Gzk paradox and expanding universe

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Discussion Overview

The discussion revolves around the GZK paradox and its potential explanations in the context of an expanding universe. Participants explore various theoretical models and implications related to cosmic rays, supernovae, and relativistic effects, focusing on both conceptual and mathematical aspects.

Discussion Character

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

Main Points Raised

  • One participant suggests that if the universe were divided into two mass zones that repel each other, this could explain why cosmic rays have not been stopped by the cosmic microwave background (CMBR), despite expectations based on the GZK limit.
  • Another participant questions the connection between the acceleration of distant supernovae and the GZK limit, noting that the distances involved are significantly different.
  • A participant proposes that if quarks in cosmic ray protons are considered to have a size and undergo relativistic length contraction, this could reduce the probability of collisions with CMBR photons, allowing protons to reach Earth.
  • Reference to Stecker's discussion of the GZK effect is made, emphasizing that relativistic effects were considered in calculations regarding photomeson production cross sections.
  • One participant shares a calculation indicating that the size of a charge sphere in a quark is much smaller than that of a proton at rest, suggesting that this could affect interaction probabilities with CMBR photons.
  • Concerns are raised about how these considerations might also apply to high-energy protons colliding with other particles, potentially leading to different behaviors in air showers than what has been observed.
  • Another participant notes that while the size of quarks affects collision probabilities, it does not determine the outcomes of collisions, assuming a similar number of oxygen quarks to CMBR photons encountered by cosmic rays.

Areas of Agreement / Disagreement

Participants express differing views on the relationship between supernovae acceleration and the GZK limit, with some proposing alternative models involving relativistic effects. The discussion remains unresolved with multiple competing perspectives presented.

Contextual Notes

Participants highlight the complexity of the GZK paradox and the need for careful consideration of relativistic effects, collision probabilities, and the implications of different theoretical models. Some assumptions and definitions remain unaddressed, contributing to the ongoing debate.

kurious
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If the universe were divided into two mass zones, and one zone
repelled the other,supernovae would not only accelerate away from us
but the zone in which we are living would accelerate away from the
supernovae.Also cosmic rays could be repelled by one zone and pushed
through another.Could this explain the GZK paradox where highly
energetic cosmic rays that should have been stopped from reaching the
Earth by the microwave background have not been stopped?
 
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I'm not sure I understand what you're saying here; perhaps a few numbers might help.

First, re supernovae 'accelerating away from us': the 'high-z' supernovae (SN) which provide evidence for the 'acceleration' are ~5 to 10 billion light years away (well, more accurately, the light which we now see from them has traveled for 5 to 10 billion years to get to us). Closer SN do not really show a deviation from the Hubble expansion rate (~71 km/s/Mpc), though the 'acceleration' surely affects what we see of them too (there are also plenty of SN which seem to be further, or closer, to us than the Hubble relation would suggest; however, these deviations are well understood as the result of the motion of the host galaxies in the gravitational field of the cluster - or super-cluster - in which they reside).

Then the GZK limit: based on the density of CMBR photons (~400 per cubic centimetre), cosmic ray protons with an energy of ~>50 EeV (1 EeV = 1018 eV) should only be able to travel ~<100 Mly before they collide with a CMBR photon and produce lots of pions.

You can see that these distances are quite different, so it's hard to see how the acceleration of distant SN and the GZK limit they would be connected.
 
see reply below
 
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You can see that these distances are quite different, so it's hard to see how the acceleration of distant SN and the GZK limit they would be connected

I agree with what you have said. Suppose the quarks in cosmic ray protons have a size i.e
if they consisted of spheres of charge, and by special relativity length contraction these spheres got small at high speeds and energies, this would reduce the probability of a collision with a CMBR photon and allow the proton to reach the Earth.
 
Stecker has a good discussion of the GZK effect (see Section 2.2, starting on p7). It also contains references to the original papers by Griesen, Zatsepin, and Kuz'min, as well as several others on the topic.

I think you will find that relativity effects were taken into account in making the calculations, particulary wrt the "energy dependence of the photomeson production cross sections and inelasticities", i.e. how likely it is that a proton of energy x will collide with a CMBR photon, for different kinds of collision.
 
Thanks for the reference.It's full of useful reading.
think you will find that relativity effects were taken into account in making the calculations, particulary wrt the "energy dependence of the photomeson production cross sections and inelasticities", i.e. how likely it is that a proton of energy x will collide with a CMBR photon, for different kinds of collision.



I've done a calculation that shows that a sphere of charge in a quark is 10^-18 m when the quark has no speed.This is one thousand times smaller than a proton at rest.So relativistic length contraction would make the quark even smaller and less likely to interact with the CMBR than expected using the normal proton size.
 
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kurious said:
I've done a calculation that shows that a sphere of charge in a quark is 10^-18 m when the quark has no speed.This is one thousand times smaller than a proton at rest.So relativistic length contraction would make the quark even smaller and less likely to interact with the CMBR than expected using the normal proton size.
The same considerations would surely also need to have been made re high energy protons colliding with particles such as oxygen nuclei, leading to different behaviour for air showers (for example) than what has been observed. The same effects would also occur - at much lower energies - in the LHC and its predecessors.

There's certainly some interesting physics in the >100 GeV regime, such as the formation of a new state of matter, http://www.bnl.gov/rhic/QGP.htm, but AFAIK studies of these phenomena haven't lead to big changes in estimates of collision cross-sections.
 
gzk paradox

The same considerations would surely also need to have been made re high energy protons colliding with particles such as oxygen nuclei, leading to different behaviour for air showers (for example) than what has been observed. The same effects would also occur - at much lower energies - in the LHC and its predecessors.

But the size of the quarks only determines the chance of a collision - not the outcome of the collision - assuming the number of oxygen quarks is similar to the number of microwaves a cosmic ray proton encounters on its journey.
 
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