yukawa-type interactions. The new sectors are classified according to their transformation properties under the Standard Model gauge group and all models are systematically confronted with a variety of experimental constraints: LEP mass bounds, direct LHC searches, electroweak precision observables, and direct searches for dark matter. We show that scenarios featuring only one type of new fermions become very predictive once the relic density and collider constraints are taken into account, as in this case (g − 2) μ is not enhanced by chirality flip. Conversely, for models where an additional source of chiral-symmetry violation is generated via fermion mixing, the constraints are much looser and new precision experiments with highly suppressed systematic uncertainties may be required to test the parameter space.http://link.springer.com/article/10.1007/JHEP09(2017)112Phenomenological Models
collection DOAJ
language English
format Article
sources DOAJ
author Kamila Kowalska
Enrico Maria Sessolo
spellingShingle Kamila Kowalska
Enrico Maria Sessolo
Expectations for the muon g − 2 in simplified models with dark matter
Journal of High Energy Physics
Phenomenological Models
author_facet Kamila Kowalska
Enrico Maria Sessolo
author_sort Kamila Kowalska
title Expectations for the muon g − 2 in simplified models with dark matter
title_short Expectations for the muon g − 2 in simplified models with dark matter
title_full Expectations for the muon g − 2 in simplified models with dark matter
title_fullStr Expectations for the muon g − 2 in simplified models with dark matter
title_full_unstemmed Expectations for the muon g − 2 in simplified models with dark matter
title_sort expectations for the muon g − 2 in simplified models with dark matter
publisher SpringerOpen
series Journal of High Energy Physics
issn 1029-8479
publishDate 2017-09-01
description Abstract We investigate simplified models of new physics that can accommodate the measured value of the anomalous magnetic moment of the muon and the relic density of dark matter. We define a set of renormalizable, SU(2)×U(1) invariant extensions of the Standard Model, each comprising an inert ℤ 2-odd scalar field and one or more vector-like pairs of colorless fermions that communicate to the muons through Yukawa-type interactions. The new sectors are classified according to their transformation properties under the Standard Model gauge group and all models are systematically confronted with a variety of experimental constraints: LEP mass bounds, direct LHC searches, electroweak precision observables, and direct searches for dark matter. We show that scenarios featuring only one type of new fermions become very predictive once the relic density and collider constraints are taken into account, as in this case (g − 2) μ is not enhanced by chirality flip. Conversely, for models where an additional source of chiral-symmetry violation is generated via fermion mixing, the constraints are much looser and new precision experiments with highly suppressed systematic uncertainties may be required to test the parameter space.
topic Phenomenological Models
url http://link.springer.com/article/10.1007/JHEP09(2017)112
work_keys_str_mv AT kamilakowalska expectationsforthemuong2insimplifiedmodelswithdarkmatter
AT enricomariasessolo expectationsforthemuong2insimplifiedmodelswithdarkmatter
_version_ 1725920351000461312