Black holes with q>e, or a charge greater than the mass of the black hole, are considered singular because the equations of general relativity break down at the singularity. This means that we do not fully understand the physics at this point, and it is a subject of ongoing research and debate.
The charge of a black hole affects the singularity by altering the shape and properties of the event horizon. A charged black hole has an inner and outer event horizon, and the singularity lies between these horizons. The charge also affects the strength of the gravitational pull at the singularity.
It is currently unknown if black holes with q>e can exist in nature, as the conditions required for such a black hole to form are not fully understood. However, some theories suggest that primordial black holes with q>e may have formed in the early universe, and they could potentially exist in extreme environments such as near supermassive black holes.
If a charged object were to fall into a black hole with q>e, it would experience a force known as the Coulomb force, which is similar to the electromagnetic force. This force would cause the object to repel from the singularity and potentially prevent it from reaching the event horizon. However, the exact behavior of the object would depend on its mass, charge, and the strength of the gravitational pull.
The singularity of a black hole with q>e differs from a non-charged black hole in several ways. One key difference is that the charged black hole has an inner and outer event horizon, while a non-charged black hole only has one event horizon. Additionally, the singularity of a charged black hole has a different shape and properties due to the presence of the charge. The behavior of particles and objects falling towards the singularity also differs between charged and non-charged black holes.