Ill Illustrating SUSY breaking effects
- n various in
inflation models
山田 悠介 (早稲田大) 共同研究者 安倍 博之、青木 俊太朗、長谷川史憲 (早稲田大)
- H. Abe, S. Aoki, F. Hasegawa and Y. Y, arXiv:1408.XXXX
7/29 基研研究会 素粒子物理学の進展2014
on various in inflation models ( ) - - PowerPoint PPT Presentation
7/29 2014 Ill Illustrating SUSY breaking effects on various in inflation models ( ) ( ) H.
7/29 基研研究会 素粒子物理学の進展2014
7/29 基研研究会 素粒子物理学の進展2014
+ 1 loop effective potential
D-term hybrid inflation Universal attractor inflation
D-term hybrid inflation Universal attractor inflation
D-term hybrid inflation Universal attractor inflation
D-term hybrid inflation
Universal attractor inflation
generators
Translation SUSY Lorentz rotation Dilatation Chiral U(1) S-SUSY Conformal boost
generators
Translation SUSY Lorentz rotation Dilatation Chiral U(1) S-SUSY Conformal boost
generators
Translation SUSY Lorentz rotation Gauge fixing Compensator multipletが必要
+global U(1)R, Kahler symmetry
D-gauge fixing condition (Einstein frame) (Jordan frame)
D-gauge fixing condition (Einstein frame) A-gauge fixing condition
&
&
D-term hybrid inflation Universal attractor inflation
D-term hybrid inflation Universal attractor inflation
“compensated” terms → enhancement/suppression effectsが生じる Minimal Kahler models:
Higher derivative extensionをしても同様の議論が出来る!
(青木くんのポスター)
補助場を消去する前のF-termポテンシャル
Global SUSY like scalar potential !
もし なら 補助場を消去する前のF-termポテンシャル
Global SUSY like scalar potential ! もし なら
補助場を消去する前のF-termポテンシャル
インフレーション中 Chaotic inflation in SUGRA
インフレーション中 Chaotic inflation in SUGRA
No-scale model
No-scale model
② No-scale structureでSUGRA correctionを消去
No-scale model
apploximately No-scale model (e.g. LARGE volume scenario のとき
Application to the tadpole problem in hybrid inflation
D7-brane chaotic inflation
(In string theory )
② No-scale structureでSUGRA correctionを消去
LVS in effective theory of 5D SUGRA
Approximately No-scale !
をintegrate out Global SUSY like parts Suppressed SUGRA corrections
※compensatorからの寄与は残る
Simple chaotic inflation
全ての“compensated” termのEnhancement/Suppression effects “gravity” mediated interactionsの原因
SUGRA potential without SUGRA corrections
Hubble correctionによって、 がポテンシャル障壁を超えないためには 次の条件が必要 High scale SUSY breaking !