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I've been looking for a literature value and can't find one, even from the PDG. Does anyone know where I could find the branching fractions for the $\Delta^0$ decay modes, specifically $\Delta^0 \rightarrow n + \pi^0$ $\Delta^0 \rightarrow p + \pi^-$?

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Except for small electromagnetic decay branching ratios like $\Delta\to N\gamma$, essentially 100% of the branching ratio of the $\Delta$ is to $N\pi$ final states. This is just kinematics. The only other hadronic final state with baryon number one that is energetically allowed is $N\pi\pi$, which has an extremely small phase (it is just barely allowed).

The relative rates for $\Delta^0\to n+\pi^0$ and $\Delta^0\to p+\pi^-$ are determined by isospin. The relevant Clebsch-Gordon coefficients are $$ \langle 3/2,-1/2|1/2,-1/2;1,0\rangle = \sqrt{2/3}\\ \langle 3/2,-1/2|1/2,1/2;1,-1\rangle = \sqrt{1/3} $$ so the relative rates are 2/3 and 1/3.

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The resonance has an isospin and as a strong interaction resonance, the decay channels are treated in the PDG as one "Nucleon pi" decay

delta1232

The correct ratio is given in the answer by @Thomas, who gives the algebra of the SU(2) isospin case. 2:1

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  • $\begingroup$ This is not right. The rates are determined by Clebsch-Gordan coefficients, which are 2:1. $\endgroup$
    – Thomas
    Commented Feb 12, 2017 at 22:09
  • $\begingroup$ @Thomas yes, the way to get the numbers are clebsch gordan coefficients, I just guessed at them because I am too rusty. $\endgroup$
    – anna v
    Commented Feb 13, 2017 at 4:41
  • $\begingroup$ OP please choose the other answer as the correct one as I had a mistaken ratio . You are allowed to change mind on which answer you chose. Sorry if this was a homeork problem, but in any case for a homework problem you have to show the calculation $\endgroup$
    – anna v
    Commented Feb 13, 2017 at 4:45
  • $\begingroup$ Not a homework problem and it's all right, I was only looking for these as confirmation of a calculation, I had used CG coefficients. $\endgroup$
    – user13948
    Commented Feb 15, 2017 at 10:44

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