Built on

Coxeter, H.S.M. “Crystal symmetry and its generalizations”, Royal Society of Canada (3), 51
1957
Earlier work this paper cites.
E. Cremmer, J. Scherk and S. Ferrara, “SU(4) Invariant Supergravity Theory,” Phys. Lett. 74B
1978
Earlier work this paper cites.
A. A. Starobinsky, “A New Type of Isotropic Cosmological Models Without Singularity,” Phys. Lett. B 91
1980
Earlier work this paper cites.
J. E. Lidsey, A. R. Liddle, E. W. Kolb, E. J. Copeland, T. Barreiro and M. Abney, “Reconstructing the inflation potential : An overview,” Rev. Mod. Phys. 69
Original
1997
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.
V. Balasubramanian, P. Berglund, J. P. Conlon and F. Quevedo, “Systematics of moduli stabilisation in Calabi-Yau flux compactifications,” JHEP 0503
2005
Earlier work this paper cites.
D. S. Salopek, J. R. Bond and J. M. Bardeen, “Designing density fluctuation spectra in inflation,” Phys. Rev. D40
Original
2008
Earlier work this paper cites.
V. Demozzi, A. Linde and V. Mukhanov, “Supercurvaton,” JCAP 1104
Original
2011
Earlier work this paper cites.
R. Kallosh and A. Linde, “Universality Class in Conformal Inflation,” JCAP 1307
Original
2013
Earlier work this paper cites.
S. Ferrara, R. Kallosh, A. Linde and M. Porrati, “Minimal Supergravity Models of Inflation,” Phys. Rev. D 88
Original
2013
Earlier work this paper cites.
R. Kallosh, A. Linde and D. Roest, “Superconformal Inflationary α \alpha -Attractors,” JHEP 1311
Original
2013
Earlier work this paper cites.
V. Mukhanov, “Quantum Cosmological Perturbations: Predictions and Observations,” Eur. Phys. J. C 73
Original
2013
Earlier work this paper cites.

Similar

E. Bergshoeff, M. de Roo and B. de Wit, “Extended Conformal Supergravity,” Nucl. Phys. B 182
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.
D. Roest, “Universality classes of inflation,” JCAP 1401
Original
2014
Cited alongside, same era.
S. Ferrara, R. Kallosh and A. Linde, “Cosmology with Nilpotent Superfields,” JHEP 1410
Original
2014
Cited alongside, same era.
S. Cecotti and R. Kallosh, “Cosmological Attractor Models and Higher Curvature Supergravity,” JHEP 1405
Original

Then

A. S. Goncharov and A. D. Linde, “Chaotic Inflation Of The Universe In Supergravity,” Sov. Phys. JETP 59
Original
2015
Later among the works it cites.
R. Kallosh and T. Wrase, “Emergence of Spontaneously Broken Supersymmetry on an Anti-D3-Brane in KKLT dS Vacua,” JHEP 1412
Original
2015
Later among the works it cites.
B. J. Broy, M. Galante, D. Roest and A. Westphal, “Pole inflation - Shift symmetry and universal corrections,” JHEP 1512
Original
2015
Later among the works it cites.
R. Kallosh and A. Linde, “Planck, LHC, and α \alpha -attractors,” Phys. Rev. D 91
Original
2015
Later among the works it cites.
S. Ferrara and R. Kallosh, “Seven-disk manifold, α \alpha -attractors, and B B modes,” Phys. Rev. D 94

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…

2017

Maximal Supersymmetry and B-Mode Targets

Kallosh, Renata, Linde, Andrei, Wrase, Timm et al.

Understand

Extending the work of Ferrara and one of the authors, we present dynamical cosmological models of $\alpha$-attractors with plateau potentials for $3\alpha=1,2,3,4,5,6,7$.

These models are motivated by geometric properties of maximally supersymmetric theories: M-theory, superstring theory, and maximal $N = 8$ supergravity.
After a consistent truncation of maximal to minimal supersymmetry in a seven-disk geometry, we perform a two-step procedure: 1) we introduce a superpotential, which stabilizes the moduli of the seven-disk geometry in a supersymmetric minimum, 2) we add a cosmological sector with a nilpotent stabilizer, which breaks supersymmetry spontaneously and leads to a desirable class of cosmological attractor models.
These models with $n_s$ consistent with observational data, and with tensor-to-scalar ratio $r \approx 10^{-2}- 10^{-3}$, provide natural targets for future B-mode searches.