In an alternative universe the energy conservation equation is given by p+4- + = 0, a c2 and the Friedmann equation takes the form 2 a 8πG = p², 3 where all variables have their usual meaning, and a, p, and P depend on time t only. Assume this alternative universe is dominated by a fluid with equation of state P = c² wp, where the equation of state parameter w is a constant (with w -1). a) Calculate p(a), the dependence of the energy density p on the scale factor a. b) Calculate the time evolution of the scale factor a(t).

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Chapter1: Units, Trigonometry. And Vectors
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In an alternative universe the energy conservation equation is given by
p+4-
+
= 0,
a
c2
and the Friedmann equation takes the form
2
a
8πG
=
p²,
3
where all variables have their usual meaning, and a, p, and P depend on time t only. Assume this
alternative universe is dominated by a fluid with equation of state P = c² wp, where the equation
of state parameter w is a constant (with w -1).
a)
Calculate p(a), the dependence of the energy density p on the scale factor a.
b) Calculate the time evolution of the scale factor a(t).
Transcribed Image Text:In an alternative universe the energy conservation equation is given by p+4- + = 0, a c2 and the Friedmann equation takes the form 2 a 8πG = p², 3 where all variables have their usual meaning, and a, p, and P depend on time t only. Assume this alternative universe is dominated by a fluid with equation of state P = c² wp, where the equation of state parameter w is a constant (with w -1). a) Calculate p(a), the dependence of the energy density p on the scale factor a. b) Calculate the time evolution of the scale factor a(t).
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