Lepton asymmetry in the primordial gravitational wave spectrum
arXiv:hep-ph/0611121 · doi:10.1103/PhysRevD.75.084017
Abstract
Effects of neutrino free streaming is evaluated on the primordial spectrum of gravitational radiation taking both neutrino chemical potential and masses into account. The former or the lepton asymmetry induces two competitive effects, namely, to increase anisotropic pressure, which damps the gravitational wave more, and to delay the matter-radiation equality time, which reduces the damping. The latter effect is more prominent and a large lepton asymmetry would reduce the damping. We may thereby be able to measure the magnitude of lepton asymmetry from the primordial gravitational wave spectrum.
arXiv comment14 pages, 5 figures
References in corpus (31)
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
- First Results from KamLAND: Evidence for Reactor Anti-Neutrino Disappearance
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Implications for Inflation
- Neutrinos in cosmology
- Primordial Nucleosynthesis: Theory and Observations
- Cosmological bounds on neutrino degeneracy improved by flavor oscillations
- Improved Calculation of the Primordial Gravitational Wave Spectrum in the Standard Model
- Damping of Tensor Modes in Cosmology
- Review of Big Bang Nucleosynthesis and Primordial Abundances
- Large neutrino asymmetries from neutrino oscillations
- Constraining neutrino physics with BBN and CMBR
- Probing the equation of state of the early universe with a space laser interferometer
- The first second of the Universe
- Cosmological implications of a Relic Neutrino Asymmetry
- Chaotic Amplification of Neutrino Chemical Potentials by Neutrino Oscillations in Big Bang Nucleosynthesis
- Comment on "Damping of Tensor Modes in Cosmology"
- Large lepton asymmetry from Q-balls
- Generation of Large Lepton Asymmetries
- The Small Observed Baryon Asymmetry from a Large Lepton Asymmetry
- Naturally Large Cosmological Neutrino Asymmetries in the MSSM
- Spontaneous baryogenesis in flat directions
- Limit on the Neutrino Mass from the WMAP Three Year Data
- Baryogenesis in a flat direction with neither baryon nor lepton charge
- Evolution of gravitational waves through the cosmological QCD transition
- Generation of cosmological large lepton asymmetry from a rolling scalar field
- Constraints on Neutrino Degeneracy from the Cosmic Microwave Background and Primordial Nucleosynthesis
- Blocking Active-Sterile Neutrino Oscillations in the Early Universe with a Majoron Field
- Do neutrino flavor oscillations forbid large lepton asymmetry of the universe ?
- Joint constraints on the lepton asymmetry of the Universe and neutrino mass from the Wilkinson Microwave Anisotropy Probe
- Remarks on the Cosmic Density of Degenerate Neutrinos
Cited by in corpus (15)
- Space laser interferometers can determine the thermal history of the early Universe
- Probing dark radiation with inflationary gravitational waves
- Probing the properties of relic neutrinos using the cosmic microwave background, the Hubble Space Telescope and galaxy clusters
- Impact of anisotropic stress of free-streaming particles on gravitational waves induced by cosmological density perturbations
- WMAP 5-year constraints on lepton asymmetry and radiation energy density: Implications for Planck
- Perturbations of Matter Fields in the Second-order Gauge-invariant Cosmological Perturbation Theory
- Inflationary Gravitational Waves and the Evolution of the Early Universe
- Probing neutrino interactions and dark radiation with gravitational waves
- Cosmological evidence for leptonic asymmetry after Planck
- Gravitational Waves from Q-ball Formation
- Constraints on neutrino masses from WMAP5 and BBN in the lepton asymmetric universe
- Forecast on lepton asymmetry from future CMB experiments
- Effective Search Templates for a Primordial Stochastic Gravitational Wave Background
- Kinetic theory and evolution of cosmological fluctuations with neutrino number asymmetry
- Subdominant Dark Matter sterile neutrino resonant production in the light of Planck