Why three generations?
arXiv:1602.03003 · doi:10.1016/j.physletb.2016.05.025
Abstract
We discuss an anthropic explanation of why there exist three generations of fermions. If one assumes that the right-handed neutrino sector is responsible for both the matter-antimatter asymmetry and the dark matter, then anthropic selection favors three or more families of fermions. For successful leptogenesis, at least two right-handed neutrinos are needed, while the third right-handed neutrino is invoked to play the role of dark matter. The number of the right-handed neutrinos is tied to the number of generations by the anomaly constraints of the gauge symmetry. Combining anthropic arguments with observational constraints, we obtain predictions for the -ray observations, as well as for neutrinoless double-beta decay.
arXiv comment7pages, 2 figures
References in corpus (45)
- Sterile Neutrinos as Dark Matter
- Leptogenesis
- Detection of An Unidentified Emission Line in the Stacked X-ray spectrum of Galaxy Clusters
- An unidentified line in X-ray spectra of the Andromeda galaxy and Perseus galaxy cluster
- Leptogenesis as the origin of matter
- Sterile Neutrino Hot, Warm, and Cold Dark Matter
- Search for Majorana neutrinos with the first two years of EXO-200 data
- Status of three-neutrino oscillation parameters, circa 2013
- Cosmological Sign of Neutrino CP Violation
- Massive sterile neutrinos as warm Dark Matter
- Dimensionless constants, cosmology and other dark matters
- Sterile neutrinos: the dark side of the light fermions
- Sterile neutrinos, dark matter, and the pulsar velocities in models with a Higgs singlet
- Can sterile neutrinos be the dark matter?
- Dark-matter sterile neutrinos in models with a gauge singlet in the Higgs sector
- Direct Detection of Warm Dark Matter in the X-ray
- Lightest sterile neutrino abundance within the nuMSM
- Opening a new window for warm dark matter
- Constraints on sterile neutrino as a dark matter candidate from the diffuse X-ray background
- Pulsar kicks from a dark-matter sterile neutrino
- Checking the dark matter origin of 3.53 keV line with the Milky Way center
- Number of Fermion Generations Derived from Anomaly Cancellation
- Production and Evolution of Perturbations of Sterile Neutrino Dark Matter
- Neutral current induced neutrino oscillations in a supernova
- Dark Matter from Split Seesaw
- Direct X-ray Constraints on Sterile Neutrino Warm Dark Matter
- Constraining DM properties with SPI
- Constraints on the parameters of radiatively decaying dark matter from the dark matter halo of the Milky Way and Ursa Minor
- Restrictions on parameters of sterile neutrino dark matter from observations of galaxy clusters
- New Limits on Sterile Neutrinos from Suzaku Observations of the Ursa Minor Dwarf Spheroidal Galaxy
- Constraining sterile neutrino dark matter by phase-space density observations
- Dark Matter Search Using Chandra Observations of Willman 1, and a Spectral Feature Consistent with a Decay Line of a 5 keV Sterile Neutrino
- Searching for dark matter in X-rays: how not to check the dark matter origin of a spectral feature
- Seesaw Mechanism with Occam's Razor
- Small-scale structure formation properties of chilled sterile neutrinos as dark matter
- Diluted equilibrium sterile neutrino dark matter
- Improved Limits on Sterile Neutrino Dark Matter using Full-Sky Fermi Gamma-Ray Burst Monitor Data
- Dark Matter Search Using XMM-Newton Observations of Willman 1
- Dark Matter and The Anthropic Principle
- Effective Majorana Mass and Neutrinoless Double Beta Decay
- Delayed pulsar kicks from the emission of sterile neutrinos
- Gauged Discrete Symmetries and Proton Stability
- Non-Anomalous Discrete R-symmetry Decrees Three Generations
- Longevity Problem of Sterile Neutrino Dark Matter
- Semi-Simple Unification on T^6/Z_12 Orientifold in the Type IIB Supergravity
Cited by in corpus (9)
- Three generations, two unbroken gauge symmetries, and one eight-dimensional algebra
- The Degree of Fine-Tuning in our Universe -- and Others
- Right-handed Neutrino Dark Matter in a U(1) Extension of the Standard Model
- Dark Photon Dark Matter in the minimal Model
- Right-Handed Neutrino Dark Matter with Forbidden Annihilation
- Dark Matter Annihilation via Breit-Wigner Enhancement with Heavier Mediator
- Three Generations and a Trio of Trialities
- Thermal Relic Right-Handed Neutrino Dark Matter
- A Superalgebra Within: representations of lightest standard model particles form a -graded algebra