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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![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?](/v2/_next/image?url=https%3A%2F%2Fcontent.bartleby.com%2Fqna-images%2Fquestion%2F88e7e02f-602b-4daf-a6f1-9ccf3f083a32%2F3cb52888-6fee-427d-ac93-8888dea4e866%2Flihzdl_processed.jpeg&w=3840&q=75)
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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