Nonminimal macroscopic models of a scalar field based on microscopic dynamics: extension of the theory to negative masses

DOI10.1134/S0202289315040076zbMath1333.83158arXiv1504.02768WikidataQ125825175 ScholiaQ125825175MaRDI QIDQ253765

F. Blanchet-Sadri, M. Dambrine

Publication date: 8 March 2016

Published in: Gravitation \& Cosmology (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1504.02768

zbMATH Keywords

action functionalmultiple scalar fieldsnegative masses

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Equations of motion in general relativity and gravitational theory (83C10)

Related Items (9)

Collisionless self-gravitating statistical systems of scalarly interacting particles ⋮ Statistical cosmological fermion systems with phantom scalar interaction of particles ⋮ Cosmological evolution of the Boltzmann plasma with phantom scalar interparticle interaction. II: Multicomponent system without charge symmetry ⋮ Qualitative and numerical analysis of a cosmological model based on a phantom scalar field with self-interaction ⋮ Cosmological evolution of a scalar-charged degenerate cosmological plasma with Higgs scalar fields ⋮ Complete cosmological model based on an asymmetric scalar Higgs doublet ⋮ Cosmological models based on a statistical system of scalar charged degenerate fermions and an asymmetric Higgs scalar doublet ⋮ Peculiarities of cosmological models based on a nonlinear asymmetric scalar doublet with minimal interaction. I. Qualitative analysis ⋮ Cosmological evolution of a statistical system of degenerate scalarly charged fermions with an asymmetric scalar doublet. I: two-component system of assorted charges

Cites Work

• Statistical systems with phantom scalar interaction in gravitation theory. I. Microscopic dynamics
• Statistical systems with phantom scalar interaction in gravitation theory. II. Macroscopic equations and cosmological models
• Cosmological evolution of plasma with scalar interparticle interaction. I. canonical formulation of classical scalar interaction
• Statistical dynamics of a classical particle ensemble in the gravitational field
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