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

July 31- August 01, 2017

6th International Conference on Photonics

Milan, Italy
July 31- August 02, 2017

7th International Conference on Laser Optics

Milan,Italy
August 28-30, 2017

2nd International Conference on Physics

Brussels, Belgium
Nov 08-09, 2017

2nd International Conference on Atomic and Nuclear Physics

Las Vegas, Nevada, USA
November 13-15, 2017

2nd International Conference on Astrophysics and Particle Physics

San Antonio, Texas, USA
November 20-22, 2017

Physics- 2017 (CME & CPD Accredited)

Rome, Italy
December 11-12, 2017

3rd International Conference on High Energy Physics

Rome,Italy

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