Gzk paradox and expanding universe

In summary, 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. This could explain the GZK paradox where highly energetic cosmic rays that should have been stopped from reaching the Earth have not been stopped.
  • #1
kurious
641
0
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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  • #2
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.
 
  • #3
see reply below
 
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  • #4
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.
 
  • #5
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.
 
  • #6
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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  • #7
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.
 
  • #8
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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1. What is the Gzk paradox?

The Gzk paradox refers to the observation that high-energy cosmic rays from outside our galaxy should not be able to reach Earth due to interactions with the cosmic microwave background radiation. This is because these high-energy particles should lose energy and become less energetic as they travel through space, making it unlikely for them to reach us. However, these high-energy cosmic rays have been observed on Earth, creating a paradox.

2. How does the expanding universe play a role in the Gzk paradox?

The expanding universe plays a crucial role in the Gzk paradox because it affects the energy loss of high-energy cosmic rays as they travel through space. As the universe expands, the cosmic microwave background radiation becomes less dense, allowing high-energy particles to travel further without losing as much energy. This could potentially explain how these particles are able to reach Earth despite the Gzk paradox.

3. What evidence supports the Gzk paradox?

Several experiments and observations have provided evidence for the Gzk paradox. For example, the Pierre Auger Observatory in Argentina has detected ultra-high-energy cosmic rays that should not be able to reach Earth according to the Gzk paradox. Additionally, the Planck satellite has measured the cosmic microwave background radiation and confirmed its existence, further supporting the paradox.

4. How do scientists attempt to solve the Gzk paradox?

Scientists have proposed several theories to solve the Gzk paradox, such as the "top-down" theory which suggests that these high-energy cosmic rays may actually originate from supermassive particles decaying into smaller particles. Another theory is that these particles may be produced by cosmic strings, which are theoretical objects that could generate extremely high-energy particles.

5. What are the implications of solving the Gzk paradox?

If the Gzk paradox is solved, it could provide a better understanding of the origin and nature of high-energy cosmic rays. It could also potentially lead to advancements in our understanding of the universe and its evolution. Additionally, solving the Gzk paradox could help confirm or rule out various theories and models of the universe, providing further insights into its mysteries.

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