Stable nuclides are those whose n/p ratio is | vedclass

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(A) For light elements with low atomic numbers (up to $Z = 20$),stable nuclides typically have a neutron-to-proton ratio of approximately $1$ $(n/p =

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$n/p = 1$

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(A) For light elements with low atomic numbers (up to $Z = 20$),stable nuclides typically have a neutron-to-proton ratio of approximately $1$ $(n/p = 1)$.As the atomic number increases,the number of neutrons required for stability increases,leading to an $n/p$ ratio greater than $1$ for heavier elements.However,in the context of general introductory chemistry,the ideal ratio for stability is often represented as $n/p = 1$.

Stable nuclides are those whose $n/p$ ratio is

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