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Dr. A.R. Fazely

                            
                           

                  Ali R. Fazely

Title:
   Emeritus Professor 
Office:

   Department of Physics, Rm. 237, William James Hall, Southern University,

   Baton Rouge, LA 70813

Phone:
   225-267-7254
Email:
   fazely@icecube.wisc.edu
        CV:    Detailed Curriculum Vita & CV

 

 

 

Education

  • Ph.D., Kent State University, Kent, OH, USA, 1982, Intermediate Energy Nuclear Physics
  • M.A., Physics, Kent State University, Kent, OH, USA, 1980
  • M.S., Mechanical Engineering, Oklahoma State University, Stillwater, OK, USA, 1977
  • B.S., Mechanical Engineering, Oklahoma State University, Stillwater, OK, USA, 1975

Work Experience

  • Southern University, Department of Physics 8/1998-2013: Professor, Doctoral Research Faculty, Graduate Coordinator
  • Southern University, Department of Physics 8/1996-7/1998: Associate Professor, Doctoral Research Faculty, Graduate Coordinator 8/1996-7/1997: Associate Professor, tenured
  • Southern University, Department of Physics 8/1992-7/1996: Associate Professor, Associate Professor, tenure-track
  • Southern University, Department of Physics 8/1991-7/1992: Assistant Professor
  • Louisiana State University, Department of Physics 1/1991-8/1991: Assistant Professor-Research
  • Louisiana State University, Department of Physics 9/1985-12/1990: Senior Research Associate
  • Louisiana State University, Department of Physics, Visiting Scientist, Los Alamos National Laboratory 2/1983-8/1985: Research Associate
  • Kent State University, Department of Physics 9/1982-3/1983: Research Associate
  • Langston University, Department of Physical Science 9/1977-3/1978: Physics Instructor

Research Accomplishments

  • For the latest Research (CV)
  • Over 200 refereed publications, including two (2) Liquid Scintillator Neutrino Detector (LSND) renowned (over 500 citations) papers. CV
  • More than 200 presentations and proceedings, more than 19 invited talks. 
  • Had leading and pivotal role as the Deputy Spokesman and as the major author of the Oak Ridge Large Neutrino Detector (ORLaND)  proposal

Administrative Experience/Grant & Contract Activities

  • Established the Southern University Radiation Safety Office,
  • Chairman of the Department Tenure and Promotion Committee,
  • Chair of the Graduate Admission and Assistantship Committee,
  • Details are available in my CV CV

Awards, Honors, Scientific Leadership & Offices Held

  • Member of Sigma Xi
  • Member of the American Physical Society
  • Graduate Student Achievement Award in Research, Academic Year 1981-82
  • Co-spokesman of Experiment 999 at the Los Alamos Meson Physics Facility (LAMPF)
  • Co-spokesman of Experiment 1161 at LAMPF
  • Chairman of Neutrino Facilities at the Los Alamos Meson Physics Facility (LAMPF) (1992-1994)
  • Member of LAMPF Technical Advisory Panel (1992-1994)
  • Deputy Spokesman for the Oak Ridge Laboratory for Neutrino Detectors (ORLaND), (1999-2001)
  • University Outstanding Research/Investigator, Academic Year 04-05

 

BELOW ARE SELECTED GEANT SIMULATIONS FOR THE ICECUBE DETECTOR

 

 

 

 

 

 

 
 


Ali R. Fazely, Samvel Ter-Antonyan, Xianwu Xu
Southern University, Baton Rouge

fazely@icecube.wisc.edu

Description
  • I3geant Simulation for Supernova Neutrinos
  • The same MC also simulates atmospheric muon events. Please click on the following link. Atmospheric Muons
  • Full Geant-3.21/GCALOR Simulation of the IceCube Detector. The AHA ice model was used.



Current Results for the Final IceCube Geometry (78 + 8). A SN temprature of T = 6.5 MeV is assumed. A total of 1,000,000 e+'s were simulated. These results use the latest DOM acceptance datafiles from Chiba. A 15% threshold for PE detection has been applied.

  • The SN neutrino energy distribution according to a Fermi function with T = 6.5 MeV (top),
  • and the positron energy distribution from the inverse beta decay reaction (bottom).
  • The flux-integrated cross section for the inverse beta decay reaction is 0.37 x 10^-40 cm^2

       
  • The fiducial volume peppered by 740,000 positrons.

       
  • Two-DOM fraction coincidence plots (left). Ratio of 2+ DOM hits to all hits is about 2%. Number of hits per DOM (right). Note, these plots are for the whole detector (5160 DOMs).

           
  • Two-DOM fraction coincidence plots (left). Ratio of 2+ DOM hits to all hits is about 5.6%. Number of hits per DOM (right). Note, these plots are for the DeepCore only.

           
  • DOM sensitivity range for IC-86 to C-light from the SN positrons (left) and DOM sensitivity range for DC to C-light from the SN positrons (right).

           

    Results for the Final IceCube Geometry (78 + 8). A SN temprature of T = 6.5 MeV is assumed. A total o:0 f 10,000,000 e+'s were simulated. These results use the old DOM acceptance datafiles

    • Hit distributions for single DOM hits

                 
    • Two-DOM fraction coincidence plots (left); Number of hits per DOM (right)

             
    • DOM Occupancy Plot for SN Positrons. Note the bottom of the detector has much clearer ice.

         

      Results for IceCube Geometry (80 + 6)

      • Hit distributions for single DOM hits

               
      • Two-DOM fraction coincidence plots

           
      • Hit distribution and the corresponding hit times in mu-sec.

               
      • An event display of a sample of e+ SN events. Note the scattering and absorption are taken from the AHA ice model.

           


    Last update 12.23.10