Starobinsky inflation in the swampland

被引:1
|
作者
Luest, Dieter [1 ,2 ]
Masias, Joaquin [2 ]
Muntz, Benjamin [2 ,3 ,4 ]
Scalisi, Marco [2 ]
机构
[1] Ludwig Maximilians Univ Munchen, Arnold Sommerfeld Ctr Theoret Phys, D-80333 Munich, Germany
[2] Max Planck Inst Phys & Astrophys, Werner Heisenberg Inst, Boltzmannstr 8, D-85748 Garching, Germany
[3] Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England
[4] Nottingham Ctr Grav, Nottingham NG7 2RD, England
来源
基金
英国科学技术设施理事会;
关键词
Cosmological models; Early Universe Particle Physics; String and Brane Phenomenology; BLACK-HOLES; QUANTUM; COSMOLOGY; FIELD;
D O I
10.1007/JHEP07(2024)186
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We argue that the Starobinsky model of inflation, realised via an R2 term in the Lagrangian, can originate from quantum effects due to a tower of light species. By means of two separate arguments, we show how this implies that the scale of the R2 term must be of order of the species scale Lambda s, namely the energy at which gravity becomes strongly coupled. We discuss the implications and challenges of this scenario for inflation, inflationary reheating, and string theory embeddings. In this context, we collect strong evidence to conclude that Starobinsky inflation lies in the Swampland.
引用
收藏
页数:30
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