Which property of reversible linear evolution preserves total probability for every normalized initial state?
For a closed system with time-independent, self-adjoint H, which operator evolves its state from zero to t? Keep hbar explicit.
In the Heisenberg picture, the state stays at its initial value and observables carry the evolution-related time dependence.
Circle one: True False
H|0>=0 and H|1>=Δ|1>, with orthonormal states. Initially psi0=(|0>+3|1>)/sqrt(10). At Δt/hbar=pi, what is U(t)psi0?
A normalized superposition evolves under time-independent H. Which statement holds in a fixed orthonormal energy eigenbasis?
For arbitrary unitary U and observable A in a finite-dimensional system, psi_S=U psi0. Which expression always equals <psi_S|A|psi_S> in the Heisenberg picture?
H is time independent. A finite-dimensional observable A has no explicit time dependence and [H,A]=0. What follows in the Heisenberg picture?
H|0>=0 and H|1>=epsilon|1>, with orthonormal states. Initially psi0=|+>=(|0>+|1>)/sqrt(2). At epsilon t/hbar=pi, a student adds the energy probabilities and reports P(+)=1. What is P(+)?