  Carroll black holes with an associated Carroll temperature were introduced
recently. So far, it is unclear if they exhibit a Hawking-like effect. To solve
this, we study scalar fields on Carroll black hole backgrounds. Inspired by
anomaly methods, we derive a Hawking-like energy-momentum tensor compatible
with the Carroll temperature and the Stefan-Boltzmann law. Key steps in our
derivation are the finiteness of energy at the Carroll extremal surface and
compatibility with the Carroll Ward identities, thereby eliminating,
respectively, the Carroll-analogs of the Boulware and Unruh vacua.
