Cosmic backgrounds from the radio to the far-infrared: recent results and perspectives from cosmological and astrophysical surveys
arXiv:2111.11472 · doi:10.1142/S0218271822300129
Abstract
Cosmological and astrophysical surveys in various wavebands, in particular from the radio to the far-infrared, offer a unique view of the universe's properties and the formation and evolution of its structures. After a preamble on the so-called tension problem, which occurs when different types of data are used to determine cosmological parameters, we discuss the role of fast radio bursts in cosmology, in particular for the missing baryon problem, and the perspectives from the analysis of the 21 cm redshifted line from neutral hydrogen. We then describe the Planck Legacy Archive, its wealth of scientific information and next developments, and the promising perspectives expected from higher resolution observations, in particular for the analysis of the thermal Sunyaev-Zel'dovich effect. Three cosmological results of the Planck mission are presented next: the implications of the map of Comptonization fluctuations, the dipole analysis from cross-correlating cosmic microwave background anisotropy and Comptonization fluctuation maps, and the constraints on the primordial tensor-to-scalar perturbation ratio. Finally, we discuss some future perspectives and alternative scenarios in cosmology, such as the study of the Lorentz invariance violation with the cosmic microwave background polarization, the introduction of new gravitational degrees of freedom to solve the dark matter problem, and the exploitation of the magnification bias with high-redshift sub-millimeter galaxies to constrain cosmological parameters.
v2: 31 pages, 5 figures. IJMPD (World Scientific), in press. v1: 30 pages, 7 figures. Will appear in the Proc. of the MG16 Meeting, online, 5-10 July 2021, eds. R. Ruffini (Intern. Center for Relativistic Astrophysics Network (ICRANet), Italy & University of Rome La Sapienza, Italy) & G. Vereshchagin (Intern. Center for Relativistic Astrophysics Network (ICRANet), Italy), World Scientific, 2022
References in corpus (38)
- In the Realm of the Hubble tension a Review of Solutions
- A bright millisecond radio burst of extragalactic origin
- Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
- A Joint Analysis of BICEP2/Keck Array and Planck Data
- KiDS-1000 Cosmology: Multi-probe weak gravitational lensing and spectroscopic galaxy clustering constraints
- The Host Galaxy and Redshift of the Repeating Fast Radio Burst FRB 121102
- A census of baryons in the Universe from localized fast radio bursts
- Improved upper limits on the 21-cm signal power spectrum of neutral hydrogen at from LOFAR
- Planck intermediate results. LVII. Joint Planck LFI and HFI data processing
- A new relativistic theory for Modified Newtonian Dynamics
- Deep multi-redshift limits on Epoch of Reionisation 21cm Power Spectra from Four Seasons of Murchison Widefield Array Observations
- First Results from HERA Phase I: Upper Limits on the Epoch of Reionization 21 cm Power Spectrum
- Signature of Excess Radio Background in the 21-cm Global Signal and Power Spectrum
- First Season MWA EoR Power Spectrum Results at Redshift 7
- Planck constraints on the tensor-to-scalar ratio
- Can Cosmic Structure form without Dark Matter?
- Improving the Epoch of Reionization Power Spectrum Results from Murchison Widefield Array Season 1 Observations
- First Season MWA Phase II EoR Power Spectrum Results at Redshift 7
- CMB polarization power spectra contributions from a network of cosmic strings
- An EAGLE view of the missing baryons
- Can primordial magnetic fields be the origin of the BICEP2 data?
- Cosmic Magnetic Fields and the CMB
- Simple halo model formalism for the cosmic infrared background and its correlation with the thermal Sunyaev Zel'dovich effect
- Planck intermediate results. LVI. Detection of the CMB dipole through modulation of the thermal Sunyaev-Zeldovich effect: Eppur si muove II
- Kinetic Inductance Detectors for the OLIMPO experiment: in--flight operation and performance
- A hint on the metal-free star formation rate density from 21cm-EDGES data
- The local B-polarization of the CMB: a very sensitive probe of cosmic defects
- Cosmology with the sub-millimetre galaxies magnification bias: Tomographic Analysis
- Delay Spectrum with Phase-Tracking Arrays: Extracting the HI power spectrum from the Epoch of Reionization
- A direct and robust method to observationally constrain the halo mass function via the submillimeter magnification bias: Proof of concept
- Cosmological constraints with the sub-millimetre galaxies Magnification Bias after large scale bias corrections
- Cosmology with the submillimetre galaxies magnification bias: Proof of concept
- Implications of the Lyman- forest for the 21-cm power spectrum from the epoch of reionization
- Kinetic Inductance Detectors and readout electronics for the OLIMPO experiment
- Over-density of SMGs in fields containing z~0.3 galaxies: magnification bias and the implications for studies of galaxy evolution
- Effects of observer peculiar motion on the isotropic background frequency spectrum: from monopole to higher multipoles
- Impact of the vector dark matter on polarization of the CMB photon
- Fast Radio Burst Cosmology and HIRAX