Are cosmological neutrinos free-streaming?
arXiv:0806.1735 · doi:10.1103/PhysRevD.79.043512
Abstract
Precision data from cosmology suggest neutrinos stream freely and hence interact very weakly around the epoch of recombination. We study this issue in a simple framework where neutrinos recouple instantaneously and stop streaming freely at a redshift z_i. The latest cosmological data imply z_i < 1500, the exact constraint depending somewhat on the assumed prior on z_i. This bound translates into a limit on the coupling strength between neutrinos and majoron-like particles phi, implying tau > 1 x 10^10 s (m_2/50 meV)^3 for the decay nu_2 -> nu_1+phi.
4 pages, 2 figures
References in corpus (34)
- Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
- Cosmological parameters from CMB and other data: a Monte-Carlo approach
- Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant
- The 2dF Galaxy Redshift Survey: Power-spectrum analysis of the final dataset and cosmological implications
- Cosmological Perturbation Theory in the Synchronous and Conformal Newtonian Gauges
- Cosmological Perturbation Theory in the Synchronous vs. Conformal Newtonian Gauge
- Cosmological Constraints from the SDSS Luminous Red Galaxies
- Massive neutrinos and cosmology
- Relic neutrino decoupling including flavour oscillations
- Cosmological parameters from combining the Lyman-alpha forest with CMB, galaxy clustering and SN constraints
- Scrutinizing Exotic Cosmological Models Using ESSENCE Supernova Data Combined with Other Cosmological Probes
- Neutrino masses and the number of neutrino species from WMAP and 2dFGRS
- Neutrinoless Universe
- Constraining invisible neutrino decays with the cosmic microwave background
- The neutrino mass bound from WMAP-3, the baryon acoustic peak, the SNLS supernovae and the Lyman-alpha forest
- Structure formation with strongly interacting neutrinos - implications for the cosmological neutrino mass bound
- Cosmological Signatures of Interacting Neutrinos
- Observables sensitive to absolute neutrino masses: A reappraisal after WMAP-3y and first MINOS results
- Primordial Neutrinos
- Observational bounds on the cosmic radiation density
- Recovering the Inflationary Potential and Primordial Power Spectrum With a Slow Roll Prior: Methodology and Application to WMAP 3 Year Data
- Present bounds on the relativistic energy density in the Universe from cosmological observables
- Cosmology of neutrinos and extra light particles after WMAP3
- Constraint on the Effective Number of Neutrino Species from the WMAP and SDSS LRG Power Spectra
- New CMBR data and the cosmic neutrino background
- Cosmological neutrino mass detection: The best probe of neutrino lifetime
- Nonlinear corrections to the cosmological matter power spectrum and scale-dependent galaxy bias: implications for parameter estimation
- Bulk viscosity of a gas of neutrinos and coupled scalar particles, in the era of recombination
- Anisotropies in the Cosmic Neutrino Background after WMAP 5-year Data
- Interacting Hot Dark Matter
- Revised WMAP constraints on neutrino masses and other extensions of the minimal CDM model
- Conservative Estimates of the Mass of the Neutrino from Cosmology
- New constraint on the cosmological background of relativistic particles
- The Impact of Prior Assumptions on Bayesian Estimates of Inflation Parameters and the Expected Gravitational Waves Signal from Inflation
Cited by in corpus (48)
- The Neutrino Puzzle: Anomalies, Interactions, and Cosmological Tensions
- Constraining the Self-Interacting Neutrino Interpretation of the Hubble Tension
- Limits on Neutrino-Neutrino Scattering in the Early Universe
- Updated constraints on non-standard neutrino interactions from Planck
- The Case for Dark Radiation
- Interacting neutrinos in cosmology: exact description and constraints
- Observational Constraints on Secret Neutrino Interactions from Big Bang Nucleosynthesis
- Cosmology with self-interacting sterile neutrinos and dark matter - A pseudoscalar model
- Small neutrino masses from gravitational -term
- Neutrino physics from precision cosmology
- Cosmological Constraints on Invisible Neutrino Decays Revisited
- Cosmological constraints on neutrino self-interactions with a light mediator
- Boltzmann hierarchy for interacting neutrinos I: formalism
- Snowmass White Paper: Beyond the Standard Model effects on Neutrino Flavor
- Constraints on neutrino and dark radiation interactions using cosmological observations
- Invisible neutrino decay in precision cosmology
- Visible Decay of Astrophysical Neutrinos at IceCube
- Probing secret interactions of eV-scale sterile neutrinos with the diffuse supernova neutrino background
- How to relax the cosmological neutrino mass bound
- Solving the Hubble tension without spoiling Big Bang Nucleosynthesis
- Leptonic Scalars at the LHC
- Constraining the invisible neutrino decay with KM3NeT-ORCA
- Detecting the cosmological neutrino background in the CMB
- Long-Range Lepton Flavor Interactions and Neutrino Oscillations
- Confronting interacting dark radiation scenarios with cosmological data
- Dark Radiation in extended cosmological scenarios
- Precision CMB constraints on eV-scale bosons coupled to neutrinos
- Origin of Delta N_eff as a Result of an Interaction between Dark Radiation and Dark Matter
- Neutrino meets ultralight dark matter: decay and cosmology
- Massive neutrino self-interactions with a light mediator in cosmology
- Probing neutrino interactions and dark radiation with gravitational waves
- Global view of neutrino interactions in cosmology: The freestreaming window as seen by Planck
- Diffuse Ultra-High Energy Neutrino Fluxes and Physics Beyond the Standard Model
- Galactic Dark Matter Population as the Source of Neutrino Masses
- The Cosmic Neutrino Background Anisotropy - Linear Theory
- Analytic treatment of 3-flavor neutrino oscillation and decay in matter
- Probing nonstandard neutrino cosmology with terrestrial neutrino experiments
- Visible neutrino decay at DUNE
- Self-interacting neutrinos, the Hubble parameter tension, and the Cosmic Microwave Background
- Massive Fermi Gas in the Expanding Universe
- Decaying neutrinos: The long way to isotropy
- Exploring the vacuum structure of gravitationally induced neutrino masses
- Neutrino decays as a natural explanation of the neutrino mass tension
- Cosmic Neutrino Background as a Ferromagnet
- Damping of cosmological tensor modes in Horndeski theories after GW170817
- Majorana CP Violation Insights from Decaying Neutrinos
- Improved cosmological constraints on the neutrino mass and lifetime
- Sound Speed and Viscosity of Semi-Relativistic Relic Neutrinos