BICEP2 implications for single-field slow-roll inflation revisited

被引:43
|
作者
Antusch, Stefan [1 ,2 ]
Nolde, David [1 ]
机构
[1] Univ Basel, Dept Phys, CH-4056 Basel, Switzerland
[2] Max Planck Inst Phys & Astrophys, Werner Heisenberg Inst, D-80805 Munich, Germany
基金
瑞士国家科学基金会;
关键词
inflation; physics of the early universe;
D O I
10.1088/1475-7516/2014/05/035
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
It is generally believed that in single-field slow-roll inflation, a large tensor-to-scalar ratio r > 0.1 requires inflaton field values close to or above the Planck scale. Recently, it has been claimed that r > 0.15 can be achieved with much smaller inflaton field values Delta phi < M-pl/10. We show that in single-field slow-roll inflation, it is impossible to reconcile r > 0.1 with such small field values, independently of the form of the potential, and that the recent claim to the contrary is based on an invalid approximation. We conclude that the result of the BICEP2 measurement of r > 0.1, if confirmed, truly has the potential to rule out small-field models of single-field slow-roll inflation.
引用
收藏
页数:10
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