Updated Cosmological Constraints in Extended Parameter Space with Planck PR4, DESI Baryon Acoustic Oscillations, and Supernovae: Dynamical Dark Energy, Neutrino Masses, Lensing Anomaly, and the Hubble Tension
| Autor: | Shouvik Roy Choudhury, Teppei Okumura |
|---|---|
| Jazyk: | angličtina |
| Rok vydání: | 2024 |
| Předmět: | |
| Zdroj: | The Astrophysical Journal Letters, Vol 976, Iss 1, p L11 (2024) |
| Druh dokumentu: | article |
| ISSN: | 2041-8213 2041-8205 |
| DOI: | 10.3847/2041-8213/ad8c26 |
| Popis: | We present updated constraints on cosmological parameters in a 12-parameter model, extending the standard six-parameter ΛCDM by including dynamical dark energy (DE ; w _0 , w _a ), the sum of neutrino masses (∑ m _ν ), the effective number of non-photon radiation species ( N _eff ), the lensing amplitude scaling ( A _lens ), and the running of the scalar spectral index ( α _s ). For cosmic wave background (CMB) data, we use the Planck Public Release (PR) 4 (2020) HiLLiPoP and LoLLiPoP likelihoods, Planck PR4+Atacama Cosmology Telescope (ACT) DR6 lensing, and Planck 2018 low- ℓ TT likelihoods, along with DESI DR1 baryon acoustic oscillations (BAO) and Pantheon+ and DESY5 uncalibrated Type Ia supernovae (SNe) likelihoods. Key findings are the following: (i) Contrary to DESI results, CMB+BAO+Pantheon+ data include a cosmological constant within 2 σ , while CMB+BAO+DESY5 excludes it at over 2 σ , indicating the dynamical nature of DE is not yet robust. Potential systematics in the DESY5 sample may drive this exclusion. (ii) Some data combinations show a 1 σ + detection of nonzero ∑ m _ν , indicating possible future detection. We also provide a robust upper bound of ∑ m _ν ≲ 0.3 eV (95% confidence limit (CL)). (iii) With CMB+BAO+SNe, A _lens = 1 is included at 2 σ (albeit not at 1 σ ), indicating no significant lensing anomaly in this extended cosmology with Planck PR4 likelihoods. (iv) The Hubble tension persists at 3.2 to 3.9 σ , suggesting these simple extensions do not resolve it. (v) The S _8 tension with Dark Energy Survey Year 3 weak lensing is reduced to 1.4 σ , likely due to additional parameters and the Planck PR4 likelihoods. |
| Databáze: | Directory of Open Access Journals |
| Externí odkaz: |
|