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The dynamics of hybrid models is usually approximated by the evolution of a scalar field slowly rolling along a nearly flat valley.
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False vacuum inflation with Einstein gravity
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Formalizing the slow roll approximation in inflation
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Cosmic strings and other topological defects
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From the Big Bang theory to the theory of a stationary universe
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M. B. Hindmarsh and T. W. B. Kibble · 1995
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Spin networks and quantum gravity
Carlo Rovelli and Lee Smolin · 1995
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Smooth hybrid inflation
George Lazarides and C. Panagiotakopoulos · 1995
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Renata Kallosh, Andrei D. Linde, Dmitri A. Linde, and Leonard Susskind · 1995
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Arjun Berera · 1995
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Initial conditions for smooth hybrid inflation
George Lazarides, C. Panagiotakopoulos, and N. D. Vlachos · 1996
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Density perturbations and black hole formation in hybrid inflation
Juan Garcia-Bellido, Andrei D. Linde, and David Wands · 1996
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Inflation in supersymmetric unified theories
R. Jeannerot · 1997
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L. P. Grishchuk and Jerome Martin · 1997
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Lev Kofman, Andrei D. Linde, and Alexei A. Starobinsky · 1997
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Initial conditions for supersymmetric inflation
George Lazarides and N. D. Vlachos · 1997
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SIAM Journal on Numerical Analysis
L. Dieci, R. D. Russel, and E. S. V. Vleck · 1997
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George F. Smoot and D. Scott · 1998
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Matthew Colless · 1998
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Preheating in hybrid inflation
Juan Garcia-Bellido and Andrei D. Linde · 1998
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Fine tuning of the initial conditions for hybrid inflation
N. Tetradis · 1998
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Tanmay Vachaspati and Mark Trodden · 2000
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Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant
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