Phenomenological aspects of no-scale inflation models

Ellis, John; Garcia, Marcos A. G.; Nanopoulos, Dimitri V.; Olive, Keith A.

doi:10.1088/1475-7516/2015/10/003

Phenomenological aspects of no-scale inflation models

Journal Article · Thu Oct 01 00:00:00 EDT 2015 · Journal of Cosmology and Astroparticle Physics

DOI:https://doi.org/10.1088/1475-7516/2015/10/003· OSTI ID:1437112

Ellis, John ^[1]; Garcia, Marcos A. G. ^[2]; Nanopoulos, Dimitri V. ^[3]; Olive, Keith A. ^[2]

King's College London (United Kingdom). Theoretical Particle Physics and Cosmology Group. Dept. of Physics; European Organization for Nuclear Research (CERN), Geneva (Switzerland). Theory Division; University of Minnesota
Univ. of Minnesota, Minneapolis, MN (United States). William I. Fine Theoretical Physics Inst. School of Physics and Astronomy
Texas A & M Univ., College Station, TX (United States). George P. and Cynthia W. Mitchell Inst. for Fundamental Physics and Astronomy; Houston Advanced Research Center (HARC), Woodlands, TX (United States). Astroparticle Physics Group; Academy of Athens (Greece). Division of Natural Sciences

We discuss phenomenological aspects of inflationary models wiith a no-scale supergravity Kähler potential motivated by compactified string models, in which the inflaton may be identified either as a Kähler modulus or an untwisted matter field, focusing on models that make predictions for the scalar spectral index n_s and the tensor-to-scalar ratio r that are similar to the Starobinsky model. We discuss possible patterns of soft supersymmetry breaking, exhibiting examples of the pure no-scale type m₀ = B₀ = A₀ = 0, of the CMSSM type with universal A₀ and m₀ ≠ 0 at a high scale, and of the mSUGRA type with A₀ = B₀ + m₀ boundary conditions at the high input scale. These may be combined with a non-trivial gauge kinetic function that generates gaugino masses m_1/2 ≠ 0, or one may have a pure gravity mediation scenario where trilinear terms and gaugino masses are generated through anomalies. We also discuss inflaton decays and reheating, showing possible decay channels for the inflaton when it is either an untwisted matter field or a Kähler modulus. Reheating is very efficient if a matter field inflaton is directly coupled to MSSM fields, and both candidates lead to sufficient reheating in the presence of a non-trivial gauge kinetic function.

View Accepted Manuscript (DOE)

Research Organization:: European Organization for Nuclear Research (CERN), Geneva (Switzerland); King's College London (United Kingdom); Univ. of Minnesota, Minneapolis, MN (United States)

Sponsoring Organization:: European Research Council (ERC); Science and Technology Facilities Council (STFC) (United Kingdom); USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25)

Grant/Contract Number:: SC0011842

OSTI ID:: 1437112

Alternate ID(s):: OSTI ID: 22458384
OSTI ID: 22525305

Journal Information:: Journal of Cosmology and Astroparticle Physics, Journal Name: Journal of Cosmology and Astroparticle Physics Journal Issue: 10 Vol. 2015; ISSN 1475-7516

Publisher:: Institute of Physics (IOP)Copyright Statement

Country of Publication:: United States

Language:: English

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Phenomenological aspects of no-scale inflation models

Journal Article · Thu Oct 01 00:00:00 EDT 2015 · Journal of Cosmology and Astroparticle Physics · OSTI ID:22525305

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Journal Article · Thu Oct 01 00:00:00 EDT 2015 · Journal of Cosmology and Astroparticle Physics · OSTI ID:22458384

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72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
79 ASTRONOMY AND ASTROPHYSICS
cosmology connection
inflation
particle physics
supersymmetry and cosmology

Phenomenological aspects of no-scale inflation models

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