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Scale-independent inflation and hierarchy generation

Abstract:
We discuss models involving two scalar fields coupled to classical gravity that satisfy the general criteria: (i) the theory has no mass input parameters, (ii) classical scale symmetry is broken only through −ςϕ 2 R couplings where ς departs from the special conformal value of 1; (iii) the Planck mass is dynamically generated by the vacuum expectations values (VEVs) of the scalars (iv) there is a stage of viable inflation associated with slow roll in the two-scalar potential; (v) the final vacuum has a small to vanishing cosmological constant and an hierarchically small ratio of the VEVs and the ratio of the scalar masses to the Planck scale. This assumes the paradigm of classical scale symmetry as a custodial symmetry of large hierarchies.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1016/j.physletb.2016.10.036

Authors


More by this author
Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics; Astrophysics
Oxford college:
Oriel College
Role:
Author
More by this author
Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics; Theoretical Physics
Role:
Author


Publisher:
Elsevier
Journal:
Physics Letters B More from this journal
Volume:
763
Pages:
174-178
Publication date:
2016-10-01
Acceptance date:
2016-10-17
DOI:
EISSN:
1873-2445
ISSN:
0370-2693


Keywords:
Pubs id:
pubs:611975
UUID:
uuid:a61da81e-9bee-40ba-ad7e-24c45d16883c
Local pid:
pubs:611975
Source identifiers:
611975
Deposit date:
2018-01-23

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