Abstract <p>We establish a new <InlineEquation ID="IEq3"> <EquationSource Format="TEX">\(SU(N)\)</EquationSource> <!--GravCos2670004Balakin-m3--> </InlineEquation> symmetric model of interaction between the fields of four types: a multiplet of vector fields, which describes the so-called color aether, a multiplet of pseudoscalar fields, which is associated with a multi-component cosmic dark matter, gauge and gravitational fields. The extended Lagrangian of the model contains a new constructive element based on the covariant <InlineEquation ID="IEq4"> <EquationSource Format="TEX">\(SU(N)\)</EquationSource> <!--GravCos2670004Balakin-m4--> </InlineEquation> symmetric divergence of the multiplet of vector fields; this new element, being a multiplet of scalars from the point of view of space-time transformations, and a color vector from the point of view of the <InlineEquation ID="IEq5"> <EquationSource Format="TEX">\(SU(N)\)</EquationSource> <!--GravCos2670004Balakin-m5--> </InlineEquation> group space, gives us a possibility to properly formulate a multi-axionic extension of the Peccei-Quinn theory. A hypothesis of a spontaneous polarization of the multi-axionic color aether in the early Universe is presented. A set of self-consistent master equations of the model is derived. An application to cosmology is considered: the obtained master equations are solved for a truncated test model based on the Bianchi-I space-time platform.</p>

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Decay of a Multi-Axionic \(\boldsymbol{SU(N)}\) Symmetric Color Aether in the Early Universe as an Origin of Emergence of Multicomponent Dark Matter

  • Alexander B. Balakin,
  • Gleb B. Kiselev

摘要

Abstract

We establish a new \(SU(N)\) symmetric model of interaction between the fields of four types: a multiplet of vector fields, which describes the so-called color aether, a multiplet of pseudoscalar fields, which is associated with a multi-component cosmic dark matter, gauge and gravitational fields. The extended Lagrangian of the model contains a new constructive element based on the covariant \(SU(N)\) symmetric divergence of the multiplet of vector fields; this new element, being a multiplet of scalars from the point of view of space-time transformations, and a color vector from the point of view of the \(SU(N)\) group space, gives us a possibility to properly formulate a multi-axionic extension of the Peccei-Quinn theory. A hypothesis of a spontaneous polarization of the multi-axionic color aether in the early Universe is presented. A set of self-consistent master equations of the model is derived. An application to cosmology is considered: the obtained master equations are solved for a truncated test model based on the Bianchi-I space-time platform.