scholarly journals Inflation, scale of supersymmetry breaking and moduli stabilization

2016 ◽  
Author(s):  
Emilian Dudas ◽  
Clemens Wieck
2006 ◽  
Vol 2006 (06) ◽  
pp. 048-048 ◽  
Author(s):  
Andrey Katz ◽  
Michele Redi ◽  
Yael Shadmi ◽  
Yuri Shirman

2012 ◽  
Vol 85 (6) ◽  
Author(s):  
Andrei Linde ◽  
Yann Mambrini ◽  
Keith A. Olive

2019 ◽  
Vol 2019 (9) ◽  
Author(s):  
Tatsuo Kobayashi ◽  
Osamu Seto ◽  
Shintaro Takada ◽  
Takuya H Tatsuishi ◽  
Shohei Uemura ◽  
...  

Abstract We study Kähler moduli stabilization in type IIB superstring theory. We propose a new moduli stabilization mechanism by the supersymmetry breaking chiral superfield which is coupled to Kähler moduli in the Kähler potential. We also study its uplifting of the Large Volume Scenario (LVS). In both cases, the form of the superpotential is crucial for moduli stabilization. We confirm that our uplifting mechanism does not destabilize the vacuum of the LVS drastically.


2017 ◽  
Vol 32 (29) ◽  
pp. 1750150
Author(s):  
Noriaki Kitazawa

We discuss the effect of the dynamics of D-branes on moduli stabilization in type IIB string theory compactifications, with reference to a concrete toy model of [Formula: see text] orientifold compactification with fractional D3-branes and anti-D3-branes at orbifold fixed points. The resulting attractive forces between anti-D3-branes and D3-branes, together with the repulsive forces between anti-D3-branes and O3-planes, can affect the stability of the compact space. There are no complex structure moduli in [Formula: see text] orientifold, which should thus capture some generic features of more general settings where all complex structure moduli are stabilized by three-form fluxes. The simultaneous presence of branes and anti-branes brings along the breaking of supersymmetry. Non-BPS combinations of this type are typical of “brane supersymmetry breaking” and are a necessary ingredient in the KKLT scenario for stabilizing the remaining Kähler moduli. The conclusion of our analysis is that, while mutual D-brane interactions sometimes help Kähler moduli stabilization, this is not always the case.


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