Can the Mass of Cosmic Rays in the Universe Be Calculated?

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Discussion Overview

The discussion centers around the calculation of the mass of cosmic rays in the universe, exploring their origins, characteristics, and whether their mass can be considered constant or uniform. It touches on theoretical aspects, implications for space travel, and the nature of cosmic rays as a form of radiation.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant notes that cosmic rays are high-energy particles, including protons and alpha particles, and questions the possibility of calculating their total mass in the universe.
  • Another participant suggests that the article may have oversimplified the nature of cosmic rays, which also include other forms of radiation and have multiple sources beyond supernovae.
  • A participant introduces the concept of "Galactic Cosmic Radiation," comparing it to solar wind and mentioning its varied energy spectrum, with some particles traveling near the speed of light.
  • One participant expresses skepticism about accurately estimating the overall mass of cosmic rays due to uncertainties in cosmic ray acceleration theories, while noting that the energy density is comparable to other cosmic components but negligible compared to critical density.
  • It is mentioned that cosmic ray density is not constant and may vary with star formation rates and proximity to galaxies and clusters, where large-scale magnetic fields can influence their distribution.
  • Another participant adds that local variations in cosmic ray density can occur near gamma-ray bursts, quasars, and supernova remnants.

Areas of Agreement / Disagreement

Participants express differing views on the nature and calculation of cosmic rays, with no consensus reached on whether their mass can be calculated or if it remains constant across the universe.

Contextual Notes

Participants highlight uncertainties regarding cosmic ray acceleration mechanisms and the implications of varying densities in different cosmic environments.

Qmon
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I read an article in this months Discover magazine that stated that cosmic rays are atoms of the elements from hydrogen up to iron traveling at close to the speed of light that originate from exploding stars. Can the mass of cosmic rays be calculated for the universe? Is it a constant? As some rays are absorbed new ones are formed but is it generally uniform?

Q
 
Space news on Phys.org
Sounds like crackpot science to me.

Cosmic Rays is not a sole "thing". It is radiation consisting of high-energy particles (protons, alpha particles are the most common ones). Atomic nuclei, electrons and gamma rays and high-energy neutrinos is also included.

Futhermore, there are more sources of cosmic rays that just supernovae. I do not know if it possible to somehow measure or calulate the total mass of all the cosmic rays in the universe.
 
Perhaps they were only describing certain aspects of cosmic rays. The artical was all about how we won't be able to travel to other planets unless we can eliminate the affects of cosmic rays on the human body.

Q
 
There is what is known as "Galactic Cosmic Radiation", which is much the same as the solar wind (high energy atoms, ions and electrons) from our own sun, but comes from all other sources in the galaxy, and perhaps other galaxies.

See -

http://www.sievert-system.org/WebMasters/en/contenu_rayonnement.html[/URL]

[PLAIN]http://rise.hao.ucar.edu/iscs/abstracts/node99.html[/URL]

[url]http://hesperia.gsfc.nasa.gov/sspvse/oral/Ken_McCracken/wintergreen1.pdf[/url] (use save target as)

[PLAIN]http://aoss.engin.umich.edu/Radiation/presentations/Shea-Smart.pdf[/URL]

http://www.nature.com/nature/journal/v255/n5511/abs/255687a0.html;jsessionid=D3C86159CC3D1A72216F9744FB4527D1

There exists an spectrum of energy of Galactic Cosmic Radiation, with the higher energies >> being relatively rare.

Particles with energy as high as 10[sup]20[/sup] eV have been reported, and these are certainly near the speed of light. Consider that a single nucleon (proton or neutron) has rest mass slight less than 0.940 GeV.
 
Last edited by a moderator:
Qmon said:
I read an article in this months Discover magazine that stated that cosmic rays are atoms of the elements from hydrogen up to iron traveling at close to the speed of light that originate from exploding stars. Can the mass of cosmic rays be calculated for the universe?

Our theories of cosmic ray acceleration are a bit fuzzy, so I don't think one could do a very accurate estimate of the overall mass of cosmic rays in the universe, but the total mass would be very, very small. The energy density, on the other hand, is about an eV per cubic centimeter in the Milky Way. This is comparable to the local energy density of the cosmic microwave background, starlight, and magnetic fields, but negligible compared to the critical density.
Is it a constant?

No, if they are reallly accelerated in supernovae or gamma-ray bursts, then their density should be changing along with the star formation rate density (which has been decreasing since z~2).
As some rays are absorbed new ones are formed but is it generally uniform?

No, the density of cosmic rays should be greatly enhanced near galaxies and clusters. Large-scale magnetic fields in the host galaxies will trap many of the charged cosmic rays.
 
If you go down to more local levels, you will probably find some other extreme variations.

For example, along the beams from GRBs, and (especially) in and along jets, from quasars and AGNs, as well as micro-quasars (this is in addition to the environs of supernovae and their remnants, as has already been pointed out).
 
Thanks guys.
 

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