by Jarek » Wed Oct 13, 2021 6:59 am
It is close to zero, but cannot be neglected: can add to non-negligible contributions in arbitrarily large distance ... gravity is muuuuch weaker and adds to essential contributions in cosmological scales deciding evolution of the Universe.
And generally there is no problem with long-range behavior, only short-range: we don't know what is energy density e.g. 1fm from electron - we need rho(r) energy density function.
It is close to zero, but cannot be neglected: can add to non-negligible contributions in arbitrarily large distance ... gravity is muuuuch weaker and adds to essential contributions in cosmological scales deciding evolution of the Universe.
And generally there is no problem with long-range behavior, only short-range: we don't know what is energy density e.g. 1fm from electron - we need rho(r) energy density function.