Planck constraints on Higgs modulated reheating of renormalization group improved inflation

被引:23
作者
Cai, Yi-Fu [1 ]
Chang, Yu-Chiao [2 ,3 ]
Chen, Pisin [2 ,3 ,4 ,5 ]
Easson, Damien A. [6 ]
Qiu, Taotao [2 ,3 ]
机构
[1] McGill Univ, Dept Phys, Montreal, PQ H3A 2T8, Canada
[2] Natl Taiwan Univ, Dept Phys, Taipei 10617, Taiwan
[3] Natl Taiwan Univ, Leung Ctr Cosmol & Particle Astrophys, Taipei 10617, Taiwan
[4] Natl Taiwan Univ, Grad Inst Astrophys, Taipei 10617, Taiwan
[5] Stanford Univ, SLAC, Kavli Inst Particle Astrophys & Cosmol, Stanford, CA 94305 USA
[6] Arizona State Univ, Dept Phys, Tempe, AZ 85287 USA
关键词
STANDARD MODEL; PERTURBATIONS; UNIVERSE; SCENARIO; FLATNESS; GRAVITY; HORIZON;
D O I
10.1103/PhysRevD.88.083508
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Within the framework of renormalization group improved inflationary cosmology motivated by asymptotically safe gravity, we study the dynamics of a scalar field which can be interpreted as the Higgs field. The background trajectories of this model can provide sufficient inflationary e-folds and a graceful exit to a radiation dominated phase. We study the possibility of generating primordial curvature perturbations through the Standard Model Higgs boson. This can be achieved under finely tuned parameter choices by making use of the modulated reheating mechanism. The primordial non-Gaussianity is expected to be sizable in this model. Though tightly constrained by the newly released Planck cosmic microwave background data, this model provides a potentially interesting connection between collider and early Universe physics.
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页数:13
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