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Dr. Strange
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Wikipedia gives the redshift of recombination at z = 1500 (roughly 4,000 K). The Plank report list a 'redshift for which the optical length equals unity' and gives a value of 1090. What is the difference between the two?
Hi @Dr. Strange:Dr. Strange said:could you also give a layman's description of optical depth,
Yes, that was very helpful. Is there any relation between the first peak of the BAO spectrum and one of these z values (for example, the 1090 value quoted in the Plank final results).Buzz Bloom said:I think my post #9 in another thread might help.
https://www.physicsforums.com/threads/depth-of-the-cmb.843673/#post-5295553
Hi Dr. Strange:Dr. Strange said:Is there any relation between the first peak of the BAO spectrum and one of these z values
Recombination redshift refers to the time in the early universe when neutral hydrogen atoms formed from free protons and electrons. This event occurred approximately 380,000 years after the Big Bang and is responsible for the cosmic microwave background radiation we observe today.
Recombination redshift is measured using the cosmic microwave background (CMB) radiation. This radiation was emitted at the time of recombination and has been redshifted as the universe expands. By studying the frequency and intensity of the CMB, scientists can determine the redshift value of recombination.
The recombination redshift has significant implications for our understanding of the universe. It marks the transition from a hot, opaque universe to a cooler, transparent one. It also allows us to study the properties of the early universe and make predictions about its evolution.
The precise value of recombination redshift is an important factor in cosmological models. It can help determine the age of the universe, the density of matter and energy, and the expansion rate of the universe. It also provides constraints on the theories of the universe's formation and evolution.
No, recombination redshift cannot be observed directly. However, its effects can be seen in the cosmic microwave background radiation, which can be observed using telescopes and other instruments. By studying this radiation, scientists can indirectly observe the recombination redshift and its impact on the early universe.