Built on

A. A. Starobinsky, “A New Type of Isotropic Cosmological Models Without Singularity,” Phys. Lett. B 91
1980
Earlier work this paper cites.
A. H. Guth, “The Inflationary Universe: A Possible Solution to the Horizon and Flatness Problems,” Phys. Rev. D 23
1981
Earlier work this paper cites.
A. D. Linde, “A New Inflationary Universe Scenario: A Possible Solution of the Horizon, Flatness, Homogeneity, Isotropy and Primordial Monopole Problems,” Phys. Lett. B 108
1982
Earlier work this paper cites.
B. Whitt, “Fourth Order Gravity as General Relativity Plus Matter,” Phys. Lett. B 145
1988
Earlier work this paper cites.
D. S. Salopek, J. R. Bond and J. M. Bardeen, “Designing density fluctuation spectra in inflation,” Phys. Rev. D40
1989
Earlier work this paper cites.
A. D. Linde, “Chaotic Inflation,” Phys. Lett. B 129
1990
Earlier work this paper cites.
R. Bousso and J. Polchinski, “Quantization of four form fluxes and dynamical neutralization of the cosmological constant,” JHEP 0006
2000
Earlier work this paper cites.
M. Kawasaki, M. Yamaguchi and T. Yanagida, “Natural chaotic inflation in supergravity,” Phys. Rev. Lett. 85
2000
Earlier work this paper cites.
S. Kachru, R. Kallosh, A. D. Linde and S. P. Trivedi, “De Sitter vacua in string theory,” Phys. Rev. D 68
2003
Earlier work this paper cites.
M. R. Douglas, “The Statistics of string / M theory vacua,” JHEP 0305
2003
Earlier work this paper cites.
A. Aazami and R. Easther, “Cosmology from random multifield potentials,” JCAP 0603
2006
Earlier work this paper cites.
C. Destri, H. J. de Vega and N. G. Sanchez, “MCMC analysis of WMAP3 and SDSS data points to broken symmetry inflaton potentials and provides a lower bound on the tensor to scalar ratio,” Phys. Rev. D 77
2008
Earlier work this paper cites.
F. L. Bezrukov and M. Shaposhnikov, “The Standard Model Higgs boson as the inflaton,” Phys. Lett. B 659
Original
2008
Earlier work this paper cites.
R. Kallosh and A. Linde, “New models of chaotic inflation in supergravity,” JCAP 1011
Original
2011
Earlier work this paper cites.
J. Frazer and A. R. Liddle, “Exploring a string-like landscape,” JCAP 1102
Original
2012
Earlier work this paper cites.

Similar

D. Battefeld, T. Battefeld and S. Schulz, “On the Unlikeliness of Multi-Field Inflation: Bounded Random Potentials and our Vacuum,” JCAP 1206
Original
2012
Cited alongside, same era.
K. Nakayama, F. Takahashi and T. T. Yanagida, “Polynomial Chaotic Inflation in the Planck Era,” Phys. Lett. B 725
Original
2013
Cited alongside, same era.
R. Kallosh and A. Linde, “Superconformal generalization of the chaotic inflation model λ 4 ϕ 4 − ξ 2 ϕ 2 R \frac{\lambda}{4}\phi^{4}-\frac{\xi}{2}\phi^{2}R ,” JCAP 1306
Original
2013
Cited alongside, same era.
R. Kallosh and A. Linde, “Superconformal generalizations of the Starobinsky model,” JCAP 1306
Original
2013
Cited alongside, same era.
R. Kallosh and A. Linde, “Universality Class in Conformal Inflation,” JCAP 1307

Then

R. Kallosh and A. Linde, “Multi-field Conformal Cosmological Attractors,” JCAP 1312
Original
2015
Later among the works it cites.
M. Galante, R. Kallosh, A. Linde and D. Roest, “Unity of Cosmological Inflation Attractors,” Phys. Rev. Lett. 114
Original
2015
Later among the works it cites.
R. Kallosh and A. Linde, “Escher in the Sky,” Comptes Rendus Physique 16
Original
2015
Later among the works it cites.
S. Ferrara, R. Kallosh and A. Linde, “Cosmology with Nilpotent Superfields,” JHEP 1410
Original
2015
Later among the works it cites.
R. Kallosh and A. Linde, “Inflation and Uplifting with Nilpotent Superfields,” JCAP 1501
Original

Beyond the bibliography

alphaXiv searches the wider corpus for related work and actual follow-ups.

Open on alphaXiv

alphaXiv is searching for related work…

Reading the bibliography…

2016

Random Potentials and Cosmological Attractors

Linde, Andrei

Understand

I show that the problem of realizing inflation in theories with random potentials of a limited number of fields can be solved, and agreement with the observational data can be naturally achieved if at least one of these fields has a non-minimal kinetic term of the type used in the theory of cosmological $\alpha$-attractors.