No I really just mean the plain and simple scenario. Imagine you knew nothing about escape velocity or black holes, then you would not be confused at all by the idea that an object can move away from the Earth at any speed whatsoever, so long as its direction was away from the Earth. You don't need to move at Earth's escape velocity to move arbitrarily far away from the Earth. You could in principle travel all the way to the Andromeda galaxy without ever exceeding the Earth's escape velocity at any point.
Now for some reason when people talk about black holes existing because the escape velocity exceeds the speed of light, then it tricks people into thinking things they would never have otherwise thought, like in order to move away from an object you need to be moving at that object's escape velocity. Like somehow if you don't move away from an object at its escape velocity then you can't move away from that object at all.
Ignoring general relativity, if a black hole was nothing more than an object that had an escape velocity greater than the speed of light, then there's no reason why you couldn't enter the event horizon and then very slowly come back out, go back in, then sloooowly come back out, heck even come out and travel to an arbitrarily far galaxy and tell people about your adventure.
Escape velocity does not mean being unable to move away from an object, not for Earth and not for a black hole either. Escape velocity just means the velocity where no further propulsion or acceleration is needed to continue moving away from an object.
In general relativity, it's not simply that the escape velocity at the event horizon is equal to the speed of light, for if that were all there was to it, then simply bring some fuel with you to propel yourself away from the event horizon, feel free to do so at 1 cm an hour. In general relativity there are two perspectives, the perspective of the object entering the black hole where space-time curvature becomes so extreme that the spatial coordinate swaps places with the time coordinate in such a way that every future point is closer and closer to the singularity, and there is the perspective of an outside observer who sees an object getting closer to the event horizon undergo extreme time dilation and effectively freeze as their position perpetually smears itself across the entirety of the event horizon.