Raising the reionization optical depth with inflationary CMB features
Tanisha Jhaveri, Wayne Hu, Vivian Miranda
astro-ph.CO
Submitted: 2026-06-18
Code: https://github.com/lesgourg/class_public
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Wilkinson Microwave Anisotropy Probe (WMAP) First Year Observations: TE Polarization
- Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results
- Planck 2013 results. XVI. Cosmological parameters
- Planck 2015 results. XIII. Cosmological parameters
- Planck 2018 results. VI. Cosmological parameters
- Reionization optical depth determination from Planck HFI data with ten percent accuracy
- Planck intermediate results. LI. Features in the cosmic microwave background temperature power spectrum and shifts in cosmological parameters
- DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints
- Turning a negative neutrino mass into a positive optical depth
- Dispu$\tau$able: the high cost of a low optical depth
- The Complete CEERS Early Universe Galaxy Sample: A Surprisingly Slow Evolution of the Space Density of Bright Galaxies at z ~ 8.5-14.5
- Early results from GLASS-JWST. III: Galaxy candidates at z$\sim$9-15
- Overview of the JWST Advanced Deep Extragalactic Survey (JADES)
- A Comprehensive Study on Galaxies at z~9-16 Found in the Early JWST Data: UV Luminosity Functions and Cosmic Star-Formation History at the Pre-Reionization Epoch
- Planck 2018 results. VII. Isotropy and Statistics of the CMB
- Evidence for horizon-scale power from CMB polarization
- Reionization optical depth and CMB-BAO tension in punctuated inflation
- Updated Constraints on Infrared Cutoff Models and Implications for Large-Scale CMB Anomalies
- Inflationary vs. Reionization Features from Planck 2015 Data
- Generalized Slow Roll for Large Power Spectrum Features
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