Using the time evolution operator

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The discussion centers on the application of the time evolution operator in a 2D Hilbert space using the Pauli matrix in the y-direction as the Hamiltonian. The eigenvectors of the Hamiltonian are expressed as |±>_y, which are linear combinations of the orthonormal basis e1 and e2. The time evolution operator is applied to these eigenvectors, leading to an expression involving an exponential function. The simplification occurs because the eigenvalues of the Pauli matrix σ_y are ±1, allowing for a straightforward reduction of the expression. This clarification helps in understanding the relationship between the eigenvalues and the time evolution of the system.
ian2012
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I hope someone can help me out here,

I am confused with a line of text I read - it is an example of a 2D Hilbert space with orthonormal basis e1, e2. The Hamiltonian of the system is the Pauli matrix in the y-direction. Given by the matrix:

\sigma_{y} = (\frac{0, -i}{i, 0})

The eigenvectors of the Hamiltonian are given by:

| \pm >_{y}= \frac{1}{\sqrt{2}}(| e_{1} > \pm i|e_{2}>)

So, applying the time evolution operator to the eigenvectors gives:

U| \pm >_{y}=exp(\frac{-i(t-t_{0}) \sigma_{y}}{\hbar})| \pm >_{y}
U| \pm >_{y}=exp(\frac{\mp i(t-t_{0})}{\hbar})| \pm >_{y}

I don't understand how the last line came about?
 
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The last line follows because the eigenvalues of \sigma_y are +/- 1.
 
Oh right, of course, so it let's you simplify the expression.
 
Time reversal invariant Hamiltonians must satisfy ##[H,\Theta]=0## where ##\Theta## is time reversal operator. However, in some texts (for example see Many-body Quantum Theory in Condensed Matter Physics an introduction, HENRIK BRUUS and KARSTEN FLENSBERG, Corrected version: 14 January 2016, section 7.1.4) the time reversal invariant condition is introduced as ##H=H^*##. How these two conditions are identical?

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