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Title

A SIMULATION ON THE PROPAGATION OF SUPERNOVA COSMIC PARTICLES IN A FRACTAL MEDIUM

Author(s)

KETABI N. | FATEMI J.

Pages

  269-272

Abstract

 In this paper, we present a Mont Carlo simulation by using the inhomogeneous diffusion equation suggested by Lagutin et al. in a fractal interstellar medium for a SUPERNOVA, as being the main source of Galactic COSMIC RAYS in an energy range up to 1016ev. When the numerical results of this simulation are compared with the predicted energy density of COSMIC RAYS from the SUPERNOVA model of Erlikyn and Wolfendale (EW), they show a strong consistency with the observed experimental parameters of COSMIC RAYS, i.e. Galactic radial gradient, percentage of total SUPERNOVA energy transfer to cosmic particles etc., which is also confirmation of a SUPERNOVA being of cosmic ray origin.

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    APA: Copy

    KETABI, N., & FATEMI, J.. (2009). A SIMULATION ON THE PROPAGATION OF SUPERNOVA COSMIC PARTICLES IN A FRACTAL MEDIUM. SCIENTIA IRANICA, 16(3 (TRANSACTION B: MECHANICAL ENGINEERING)), 269-272. SID. https://sid.ir/paper/289800/en

    Vancouver: Copy

    KETABI N., FATEMI J.. A SIMULATION ON THE PROPAGATION OF SUPERNOVA COSMIC PARTICLES IN A FRACTAL MEDIUM. SCIENTIA IRANICA[Internet]. 2009;16(3 (TRANSACTION B: MECHANICAL ENGINEERING)):269-272. Available from: https://sid.ir/paper/289800/en

    IEEE: Copy

    N. KETABI, and J. FATEMI, “A SIMULATION ON THE PROPAGATION OF SUPERNOVA COSMIC PARTICLES IN A FRACTAL MEDIUM,” SCIENTIA IRANICA, vol. 16, no. 3 (TRANSACTION B: MECHANICAL ENGINEERING), pp. 269–272, 2009, [Online]. Available: https://sid.ir/paper/289800/en

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