4.1 Suppose the energy density of the cosmological constant is equal to the present critical density ɛa = Ec.0 energy of the cosmological constant within a sphere 1 AU in radius? What is the rest energy of the Sun (Eo = Moc²)? Comparing these two numbers, do you expect the cosmological constant to have a significant effect on the motion of planets within the solar system? = 4870 MeVm-3. What is the total
4.1 Suppose the energy density of the cosmological constant is equal to the present critical density ɛa = Ec.0 energy of the cosmological constant within a sphere 1 AU in radius? What is the rest energy of the Sun (Eo = Moc²)? Comparing these two numbers, do you expect the cosmological constant to have a significant effect on the motion of planets within the solar system? = 4870 MeVm-3. What is the total
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Transcribed Image Text:4.1 Suppose the energy density of the cosmological constant is equal to the
present critical density ɛa = Ec0 = 4870 MeVm3. What is the total
energy of the cosmological constant within a sphere 1 AU in radius?
What is the rest energy of the Sun (Eo = Moc²)? Comparing these two
numbers, do you expect the cosmological constant to have a significant
effect on the motion of planets within the solar system?
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