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It is possible to combine both Friedmann-Lemaitre equations to create another useful equation for cosmology (the...

It is possible to combine both Friedmann-Lemaitre equations to create another useful equation for cosmology (the so-called fluid equation). Derive that equation by first taking the time derivative of the first Friedmann-Lemaitre equation and then by using the second one to redefine the terms. Assume ? = 0.

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Applied to a fluid with a given equation of state, the Friedmann equations yield the time evolution and geometry of the universe as a function of the fluid density. Some cosmologists call the second of these two equations the Friedmann acceleration equation and reserve the term Friedmann equation for only the first equation.

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