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Journal Article

Fits to SO(10) Grand Unified Models

MPS-Authors
http://pubman.mpdl.mpg.de/cone/persons/resource/persons30429

Dück,  Alexander
Werner Rodejohann - ERC Starting Grant, Junior Research Groups, MPI for Nuclear Physics, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons30951

Rodejohann,  Werner
Werner Rodejohann - ERC Starting Grant, Junior Research Groups, MPI for Nuclear Physics, Max Planck Society;

Fulltext (public)

1306.4468.pdf
(Preprint), 418KB

Supplementary Material (public)
There is no public supplementary material available
Citation

Dück, A., & Rodejohann, W. (2013). Fits to SO(10) Grand Unified Models. Journal of high energy physics: JHEP, 2013(09): 24, pp. 1-34. doi:10.1007/JHEP09(2013)024.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0014-5482-8
Abstract
We perform numerical fits of Grand Unified Models based on SO(10), using various combinations of 10-, 120- and 126-dimensional Higgs representations. Both the supersymmetric and non-supersymmetric versions are fitted, as well as both possible neutrino mass orderings. In contrast to most previous works, we perform the fits at the weak scale, i.e. we use RG evolution from the GUT scale, at which the GUT-relations between the various Yukawa coupling matrices hold, down to the weak scale. In addition, the right-handed neutrinos of the seesaw mechanism are integrated out one by one in the RG running. Other new features are the inclusion of recent results on the reactor neutrino mixing angle and the Higgs mass (in the non-SUSY case). As expected from vacuum stability considerations, the low Higgs mass and the large top-quark Yukawa coupling cause some pressure on the fits. A lower top-quark mass, as sometimes argued to be the result of a more consistent extraction from experimental results, can relieve this pressure and improve the fits. We give predictions for neutrino masses, including the effective one for neutrinoless double beta decay, as well as the atmospheric neutrino mixing angle and the leptonic CP phase for neutrino oscillations.