General Relativity: An Introduction for Physicists · Problem 15.11

Cosmological models — Hobson, Efstathiou & Lasenby

Physics · conformal-time-field-equation

Problem

The conformal time variable is defined by dη=c dt/Rd\eta = c\, dt/R. Hence show that the second cosmological field equation can be written as (dadη)2=−kΩk,0(Ωm,0 a+Ωr,0+ΩΛ,0 a4+Ωk,0 a2).\left(\frac{da}{d\eta}\right)^2 = -\frac{k}{\Omega_{k,0}}\left(\Omega_{\mathrm{m},0}\, a + \Omega_{\mathrm{r},0} + \Omega_{\Lambda,0}\, a^4 + \Omega_{k,0}\, a^2\right).

Related theory

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