gluon
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Can someone tell me how i can determine the one degree peak from power spectrum ?
The discussion revolves around understanding the one degree peak in the cosmic microwave background (CMB) power spectrum. Participants explore the implications of this peak in terms of temperature differences and the underlying physics related to sound waves in the early universe.
Participants express differing views on the nature of temperature differences at the sound horizon and the implications of the one degree peak. There is no consensus on whether the temperature difference should be zero or the specific contributions of various waves to the observed phenomena.
Limitations include the complexity of the interactions between different waves, the dependence on definitions of temperature differences, and the unresolved mathematical steps regarding the calculations of distances and angles.
This discussion may be useful for those interested in cosmology, the cosmic microwave background, and the physics of sound waves in the early universe.
This post is useful for the plots, and has a good description of how the power spectrum is derived:gluon said:Can someone tell me how i can determine the one degree peak from power spectrum ?
One degree is the "sound horizon", which is the distance that sound waves in the CMB were capable of traveling since the big bang.gluon said:the temperature difference at 1 degree why is so big?it measures the difference between two points that the sound wave have reached at the time of recombination or from the initial overdense which became underdense and the point that the wave have reached at the time of recombination?
Why would it be zero?gluon said:and why the temprature difference is big?the temprature difference of two points of sound horizon isn t zero ?
Not just overtones. Different waves at the same wavelength. At ##\ell = 180##, there are 361 different possible orientations for the waves. Each of those orientations will have its own randomized amplitude.gluon said:yes i know its the overtone modes which are at smaller angles.but in the fundumental mode if i measure the temprature difference between two points which is diametrically opposite in the sound horizon, this spherical shell ,with the center in the initial overdense region ,isn't have the same density and thus the same temprature?