INDIAN INSTITUTE OF SCIENCE EDUCATION AND RESEARCH BHOPAL

 

Name: Dr. Sukanta Panda
Designation: Assistant Professor
Department: Physics
E-Mail: sukanta@iiserb.ac.in
Phone: +91-755-4092303
Fax: +91-755-4092392

Academic Profile:

  • Assistant Professor (November 2008-), Physics, Indian Institute of Science Education and Research, Bhopal, India.
  • Post-doc. Position from Spanish Ministry of Education and Science at Universidad Autonoma de Madrid, Madrid, Spain from 01.02.2006 to 31.09.2008.
  • Post-doc. Harish-Chandra Research Institute from 01.04.2004 to 31.01.2006.
  • Ph.D. Signatures of Low Scale Gravity in Ultra High Energy Cosmic Rays, Department of Physics, Indian Institute of Technology, Kanpur with Dr. Pankaj Jain.

Research Interest:

  • High Energy Cosmic Rays


Selected Publications:

  1. Extra Dimensions and Strong Neutrino-Nucleon Interactions Above 1019 eV :
    Breaking the GZK Barrier (hep-ph/0001031), Phys Lett. B 484, 267 (2000).
    Pankaj Jain, Douglas W. Mckay, S. Panda and John P. Ralston.

  2. Angular Dependence of Neutrino Flux in KM3 Detectors in Low Scale Gravity
    Models (hep-ph/0205052) Phys. Rev. D 66, 065018 (2002). Pankaj Jain, Supriya Kar, Douglas W. Mckay, Sukanta Panda and John P.Ralston.

  3. Brane-Production and the Neutrino-Nucleon Cross Section at Ultra High
    Energies in Low Scale Gravity Models (hep-ph/0201232)Int. J. Mod. Phys D 12, 1593 (2003).Pankaj Jain, Supriya Kar and Sukanta Panda.

  4. Probing Very High Energy Prompt Muonand Neutrino fluxes and Cosmic Ray Knee via Underground Muons (hepph/0512179) JCAP07, 011 (2006).Raj Gandhi and Sukanta Panda.

  5. High Energy Atmospheric Muon flux Expected at India-Based NeutrinoObservatory, hep-ph/0710.3125, accepted for publication in IJMPA.Sukanta Panda and Sergei Sinegovskii.

  6. Prospects for detection of the lunar Cerenkov emission by the UHE Cosmic Rays and Neutrinos using the GMRT and the Ooty Radio Telescope,arXiv:0805.4304.Govind Swarup and Sukanta Panda.

  7. Stau detection at neutrino telescopes in scenarios with supersymmetric dark
    matterarXiv:0812.1067, Accepted in JCAP.

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