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Implication of the Hubble tension for the primordial Universe in light of recent cosmological data

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arxiv 2103.09729 v2 pith:ZVW4QZHK submitted 2021-03-17 astro-ph.CO gr-qchep-th

Gen Ye , Bin Hu , Yun-Song Piao This is my paper · ORCID
classification astro-ph.COgr-qchep-th
keywords deltahubbletensioncosmologicalprimordialshiftsacousticanalysis
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abstract

In prerecombination resolutions of the Hubble tension, such as early dark energy, new physics before recombination shifts the values of relevant cosmological parameters so that the models can fit with cosmic microwave background and baryon acoustic oscillations observations as well as $\Lambda$CDM does. In this paper, we clarify how the parameter shifts are related with $\delta H_0$, particularly we find the shift of primordial scalar spectral index scales as ${\delta n_s}\simeq 0.4{\delta H_0\over H_0}$ by performing the Monte Carlo Markov chain analysis with the Planck2018+BAO+Pantheon+R19+Keck Array/BICEP dataset. A novel point of our result is that if the current $H_0$ measured locally is correct, complete resolution of the Hubble tension seems to be pointing to a scale invariant Harrison-Zeldovich spectrum, i.e. $n_s= 1$ for $H_0\sim 73$km/s/Mpc.

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Cited by 11 Pith papers

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    Fitting a model of supermassive primordial black holes to JWST data at z=11 reproduces the excess of bright galaxies, but the agreement reflects parameter tuning rather than an independent test.

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