Information Information

Contact
Room 430
P.O.Box: 11155-9161
Tel: 098 21 6616 4528
Fax: +98 21 6602 2711
E-Mail: bahmanabadi@sharif.edu
Personal Page: http://sina.sharif.edu/~bahmanabadi
Group Page: http://physics.sharif.edu/~cosmicrays

 

Research Interests

Cosmic rays Gamma Rays Astronomy.

 

Research Plan

The earth is bombarding by elementary particles and atomic nuclei of very high energies. They are Oriented from outer space, such as the sun, neutron stars, black holes, and etc. These particles may produce secondary particles that penetrate Earth's atmosphere. The number of particles start to increase rapidly as this shower or cascade of particles mores downwards in the atmosphere. We call this an Extensive air shower. Extensive air showers can be detected with different kinds of particle detectors. We carry out the detection by scintillation detectors. So, we can find direction and energy of primary particles and finally their sources.

 

Selected Publications

  • F. Sheidaei, M. Bahmanabadi, and J. Samimi, "Moon shadow on high energy cosmic ray in data of a small extensive air shower array", Astroparticle Physics, Accepted, 2010
  • F. Sheidaei, M. Bahmanabadi, A. Keivani and J. Samimi, "Instrumentation development for an array of water Cherenkov detectors for extensive air shower experiments", JOURNAL OF PHYSICS G: NUCLEAR AND PARTICLE PHYSICS, 36 (2009) 115201 (9pp)
  • S.M.H. Halataei, M. Bahmanabadi, M. Khakian Ghomi, and J. Samimi "Simulation study on Number of secondary particles in extensive air showers using CORSIKA Code", PHYSICAL REVIEW D 77, 083001 (2008)
  • F. Sheidaei, M. Bahmanabadi A. Keivani, M. Khakian Ghomi, J. Samimi, and A. Shadkam "Study on anisotropy of cosmic ray distribution with a small array of water Cherenkov detectors", PHYSICAL REVIEW D 76, 082002 (2007)
  • M. Bahmanabadi, M. Khakian Ghomi, F. Sheidaei, J. Samimi "Galactic Anisotropy of Cosmic Ray Intensity Observed by an Air Shower Experiment", Publications of the Astronomical Society of Australia 23, 1-6 (2006)