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Models of cosmic inflation suggest that our universe underwent an early phase of accelerated expansion, driven by the dynamics of one or more scalar fields.
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1998
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S. V. Ketov, Quantum Nonlinear Sigma Models
2000
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2002
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Y. Fujii and K.-i. Maeda, The Scalar-Tensor Theory of Gravitation
2003
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J. M. Maldacena, “Non-Gaussian features of primordial fluctuations in single field inflationary models,” J. High Energy Phys. 0305 (2003): 013, arXiv:astro-ph/0210603
2003
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V. Faraoni, Cosmology in Scalar-Tensor Gravity
2004
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M. Janssen, “Of pots and holes: Einstein’s bumpy road to general relativity,” Ann. Phys. (Leipzig) 14, Supplement (2005): 58
2005
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B. A. Bassett, S. Tsujikawa, and D. Wands, “Inflation dynamics and reheating,” Rev. Mod. Phys. 78 (2006): 537, arXiv:astro-ph/0507632
2006
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D. I. Kaiser, “When fields collide,” Sci. Am. 296 (June 2007): 62
2007
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2008
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L. E. Parker and D. J. Toms, Quantum Field Theory in Curved Spacetime
2009
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