scholarly journals Kinetically modified nonminimal chaotic inflation

2015 ◽  
Vol 91 (12) ◽  
Author(s):  
Constantinos Pallis
Keyword(s):  
2010 ◽  
Vol 25 (31) ◽  
pp. 2697-2713
Author(s):  
KOUROSH NOZARI ◽  
SIAMAK AKHSHABI

We construct an inflation model on the Randall–Sundrum I (RSI) brane where a bulk scalar field stabilizes the inter-brane separation. We study impact of the bulk scalar field on the inflationary dynamics on the brane. We proceed in two different approaches: in the first approach, the stabilizing field potential is directly appeared in the Friedmann equation and the resulting scenario is effectively a two-field inflation. In the second approach, the stabilization mechanism is considered in the context of a warp factor so that there is just one field present that plays the roles of both inflaton and stabilizer. We study constraints imposed on the model parameters from recent observations.


2014 ◽  
Vol 738 ◽  
pp. 196-200 ◽  
Author(s):  
Hitoshi Murayama ◽  
Kazunori Nakayama ◽  
Fuminobu Takahashi ◽  
Tsutomu T. Yanagida
Keyword(s):  

2018 ◽  
Vol 98 (12) ◽  
Author(s):  
Shinta Kasuya ◽  
Mayuko Taira
Keyword(s):  

2015 ◽  
Vol 741 ◽  
pp. 267-271 ◽  
Author(s):  
Keisuke Harigaya ◽  
Masahiro Kawasaki ◽  
Tsutomu T. Yanagida

1991 ◽  
Vol 43 (2) ◽  
pp. 362-368 ◽  
Author(s):  
Insu Yi ◽  
Ethan T. Vishniac ◽  
Shin Mineshige

2019 ◽  
Vol 79 (10) ◽  
Author(s):  
Matías López ◽  
Jorge Maggiolo ◽  
Nelson Videla ◽  
Pablo González ◽  
Grigoris Panotopoulos

Abstract We study chaotic inflation with a Galileon-like self-interaction $$G(\phi ,X)\Box \phi $$G(ϕ,X)□ϕ, where $$G(\phi ,X)\propto X^{n}$$G(ϕ,X)∝Xn. General conditions required for successful inflation are deduced and discussed from the background and cosmological perturbations under slow-roll approximation. Interestingly, it is found that in the regime where the Galileon term dominates over the standard kinetic term, the tensor-to-scalar ratio becomes significantly suppressed in comparison to the standard expression in General Relativity (GR). Particularly, we find the allowed range in the space of parameters characterizing the chaotic quadratic and quartic inflation models by considering the current observational data of Planck from the $$n_{\mathcal {S}}-r$$nS-r plane. Finally, we discuss about the issue if the Galileon term is dominant by the end of inflation, this can affect the field oscillation during reheating.


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