Quantum Field Hamiltonian
We are given a Hamiltonian: \[ H=\int dx\left[\Psi^\dagger(x)\left(-\frac{\nabla^2}{2m}\right)\Psi(x)+V(x)\Psi^\dagger(x)\Psi(x)\right]. \] Here we take \(\hbar=1\). The first term is the kinetic energy term, because in single-particle quantum mechanics, \(\hat p^2/(2m)\) in the position representation corresponds to \(-\nabla^2/(2m)\). The second term is the potential energy term, where \(\Psi^\dagger(x)\Psi(x)\) is the particle number density at position \(x\), so \(V(x)\Psi^\dagger(x)\Psi(x)\) represents the potential energy density at \(x\). If we take \(V(x)=mc^2\), it just adds a rest energy to each particle; there is still no interaction force between particles here. ...