Finding the One Degree Peak in a Power Spectrum

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Discussion Overview

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.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • Some participants suggest plotting the angular separation between CMB temperature differences to visualize the one degree peak.
  • It is noted that the power spectrum is typically plotted with ##\ell## on the x-axis, where the peak near ##\ell = 180## corresponds to fluctuations with a wavelength of approximately one degree.
  • Questions are raised about the significance of the temperature difference at one degree, with some participants linking it to the sound horizon and the behavior of sound waves at the time of recombination.
  • There is a discussion about whether the temperature difference between two points at the sound horizon should be zero, with some arguing that it cannot be zero due to the nature of matter falling into potential wells.
  • Participants explore the concept of multiple waves contributing to the CMB, with one noting that the peak arises from constructive interference of waves at the sound horizon.
  • Clarifications are made regarding the presence of different waves at the same wavelength but in different directions, leading to variations in amplitude and temperature differences.
  • Some participants express confusion about the relationship between the initial overdense region and the resulting temperature differences measured at the sound horizon.

Areas of Agreement / Disagreement

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.

Contextual Notes

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.

Who May Find This Useful

This discussion may be useful for those interested in cosmology, the cosmic microwave background, and the physics of sound waves in the early universe.

gluon
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Can someone tell me how i can determine the one degree peak from power spectrum ?
 
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You plot the angular separation between CMB temperature differences.
 
gluon said:
Can someone tell me how i can determine the one degree peak from power spectrum ?
This post is useful for the plots, and has a good description of how the power spectrum is derived:
http://backreaction.blogspot.com/2007/12/cmb-power-spectrum.html

As for how you can see the 1-degree peak, the power spectrum of the CMB is usually plotted with ##\ell## along the x-axis. The approximate wavelength of a fluctuation is ##180 / \ell## degrees. So the peak that appears close to ##\ell = 180## represents waves with a wavelength of approximately one degree. The plot at the above blog post also lists the angular scale along the top.
 
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?
 
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?
One degree is the "sound horizon", which is the distance that sound waves in the CMB were capable of traveling since the big bang.
 
and why the temprature difference is big?the temprature difference of two points of sound horizon isn t zero ?
 
gluon said:
and why the temprature difference is big?the temprature difference of two points of sound horizon isn t zero ?
Why would it be zero?

One degree represents matter that fell into a potential well. The next (shorter) peak come from matter that fell into a potential well, then bounced back out.
 
because the two points at the sound horizon have the same temprature or am i wrong?
 
No, definitely not. Where are you getting this idea from?
 
  • #10
The y-axis is temprature difference between two points and the horizontal is the angle separation.the first peak giving as the fundamental frequency of sound wave right?
if we suppose that we have a overdense region at the time of inflation and until recombination it gets underdense and the wave have propagated at known distance which is given by d=c*t ,c is the speed of sound wave 0,6c and t is the time at recombination 375.000,which giving a distance d=225.000 ly and we know that the distance from cmb surface is 41billion ly away so we get a angle which is 0,5 degree .But if i take that the wave went spherical away from overdense point we get a diameter of 716.000 ly which is giving 1 degree angle.

which difference in temprature we measure? 1) from the initial overdence ,which became underdense,until the region which sound wave reach?or 2) from two positions that sound wave have reached at the time of recombintaion which is separated by distance 716.000 ly ? if we take the 1) case i understand why the temprature difference is so big,but the angle is 0,5 degree not 1.In case 2) the degree is 1 but i can't see why we have temprature difference between this points.should it have zero temprature difference or not?

Sorry for my English!
 
  • #11
I think the mistake you're making is that it's not just one wave. The CMB is made out of a large, random assortment of waves all traveling in different directions. A peak shows up at the same wavelength as the sound horizon because that's the longest wavelength where constructive interference becomes possible.
 
  • #12
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?
 
  • #13
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?
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.
 
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  • #14
do you mean 361 different waves with the same wavenumber?and this waves can cancel each other or amplifying?
 
  • #15
Yes. Same wavenumber, different directions. If you want to get some detail on how this works, you can try reading up on spherical harmonics.
 
  • #16
Thanks Chalnoth!
 

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