Question about pre-CMB & Lepton Number

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In summary, prior to recombination, the vast majority of leptons and antileptons annihiliated into photons, leaving a small number of remaining leptons. During the 380,000 years when the universe was opaque to photons, the photons interacted strongly with electrons, continuously bouncing off of them. Despite there being a large number of photons relative to electrons and nucleons, the lack of space for them to "stream free" allowed for continuous interaction until recombination.
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I have a question about the interaction between photons and leptons prior to recombination

I understand that once the threshold temperature for electrons was reached early in the universe' history, the vast majority of the leptons and antileptons annihiliated into photons. Except for possibly the neutrinos and antineutrinos which interact very weakly. I also understand that the number of remaining leptons (the lepton number) after this annihilation event was very small relative to the number of photons. Something like 1*10(minus 9). So during the 380,000 years prior to recombination, when the universe was opaque to photons, it is said that the photons interacted very strongly with the electrons, continuously bouncing off of them, which is why the universe was opaque. However, if at this time there were something like 1,000 million photons for every electron and 1,000 million photons for every nucleon, how is this possible? It would seem that the universe would be so overwhelmed by photons relative to electrons that not all of the photons would interact with electrons and would indeed stream free. But according to BB cosmology they did not stream free until recombination. What am I missing in my understanding?
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Remember that there was literally nowhere to "stream free" to. The entirety of the universe was this way. Even if a photon takes days to interact with a particle, it still had 380,000 years to do so.
 

Related to Question about pre-CMB & Lepton Number

What is pre-CMB?

Pre-CMB (cosmic microwave background) refers to the period before the formation of the cosmic microwave background radiation, which is the oldest light in the universe. It is believed to have formed about 380,000 years after the Big Bang.

What is the significance of the CMB?

The CMB is significant because it provides important information about the early universe, such as its age, expansion rate, and composition. It also supports the Big Bang theory and helps us understand the structure and evolution of the universe.

What is the connection between pre-CMB and lepton number?

The lepton number is a fundamental property of subatomic particles, specifically leptons. The study of pre-CMB can provide insight into the lepton number and its possible variations in the early universe, which can help us understand the fundamental laws of physics.

How is the lepton number related to the asymmetry between matter and antimatter in the universe?

The lepton number is believed to be linked to the asymmetry between matter and antimatter in the universe. This is because leptons and antileptons have opposite lepton numbers, and any deviations in the lepton number could have resulted in the dominance of matter over antimatter in the early universe.

What are some current research efforts in understanding pre-CMB and lepton number?

Scientists are currently studying the cosmic microwave background radiation to gather more information about the early universe and its fundamental properties, including the lepton number. They are also conducting experiments with particle accelerators to simulate conditions of the early universe and test theories about the lepton number and its potential variations.

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