Naturalness and stability of the generalized Chaplygin gas in the seesaw cosmon scenario

Journal Article · Tue Jun 15 04:00:00 EDT 2010 · Physical Review. D, Particles Fields

DOI:https://doi.org/10.1103/PHYSREVD.81.123013· OSTI ID:21408033

Bernardini, A E; Bertolami, O ^[1]

---

1. Departamento de Fisica, Universidade Federal de Sao Carlos, PO Box 676, 13565-905, Sao Carlos, SP (Brazil)

The seesaw mechanism is conceived on the basis that a mass scale, {xi}, and a dimensionless scale, s, can be fine-tuned in order to control the dynamics of active and sterile neutrinos through cosmon-type equations of motion: the seesaw cosmon equations. This allows for sterile neutrinos to be a dark matter candidate. In this scenario, the dynamical masses and energy densities of active and sterile neutrinos can be consistently embedded into the generalized Chaplygin gas (GCG), the unified dark sector model. In addition, dark matter adiabatically coupled to dark energy allows for a natural decoupling of the (active) mass varying neutrino component from the dark sector. Thus mass varying neutrinos turn into a secondary effect. Through the scale parameters, {xi} and s, the proposed scenario allows for a convergence among three distinct frameworks: the cosmon scenario, the seesaw mechanism for mass generation, and the GCG model. It is found that the equation of state of the perturbations is the very one of the GCG background cosmology so that all the results from this approach are maintained, being smoothly modified by active neutrinos. Constrained by the seesaw relations, it is shown that the mass varying mechanism is responsible for the stability against linear perturbations and is indirectly related to the late time cosmological acceleration.

• OSTI ID: 21408033
• Journal Information: Physical Review. D, Particles Fields, Journal Name: Physical Review. D, Particles Fields Journal Issue: 12 Vol. 81; ISSN PRVDAQ; ISSN 0556-2821
• Country of Publication: United States
• Language: English

Related Subjects

72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
79 ASTRONOMY AND ASTROPHYSICS
ACCELERATION
CONVERGENCE
COSMOLOGY
DECOUPLING
DIFFERENTIAL EQUATIONS
DISTURBANCES
ELEMENTARY PARTICLES
ENERGY DENSITY
EQUATIONS
EQUATIONS OF MOTION
EQUATIONS OF STATE
FERMIONS
LEPTONS
MASS
MASSLESS PARTICLES
MATTER
NEUTRINOS
NONLUMINOUS MATTER
PARTIAL DIFFERENTIAL EQUATIONS
PERTURBATION THEORY
SIMULATION
STABILITY