Particle physics: calculating the phase space factor for pion to muon decay

ncs22
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Show that the phase space factor \rho \propto p^2 dp/dE for the decay \pi\rightarrow \mu + \upsilon is

\rho \propto \frac{({m_\pi}^2 - {m_\mu}^2)^2}{{m_\pi}^3}E_\mu

where E is the total energy.I can show that p^2 = ({m_\pi}^2 - {m_\mu}^2)^2/4{m_\pi}^2

but then I get stuck, I don't know how to evaluate dp/dE and I'm not sure what p here is referring to i.e. which particle and in which frame. I worked out the above expression for p2 taking it to be the energy for the muon (or neutrino) in the center of mass frame.
 
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I'm not sure what exactly is meant by phase-space factor, but I would assume that a Dirac delta (for 4-momentum conservation) has already been factored out, which means that you can treat the momentum as the final-state momentum of the particle of your choice. Usually, you choose the visible one (e.g. the muon).
 
Thanks for the reply.

ok cool at least that means the first bit is probably right :-)

The phase space factor is the number of final states per initial energy, for example the term in Fermi's Golden rule usually denoted by a \rho. Yes I know you can write the phase space as a product of integrals over every particles momentum in which case a delta function has to be introduced to account for the fact that not every momentum is independent.

When I find the answer I will post it here.
 
I understand I can't post solutions to homework questions until the OP has solved the problem or the thread has been dormant a long time. However, it has been over 15 years and I just solved this same problem, so I would like to finally put this thread to rest.

To start, note that ##p## here is the magnitude of the muon's momentum ##\mathbf{p}## in the COM frame. As this is a two-body decay, ##\mathbf{p_\nu} = -\mathbf{p}## by conservation of momentum. As stated in the original post, ##E## is the total energy in the COM frame, so ##E = m_\pi## (we set ##c=1## throughout).

The 4-momenta of the particles in the COM frame can be written as $$(p_\pi)^\lambda = (m_\pi, \mathbf{0})$$ $$(p_\mu)^\lambda = (E_\mu, \mathbf{p})$$ $$(p_\nu)^\lambda = (p, -\mathbf{p})$$ where we assume the neutrino is massless. By conservation of 4-momentum, $$(p_\pi)^\lambda - (p_\nu)^\lambda = (p_\mu)^\lambda$$ By squaring both sides (recalling the Minkowski metric) we get $$-m_\pi^2+2m_\pi p = -m_\mu^2$$ $$\implies\quad p^2=\frac{(m_\pi^2-m_\mu^2)^2}{4m_\pi^2} \tag{1}$$ Now we consider ##\frac{dp}{dE}##. Equating the zeroth component of the 4-momenta we find $$m_\pi=E_\mu+p=\sqrt{m_\mu^2+p^2} + p$$ From earlier we know ##m_\pi=E##, so we get $$E=\sqrt{m_\mu^2+p^2} + p$$ Differentiating both sides wrt ##E##, we find $$1=\frac{1}{2}(m_\mu^2+p^2)^{-\frac{1}{2}}\cdot2p \frac{dp}{dE}+\frac{dp}{dE}$$ $$\implies \quad 1=\frac{dp}{dE} [1+\frac{p}{(m_\mu^2+p^2)^{\frac{1}{2}}}]=\frac{dp}{dE} [1+\frac{p}{E_\mu}]$$ $$\implies \quad \frac{dp}{dE} = [1+\frac{p}{E_\mu}]^{-1} = \frac{E_\mu}{E_\mu+p}$$ $$\implies\quad \frac{dp}{dE} = \frac{E_\mu}{m_\pi}\tag{2}$$ Combining equations ##1## and ##2## and ignoring the constant gives the required answer.
 
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