Home page of KAMALES KAR

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  • Ph.D. University of Rochester, 1979; Senior Professor, Saha Institute of Nuclear Physics

    Fields of interest

    Publications/Preprints since 2003

    1. Localisation in 2p1f nuclear shell model wavefunctions, J.M.G. Gomez, K. Kar, V.K.B. Kota, R.A. Molina and J. Retamosa, Phys. Letts B 567 251 (2003)
    2. Working group report: Neutrinos and astroparticle physics, R. Gandhi, K. Kar and S. Uma Sankar, Pramana 60 405 (2003)
    3. Number of principal components and localization length in E2 and M1 transition strengths in 46V, J.M.G. Gomez, K. Kar, V.K.B. Kota, R.A. Molina and J. Retamosa, Phys Letts B 506 333 (2003)
    4. Prospects of probing theta13 and neutrino mass hierarchy by supernova neutrinos in KamLAND, Abhijit Bandyopadhyay, Sandhya Choubey, Srubabati Goswami and Kamales Kar, hep-ph/0312315
    5. Neutrinos from supernovae, Sandhya Choubey and Kamales Kar,hep-ph/0212326 , Proceedings INSA 70A (2004) 123
    6. India-based Neutrino Observatory: Project Report. Volume 1 by INO Collaboration- M. Sajjad Athar et al, INO-2006-01, May (2006)
    7. Beta decay rates for nuclei with 115 Possible violation of the spin-statistics relation for neutrinos: checking through future galactic supernova, Sandhya Choubey and Kamales Kar, Phys Letts B B364 (2006) 14
    8. Beta decay rates for nuclei with 65 A GEANT-Based study of atmospheric neutrino oscillation parameters at INO, A Samanta, S. Bhattacharya, A.Ghosal, K. Kar, D. Majumdar and A. Raychaudhuri, Intl Jour of Mod Phys A 23 (2008) 233
    9. Upper limit on the cosmic gamma-ray burst rate from high energy diffuse neutrino background, Pijushpani Bhattacharjee, Sovan Chakraborty, Srirupa Das Gupta and Kamales Kar, Phys Rev D 77 (2008) 043008 (astro-ph/0710.5922)
    10. Effect of collective flavor oscillations on the diffuse supernova neutrino background, Sovan Chakraborty, Sandhya Choubey, Basudeb Dasgupta and Kamales Kar, Jour Cosmology and Astropart Phys 0809:013 (2008) (hep-ph/0805.3131)
    11. Beta decay rates for r-process for nuclei near neutron number N=82, Kamales Kar and Soumya Chakravarti, astro-ph/0811.0872
    12. Weak interaction rates for stellar evolution, supernovae and nucleosynthesis, Kamales Kar, Proc. School on synthesis of elements in stars and cosmic abundances (Kodaikanal, 2008) (Spriger-Verlag, 2009) (to appear)

    How to reach me

    mailing address:

    KAMALES KAR
    Theory Division
    Saha Institute of Nuclear Physics
    Sector 1, Block AF, Bidhan Nagar
    Calcutta 700064 India

    e-mail: kamales.kar@saha.ac.in

    phone: 91 33 2337 5345 ext 2345

    fax: 91 33 2337 4637

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