accepted \titou changes
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@ -331,14 +331,14 @@ Expanding the wave function and energy as power series in $\lambda$ as
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\end{align}
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\end{subequations}
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and solving the corresponding perturbation equations up to a given order $k$, then
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yields approximate solutions to Eq.~\eqref{eq:SchrEq} \titou{by setting $\lambda = 1$}.
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yields approximate solutions to Eq.~\eqref{eq:SchrEq} by setting $\lambda = 1$.
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% MATHEMATICAL REPRESENTATION
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Mathematically, Eq.~\eqref{eq:E_expansion} corresponds to a Taylor series expansion of the exact energy
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around the reference system $\lambda = 0$.
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The energy of the target ``physical'' system is then recovered at the point $\lambda = 1$.
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However, like all series expansions, the Eq.~\eqref{eq:E_expansion} has a radius of convergence $\rc$.
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When $\rc \titou{\le} 1$, the Rayleigh--Sch\"{r}odinger expansion will diverge
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When $\rc \le 1$, the Rayleigh--Sch\"{r}odinger expansion will diverge
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for the physical system.
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The value of $\rc$ can vary significantly between different systems and strongly depends on the particular decomposition
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of the reference and perturbation Hamiltonians in Eq.~\eqref{eq:SchrEq-PT}.\cite{Mihalka_2017b}
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@ -377,7 +377,7 @@ We will demonstrate how the choice of reference Hamiltonian controls the positio
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ultimately determines the convergence properties of the perturbation series.
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\titou{Practically, to locate EPs in a more complicated systems, one must solve simultaneously the following equations:\cite{Cejnar_2007}
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Practically, to locate EPs in a more complicated systems, one must simultaneously solve\cite{Cejnar_2007}
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\begin{subequations}
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\begin{align}
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\label{eq:PolChar}
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@ -388,9 +388,11 @@ ultimately determines the convergence properties of the perturbation series.
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\end{align}
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\end{subequations}
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where $\hI$ is the identity operator.
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Equation \eqref{eq:PolChar} is the well-known secular equation providing us with the (eigen)energies of the system.
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If an energy is also solution of Eq.~\eqref{eq:DPolChar}, then this energy value is, at least, two-fold degenerate.
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These degeneracies can be conical intersections between two states with different symmetries for real values of $\lambda$ \cite{Yarkony_1996} or EPs between two states with the same symmetry for complex values of $\lambda$.}
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Equation \eqref{eq:PolChar} is the well-known secular equation providing the (eigen)energies of the system.
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If the energy is also solution of Eq.~\eqref{eq:DPolChar}, then this energy value is at least two-fold degenerate.
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These degeneracies can be conical intersections between two states with different symmetries
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for real values of $\lambda$\cite{Yarkony_1996} or EPs between two states with the
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same symmetry for complex values of $\lambda$.
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%============================================================%
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