Testing multifield inflation: A geometric approach

被引:44
|
作者
Peterson, Courtney M. [1 ]
Tegmark, Max [2 ,3 ]
机构
[1] Harvard Univ, Dept Phys, Cambridge, MA 02138 USA
[2] MIT, Dept Phys, Cambridge, MA 02139 USA
[3] MIT, MIT Kavli Inst, Cambridge, MA 02139 USA
关键词
COSMOLOGICAL PERTURBATIONS; DENSITY PERTURBATIONS; MULTICOMPONENT INFLATON; QUANTUM FLUCTUATIONS; SPECTRUM; DYNAMICS; 2ND-ORDER; UNIVERSE; HORIZON;
D O I
10.1103/PhysRevD.87.103507
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We develop an approach for linking the power spectra, bispectrum, and trispectrum to the geometric and kinematical features of multifield inflationary Lagrangians. Our geometric approach can also be useful in determining when a complicated multifield model can be well approximated by a model with one, two, or a handful of fields. To arrive at these results, we focus on the mode interactions in the kinematical basis, starting with the case of no sourcing and showing that there is a series of mode conservation laws analogous to the conservation law for the adiabatic mode in single-field inflation. We then treat the special case of a quadratic potential with canonical kinetic terms, showing that it produces a series of mode sourcing relations identical in form to that for the adiabatic mode. We build on this result to show that the mode sourcing relations for general multifield inflation are an extension of this special case but contain higher-order covariant derivatives of the potential and corrections from the field metric. In parallel, we show how the mode interactions depend on the geometry of the inflationary Lagrangian and on the kinematics of the associated field trajectory. Finally, we consider how the mode interactions and effective number of fields active during inflation are reflected in the spectra and introduce a multifield consistency relation, as well as a multifield observable beta(2) that can potentially distinguish two-field scenarios from scenarios involving three or more effective fields.
引用
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页数:20
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