Neutrino Clouds
arXiv:hep-ph/9603392 · doi:10.1142/S0217751X98001414
Abstract
We consider the possibility that neutrinos are coupled very weakly to an extremely light scalar boson. We first analyze the simple problem of one generation of neutrino and show that, for ranges of parameters that are allowed by existing data, such a system can have serious consequences for the evolution of stars and could impact precision laboratory measurements. We discuss the extension to more generations and show that the general conclusion remains viable. Finally, we note that, should such a scalar field be present, experiments give information about effective masses, not the masses that arise in unified field theories.
23 pages, LaTex, 9 Postscript figures included; submitted to Phys. Rev. D
References in corpus (1)
Cited by in corpus (42)
- Study of the anomalous acceleration of Pioneer 10 and 11
- Indication, from Pioneer 10/11, Galileo, and Ulysses Data, of an Apparent Anomalous, Weak, Long-Range Acceleration
- Dark Energy from Mass Varying Neutrinos
- Gravitational clustering of relic neutrinos and implications for their detection
- Cosmological Signatures of Interacting Neutrinos
- Solar mass-varying neutrino oscillations
- Distorted Neutrino Oscillations From Ultralight Scalar Dark Matter
- Supersymmetric Theories of Neutrino Dark Energy
- Model of Mass Varying Neutrinos in SUSY
- Non-standard Hamiltonian effects on neutrino oscillations
- Speed of Sound in the Mass Varying Neutrinos Scenario
- Confronting mass-varying neutrinos with MiniBooNE
- A New Light Higgs Boson and Short-Baseline Neutrino Anomalies
- Probing Neutrino Dark Energy with Extremely High-Energy Cosmic Neutrinos
- Sensitivity of Neutrino Mass Experiments to the Cosmic Neutrino Background
- Annual Modulation of Cosmic Relic Neutrinos
- Neutrino Lumps in Quintessence Cosmology
- Neutrino bound states and bound systems
- New Matter Effects and BBN Constraints for Mass Varying Neutrinos
- Measuring Active-Sterile Neutrino Oscillations with a Stopped Pion Neutrino Source
- Mass-Varying Neutrinos from a Variable Cosmological Constant
- Analysis of Beta-Decay Rates for Ag108, Ba133, Eu152, Eu154, Kr85, Ra226 And Sr90, Measured at the Physikalisch-Technische Bundesanstalt from 1990 to 1996
- Tritium Beta Decay, Neutrino Mass Matrices and Interactions Beyond the Standard Model
- Embedding the Texture of the Neutrino Mass Matrix into the MaVaNs Scenario
- Mass Varying Neutrinos, Quintessence, and the Accelerating Expansion of the Universe
- UHE neutrino damping in a thermal gas of relic neutrinos
- Upper Limits on the Cosmic Neutrino Background from Cosmic Rays
- Stability of mass varying particle lumps
- New Constraints on Dark Matter and Cosmic Neutrino Profiles through Gravity
- Spin light of neutrino in astrophysical environments
- Probing nonstandard neutrino cosmology with terrestrial neutrino experiments
- Detection of cosmic neutrino clustering by cosmic ray spectra
- Symmetry breaking, and the effect of matter density on neutrino oscillation
- Probing Long-Range Forces Between Neutrinos with Cosmic Structures
- The effect of supersymmetry breaking in the Mass Varying Neutrinos
- A Mesonic Analog of the Deuteron
- Neutrino Clustering in the Galaxy with a Global Monopole
- Neutrino masses and mixing
- Daemons, the "Troitsk anomaly" in tritium beta spectrum, and the KATRIN experiment
- Equilibrium and stability of neutrino lumps as TOV solutions
- Superfluidity in neutrino clusters
- New Constraint on the Local Relic Neutrino Background Overdensity with the First KATRIN Data Runs