Primordial tensor mode from the neutrino sector
Shohei Saga, Shuichiro Yokoyama
astro-ph.CO
Submitted: 2026-07-16
Comments: 9 pages, 4 figures
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- An All-Sky Analysis of Polarization in the Microwave Background
- Statistics of Cosmic Microwave Background Polarization
- CMB Anisotropies: Total Angular Momentum Method
- Planck 2018 results. VI. Cosmological parameters
- BICEP / Keck XIII: Improved Constraints on Primordial Gravitational Waves using Planck, WMAP, and BICEP/Keck Observations through the 2018 Observing Season
- LiteBIRD: JAXA's new strategic L-class mission for all-sky surveys of cosmic microwave background polarization
- Probing Cosmic Inflation with the LiteBIRD Cosmic Microwave Background Polarization Survey
- Cosmological perturbations
- Planck 2013 results. XXII. Constraints on inflation
- Kinetic vs. Thermal-Field-Theory Approach to Cosmological Perturbations
- Observable primordial vector modes
- Constraint on the primordial vector mode and its magnetic field generation from seven-year Wilkinson Microwave Anisotropy Probe Observations
- Constraining primordial vector mode from B-mode polarization
- Resurrecting Gravitational Vector Modes and their Magnetogenesis
- The Status of Gravitational Vector Perturbations with Recent CMB Data
- Revisiting constraints on primordial vector modes and implications for sourced magnetic fields and observed $EB$ power spectrum
- Massive Neutrinos and Magnetic Fields in the Early Universe
- CMB anisotropies from primordial inhomogeneous magnetic fields
- Efficient Computation of CMB anisotropies in closed FRW models
- Planck 2018 results. V. CMB power spectra and likelihoods
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