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WMAP5 constraints on the unified model of dark energy and dark matter

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arxiv 0805.0731 v1 pith:RIOUIJEK submitted 2008-05-06 astro-ph

T. Barreiro , O. Bertolami , P. Torres This is my paper · ORCID
classification astro-ph
keywords darkconstraintsenergyfirstmattermodelunifiedamplitudes
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We derive constraints on the parameter space of the unified model of dark energy and dark matter, the Generalized Chaplygin Gas (GCG), from the amplitudes and positions of the first few peaks and first trough of the cosmic microwave background radiation (CMBR) power spectrum, using the latest WMAP five year data.

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    hep-ph 2019-08 conditional novelty 4.0 of 10

    Fermionic dipole dark matter can match the observed relic abundance and Planck CMB bounds only in a narrow mass-dipole window, with an upper cutoff M16* = 0.44 (dipole ~0.44 x 10^-16 e cm) when electric and magnetic m...

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