Particle decay is a Poisson process, and hence the probability that a particle survives for time t before decaying (the survival function) is given by an exponential distribution whose time constant depends on the particle's velocity:
P ( t ) = exp ( − t γ τ ) {\displaystyle P(t)=\exp \left(-{\frac {t}{\gamma \tau }}\right)}
All data are from the Particle Data Group.
This section uses natural units, where c = ℏ = 1. {\displaystyle c=\hbar =1.\,}
The lifetime of a particle is given by the inverse of its decay rate, Γ, the probability per unit time that the particle will decay. For a particle of a mass M and four-momentum P decaying into particles with momenta pi, the differential decay rate is given by the general formula (expressing Fermi's golden rule) d Γ n = S | M | 2 2 M d Φ n ( P ; p 1 , p 2 , … , p n ) {\displaystyle d\Gamma _{n}={\frac {S\left|{\mathcal {M}}\right|^{2}}{2M}}d\Phi _{n}(P;p_{1},p_{2},\dots ,p_{n})\,}
The factor S is given by S = ∏ j = 1 m 1 k j ! {\displaystyle S=\prod _{j=1}^{m}{\frac {1}{k_{j}!}}\,}
The phase space can be determined from d Φ n ( P ; p 1 , p 2 , … , p n ) = ( 2 π ) 4 δ 4 ( P − ∑ i = 1 n p i ) ∏ i = 1 n d 3 p → i 2 ( 2 π ) 3 E i {\displaystyle d\Phi _{n}(P;p_{1},p_{2},\dots ,p_{n})=(2\pi )^{4}\delta ^{4}\left(P-\sum _{i=1}^{n}p_{i}\right)\prod _{i=1}^{n}{\frac {d^{3}{\vec {p}}_{i}}{2(2\pi )^{3}E_{i}}}}
One may integrate over the phase space to obtain the total decay rate for the specified final state.
If a particle has multiple decay branches or modes with different final states, its full decay rate is obtained by summing the decay rates for all branches. The branching ratio for each mode is given by its decay rate divided by the full decay rate.
Say a parent particle of mass M decays into two particles, labeled 1 and 2. In the rest frame of the parent particle, | p → 1 | = | p → 2 | = [ M 2 − ( m 1 + m 2 ) 2 ] [ M 2 − ( m 1 − m 2 ) 2 ] 2 M , {\displaystyle |{\vec {p}}_{1}|=|{\vec {p}}_{2}|={\frac {\sqrt {[M^{2}-(m_{1}+m_{2})^{2}][M^{2}-(m_{1}-m_{2})^{2}]}}{2M}},\,} which is obtained by requiring that four-momentum be conserved in the decay, i.e. ( M , 0 → ) = ( E 1 , p → 1 ) + ( E 2 , p → 2 ) . {\displaystyle (M,{\vec {0}})=(E_{1},{\vec {p}}_{1})+(E_{2},{\vec {p}}_{2}).\,}
Also, in spherical coordinates, d 3 p → = | p → | 2 d | p → | d ϕ d ( cos θ ) . {\displaystyle d^{3}{\vec {p}}=|{\vec {p}}\,|^{2}\,d|{\vec {p}}\,|\,d\phi \,d\left(\cos \theta \right).\,}
Using the delta function to perform the d 3 p → 2 {\displaystyle d^{3}{\vec {p}}_{2}} and d | p → 1 | {\displaystyle d|{\vec {p}}_{1}|\,} integrals in the phase-space for a two-body final state, one finds that the decay rate in the rest frame of the parent particle is
d Γ = | M | 2 32 π 2 | p → 1 | M 2 d ϕ 1 d ( cos θ 1 ) . {\displaystyle d\Gamma ={\frac {\left|{\mathcal {M}}\right|^{2}}{32\pi ^{2}}}{\frac {|{\vec {p}}_{1}|}{M^{2}}}\,d\phi _{1}\,d\left(\cos \theta _{1}\right).\,}
The angle of an emitted particle in the lab frame is related to the angle it has emitted in the center of momentum frame by the equation tan θ ′ = sin θ γ ( β / β ′ + cos θ ) {\displaystyle \tan {\theta '}={\frac {\sin {\theta }}{\gamma \left(\beta /\beta '+\cos {\theta }\right)}}}
Further information: Resonance § Atomic, particle, and molecular resonance; and Resonance (particle physics)
The mass of an unstable particle is formally a complex number, with the real part being its mass in the usual sense, and the imaginary part being its decay rate in natural units. When the imaginary part is large compared to the real part, the particle is usually thought of as a resonance more than a particle. This is because in quantum field theory a particle of mass M (a real number) is often exchanged between two other particles when there is not enough energy to create it, if the time to travel between these other particles is short enough, of order 1 M , {\displaystyle {\tfrac {1}{M}},} according to the uncertainty principle. For a particle of mass M + i Γ {\displaystyle M+i\Gamma } , the particle can travel for time 1 M , {\displaystyle {\tfrac {1}{M}},} but decays after time of order of 1 Γ . {\displaystyle {\tfrac {1}{\Gamma }}.} If Γ > M {\displaystyle \Gamma >M} then the particle usually decays before it completes its travel.4
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