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

March 09-10, 2020

International Conference on Physics

Rome, Italy
March 09-10, 2020

International Conference on Physics

Rome, Italy
MARCH 20-21, 2020

World Congress on Physics

Paris, France
June 15-16, 2020

6th International Conference on Physics

Barcelona, Spain
2020-08-24

Atomic Physics, Molecular and Plasma Physics

Vancouver, Canada
September 22-23, 2020

International Conference on Optometry

Dubai, UAE
September 22-23, 2020

International Conference on Nucleic Acids

Dubai, UAE
November 02-03, 2020

GlobaL Meet on Optoelectronics and Quantum Physics

Sydney, Australia
November 12-13, 2020

European Meet on Laser, Optics & Photonics

Budapest, Hungary

Neutrino Astronomy Conference Speakers

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