# Introducing the Dirac-Milne universe

@article{BenoitLvy2011IntroducingTD,
title={Introducing the Dirac-Milne universe},
author={Aur{\'e}lien Benoit-L{\'e}vy and Gabriel Chardin},
journal={Astronomy and Astrophysics},
year={2011},
volume={537},
pages={78}
}
• Published 13 October 2011
• Physics
• Astronomy and Astrophysics
The ΛCDM standard model, although an excellent parametrization of the present cosmological data, contains two as yet unobserved components, dark matter and dark energy, that constitute more than 95% of the Universe. Faced with this unsatisfactory situation, we study an unconventional cosmology, the Dirac-Milne universe, a matter-antimatter symmetric cosmology, in which antimatter is supposed to present a negative active gravitational mass. The main feature of this cosmology is the linear…

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## References

SHOWING 1-10 OF 73 REFERENCES

### FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE OBSERVATIONS: COSMOLOGICAL INTERPRETATION

• Physics
• 2008
The Wilkinson Microwave Anisotropy Probe (WMAP) 5-year data provide stringent limits on deviations from the minimal, six-parameter Λ cold dark matter model. We report these limits and use them to

### Anisotropies in the cosmic microwave background : an analytic approach

• Physics
• 1995
We introduce a simple yet powerful {\it analytic} method which obtains the structure of cosmic microwave background anisotropies to better than 5-10\% in temperature fluctuations on {\it all} scales.

### Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant

• Physics
• 1998
We present spectral and photometric observations of 10 Type Ia supernovae (SNe Ia) in the redshift range 0.16 ≤ z ≤ 0.62. The luminosity distances of these objects are determined by methods that

### Observational constraints on power-law cosmologies

• Physics
• 1999
In a class of models designed to solve the cosmological constant problem by coupling scalar or tensor classical fields to the space-time curvature, the universal scale factor grows as a power law in

### First-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters

• Physics
• 2003
WMAP precision data enable accurate testing of cosmological models. We find that the emerging standard model of cosmology, a flat Λ-dominated universe seeded by a nearly scale-invariant adiabatic

### Updated Nucleosynthesis Constraints on Unstable Relic Particles

• Physics
• 2003
We revisit the upper limits on the abundance of unstable massive relic particles provided by the success of Big-Bang Nucleosynthesis calculations. We use the cosmic microwave background data to

### Production of heavy elements in inhomogeneous cosmologies

• Physics
• 1994
The incorporation of quantum chromodynamics into big bang cosmology predicts that the universe shifted from a quark-gluon plasma to a meson gas when it was roughly 10 μs old. If this change is due to

### Limits on cosmic matter-antimatter domains from big bang nucleosynthesis

• Physics
• 2001
We present detailed numerical calculations of the light element abundances synthesized in a Universe consisting of matter- and antimatter- domains, as predicted to arise in some electroweak

### The first second of the Universe

The history of the Universe after its first second is now tested by high quality observations of light element abundances and temperature anisotropies of the cosmic microwave background. The epoch of