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- W3099973718 abstract "We investigate how the constraint results of inflation models are affected by considering the latest local measurement of $H_0$ in the global fit. We use the observational data, including the Planck CMB full data, the BICEP2 and Keck Array CMB B-mode data, the BAO data, and the latest measurement of Hubble constant, to constrain the $Lambda$CDM+$r$+$N_{rm eff}$ model, and the obtained 1$sigma$ and 2$sigma$ contours of $(n_s, r)$ are compared to the theoretical predictions of selected inflationary models. We find that, in this fit, the scale invariance is only excluded at the 3.3$sigma$ level, and $Delta N_{rm eff}>0$ is favored at the 1.6$sigma$ level. The natural inflation model is now excluded at more than 2$sigma$ level; the Starobinsky $R^2$ model becomes only favored at around 2$sigma$ level; the most favored model becomes the spontaneously broken SUSY inflation model; and, the brane inflation model is also well consistent with the current data, in this case." @default.
- W3099973718 created "2020-11-23" @default.
- W3099973718 creator A5020810072 @default.
- W3099973718 date "2017-04-19" @default.
- W3099973718 modified "2023-10-16" @default.
- W3099973718 title "Impact of the latest measurement of Hubble constant on constraining inflation models" @default.
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- W3099973718 doi "https://doi.org/10.1007/s11433-017-9017-7" @default.
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