Report/Internal Report PUBDB-2015-01152

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Challenges for Large-Field Inflation and Moduli Stabilization

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2015

Red Report 44 pp. ()  GO

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Report No.: CPHT-RR002.0115; DESY-15-014; arXiv:1501.0581

Abstract: We analyze the interplay between K\'ahler moduli stabilization and chaotic inflation in supergravity. While heavy moduli decouple from inflation in the supersymmetric limit, supersymmetry breaking generically introduces non-decoupling effects. These lead to inflation driven by a soft mass term, $m_\varphi^2 \sim m m_{3/2}$, where $m$ is a supersymmetric mass parameter. This scenario needs no stabilizer field, but the stability of moduli during inflation imposes a large supersymmetry breaking scale, $m_{3/2} \gg H$, and a careful choice of initial conditions. This is illustrated in three prominent examples of moduli stabilization: KKLT stabilization, K\'ahler Uplifting, and the Large Volume Scenario. Remarkably, all models have a universal effective inflaton potential which is flattened compared to quadratic inflation. Hence, they share universal predictions for the CMB observables, in particular a lower bound on the tensor-to-scalar ratio, $r \gtrsim 0.05$.


Note: OA

Contributing Institute(s):
  1. Theorie-Gruppe (T)
Research Program(s):
  1. 611 - Fundamental Particles and Forces (POF3-611) (POF3-611)
  2. VH-GS-500 - PIER Helmholtz Graduate School (2015_IFV-VH-GS-500) (2015_IFV-VH-GS-500)
  3. MASSTEV - Mass hierarchy and particle physics at the TeV scale (226371) (226371)
Experiment(s):
  1. No specific instrument

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Challenges for large-field inflation and moduli stabilization
Journal of high energy physics 1504(4), 58 () [10.1007/JHEP04(2015)058]  GO OpenAccess  Download fulltext Files  Download fulltextFulltext by arXiv.org BibTeX | EndNote: XML, Text | RIS


 Record created 2015-02-03, last modified 2021-11-10