Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
2010-12-29
JHEP 04 (2011) 009
Physics
High Energy Physics
High Energy Physics - Phenomenology
27 pages, 6 figures; v2, published version, minor adjustments to the introduction, minor corrections to section 2.2 for improv
Scientific paper
10.1007/JHEP04(2011)009
We argue that the eta-problem in supergravity inflation cannot be solved without knowledge of the ground state of hidden sectors that are gravitationally coupled to the inflaton. If the hidden sector breaks supersymmetry independently, its fields cannot be stabilized during cosmological evolution of the inflaton. We show that both the subsequent dynamical mixing between sectors as well as the lightest mass of the hidden sector are set by the scale of supersymmetry breaking in the hidden sector. The true cosmological eta-parameter arises from a linear combination of the lightest mode of the hidden sector with the inflaton. Generically, either the true eta deviates considerably from the na\"ive eta implied by the inflaton sector alone, or one has to consider a multifield model. Only if the lightest mass in the hidden sector is much larger than the inflaton mass and if the inflaton mass is much larger than the scale of hidden sector supersymmetry breaking, is the effect of the hidden sector on the slow-roll dynamics of the inflaton negligible.
der Aalst Ted van
Hardeman Sjoerd
Oberreuter Johannes M.
Palma Gonzalo A.
Schalm Koenraad
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