Power Suppression and Lensing Anomaly -- A phenomenological investigation
arXiv:2504.21386 · doi:10.1103/ksdc-pb3h
Abstract
Primordial power spectra with low power at long wavelengths can alleviate lensing anomaly. However the extent to which data favours such a primordial spectra is not clear. In this work, we investigate power suppression and related mitigation of lensing anomaly with the help of phenomenological models which are valid over scales of interest. We consider simple extensions to nearly scale invariant power spectra such as those which includes running and running of running of spectral index. We perform Bayesian analysis of these models, which are agnostic about power suppression, with Planck legacy data and show that data tend to choose parameters which leads to power suppression at low multipoles. We then investigate the connection between power suppression and alleviation of lensing anomaly and show that lensing anomaly is mitigated the most in models with maximum suppression of power at low multipoles. We also analyse the significance of these findings using information criteria. These results are further analyzed in the light of Planck Release 4 data using CamSpec, HiLLiPoP and LoLLiPoP likelihoods in which departure of lensing parameter from one is significantly reduced. Furthermore, we investigate the ability of near-ultimate future CMB missions such as ECHO to put tighter constraints on these models and to settle the issue. We conclude that we can make stronger conclusions about the presence of power suppression in the future by studying such simple phenomenological models.
Version accepted for publication in Physical Review D; 28 pages, 10 figures and 16 tables
References in corpus (59)
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
- The Sloan Digital Sky Survey: Technical Summary
- HEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere
- Efficient Computation of CMB anisotropies in closed FRW models
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
- Cosmological parameters from CMB and other data: a Monte-Carlo approach
- The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant
- Planck 2018 results. X. Constraints on inflation
- The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15
- Planck 2018 results. I. Overview and the cosmological legacy of Planck
- 4-Year COBE DMR Cosmic Microwave Background Observations: Maps and Basic Results
- Dark Energy Survey Year 1 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
- Planck 2018 results. V. CMB power spectra and likelihoods
- The Dark Energy Camera
- Encyclopaedia Inflationaris
- Cobaya: Code for Bayesian Analysis of hierarchical physical models
- The Atacama Cosmology Telescope: DR4 Maps and Cosmological Parameters
- Planck 2018 results. VII. Isotropy and Statistics of the CMB
- Determination of Inflationary Observables by Cosmic Microwave Background Anisotropy Experiments
- Suppressing the lower Multipoles in the CMB Anisotropies
- CMB Anomalies after Planck
- Planck intermediate results. LVII. Joint Planck LFI and HFI data processing
- The Best Inflationary Models After Planck
- GetDist: a Python package for analysing Monte Carlo samples
- Improved limits on the tensor-to-scalar ratio using BICEP and Planck
- Likelihood Analysis of CMB Temperature and Polarization Power Spectra
- The Dark Energy Survey Image Processing Pipeline
- Cosmic Microwave Weak lensing data as a test for the dark universe
- CMB power spectra and cosmological parameters from Planck PR4 with CamSpec
- PRISM (Polarized Radiation Imaging and Spectroscopy Mission): An Extended White Paper
- Spontaneous Isotropy Breaking: A Mechanism for CMB Multipole Alignments
- Cosmological parameters derived from the final (PR4) Planck data release
- 2-Point Correlations in the COBE DMR 4-Year Anisotropy Maps
- High-redshift cosmography: auxiliary variables versus Padé polynomials
- CMB mapping experiments: a designer's guide
- Planck constraints on the tensor-to-scalar ratio
- Punctuated inflation and the low CMB multipoles
- Exploring Cosmic Origins with CORE: Survey requirements and mission design
- BINGO: A code for the efficient computation of the scalar bi-spectrum
- Constraints on mode couplings and modulation of the CMB with WMAP data
- Alleviating the Tension in the Cosmic Microwave Background using Planck-Scale Physics
- Observability of secondary Doppler peaks in the CMBR power spectrum by experiments with small fields
- Large scale anomalies in the CMB and non-Gaussianity in bouncing cosmologies
- On the scalar consistency relation away from slow roll
- High-redshift cosmography: Application and comparison with different methods
- Non-Gaussianity in Loop Quantum Cosmology
- Relieving tensions related to the lensing of CMB temperature power spectra
- Examining the consistency relations describing the three-point functions involving tensors
- Power Spectra Based Planck Constraints on Compensated Isocurvature, and Forecasts for LiteBIRD and CORE Space Missions
- -mode forecast of CMB-Bhrat
- Anomalies in the CMB from a cosmic bounce
- Predictions for the CMB from an anisotropic quantum bounce
- Numerical evaluation of the three-point scalar-tensor cross-correlations and the tensor bi-spectrum
- Observational consequences of Bianchi I spacetimes in loop quantum cosmology
- Constraining the bispectrum from bouncing cosmologies with Planck
- Alleviation of anomalies from the non-oscillatory vacuum in loop quantum cosmology
- Ideal scales for weighing the Universe
- Impact of Low ell's on Large Scale Structure Anomalies
- Estimation of imprints of the bounce in loop quantum cosmology on the bispectra of cosmic microwave background