How Does the Hamiltonian Affect the Time Evolution of a Qubit's Density Matrix?

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SUMMARY

The discussion focuses on the time evolution of a qubit's density matrix, specifically when the Hamiltonian is expressed as ##AI + BY##, where ##A## and ##B## are constants, and ##Y## is the Pauli matrix ##\left( \begin{array}{cc} 0 & -i \\ i & 0 \end{array} \right)##. The initial density matrix is given as ##\rho = \left( \begin{array}{cc} \frac{1}{2} & \frac{1}{3} \\ \frac{1}{3} & \frac{1}{2} \end{array} \right)##. The discussion suggests rewriting the density matrix in the form ##\rho = \frac{1}{2} (I + a(t)X + b(t)Y + c(t)Z)## to derive differential equations for the coefficients ##a(t)##, ##b(t)##, and ##c(t)##. The time evolution operator ##U(t,t_0) = e^{-\frac{i}{\hbar}H(t-t_0)}## is also highlighted as a key component in calculating ##\rho(t) = U\rho(t_0) U^{\dagger}##.

PREREQUISITES
  • Understanding of quantum mechanics concepts, particularly qubits and density matrices.
  • Familiarity with Hamiltonians in quantum systems.
  • Knowledge of Pauli matrices and their applications in quantum mechanics.
  • Proficiency in matrix exponentiation and Taylor series expansions.
NEXT STEPS
  • Study the derivation of the time evolution operator in quantum mechanics.
  • Learn about the Schrödinger equation and its application to density matrices.
  • Explore the properties and applications of Pauli matrices in quantum computing.
  • Investigate the implications of Hamiltonians on quantum state evolution.
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Quantum physicists, students studying quantum mechanics, and researchers working on quantum computing and information theory will benefit from this discussion.

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Homework Statement


In a computational basis, a qubit has density matrix
##
\rho = \left( \begin{array}{ccc}
\frac{1}{2} & \frac{1}{3} \\
\frac{1}{3} & \frac{1}{2} \\
\end{array} \right)##
At t=0. Find the time dependence of ##\rho## when the Hamiltonian is given by ##AI+BY##, ##A## and ##B## are constants, ##Y## is the Pauli matrix
##
\left( \begin{array}{ccc}
0 & -i \\
i & 0 \\
\end{array} \right)##
Then the hint says to write the matrix in the form ##\rho = \frac{1}{2} (I+a(t)X+b(t)Y+c(t)Z)## where
## X=
\left( \begin{array}{ccc}
0 & 1 \\
1 & 0 \\
\end{array} \right)##,
##Z=
\left( \begin{array}{ccc}
1 & 0 \\
0 & -1 \\
\end{array} \right)##
and derive differential equations for the coefficients.

Homework Equations

The Attempt at a Solution


I thought I should be using the time shift operator ##U(t,t_0) = e^{-\frac{i}{\hbar}H(t-t_0)}##, and calculating ##\rho(t) = U\rho(t_0) U^{\dagger}##, except I'm not exactly sure what the exponential of my particular Hamiltonian would mean. But if I write the density matrix in the form suggested by the hint then I don't know what to do with it from there to get a differential equation. Is it something to do with the Schrödinger equation? Should I sub it into that and treat it like a state ##\psi##?

Thank you for any help, I really appreciate it, I'm a bit lost!
 
Physics news on Phys.org
The exponential of the Hamiltonian (in this given in matrix form) is defined by its Taylor expansion. That is,
##exp(A)=\sum_{k=0}^\infty A^k/k!## for a matrix ##A##
 

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