  We study the formation of primordial black holes (PBH) in the Starobinsky
supergravity coupled to the nilpotent superfield describing Volkov-Akulov
goldstino. By using the no-scale K\"ahler potential and a polynomial
superpotential, we find that under certain conditions our model can describe
effectively single-field inflation with the ultra-slow-roll phase that appears
near a critical (nearly-inflection) point of the scalar potential. This can
lead to the formation of PBH as part of (or whole) dark matter, while keeping
the inflationary spectral tilt and the tensor-to-scalar ratio in good agreement
with the current cosmic microwave background (CMB) bounds. After inflation,
supersymmetry is spontaneously broken at the inflationary scale with the
vanishing cosmological constant.
