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Generalized G-Inflation —Inflation with the Most General Second-Order Field Equations—

TLDR
In this paper, the generalized Galileons were used as a framework to develop the most general single-field inflation models ever, Generalized G-inflation, containing yet further generalization of Ginf lation, as well as previous examples such as k-inflation, extended inflation, and new Higgs inflation as special cases.
Abstract
We study generalized Galileons as a framework to develop the most general single-field inflation models ever, Generalized G-inflation, containing yet further generalization of Ginf lation, as well as previous examples such as k-inflation, extended inflation, and new Higgs inflation as special cases. We investigate the background and perturbation evolution in this model, calculating the most general quadratic actions for tensor and scalar cosmological perturbations to give the stability criteria and the power spectra of primordial fluctuations. It is pointed out in the Appendix that the Horndeski theory and the generalized Galileons are equivalent. In particular, even the non-minimal coupling to the Gauss-Bonnet term is included in the generalized Galileons in a non-trivial manner. Subject Index: 440, 442, 453

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Citations
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Bounds from ISW-galaxy cross-correlations on generalized covariant Galileon models

TL;DR: In this article, it is shown that, after imposing all standard theoretical stability constraints, it is still possible to identify a region in the parameter space of the generalized covariant Galileon model that allows for positive ISW-galaxy cross-correlations.
Posted Content

Dimensional aspects of Lovelock-Lanczos gravity

TL;DR: In this article, a class of Lovelock-Lanczos gravity (LLG) theories with perturbative expansion around a given (A)dS vacuum can be regularized up to arbitrary order.
Journal ArticleDOI

Modified gravity in the interior of population II stars

TL;DR: In this article, the effects of a beyond-Horndeski theory of modified gravity in the interior of a population II star were studied, and a simple phenomenological model of a $1.1M −1 −1−1 star with a thin Hydrogen burning shell with a partially degenerate isothermal core was proposed.
Journal ArticleDOI

An issue with the classification of the scalar-tensor theories of gravity

TL;DR: In this paper, a specific criterion for an unambiguous identification of scalar-tensor theories and its impact on the conformal transformations issue is discussed, which carries not only pedagogical but also scientific interest since an incorrect classification of a given theory as a scalar tensor theory may lead to conceptual issues and to the consequent misunderstanding of its physical implications.
Journal ArticleDOI

Inflationary spectral tilts as a result of the dilatation symmetry breaking

TL;DR: In this paper, the spectral indices and their runnings up to the second and the third order of slow roll parameters were derived using the horizon crossing formalism, and the results were more rigorous and generic than the previous works.
References
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Journal ArticleDOI

Second-order scalar-tensor field equations in a four-dimensional space

TL;DR: In this article, the second-order Euler-Lagrange tensors are derived from a Lagrangian which is at most of second order in the derivatives of the field functions.
Journal ArticleDOI

Galileon as a local modification of gravity

TL;DR: In this article, the authors study the connection between self-acceleration and the presence of ghosts for a quite generic class of theories that modify gravity in the infrared, defined as those that at distances shorter than cosmological, reduce to a certain generalization of the Dvali-Gabadadze-Porrati (DGP) effective theory.
Journal ArticleDOI

DBI in the sky

TL;DR: In this article, the spectrum of density perturbations generated in models of the recently discovered "D-cceleration" mechanism of inflation was analyzed, and it was shown that the model has a strict lower bound on the non-Gaussianity of the CMBR power spectrum at an observable level.
Journal ArticleDOI

Imperfect Dark Energy from Kinetic Gravity Braiding

TL;DR: In this paper, the authors introduce a large class of scalar-tensor models with interactions containing the second derivatives of the scalar field but not leading to additional degrees of freedom.
Journal ArticleDOI

Strong Interactions and Stability in the DGP Model

TL;DR: The model of Dvali, Gabadadze and Porrati (DGP) as mentioned in this paper gives a simple geometrical setup in which gravity becomes 5-dimensional at distances larger than a length scale lambda(DGP).
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