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Heavy Elements Produced in Supernova Explosion and thier Propulsion in the ISM

Published online by Cambridge University Press:  29 January 2014

Rulee Baruah
Rulee Baruah*
Affiliation:
Department of Physics, HRH The Prince of Wales Institute of Engineering and Technology, Jorhat-785001, India email: ruleeb@yahoo.com
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Abstract

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We study the r-process path at temperatures from 1.0–3.0 × 109K and neutron number density from 1020-1030cm−3. At low density of 1020 cm−3 and T9 = 2.0, the path contains all the elements as given by experimental data of Wapstra et al. (2003). The element 98Cf254 shown by supernova light curves is found in our results. We take iron (Z = 26) as seed for calculation of abundances for supernova.

Keywords

r-processlight curvesabundances
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S296: Supernova Environmental Impacts , January 2013 , pp. 390 - 391
Copyright
Copyright © International Astronomical Union 2014 

References

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