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2007

Growing neutrinos and cosmological selection

Wetterich, C.

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The time evolution of a cosmological scalar field can be stopped by an increasing mass of the neutrinos.

This leads to a transition from a cosmological scaling solution with dynamical dark energy at early time to a cosmological constant dominated universe at late time.
The trigger for the transition is set at the time when the neutrinos become non-relativistic.
The characteristic mass scale for dark energy is thus related to the neutrino mass, the only known particle physics scale in its vicinity.

Growing neutrinos and cosmological selection · Around

Built on

P. Minkowski, Phys. Lett. B67
1979
Earlier work this paper cites.
M. Magg, C. Wetterich, Phys. Lett. 94B
1980
Earlier work this paper cites.
C. Wetterich, Nucl. Phys. B187
1981
Earlier work this paper cites.

Similar

C. Wetterich, Nucl. Phys. B302
1988
Cited alongside, same era.
C. Wetterich, Nucl. Phys. B302
1988
Cited alongside, same era.
C. Wetterich, Phys. Rev. Lett. 90
Original
2003
Cited alongside, same era.
L. Amendola, M. Baldi, C. Wetterich, arXiv: 0706.3064 [astro-ph]
Cited in the paper.

Then

M. Doran, G. Robbers, C. Wetterich, Phys. Rev. D75
2007
Closest in time.
P. Gu, X. Wang, X. Zhang, Phys. Rev. D68
2018
Closest in time.

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