No-scale D-term inflation with stabilized moduli
Description
We study the consistency of hybrid inflation and moduli stabilization, using the Kallosh–Linde model as an example for the latter. We find that F-term hybrid inflation is not viable since inflationary trajectories are destabilized by tachyonic modes. On the other hand, D-term hybrid inflation is naturally compatible with moduli stabilization due to the absence of a large superpotential term during the inflationary phase. Our model turns out to be equivalent to superconformal D-term inflation and it therefore successfully accounts for the CMB data in the large-field regime. Supersymmetry breaking can be incorporated via an O'Raifeartaigh model. For GUT-scale inflation one obtains stringent bounds on the gravitino mass. A rough estimate yields 105 GeV≲m3/2≲1010 GeV, contrary to naive expectation.
Availability note (English)
Available from http://dx.doi.org/10.1016/j.physletb.2014.01.040Additional details
Identifiers
- DOI
- 10.1016/j.physletb.2014.01.040;
- arXiv
- arXiv:1309.3122v2;
- PII
- S0370-2693(14)00062-8;
Publishing Information
- Journal Title
- Physics Letters. Section B
- Journal Volume
- 730
- Journal Issue
- Complete
- Journal Page Range
- p. 155-160
- ISSN
- 0370-2693
- CODEN
- PYLBAJ
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 46016589
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- COMPUTERIZED SIMULATION; GRAVITATION; HYBRID SYSTEMS; MASS; RELICT RADIATION; STABILIZATION; SUPERSYMMETRY; SYMMETRY BREAKING; TACHYONS; TRAJECTORIES
- Descriptors DEC
- ELECTROMAGNETIC RADIATION; ELEMENTARY PARTICLES; MICROWAVE RADIATION; POSTULATED PARTICLES; RADIATIONS; SIMULATION; SYMMETRY
Optional Information
- Copyright
- Copyright (c) 2014 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.