I do think that $L^0$ is nice usage. As is well-known $\lim_{p \to \infty} \|\cdot \|_{L^p} = \|\cdot\|_\infty$ for certain spaces or functions. The case for $L^0$ is not that pretty, but at least still nice.
Recall the distribution function $\mu$ of $f$ given by,
$$\mu(\alpha) := \mu_f(\alpha) := \mu\{|f|>\alpha\}.$$
Fubini gives that,
$$\|f\|_{L^p}^p = p \int_0^\infty \mu_f(\alpha) \alpha^p \frac{\mathrm{d}\alpha}{\alpha}.$$
We can define the Lorentz spaces in a similar way. And indeed, for a finite measure space, we have if $p < q$ that
$$L^q \subseteq L^p.$$
Hence, it is natural to define $L^0$ as,
$$L^0 = \bigcup_{p > 0} L^p.$$
We would like to have that $L^0$ is also complete as a metric space, otherwise the notation would be quite deceiving indeed. For this we need a notation of convergence. On $L^p$ for $0 < p < 1$ it is not the norm that induces the metric, but it is $\|\cdot\|_p^p$.
So, for $0 < p < 1$ we have,
$$d_p(f, g) = p \int_0^\infty \mu\{|f - g|>\alpha\} \alpha^p \frac{\mathrm{d}\alpha}{\alpha}.$$
$\varepsilon$-neighborhoods $N^p_\varepsilon$ of $f$ in $L^p$ are then given by
$$N^p_\varepsilon(f) = \Biggl\{g : p \int_0^\infty \mu\{|f - g|>\alpha\} \alpha^p \frac{\mathrm{d}\alpha}{\alpha} < \varepsilon \Biggr\}.$$
Too be continued, I wanted to give a brief remark, but I have decided otherwise in due progress.