The Heaviside step distribution is defined by (Abramowitz and Stegun Eq. 29.1.3, p. 1020):

Differentiating the Heaviside distribution
At first glance things are hopeless:


however, lets define a less brutal jump in the form of a linear slope
such that

in the limit
this becomes the Heaviside function
. However, lets differentiate first:

in the limit this is the Dirac delta function. Thus
![{\displaystyle {\frac {\rm {d}}{{\rm {d}}x}}[H(x)]=\delta (x)}](https://wikimedia.org/api/rest_v1/media/math/render/svg/569855ece47d384a52c8b50f405a4c64087d7d1d)
The delta function has the fundamental property that

References
- Milton Abramowitz and Irene A. Stegun "Handbook of Mathematical Functions" Dover Publications ninth printing.