An unstable particle of mass $M$ and mean lifetime $\tau$ has width $\Gamma$ that such that:
$$ \Gamma\tau \approx \hbar $$
The observed mass distribution follows that Breit Wigner resonance probability:
$$ f(E) =\frac k {(E^2-M^2)^2+M^2\Gamma^2}$$
with
$$ k = \frac{2\sqrt 2 M\Gamma\gamma}{\pi\sqrt{M^2+\gamma}}$$
where:
$$ \gamma = \sqrt{M^2(M^2+\Gamma^2)}$$
You have to have $M\gg\Gamma$ if you want to actually see the resonance, otherwise, there is no "bump" over background. (It's like a very over-damped oscillator, which will never oscillates..it just relaxes slowly back to 0).
Weak interactions are slow, e.g. charged pions have around $10^{-8}\,$s, while the neutral pion decays electromagnetically in $10^{-15}$ seconds.
One doesn't usually talk about widths until the strong interaction, e.g. the $\Delta$ resonances, which decay in $5\times 10^{-24}\,s$ for a width of $130\,{\rm MeV/c^2}$...about one tenth the mass.
Of course there are many exceptions to these rules. The $W^{\pm}$ decay weakly with a width of $2\, {\rm GeV/c^2}$, but here you are already working at the $W$-mass scale, where the weak interaction is no longer weak.
Nuclear decays span many orders of magnitude, with many long lived alpha (strong decay) emitters, and shorted lived beta (weak) emitters. There are many other factors affecting decay rate besides the coupling strength. Nevertheless, most electromagnetic metastable decays are fast.
Meanwhile, glow-in-the-dark plastics are electromagnetic molecular transitions that are macroscopically long...but again there are other factors like "forbidden" transitions and spin flips coming into play.