The multi-field, rapid-turn inflationary solution

被引:21
作者
Aragam, Vikas [1 ]
Paban, Sonia [1 ]
Rosati, Robert [1 ]
机构
[1] Univ Texas Austin, Dept Phys, Theory Grp, Austin, TX 78712 USA
基金
美国国家科学基金会;
关键词
Cosmology of Theories beyond the SM; Sigma Models;
D O I
10.1007/JHEP03(2021)009
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
There are well-known criteria on the potential and field-space geometry for determining if slow-roll, slow-turn, multi-field inflation is possible. However, even though it has been a topic of much recent interest, slow-roll, rapid-turn inflation only has such criteria in the restriction to two fields. In this work, we generalize the two-field, rapid-turn inflationary attractor to an arbitrary number of fields. We quantify a limit, which we dub extreme turning, in which rapid-turn solutions may be found efficiently and develop methods to do so. In particular, simple results arise when the covariant Hessian of the potential has an eigenvector in close alignment with the gradient - a situation we find to be common and we prove generic in two-field hyperbolic geometries. We verify our methods on several known rapid-turn models and search two type-IIA constructions for rapid-turn trajectories. For the first time, we are able to efficiently search for these solutions and even exclude slow-roll, rapid-turn inflation from one potential.
引用
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页数:32
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