What is Particle Astro Physics?

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    Astro Particle Physics
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SUMMARY

Particle Astrophysics focuses on high-energy particles and radiation originating from various cosmic sources, including the sun, stars, and galaxies. Galactic cosmic rays, primarily accelerated in supernova remnants, gain energy through interactions with magnetic fields. The maximum energy of these cosmic rays is limited by the size of the acceleration region and magnetic field strength. However, ultra-high-energy cosmic rays, exceeding supernova capabilities, may originate from active galactic nuclei, quasars, or represent new physics phenomena.

PREREQUISITES
  • Understanding of cosmic rays and their origins
  • Familiarity with supernova mechanics and remnants
  • Knowledge of magnetic fields in astrophysical contexts
  • Basic principles of particle physics
NEXT STEPS
  • Research the mechanisms of cosmic ray acceleration in supernova remnants
  • Explore the role of active galactic nuclei in cosmic ray production
  • Investigate the implications of ultra-high-energy cosmic rays on particle physics
  • Study the relationship between cosmic rays and dark matter theories
USEFUL FOR

Astronomers, astrophysicists, and researchers interested in high-energy particle physics and cosmic radiation phenomena.

TrevorRyan
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I was just curious if anybody could give me an in depth explanation. thanks!
 
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It deals with radiation and high energy particles that originate from the sun, other stars and related objects, the galaxy and sources outside the galaxy.

Galactic cosmic rays/radiation is a term that refers to high energy particles from sources outside of the solar system.
http://imagine.gsfc.nasa.gov/docs/science/know_l1/cosmic_rays.html

NASA-GSFC said:
Most galactic cosmic rays are probably accelerated in the blast waves of supernova remnants. This doesn't mean that the supernova explosion itself gets the particles up to these speeds. The remnants of the explosions, expanding clouds of gas and magnetic field, can last for thousands of years, and this is where cosmic rays are accelerated. Bouncing back and forth in the magnetic field of the remnant randomly let's some of the particles gain energy, and become cosmic rays. Eventually they build up enough speed that the remnant can no longer contain them, and they escape into the Galaxy.

Because the cosmic rays eventually escape the supernova remnant, they can only be accelerated up to a certain maximum energy, which depends upon the size of the acceleration region and the magnetic field strength.

However, cosmic rays have been observed at much higher energies than supernova remnants can generate, and where these ultra-high-energies come from is a big question. Perhaps they come from outside the Galaxy, from active galactic nuclei, quasars or gamma ray bursts. Or perhaps they're the signature of some exotic new physics: superstrings, exotic dark matter, strongly-interacting neutrinos, or topological defects in the very structure of the universe. Questions like these tie cosmic-ray astrophysics to basic particle physics and the fundamental nature of the universe.

http://helios.gsfc.nasa.gov/gcr.html

http://www.srl.caltech.edu/personnel/dick/cos_encyc.html

http://www.sotere.uni-osnabrueck.de/pubs/paper/summerschool-gaks.pdf

http://www.issibern.ch/PDF-Files/Spatium_11.pdf

http://icecube.wisc.edu/~halzen/presentations/bahcall.ppt
 
that was some pretty great info, Thanks!
 

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