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- W3212779512 abstract "differences between the reionization histories of the spatially flat and non-flat models. Although both the flat and non-flat models can accurately match the low-redshift (z ≲ 6) reionization observations, there is a clear discrepancy between high-redshift (z > 7) Lyman-α emitter data and the predictions from non-flat models. This is solely due to the fact that the non-flat models have a significantly larger electron scattering optical depth, τel, compared to the flat models, which requires an extended and much earlier reionization scenario supported by more high-redshift ionizing sources in the non-flat models. Non-flat models also require strong redshift evolution in the photon escape fraction, which can become unrealistically high (≳1) at some redshifts. However, τel is about 0.9-σ lower in the tilted flat ΛCDM model when the new Planck 2018 data are used and this reduction will partially alleviate the tension between the non-flat model predictions and the data." @default.
- W3212779512 created "2021-11-22" @default.
- W3212779512 creator A5062376442 @default.
- W3212779512 date "2020-09-22" @default.
- W3212779512 modified "2023-09-25" @default.
- W3212779512 title "Testing Non-Flat, Dynamical Dark Energy, Inflation Models: List of Publications and Summary Results" @default.
- W3212779512 doi "https://doi.org/10.2172/1644099" @default.
- W3212779512 hasPublicationYear "2020" @default.
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