On sgoldstino-less supergravity models of inflation
- ,
- Fabio Zwirner()
- Padua U. and
- INFN, Padua and
- CERN
19 pages
Published in:
- JHEP 12 (2014) 172
- Published: Dec 30, 2014
e-Print:
- 1411.2605 [hep-th]
Report number:
- CERN-PH-TH-2014-199,
- DFPD-2014-TH-16
Citations per year
Abstract: (Springer)
We go a step further in the search for a consistent and realistic supergravity model of large-field inflation by building a class of models with the following features: during slow-roll, all the scalar fields other than the inflaton are frozen by large inflatondependent masses or removed from the spectrum, at the end of inflation, supersymmetry is spontaneously broken with naturally vanishing classical vacuum energy. We achieve this by combining some geometrical properties of the Kähler potential with the consistent use of a single nilpotent chiral superfield, in one-to-one correspondence with the supersymmetrybreaking direction in field space at the vacuum.Note:
- 19 pages. v2: references added and few minor changes to the text. v3: published version
- Supersymmetry Breaking
- Supergravity Models
- Cosmology of Theories beyond the SM
- inflation: model
- supersymmetry: spontaneous symmetry breaking
- potential: Kaehler
- superfield: chiral
- supersymmetry: symmetry breaking
- field theory: scalar
- vacuum state: energy
References(32)
Figures(0)
- [1]
- [2]
- [3]
- [4]
- [5]
- [6]
- [7]
- [8]
- [9]
- [10]
- [11]
- [12]
- [13]
- [14]
- [15]
- [16]
- [17]
- [18]
- [19]
- [20]
- [21]
- [22]
- [23]
- [24]
- [25]