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Cardassian expansion: a model in which the universe is flat, matter dominated, and accelerating

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Cardassian expansion: a model in which the universe is flat, matter dominated, and accelerating (English)

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Katherine Freese

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author name string

Matthew Lewis

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2

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publication date

July 2002

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published in

Physics Letters B

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volume

540

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issue

1-2

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page(s)

1-8

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WikiProject Mathematics

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Measurements of Ω and Λ from 42 High‐Redshift Supernovae

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

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Cosmology with ultralight pseudo Nambu-Goldstone bosons.

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Cluster abundance constraints for cosmological models with a time-varying, spatially inhomogeneous energy component with negative pressure

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Cosmological Imprint of an Energy Component with General Equation of State

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Cosmological Parameter Extraction from the First Season of Observations with the Degree Angular Scale Interferometer

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Cosmological challenges in theories with extra dimensions and remarks on the horizon problem

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The baryon content of galaxy clusters: a challenge to cosmological orthodoxy

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The intracluster gas fraction in X-ray clusters: constraints on the clustered mass density

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Gravitational lensing as a probe of quintessence

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An evolution free test for non-zero cosmological constant

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A geometrical test of the cosmological energy contents using the Ly{alpha} forest

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Measuring the cosmological geometry from the Ly{alpha} forest along parallel lines of sight

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DOI

10.1016/S0370-2693(02)02122-6

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arXiv ID

astro-ph/0201229

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zbMATH Open document ID

0996.83071

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(Q56061021)

Cardassian expansion: a model in which the universe is flat, matter dominated, and accelerating

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