Phenomenology of the minimal inflation scenario: inflationary trajectories and particle production

被引:14
作者
Alvarez-Gaume, Luis [1 ]
Gomez, Cesar [2 ,3 ]
Jimenez, Raul [4 ]
机构
[1] CERN, Dept Phys, Theory Grp, CH-1211 Geneva 23, Switzerland
[2] UAM, CSIC, Inst Fis Teor, Madrid 28049, Spain
[3] UAM, CSIC, Dept Phys, Madrid 28049, Spain
[4] Univ Barcelona, IEEC, ICREA & ICC, E-08028 Barcelona, Spain
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2012年 / 03期
关键词
inflation; supersymmetry and cosmology; DENSITY PERTURBATIONS; UNIVERSE SCENARIO; PHASE-TRANSITION; COSMOLOGY; FLATNESS; HORIZON; FIELD;
D O I
10.1088/1475-7516/2012/03/017
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We discuss the phenomenology of the minimal inflation scenario. We concentrate on two aspects: inflationary trajectories and particle production. Our findings can be summarized in two main results: first, that inflationary trayectories that are very flat and provide enough number of e-foldings are natural in the scenario without fine tunning. We present a general formalism to identify attractors in multi-field inflation regardless of trajectories fulfilling the slow-roll conditions. We then explore particle production in the model and show how the inflaton naturally transmutes into a dark matter particle. One interesting feature of our model is that it provides a novel mechanism to generate particles and entropy in the universe: the filling of the Fermi sphere up to a given momentum p F due to the sea of goldstinos that are an important part of the matter generated after inflation. With this mechanism in hand we predict that the gravitino should have a mass of > 100 - 1000TeV. Another interesting feature of our model is that the predicted level of gravity waves is r = 0.10 - 0.001, which is in the range of detectability from Planck and upcoming CMB polarization experiments.
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页数:12
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