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...
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Online Access: | http://link.springer.com/article/10.1007/JHEP09(2017)112 |
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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 |