Intergallactic photons free mean path

In summary, Intergalactic photons are particles of light that travel through the vast emptiness of space between galaxies. The free mean path of intergalactic photons refers to the average distance that a photon can travel through space without encountering any other particles or objects. This distance is incredibly long, as the intergalactic medium is mostly empty. The free mean path of intergalactic photons is calculated by taking into account the density of particles in the intergalactic medium and the likelihood of photon-particle interactions. This calculation involves complex mathematical models and observations of the cosmic microwave background radiation. The free mean path of intergalactic photons is significant because it provides insight into the properties and composition of the intergalactic medium. It also helps us understand
  • #1
Luther_Harkon
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Homework Statement



Intergallactic ionized gas produces X ray photons via the bremsstrahlung process
[tex]
e^-\ p\rightarrow e^-\ p\ \gamma
[/tex]
In contrast to photons produced in a star (see previous exercises) these X ray photons escape from the galaxy cluster. Indeed, the largest galaxy clusters contain a few thousand galaxies with a total mass ∼ [tex]10^{14} M_\odot[/tex] and a radius of several Mpc.

Note. take [tex]n_{e^-}=n_p\sim\Omega_B\rho_c/m_p[/tex]

Homework Equations



Show that the mean free path of a photon is [tex]\lambda_\gamma=1/(n\sigma)\gg1Mpc[/tex], where [tex]\sigma[/tex] can be approximated by the Thomson cross-section of photons on electrons. Why not on photons?

The Attempt at a Solution



I had no problem in showing that the free mean path of photons , when given the conditions shown here, is much greater than 1 Mpc. But I am quite confused on why can't be the free mean path computed by the Thomson cross section on protons. Any clue on that?

Thanks!
 
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The reason why the mean free path cannot be computed using the Thomson cross section on protons is because the bremsstrahlung process involves the interaction between electrons and protons, not photons and protons. The Thomson cross section is a measure of the probability of interaction between photons and charged particles, but in this case, the charged particles are both electrons and protons. Therefore, the Thomson cross section cannot be used to accurately calculate the mean free path of photons in this scenario.

In addition, the Thomson cross section is only valid for low energy photons, while the photons produced in the bremsstrahlung process are high energy X-rays. This means that the Thomson cross section would not accurately represent the interactions between the photons and the charged particles in this process.

In summary, the Thomson cross section cannot be used to accurately calculate the mean free path of photons in this scenario because it does not take into account the interactions between electrons and protons, and it is only valid for low energy photons.
 

1. What are intergalactic photons?

Intergalactic photons are particles of light that travel through the vast emptiness of space between galaxies. They originate from various sources such as stars, galaxies, and other cosmic objects.

2. What is the free mean path of intergalactic photons?

The free mean path of intergalactic photons refers to the average distance that a photon can travel through space without encountering any other particles or objects. This distance is incredibly long, as the intergalactic medium is mostly empty.

3. How is the free mean path of intergalactic photons calculated?

The free mean path of intergalactic photons is calculated by taking into account the density of particles in the intergalactic medium and the likelihood of photon-particle interactions. This calculation involves complex mathematical models and observations of the cosmic microwave background radiation.

4. What is the significance of the free mean path of intergalactic photons?

The free mean path of intergalactic photons is significant because it provides insight into the properties and composition of the intergalactic medium. It also helps us understand the behavior of light in the vastness of space and its interactions with other particles.

5. How does the free mean path of intergalactic photons affect our observations of the universe?

The free mean path of intergalactic photons plays a crucial role in our observations of the universe. It affects the propagation of light from distant objects, leading to phenomena such as gravitational lensing. It also allows us to study the history of the universe through the cosmic microwave background radiation.

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