CMB-S4 forecasts for constraints on through -distortion anisotropy
Diffusion damping of the cosmic microwave background (CMB) power spectrum results from
imperfect photon-baryon coupling in the pre-recombination plasma. Energy release at …
imperfect photon-baryon coupling in the pre-recombination plasma. Energy release at …
CMB-S4: Forecasting Constraints on Through -distortion Anisotropy
D Zegeye, F Bianchini, JR Bond, J Chluba… - Phys. Rev. D, 2023 - inspirehep.net
Diffusion damping of the cosmic microwave background (CMB) power spectrum results from
imperfect photon-baryon coupling in the pre-recombination plasma. At redshift $5\times 10 …
imperfect photon-baryon coupling in the pre-recombination plasma. At redshift $5\times 10 …
CMB-S4: Forecasting Constraints on Through -distortion Anisotropy
D Zegeye, F Bianchini, JR Bond, J Chluba… - arXiv preprint arXiv …, 2023 - arxiv.org
Diffusion damping of the cosmic microwave background (CMB) power spectrum results from
imperfect photon-baryon coupling in the pre-recombination plasma. At redshift $5\times 10 …
imperfect photon-baryon coupling in the pre-recombination plasma. At redshift $5\times 10 …
[PDF][PDF] CMB-S4 forecasts for constraints on fNL through μ-distortion anisotropy
D Zegeye, F Bianchini, JR Bond, J Chluba… - … REVIEW D Phys Rev …, 2023 - research.rug.nl
The paradigm of cosmic inflation presents arguably the most compelling and plausible
scenario for the earliest moments of the existence of our Universe and provides a …
scenario for the earliest moments of the existence of our Universe and provides a …
[引用][C] CMB-S4 forecasts for constraints on fNL through μ-distortion anisotropy
D Zegeye, F Bianchini, JR Bond, J Chluba… - Physical Review …, 2023 - par.nsf.gov
CMB-S4 forecasts for constraints on f NL through μ-distortion anisotropy
D Zegeye, F Bianchini, JR Bond, J Chluba… - Physical Review. D., 2023 - osti.gov
CMB-S4 forecasts for constraints on f NL through μ -distortion anisotropy (Journal Article) |
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CMB-S4 forecasts for constraints on fNL through μ -distortion anisotropy
D Zegeye, F Bianchini, JR Bond, J Chluba… - Physical …, 2023 - ui.adsabs.harvard.edu
Diffusion damping of the cosmic microwave background (CMB) power spectrum results from
imperfect photon-baryon coupling in the pre-recombination plasma. Energy release at …
imperfect photon-baryon coupling in the pre-recombination plasma. Energy release at …
CMB-S4 forecasts for constraints on fNL through μ-distortion anisotropy
D Zegeye, F Bianchini, JR Bond, J Chluba, T Crawford… - 2023 - digital.csic.es
Diffusion damping of the cosmic microwave background (CMB) power spectrum results from
imperfect photon-baryon coupling in the pre-recombination plasma. Energy release at …
imperfect photon-baryon coupling in the pre-recombination plasma. Energy release at …
CMB-S4 forecasts for constraints on fNL through μ-distortion anisotropy
D Zegeye, F Bianchini, JR Bond, J Chluba… - Physical Review …, 2023 - research.rug.nl
Diffusion damping of the cosmic microwave background (CMB) power spectrum results from
imperfect photon-baryon coupling in the pre-recombination plasma. Energy release at …
imperfect photon-baryon coupling in the pre-recombination plasma. Energy release at …