Inflation, Quantum Field Renormalization, and CMB Anisotropies
classification
🌌 astro-ph.CO
gr-qchep-phhep-th
keywords
fieldinflationquantumrenormalizationaccountanisotropieschangeobservable
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We point out that if quantum field renormalization is taken into account the predictions of slow-roll inflation for both the scalar and tensorial power spectra change significantly for wavelengths that today are at observable scales
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