Neutrino Astronomy
We are educated some further things about the cosmos beyond the solar system by sighting cosmic rays, which are mostly prepared of either atomic nuclei minus their orbiting electrons, or one of their basic components, protons. But these positively charged particles don’t point to their place of origin due to the magnetic fields of our galaxy which affect their flight paths like a magnet affects iron filings. The total number of elementary particles in the cosmos, and these neutral weakly interacting particles arisen to us almost without any trouble straight from their sources, traveling at very close to the speed of light. A with low energy of neutrino in flight would not notice a barrier of lead 50 light years thick. When we are able to see out in neutrino light we will undoubtedly get a amazing new view of the universe.
- Neutrinos in the Universe
- Stellar Neutrinos
- High Energy Cosmic Neutrinos
- Implications for the Fate of the Universe
- Detection experiments
Related Conference of Neutrino Astronomy
7th World Congress on Emerging Trends in Science, Engineering and Technology
7th International Conference on Astronomy, Astrophysics and Space Science
Neutrino Astronomy Conference Speakers
Recommended Sessions
- Astrochemistry and Astrobiology
- Astronomy
- Astrophysics and Space Science
- Atomic and Molecular Astrophysics
- Cosmology
- Dark Matter and Dark Energy
- Gravitational Physics
- Heavy-ion physics
- Higgs Particle Physics
- High Energy Physics
- Instrumentation
- Neutrino Astronomy
- Nuclear Astrophysics
- Optical Astronomy
- Particle Physics
- Plasma Physics
- Space Missions & Satellite
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