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000275712 245__ $$aChallenges for large-field inflation and moduli stabilization
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000275712 520__ $$aWe analyze the interplay between Kähler 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 φ 2  ∼ mm 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 ≫ H, and a careful choice of initial conditions. This is illustrated in three prominent examples of moduli stabilization: KKLT stabilization, Kähler 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 ≳ 0.05.
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000275712 7001_ $$aDudas, Emilian$$b1
000275712 7001_ $$aHeurtier, Lucien$$b2
000275712 7001_ $$0P:(DE-H253)PIP1013212$$aWestphal, Alexander$$b3
000275712 7001_ $$0P:(DE-H253)PIP1018677$$aWieck, Clemens$$b4$$eCorresponding author
000275712 7001_ $$aWinkler, Martin Wolfgang$$b5
000275712 773__ $$0PERI:(DE-600)2027350-2$$a10.1007/JHEP04(2015)058$$gVol. 2015, no. 4, p. 58$$n4$$p58$$tJournal of high energy physics$$v1504$$x1029-8479$$y2015
000275712 7870_ $$0PUBDB-2015-01152$$aBuchmuller, Wilfried et.al.$$d2015$$iIsParent$$rDESY-15-014; CPHT-RR002.0115; arXiv:1501.0581$$tChallenges for Large-Field Inflation and Moduli Stabilization
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