Astrophysics

    

Basic Simulation of S and R Processes in Stars and Formation of Heavy Elements

Authors: Rajeev Singh

In this introductory project, we have studied the about the neutron capture processes which are responsible for the abundances of heavy elements than iron in different phases of stellar evolution. Our main aim is to understand the distribution of isotropic abundances in our universe. First we start with the discussion on nucleosynthesis and its types, then we discussed about the different types of neutron capture processes. After that we provide results of the simulation which we have done using Monte Carlo method. Finally we conclude with the importance of these processes and current research status.

Comments: 13 Pages.

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Submission history

[v1] 2020-08-05 05:00:17

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