The Volkov-Akulov-Starobinsky supergravity

被引:180
作者
Antoniadis, I. [1 ]
Dudas, E. [2 ]
Ferrara, S. [1 ,3 ,4 ]
Sagnotti, A. [5 ,6 ]
机构
[1] CERN, Div Theory, Dept Phys, CH-1211 Geneva 23, Switzerland
[2] Ecole Polytech, Ctr Phys Theor, F-91128 Palaiseau, France
[3] Ist Nazl Fis Nucl, Lab Nazl Frascati, I-00044 Frascati, Italy
[4] Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA
[5] Scuola Normale Super Pisa, Piazza Cavalieri 7, I-56126 Pisa, Italy
[6] Ist Nazl Fis Nucl, I-56126 Pisa, Italy
基金
欧洲研究理事会;
关键词
SUPERSYMMETRY; MODELS;
D O I
10.1016/j.physletb.2014.04.015
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We construct a supergravity model whose scalar degrees of freedom arise from a chiral superfield and are solely a scalaron and an axion that is very heavy during the inflationary phase. The model includes a second chiral superfield X, which is subject however to the constraint X-2 = 0 so that it describes only a Volkov-Akulov goldstino and an auxiliary field. We also construct the dual higher-derivative model, which rests on a chiral scalar curvature superfield R. subject to the constraint R-2 = 0, where the goldstino dual arises from the gauge-invariant gravitino field strength as gamma D-mn(m)psi(n). The final bosonic action is an R + R-2 theory involving an axial vector Am that only propagates a physical pseudoscalar mode. (C) 2014 The Authors. Published by Elsevier B.V.
引用
收藏
页码:32 / 35
页数:4
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