English
 
Help Privacy Policy Disclaimer
  Advanced SearchBrowse

Item

ITEM ACTIONSEXPORT

Released

Journal Article

Common source for scalars: Flavored axion-Higgs unification

MPS-Authors
/persons/resource/persons207410

Alanne,  Tommi
Division Prof. Dr. Manfred Lindner, MPI for Nuclear Physics, Max Planck Society;

/persons/resource/persons208912

Blasi,  Simone
Florian Goertz - Max Planck Research Group, Junior Research Groups, MPI for Nuclear Physics, Max Planck Society;

/persons/resource/persons231491

Goertz,  Florian
Florian Goertz - Max Planck Research Group, Junior Research Groups, MPI for Nuclear Physics, Max Planck Society;

External Resource
No external resources are shared
Fulltext (restricted access)
There are currently no full texts shared for your IP range.
Fulltext (public)

1807.10156.pdf
(Preprint), 484KB

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

Alanne, T., Blasi, S., & Goertz, F. (2019). Common source for scalars: Flavored axion-Higgs unification. Physical Review D, 99(01): 015028. doi:10.1103/PhysRevD.99.015028.


Cite as: https://hdl.handle.net/21.11116/0000-0003-35BC-E
Abstract
We propose a unified model of scalar particles that addresses the flavour
hierarchies, solves the strong CP problem, delivers a dark matter candidate,
and provides the trigger for electroweak symmetry breaking. Besides furnishing
a unification of the recently proposed axiflavon with a Goldstone-Higgs sector,
the scenario can also be seen as adding a model of flavour (and strong CP
conservation along with axion dark matter) to elementary Goldstone-Higgs
setups. In particular, we derive bounds on the axion decay constant from the
need to generate a SM-like Higgs potential at low energies, which we confront
with constraints from flavour physics and cosmology. In the minimal
implementation, we find that the axion decay constant is restricted to a thin
stripe of $f_a \approx (10^{11}-10^{12})$ GeV, while adding right-handed
neutrinos allows to realize a heavy-axion model at lower energies, down to $f_a
\sim 10$ TeV.