Some thoughts concerning backgroun radiation

In summary: The cosmological constant is the term for the amount of gravity that is in the universe. If it is zero, then the curvature of the universe is irrelevant.
  • #1
espen180
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Concider a patch of the universe where there is only negligible gravitational curvature. In this patch, SR applies. We know therefore that there is no preferred intertial motion there.

But with background radiation taken into the picture, that seems not to be the case anymore. I've read the phrase "being at rest wrt the Universe's expansion", which I take to mean a state where the background radiation is identical in intensity everywhere (roughly).

If we are not in such a state, there is a direction from which the intensity is greater then other directions, and this should act as a sort of "intrinsic friction" of the universe. Of course, today such radiation is negligible, but earlier in the Universe's lifetime it was considerable.
 
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  • #2
Yes, you can be at rest wrt the CMB. That doesn't violate SR if that's what you're asking.
 
  • #3
espen180 said:
Concider a patch of the universe where there is only negligible gravitational curvature. In this patch, SR applies. We know therefore that there is no preferred intertial motion there.

But with background radiation taken into the picture, that seems not to be the case anymore. I've read the phrase "being at rest wrt the Universe's expansion", which I take to mean a state where the background radiation is identical in intensity everywhere (roughly).

If we are not in such a state, there is a direction from which the intensity is greater then other directions, and this should act as a sort of "intrinsic friction" of the universe. Of course, today such radiation is negligible, but earlier in the Universe's lifetime it was considerable.

Yes Espen, you are quite right, no doubt about it. The only thing is that radiation pressure difference would be small. For example, for body moving at 0.999 c, at times when Tcmb= 100 K, pressure difference would be around 0.8 Micro Pa. Pressure goes up with 4th power of temperature, so for Tcmb=3000 K (very early times) it would be around 0.7 Pa.
 
  • #4
Calimero said:
Yes Espen, you are quite right, no doubt about it. The only thing is that radiation pressure difference would be small. For example, for body moving at 0.999 c, at times when Tcmb= 100 K, pressure difference would be around 0.8 Micro Pa. Pressure goes up with 4th power of temperature, so for Tcmb=3000 K (very early times) it would be around 0.7 Pa.

That was clarifying, thanks! So the effect was never very significant.

russ_watters said:
Yes, you can be at rest wrt the CMB. That doesn't violate SR if that's what you're asking.

No, nothing like that. I was just letting out some ideas.
 
  • #5
The background radiation is hotter in one direction - the past. When the universe was younger, the CMB termperature was greater. This has been observationally confirmed by more than one study [e.g., http://www.spaceref.com/news/viewpr.html?pid=3414]. The temperature difference matches BBT predictions.
 
  • #6
espen180 said:
Concider a patch of the universe where there is only negligible gravitational curvature. In this patch, SR applies.
Yes but this is only valid if the cosmological constant is zero.
 
  • #7
You are missing the big picture, passionflower.
 

FAQ: Some thoughts concerning backgroun radiation

What is background radiation?

Background radiation is the low levels of radiation that are present in our environment at all times. It comes from various sources such as the sun, outer space, and radioactive elements in the Earth's crust.

Is background radiation harmful?

In small doses, background radiation is not harmful to humans. In fact, we are constantly exposed to it and our bodies have natural defenses against it. However, prolonged exposure to high levels of background radiation can increase the risk of cancer and other health issues.

How is background radiation measured?

Background radiation is measured in units called millisieverts (mSv). This unit takes into account the amount and type of radiation, as well as the level of exposure. In general, the average person is exposed to around 3 mSv of background radiation per year.

What factors can affect background radiation levels?

Several factors can affect background radiation levels, including altitude, location, and human activities. For example, people living at higher altitudes are exposed to more background radiation due to less atmospheric shielding. Additionally, areas with high levels of natural radioactive elements in the soil will have higher background radiation levels.

How can we protect ourselves from background radiation?

We can protect ourselves from background radiation by limiting our exposure to sources of radiation, such as medical procedures and certain occupations. It is also important to follow safety protocols when handling radioactive materials. Additionally, maintaining a healthy lifestyle and diet can help our bodies better cope with low levels of radiation.

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