Starobinsky inflation

Starobinsky inflation is a modification of general relativity in order to explain cosmological inflation.

History

In the Soviet Union, Alexei Starobinsky noted that quantum corrections to general relativity should be important for the early universe. These generically lead to curvature-squared corrections to the Einstein–Hilbert action and a form of f(R) modified gravity. The solution to Einstein's equations in the presence of curvature squared terms, when the curvatures are large, leads to an effective cosmological constant. Therefore, he proposed that the early universe went through an inflationary de Sitter era.[1] This resolved the cosmology problems and led to specific predictions for the corrections to the microwave background radiation, corrections that were then calculated in detail. Starobinsky used the action[2]

which corresponds to the potential in the Einstein frame.

Observables

Starobinsky inflation gives a prediction for the observables of the spectral tilt and the tensor-scalar ratio : [3] where is the number of e-foldings since the start of the universe. As , these are compatible with experimental data, with 2019 CMB data from the Planck satellite giving a constraint of (95% confidence) and (68% confidence).[3]

See also

References

  1. ↑ Starobinsky, A. A. (December 1979). "Spectrum Of Relict Gravitational Radiation And The Early State Of The Universe". Journal of Experimental and Theoretical Physics Letters. 30: 682. Bibcode:1979JETPL..30..682S. ; Starobinskii, A. A. (December 1979). "Spectrum of relict gravitational radiation and the early state of the universe". Pisma Zh. Eksp. Teor. Fiz. (Soviet Journal of Experimental and Theoretical Physics Letters). 30: 719. Bibcode:1979ZhPmR..30..719S.
  2. ↑ Starobinsky, A.A (1980). "A new type of isotropic cosmological models without singularity". Physics Letters B. 91: 99–102. doi:10.1016/0370-2693(80)90670-X.
  3. 1 2 "Planck 2018 results. X. Constraints on inflation". arXiv:1807.06211.


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