Cosmology Based on f(R) Gravity Admits 1 eV Sterile Neutrinos
arXiv:1203.6828 · doi:10.1103/PhysRevLett.110.121302
Abstract
It is shown that the tension between recent neutrino oscillation experiments, favoring sterile neutrinos with masses of the order of 1 eV, and cosmological data which impose stringent constraints on neutrino masses from the free streaming suppression of density fluctuations, can be resolved in models of the present accelerated expansion of the Universe based on f(R) gravity.
5 pages, 3 figures, matches the published version in Phys. Rev. Lett
References in corpus (15)
- Big-Bang Nucleosynthesis
- Models of f(R) Cosmic Acceleration that Evade Solar-System Tests
- Disappearing cosmological constant in f(R) gravity
- The Reactor Antineutrino Anomaly
- The Large Scale Structure of f(R) Gravity
- Statistical Significance of the Gallium Anomaly
- Matter density perturbations and effective gravitational constant in modified gravity models of dark energy
- Cosmology seeking friendship with sterile neutrinos
- Cluster Constraints on f(R) Gravity
- Testing gravity with CAMB and CosmoMC
- A Singularity Problem with f(R) Dark Energy
- Aspects of cosmological expansion in F(R) gravity models
- Phantom boundary crossing and anomalous growth index of fluctuations in viable f(R) models of cosmic acceleration
- Future Oscillations around Phantom Divide in f(R) Gravity
- Matter power spectrum in f(R) gravity with massive neutrinos
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- Matter Power Spectra in Viable Gravity Models with Massive Neutrinos
- -gravity and neutrino physics
- Observational constraints on Starobinsky cosmology from cosmic expansion and structure growth data
- Clustering and redshift-space distortions in modified gravity models with massive neutrinos
- Joint reconstructions of growth and expansion histories from stage-IV surveys with minimal assumptions. II. Modified gravity and massive neutrinos
- Matter Power Spectra in Viable Gravity Models with Dynamical Background
- Neutrino spin oscillations in conformally gravity coupling models and quintessence surrounding a black hole
- Cosmology based on gravity with eV sterile neutrino
- Weighing neutrinos in gravity in light of BICEP2
- Scalaron production in contracting astrophysical objects
- Cosmological dynamics of f(R) models in dynamical system analysis
- Cosmological constraints on -corrected Appleby-Battye model
- Cosmological Inflation in a Generalized Unimodular Gravity
- Euclid: Constraints on f(R) cosmologies from the spectroscopic and photometric primary probes