A first principles warm inflation model that solves the cosmological horizon and flatness problems.¶
Berera, A., Gleiser, M., & Ramos, R. O. (1999). A first principles warm inflation model that solves the cosmological horizon and flatness problems. Physical Review Letters, 264-267.
Cited by¶
1 citation across 1 artifact.
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Domain-specific¶
- Warm Inflation
- A first-principles interacting model. Berera, Gleiser, and Ramos constructed a scalar-field model in which the inflaton interacts with additional massive scalar fields that couple to light fermions, allowing energy to pass through a decay chain into radiation while inflation proceeds.
This sourcePrimary microphysical interacting-field realization.
- A first-principles interacting model. Berera, Gleiser, and Ramos constructed a scalar-field model in which the inflaton interacts with additional massive scalar fields that couple to light fermions, allowing energy to pass through a decay chain into radiation while inflation proceeds.
Verification¶
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Registry ID ref:91811ce80a1d · see in the full table