Fine tuning in the constrained exceptional supersymmetric standard model
Fine tuning in the constrained exceptional supersymmetric standard model
Supersymmetric unified models in which the Z ? couples to the Higgs doublets, as in the E 6 class of models, have large fine tuning dominated by the experimental mass limit on the Z ? . To illustrate this, we investigate the degree of fine tuning throughout the parameter space of the constrained exceptional supersymmetric standard model (cE 6 SSM ) that is consistent with a Higgs mass m h ?125??GeV . Fixing tan?=10 , and taking specific values of the mass of the Z ? boson, with M Z ? ?2–4??TeV , we find that the minimum fine tuning is set predominantly from the mass of Z ? and varies from ?200 to 400 as we vary M Z ? from ?2 to 4 TeV. However, this is significantly lower than the fine tuning in the constrained minimal supersymmetric standard model, of O(1000) , arising from the large stop masses required to achieve the Higgs mass.
1-15
Athron, P.
5ac03b61-f44c-466f-b6ee-28fef4e3ab27
Binjonaid, Maien
f649290f-12fb-4663-836f-ff09d4d7854b
King, S. F.
f8c616b7-0336-4046-a943-700af83a1538
2013
Athron, P.
5ac03b61-f44c-466f-b6ee-28fef4e3ab27
Binjonaid, Maien
f649290f-12fb-4663-836f-ff09d4d7854b
King, S. F.
f8c616b7-0336-4046-a943-700af83a1538
Athron, P., Binjonaid, Maien and King, S. F.
(2013)
Fine tuning in the constrained exceptional supersymmetric standard model.
Physical Review D, 87 (11), .
(doi:10.1103/PhysRevD.87.115023).
Abstract
Supersymmetric unified models in which the Z ? couples to the Higgs doublets, as in the E 6 class of models, have large fine tuning dominated by the experimental mass limit on the Z ? . To illustrate this, we investigate the degree of fine tuning throughout the parameter space of the constrained exceptional supersymmetric standard model (cE 6 SSM ) that is consistent with a Higgs mass m h ?125??GeV . Fixing tan?=10 , and taking specific values of the mass of the Z ? boson, with M Z ? ?2–4??TeV , we find that the minimum fine tuning is set predominantly from the mass of Z ? and varies from ?200 to 400 as we vary M Z ? from ?2 to 4 TeV. However, this is significantly lower than the fine tuning in the constrained minimal supersymmetric standard model, of O(1000) , arising from the large stop masses required to achieve the Higgs mass.
Other
PhysRevD.87.115023
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Available under License Other.
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Published date: 2013
Organisations:
Physics & Astronomy
Identifiers
Local EPrints ID: 369411
URI: http://eprints.soton.ac.uk/id/eprint/369411
ISSN: 1550-7998
PURE UUID: 34eeac90-6723-436e-b01d-f0096e08f190
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Date deposited: 25 Sep 2014 13:50
Last modified: 14 Mar 2024 18:03
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Author:
P. Athron
Author:
Maien Binjonaid
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