Attractors, bifurcations and curvature in multi-field inflation

被引:26
作者
Christodoulidis, Perseas [1 ]
Roest, Diederik [1 ]
Sfakianakis, Evangelos, I [2 ,3 ]
机构
[1] Univ Groningen, Van Swinderen Inst Particle Phys & Grav, Nijenborgh 4, NL-9747 AG Groningen, Netherlands
[2] Nikhef, Sci Pk 105, NL-1098 XG Amsterdam, Netherlands
[3] Leiden Univ, Lorentz Inst Theoret Phys, NL-2333 CA Leiden, Netherlands
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2020年 / 08期
关键词
inflation; physics of the early universe;
D O I
10.1088/1475-7516/2020/08/006
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Recent years have seen the introduction of various multi-field inflationary scenarios in which the curvature and geodesics of the scalar manifold play a crucial role. We outline a simple description that unifies these different proposals and discuss their stability criteria. We demonstrate how the underlying dynamics is governed by an effective potential, whose critical points and bifurcations determine the late-time behaviour of the system, thus unifying hyperinflation, angular, orbital and side-tracked inflation. Interestingly, we show that hyperinflation is a special case of side-tracked inflation, relying on the enhanced isometrics of the hyperbolic manifold. We provide the explicit coordinate transformation that maps the two models into each other. Finally, we relax the assumption of a field-space isometry along the inflationary direction that has been considered a prerequisite in the literature so far. We explicitly construct inflationary solutions that do not proceed along a field-space isometry or geodesic and use them to discuss stability criteria.
引用
收藏
页数:21
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