\ The phenomenology of trapped inflation

被引:14
作者
Pearce, Lauren [1 ,2 ,3 ,5 ]
Peloso, Marco [1 ,2 ]
Sorbo, Lorenzo [4 ]
机构
[1] Univ Minnesota, Sch Phys & Astron, 116 Church St SE, Minneapolis, MN 55455 USA
[2] Univ Minnesota, Minnesota Inst Astrophys, 116 Church St SE, Minneapolis, MN 55455 USA
[3] Univ Minnesota, William I Fine Theoret Phys Inst, Sch Phys & Astron, 116 Church St SE, Minneapolis, MN 55455 USA
[4] Univ Massachusetts, Dept Phys, Amherst Ctr Fundamental Interact, 1126 Lederle Grad Res Tower LGRT, Amherst, MA 01003 USA
[5] Valparaiso Univ, Dept Phys & Astron, Neils Sci Ctr, 1610 Campus Dr East, Valparaiso, IN 46383 USA
基金
美国国家科学基金会;
关键词
cosmological perturbation theory; inflation; non-gaussianity; WARM INFLATION; MODEL;
D O I
10.1088/1475-7516/2016/11/058
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Trapped inflation is a mechanism in which particle production from the moving inflaton is the main source of friction in the inflaton equation of motion. The produced fields source inflaton perturbations, which dominate over the vacuum ones. We review the computation of the perturbations performed in the original work and in a successive analysis that makes use of the effective field theory (EFT) of inflation. This second paper employs the power spectrum of the inflaton perturbations obtained in the original work, and obtains a bispectrum which parametrically agrees with that of the original work, even if it originates from a different operator. We show that one approximation used in the original work to compute the correlators of the produced quanta is invalid. We replace this approximation with an exact solution of the system of equations developed in the original work and obtain a different amplitude for the power spectrum of the inflaton perturbations, which has a significant consequence for the allowed region of parameter space in this mechanism. We then show that the operator responsible for the bispectrum in the EFT computation does not arise from the computational scheme developed in the original paper and that the agreement between the bispectra of the two works is also caused by the invalid approximation.
引用
收藏
页数:48
相关论文
共 38 条
[1]   Planck 2015 results XX. Constraints on inflation [J].
Ade, P. A. R. ;
Aghanim, N. ;
Arnaud, M. ;
Arroja, F. ;
Ashdown, M. ;
Aumont, J. ;
Baccigalupi, C. ;
Ballardini, M. ;
Banday, A. J. ;
Barreiro, R. B. ;
Bartolo, N. ;
Battaner, E. ;
Benabed, K. ;
Benoit, A. ;
Benoit-Levy, A. ;
Bernard, J. -P. ;
Bersanelli, M. ;
Bielewicz, P. ;
Bock, J. J. ;
Bonaldi, A. ;
Bonavera, L. ;
Bondi, J. R. ;
Borrillu, J. ;
Bouchet, F. R. ;
Boulanger, F. ;
Bucher, M. ;
Burigana, C. ;
Butler, R. C. ;
Calabrese, E. ;
Cardoso, J. -F. ;
Catalano, A. ;
Challinor, A. ;
Chamballu, A. ;
Chary, R. -R. ;
Chiang, H. C. ;
Christensen, P. R. ;
Churchl, S. ;
Clements, D. L. ;
Colombi, S. ;
Colombo, L. P. L. ;
Combet, C. ;
Contreras, D. ;
Couchot, F. ;
Coulais, A. ;
Crill, B. P. ;
Curto, A. ;
Cuttaia, F. ;
Danese, L. ;
Davies, R. D. ;
Davis, R. J. .
ASTRONOMY & ASTROPHYSICS, 2016, 594
[2]  
Ade P. A. R., 2016, ASTRON ASTROPHYS, V594, pA17
[3]  
Amin M.A., 2016, JCAP, V02, P04
[4]   Naturally inflating on steep potentials through electromagnetic dissipation [J].
Anber, Mohamed M. ;
Sorbo, Lorenzo .
PHYSICAL REVIEW D, 2010, 81 (04)
[5]   Cosmological fluctuations from infrared cascading during inflation [J].
Barnaby, Neil ;
Huang, Zhiqi ;
Kofman, Lev ;
Pogosyan, Dmitry .
PHYSICAL REVIEW D, 2009, 80 (04)
[6]   Gravity waves and non-Gaussian features from particle production in a sector gravitationally coupled to the inflaton [J].
Barnaby, Neil ;
Moxon, Jordan ;
Namba, Ryo ;
Peloso, Marco ;
Shiu, Gary ;
Zhou, Peng .
PHYSICAL REVIEW D, 2012, 86 (10)
[7]   Feeding your inflaton: non-Gaussian signatures of interaction structure [J].
Barnaby, Neil ;
Shandera, Sarah .
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2012, (01)
[8]   Phenomenology of a pseudo-scalar inflaton: naturally large nongaussianity [J].
Barnaby, Neil ;
Namba, Ryo ;
Peloso, Marco .
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2011, (04)
[9]   Particle production during inflation: Observational constraints and signatures [J].
Barnaby, Neil ;
Huang, Zhiqi .
PHYSICAL REVIEW D, 2009, 80 (12)
[10]   The importance of being warm (during inflation) [J].
Bartrum, Sam ;
Bastero-Gil, Mar ;
Berera, Arjun ;
Cerezo, Rafael ;
Ramos, Rudnei O. ;
Rosa, Joao G. .
PHYSICS LETTERS B, 2014, 732 :116-121