Jerk, snap and the cosmological equation of state

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Jerk, snap and the cosmological equation of state

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Abstract. Linearizing the cosmological equation of state around the current epoch p = p0 + κ0 (ρ− ρ0) +O[(p− p0)2], is the simplest model one can consider that does not make any a priori restrictions on the nature of the cosmological fluid. Most popular cosmological models attempt to be “predictive”, in the sense that once some a priori equation of state is chosen the Friedmann equations are us...

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ژورنال

عنوان ژورنال: Classical and Quantum Gravity

سال: 2004

ISSN: 0264-9381,1361-6382

DOI: 10.1088/0264-9381/21/11/006