CMB vs Neutrino BG: Why Does Neutrino Transparency Occur First?

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Discussion Overview

The discussion centers around the timing of neutrino transparency compared to photon transparency in the early universe, particularly in relation to their respective temperatures of ~2 Kelvin for neutrinos and ~2.75 Kelvin for the Cosmic Microwave Background (CMB). Participants explore potential reasons for this sequence, including the role of neutron-to-proton decay and the interactions of neutrinos.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant suggests that neutrino transparency occurred before photon transparency due to the lower interaction cross sections of neutrinos, which only interact through the weak force and gravity.
  • Another participant speculates that after neutrons and protons cooled sufficiently to form nuclei, the stability of neutrons halted their decay into protons and antineutrinos, allowing neutrinos to become transparent.
  • A later reply questions the initial participant's understanding of the argument, emphasizing the importance of entropy conservation and thermal equilibrium in the context of neutrino and photon interactions.
  • One participant references a website that provides explanations about neutrino temperatures and their implications, indicating a preference for accessible resources.
  • Another participant discusses the temperature dynamics post-recombination, suggesting that the temperature of photons is affected differently due to their later formation compared to neutrinos.
  • There is a mention of a factor of 1.401 that influences temperature expectations after the recombination event, with a participant expressing a desire to discuss this further.

Areas of Agreement / Disagreement

Participants express differing views on the mechanisms behind neutrino and photon transparency, with no consensus reached on the explanations provided. Some participants challenge each other's understanding and reasoning, indicating a contested discussion.

Contextual Notes

Participants reference concepts such as entropy conservation and thermal equilibrium, but the discussion does not resolve the underlying assumptions or definitions related to these concepts.

Chaos' lil bro Order
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Hey,

Was reading how the CMB is ~2.75 Kelvin, while the Neutrino BG is ~2 Kelvin. Clearly this means that neutrino transparency occurred before photon transparency did in the early evolution of the universe. My question is why? Does is have anything to do with neutron-to-proton decay?

I'm guessing (probably incorrectly) that after neutrons and protons cooled sufficiently to bind in nuclei, the neutron was now stable and therefore stopped decaying into protons (as free neutrons do) + electrons + electron antineutrinos. And it was these antineutrinos that ceased to be produced, which gave normal neutrinos free reign in the universe without fear of being annihilated by their antineutrino counterparts. So then neutrino transparency was achieved and the neutrinos were free to redshift to today's cool 2 degrees Kelvin? I wonder if this makes sense.

Help appreciated, thanks.
 
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Chaos' lil bro Order said:
Was reading how the CMB is ~2.75 Kelvin, while the Neutrino BG is ~2 Kelvin. Clearly this means that neutrino transparency occurred before photon transparency did in the early evolution of the universe.

Are you sure you understand this? The argument deals with conservation of entropy and counting particles in thermal equilibrium.


My question is why?

The answer to this question actually is simple. Neutrinos, lacking electric charge, can only interact through the weak force (and, presumably, gravity), so their low-energy interaction cross sections are generally much smaller than those for electrons and photons.
 
SpaceTiger said:
Are you sure you understand this? The argument deals with conservation of entropy and counting particles in thermal equilibrium.




The answer to this question actually is simple. Neutrinos, lacking electric charge, can only interact through the weak force (and, presumably, gravity), so their low-energy interaction cross sections are generally much smaller than those for electrons and photons.


Why are you picking on my first comment. Speak to this comment, 'I'm guessing (probably incorrectly) that after neutrons and protons cooled sufficiently to bind in nuclei, the neutron was now stable and therefore stopped decaying into protons (as free neutrons do) + electrons + electron antineutrinos. And it was these antineutrinos that ceased to be produced, which gave normal neutrinos free reign in the universe without fear of being annihilated by their antineutrino counterparts. So then neutrino transparency was achieved and the neutrinos were free to redshift to today's cool 2 degrees Kelvin? I wonder if this makes sense.
'

Does that make sense or no?
 
So why did neutrino transparency occur before photon transparency then?
 
You can find a decent explanation http://hyperphysics.phy-astr.gsu.edu/Hbase/astro/neutemp.html" .
 
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St

Ya, I've read that. I really love that website, I've known about it some time now and its great at explaining physics in a semi-lay manner.
 
Chaos' lil bro Order said:
Ya, I've read that. I really love that website, I've known about it some time now and its great at explaining physics in a semi-lay manner.

hey Order, if you know the Georgia State site and you know that explanation of the factor of 1.401, then maybe what your question is you simply want to TALK ABOUT IT with someone. this is a standard non-hierarchical self-teaching approach where you just get somebody and go over it with them

neither person is actually the "teacher" per se, in that case

So go ahead and tell me about it:smile: I will listen gladly.

I really like that webpage and that simple idea of a jump in temp by the 1.4 factor (if there are any people who like to quibble about correctness of language, they might quibble with my saying "jump" so I better watch out.)

Instead of a jump it is more that the DECLINE IN TEMP that you expect with expansion is effectively DELAYED some by the e+ and e- recombination event---so that what results is that after that event all the temperatures are a factor of 1.4 HIGHER than you would have expected or that would have been the case absent that recomb event

so after that recomb ALL THE TEMPS ARE JACKED UP BY THAT FACTOR compared with the OLD formula relating expansion temp.OK you can probably say it better, or correct some mistake I've made, or say something else to fill in the picture. So try.

And neutrinos date from BEFORE that event, so their temp goes down a different curve-----as the space expands

While photons date from AFTER that event, so their temp goes down a jacked up temperature curve

step by step the same, except for being hotter by a 1.401 factor, and everybody getting colder and colder until photons are 2.7 and neutrinos are whatever they are (less by a 1.401 factor)

My copy of the first 3 minutes is gathering dust upstairs, but it is a great book it seems----probably is, a lot of people think so---and that webpage appears to be a snack of Weinberg

======================

now the entropy question. do you, the lil bro of Chaos, want to explain that part? it would seem appropriate considering the dichotomy of your name:smile:

WHY does the temp have to be higher AFTER the recomb event (when there are effectively fewer particles)?

Is this the kind of discussion you wanted to have? If so, please do some paraphrasing work yourself. (if not just ignore. 's cool)

================
Georgia State
http://www.phy-astr.gsu.edu/new_web/newmain.html

Hyperphsics about the neutrino transparency temp
http://hyperphysics.phy-astr.gsu.edu/Hbase/astro/neutemp.html
 
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