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David Strubbe edited Magnetic response.tex
over 9 years ago
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\begin{equation}
\label{eq:magnetic}
\hat{H} = \frac12\left({\hat{\vec{p}}} -\frac1c{\vec{\mathrm{A}}}\right)^2 +
\hat{v} + \vec{\mathrm{B}}\cdot{\hat{\vec{S}}}\ .
\end{equation}
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The first part describes the orbital interaction with the field, and the
...
electronic spin with the magnetic field.
As our main interest is the evaluation of the magnetic susceptibility,
in the
following following, we consider a perturbative uniform static magnetic
field \(\vec{\mathrm{B}}\)
and applied to a finite system with zero total spin. In the Coulomb gauge the
corresponding vector potential, \(\vec{A}\), is given as
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\begin{equation}
...
\sum_n\langle\varphi_n|\delta{\hat{\vec{v}}}^{\mathrm{mag}}|\varphi_{n}\rangle\ .
\end{equation}
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For the susceptibility, we need to calculate the
first order first-order response
functions in the presence of a magnetic field. This can be done in
practice by using the magnetic perturbation, Eq.~(\ref{eq:mag1}), in
the Sternheimer formalism described in
section \ref{sec:sternheimer}.
Since in this case If the system is time-reversal symmetric, since the perturbation is
purely
imaginary, antisymmetric under time-reversal (anti-Hermitian), it does not induce a change
in the density and the Sternheimer equation does not need to be solved
self-consistently. From there
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\begin{multline}
\label{eq:susc}
\chi_{ij} = \sum_k\Big[
\langle{\varphi_n}|\delta\hat{v}^{\mathrm{mag}}_j|{\delta\varphi_{n,i}}\rangle
+\langle{\delta\varphi_{n\,,\,i}}|\delta\hat{v}^{\mathrm{mag}}_j|{\varphi_{n}}\rangle\\ + {\rm cc.}
%+\langle{\delta\varphi_{n\,,\,i}}|\delta\hat{v}^{\mathrm{mag}}_j|{\varphi_{n}}\rangle\\
+\langle{\varphi_n}|\delta^2\hat{v}^{\mathrm{mag}}_{ij}|{\varphi_{n}}\rangle
\Big]\ .
\end{multline}
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the calculated observables. This broken gauge-invariance is well known
in molecular calculations with all-electron methods that make use of
localized basis sets. In this case,
the error can be traced to the
finite basis set finite-basis-set representation of the
wave-functions~\cite{Wolinski_1990,Schindler_1982}. A simple measure of the error
is to check for the fulfillment of the hyper-virial
relation~\cite{Bouman_1977}.