Gamma Ray Astronomy PeV EnergieS phase-3 (GRAPES-3) Experiment

News Excerpt: 

The GRAPES-3 experiment in Ooty, India, operated by the Tata Institute of Fundamental Research has discovered a new feature in the cosmic-ray proton spectrum.

About GRAPES-3 experiment:

The GRAPES-3 experiment is located at Ooty at an altitude of 2200 m above mean sea level in India, it was started as a collaboration of the Tata Institute of Fundamental Research and the Osaka City University (Japan). 

  • The near-equatorial placement of the experiment provides a unique advantage for measurements covering both northern and southern hemispheres significantly.
  • It is designed to study cosmic rays with an array of air shower detectors and a large area muon detector. 
  • It aims to probe acceleration of cosmic rays in the following four astrophysical settings - 
    • ~100 MeV in atmospheric electric fields through muons, 
    • ~10 GeV in Solar system through muons, 
    • ~1 PeV in our galaxy through nuclear composition of cosmic rays, 
    • ~100 EeV in nearby universe through measurement of diffuse γ-ray flux.
  • At present the array is operating with ~400 scintillators that are spread over an area of 25,000 m².
    • The energy threshold of muon detectors is 1 GeV.
  • The scintillators detect charged particles contained in extensive air showers produced by interaction of high energy cosmic rays in the atmosphere.
  • The unique capabilities of GRAPES-3 have allowed the study of cosmic rays over energies from a few TeV to tens of PeV and beyond.

Key findings of the experiment:

  • The GRAPES-3 experiment has discovered a new feature in the cosmic-ray proton spectrum at about 166 tera-electron-volt (TeV) energy while measuring the spectrum spanning from 50 TeV to a little over 1 peta-electron-volt (PeV).
  • The observed feature suggests a potential re-evaluation of our understanding of cosmic-ray sources, acceleration mechanisms, and their propagation within our galaxy.

About Cosmic rays:

  • They are high energy particles that move through space at nearly the speed of light. 
  • Cosmic rays provide one of few direct samples of matter from outside the solar system
  • Most cosmic rays are atomic nuclei without their atoms with protons (hydrogen nuclei) being the most abundant type, but nuclei of elements as heavy as lead also have been measured.
  • Within cosmic-rays, we also find other subatomic particles like neutrons, electrons and neutrinos.

Methodology used in the experiment:

  • Researchers utilized a combination of a dense array of plastic scintillator detectors and a large-area muon detector.
  • The researchers collected data with a collection area several thousand times larger than space-based detectors
    • It allowed researchers a more detailed examination of cosmic rays above 100 TeV, where space-based measurements lack precision due to low statistics.
  • A subset of about 8 million cosmic ray shower events recorded by these detectors was analyzed.
    • Researchers also used CPU-intensive computer simulations to measure the cosmic-ray spectrum.

Conclusion:

The GRAPES-3 experiment's discovery of a new feature in the cosmic-ray proton spectrum at 166 TeV prompts a reassessment of cosmic-ray origins and propagation. Utilizing advanced detector arrays and simulations, this finding enriches our understanding of high-energy astrophysical processes and their implications.

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