Briefly explain what is meant by "particle horizon" and "event horizon" in cosmology. Calculate the physical particle horizon, Ru(t), at time t. Assume a flat FRW universe which is dominated by a fluid that gives rise to scale factor evolution (-)", where n is a constant with 0
Briefly explain what is meant by "particle horizon" and "event horizon" in cosmology. Calculate the physical particle horizon, Ru(t), at time t. Assume a flat FRW universe which is dominated by a fluid that gives rise to scale factor evolution (-)", where n is a constant with 0
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![a) Briefly explain what is meant by "particle horizon" and "event horizon" in cosmology.
b) Calculate the physical particle horizon, RH (t), at time t. Assume a flat FRW universe which
is dominated by a fluid that gives rise to scale factor evolution
a(t) = ao ()*,
to
where n is a constant with 0 <n< 1, and a (to) = ao.
n](/v2/_next/image?url=https%3A%2F%2Fcontent.bartleby.com%2Fqna-images%2Fquestion%2Fb360a251-a88e-4e24-b6e1-ceeebc35a45e%2Faeeb40e5-c9d9-42f5-80bf-8be16a3f395b%2Fr5cn4bg_processed.jpeg&w=3840&q=75)
Transcribed Image Text:a) Briefly explain what is meant by "particle horizon" and "event horizon" in cosmology.
b) Calculate the physical particle horizon, RH (t), at time t. Assume a flat FRW universe which
is dominated by a fluid that gives rise to scale factor evolution
a(t) = ao ()*,
to
where n is a constant with 0 <n< 1, and a (to) = ao.
n
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