The r approach is made up of neutron seize followed, in a charge depending on the half-life of the nucleus, by beta decay, which produces a much less neutron-abundant isotope closer into the valley of beta stability. In this manner, the r procedure follows distinctive paths along the neutron-rich aspect https://zionaehhi.look4blog.com/71201233/examine-this-report-on-the-stellar-abundance-review