Construct · 1 fields · 1 citations

Starobinsky inflation: a standalone construct

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Particle physics

inflation driven by a quadratic curvature term added to the Einstein-Hilbert action, predicting a small tensor-to-scalar ratio.

In particle physics, Starobinsky inflation refers to inflation driven by a quadratic curvature term added to the Einstein-Hilbert action, predicting a small tensor-to-scalar ratio. This meaning comes from Starobinsky (1980) in Physics Letters B.[1]

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Nearby constructs

action3 fields · 6 citationsjingle · one word, three constructs curvature3 fields · 4 citationsjingle · one word, three constructs inflation3 fields · 4 citationsjingle · one word, three constructs

References

Starobinsky, A. A. (1980). A new type of isotropic cosmological models without singularity. Physics Letters B, 91(1), 99-102. https://doi.org/10.1016/0370-2693(80)90670-x

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