With or without magnetic field.

LagrangeEuler
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1d Ising model without magnetic field has hamiltonian ##H=-J\sum^{N-1}_{i=1}S_iS_{i+1}## with no boundary condition has partition function ##Z_N=2^{N}\cosh^{N-1}(\beta J)##. In this model with magnetic field people often put into the game circular boundary condition because then they could solve problem using transfer matrix method. Is there any easy way to solve 1d Ising model without boundary condition in extern magnetic field. Hamiltonian of that model would be ##H=-J\sum^{N-1}_{i=1}S_iS_{i+1}-B\sum^{N}_{i=1}S_i##.
 
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There is no problem to apply the transfer matrix method in the case of other boundary conditions. Just try it out.
 
I tried, problem is with ##Z=\sum_{allposibilities}\langle S_1|\hat{T}|S_2 \rangle \langle S_2|\hat{T}|S_3 \rangle...\langle S_N|\hat{T}|S_1 \rangle=\sum_{S_1}\langle S_1 |\hat{T}^{N}|S_1 \rangle=Tr(\hat{T}^{N})##
I can't get trace in case without circular boundary condition.
 
LagrangeEuler said:
I can't get trace in case without circular boundary condition.
So what? The term <S_1|T|S_N> is missing. Ok.
You get \sum_{S_1} \sum_{S_N} \langle S_1| T^{N-1} |S_N\rangle.
What happens when you decompose |S_1/N> into eigenfunctions of T?
 
I'm not quite sure what you think? One eigenvector is just ##|+1\rangle##.
 
\hat{T}= \left( \begin{array}{cc}<br /> \langle +|\hat{T}|+ \rangle &amp; \langle +|\hat{T}|- \rangle \\<br /> \langle -|\hat{T}|+ \rangle &amp; \langle -|\hat{T}|- \rangle \end{array} \right)
For ##|S_1/_N\rangle## there are two possibilities ##|+\rangle## or ##|-\rangle##.
But I don't know how to write that in some normal way and calculate.
 
That's a 2x2 matrix in the basis of the two states |+> and |->. I suppose you know how to find the eigenvectors of a 2x2 matrix?
 
Yes. For matrix
\left( \begin{array}{ccc}<br /> e^{j+h} &amp; e^{-j} \\<br /> e^{-j} &amp; e^{j-h} <br /> \end{array} \right)
eigenvectors are
\left( \begin{array}{ccc}<br /> \frac{1}{2}e^{-h}(-e^{2j}+e^{2h+2j}\pm \sqrt{4e^{2h}+e^{4j}-2e^{2h+4j}+e^{4h+4j}}) \\<br /> 1<br /> \end{array} \right)
 
What I meant is that you can write
U^T T U=\Lambda with \Lambda being a diagonal matrix of the eigenvalues \lambda_1 and \lambda_2. I assume \lambda_1&gt;\lambda_2 and call V_0 the matrix V with j=0.
Hence Z=Tr(V^{N-1}V_0)=Tr(U^T\Lambda^{N-1}UV_0)=Tr(\Lambda^{N-1} UV_0U^T)\approx<br /> \lambda_1^{N-1} (UV_0U^T)_{11}.
Hence Z differs from the Z for periodic boundary conditions only by the factor (UV_0U^T)_{11}/\lambda_1. As we are only interested in Log Z, this makes a term which is 1/N times smaller than Z. This is of the same order as the error resulting from the replacement of \Lambda^{N-1} by \lambda_1^{N-1}.
 
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