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2011
Vector-field model with compensated cosmological constant and radiation-dominated FRW phase Emelyanov, V., Klinkhamer, F. R.
Understand A special model of a massless vector-field is presented, which has an extra modified-gravity-type interaction term in the action.
The cosmology of the model is studied with standard noninteracting relativistic matter added. It is found that this cosmology can have an early phase where the vector-field starts to compensate a (Planck-scale) cosmological constant and a late Friedmann-Robertson-Walker (FRW) phase where the relativistic-matter energy density dominates the dynamic vacuum energy density. Vector-field model with compensated cosmological constant and radiation-dominated FRW phase · Around
Built on F.R. Klinkhamer and G.E. Volovik, “Vacuum energy density kicked by the electroweak crossover,” Phys. Rev. D
Original
1919
Earlier work this paper cites.
F.R. Klinkhamer, “Effective cosmological constant from TeV-scale physics,” Phys. Rev. D
Original
1939
Earlier work this paper cites.
A.D. Dolgov, “Field model with a dynamic cancellation of the cosmological constant,” JETP Lett
1985
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S. Weinberg, “The cosmological constant problem,” Rev. Mod. Phys
1989
Earlier work this paper cites.
F. Verhulst, Nonlinear Differential Equations and Dynamical Systems
1996
Earlier work this paper cites.
A.D. Dolgov, “Higher spin fields and the problem of cosmological constant,” Phys. Rev. D
1997
Earlier work this paper cites.
Similar V. Sahni and A.A. Starobinsky, “The case for a positive cosmological Λ \Lambda –term,” Int. J. Mod. Phys. D
2000
Cited alongside, same era.
V.A. Rubakov and P.G. Tinyakov, “Ruling out a higher spin field solution to the cosmological constant problem,” Phys. Rev. D
2000
Cited alongside, same era.
C. Charmousis, E.J. Copeland, A. Padilla, and P.M. Saffin, “General second order scalar-tensor theory, self tuning, and the Fab Four,” arXiv:1106.2000
Original
2000
Cited alongside, same era.
F.R. Klinkhamer and G.E. Volovik, “Self-tuning vacuum variable and cosmological constant,” Phys. Rev. D
Original
2008
Cited alongside, same era.
F.R. Klinkhamer and G.E. Volovik, “Dynamic vacuum variable and equilibrium approach in cosmology,” Phys. Rev. D
Original
2008
Then F.R. Klinkhamer and G.E. Volovik, “Towards a solution of the cosmological constant problem,” JETP Lett
Original
2010
Later among the works it cites.
F.R. Klinkhamer, “Effective cosmological constant from TeV-scale physics: Simple field-theoretic model,” Phys. Rev. D
Original
2011
Closest in time.
F.R. Klinkhamer and G.E. Volovik, “Dynamics of the quantum vacuum: Cosmology as relaxation to the equilibrium state,” J. Phys. Conf. Ser
Original
2011
Closest in time.
V. Emelyanov and F.R. Klinkhamer, “Reconsidering a higher-spin-field solution to the main cosmological constant problem,” Phys. Rev. D
Original
2012
Closest in time.
F.R. Klinkhamer, “Inflation and the cosmological constant,” Phys. Rev. D
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Cited alongside, same era.