goign through Hugh stuff and starting working on HF
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@ -101,10 +101,12 @@
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\newcommand{\bbR}{\mathbb{R}}
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\newcommand{\bbC}{\mathbb{C}}
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\newcommand{\Lup}{\text{L}^{\uparrow}}
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\newcommand{\Ldown}{\text{L}^{\downarrow}}
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\newcommand{\Rup}{\text{R}^{\uparrow}}
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\newcommand{\Rdown}{\text{R}^{\downarrow}}
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\newcommand{\Lup}{\mathcal{L}^{\uparrow}}
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\newcommand{\Ldown}{\mathcal{L}^{\downarrow}}
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\newcommand{\Lsi}{\mathcal{L}^{\sigma}}
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\newcommand{\Rup}{\mathcal{R}^{\uparrow}}
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\newcommand{\Rdown}{\mathcal{R}^{\downarrow}}
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\newcommand{\Rsi}{\mathcal{R}^{\sigma}}
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\newcommand{\LCPQ}{Laboratoire de Chimie et Physique Quantiques (UMR 5626), Universit\'e de Toulouse, CNRS, UPS, France.}
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@ -189,38 +191,32 @@ More importantly here, although EPs usually lie off the real axis, these singula
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\subcaption{\label{subfig:FCI_cplx}}
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\end{subfigure}
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\caption{%
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\hugh{Exact energies for the Hubbard dimer ($U=4t$) as functions of $\lambda$ on the real axis (\subref{subfig:FCI_real}) and in the complex plane (\subref{subfig:FCI_cplx}).
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Only the interacting closed-shell singlets are plotted in the complex plane, becoming degenerate at the EP (black dot).}
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Exact energies for the Hubbard dimer ($U=4t$) as functions of $\lambda$ on the real axis (\subref{subfig:FCI_real}) and in the complex plane (\subref{subfig:FCI_cplx}).
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Only the interacting closed-shell singlets are plotted in the complex plane, becoming degenerate at the EP (black dot).
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\label{fig:FCI}}
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\end{figure*}
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\hugh{To illustrate the concepts discussed throughout this article, we will consider the symmetric Hubbard dimer at half filling, \ie\ with two opposite-spin fermions.
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Using the localised Wannier basis, the Hilbert space for this system comprises the four configurations
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\begin{equation}
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\ket{\Lup \Ldown} \qquad \ket{\Lup\Rdown} \qquad \ket{\Rup\Ldown} \qquad \ket{\Rup\Rdown}
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\end{equation}
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%\begin{tabularx}{\linewidth}{YYYY}
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%$\ket{\Lup \Ldown}$ & $\ket{\Lup\Rdown}$ & $\ket{\Rup\Ldown}$ & $\ket{\Rup\Rdown}$
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%\\
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%$\uddot \quad \vac$ & $\updot \quad \dwdot$ & $\dwdot \quad \updot$ & $\vac \quad \uddot$
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%\end{tabularx}
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where $\text{L}^{\sigma}$ ($\text{R}^{\sigma}$) denotes an electron with spin $\sigma$ on the left (right) site.
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To illustrate the concepts discussed throughout this article, we will consider the symmetric Hubbard dimer at half filling, \ie\ with two opposite-spin fermions.
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Using the localised site basis, the Hilbert space for this system comprises the four configurations
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\begin{align}
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& \ket{\Lup \Ldown} & & \ket{\Lup\Rdown} & & \ket{\Rup\Ldown} & & \ket{\Rup\Rdown}
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\end{align}
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where $\Lsi$ ($\Rsi$) denotes an electron with spin $\sigma$ on the left (right) site.
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The exact Hamiltonian is then
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\begin{equation}
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\label{eq:H_FCI}
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\bH =
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\begin{pmatrix}
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U & - t & - t & 0 \\
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U & - t & + t & 0 \\
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- t & 0 & 0 & - t \\
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- t & 0 & 0 & - t \\
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0 & - t & - t & U \\
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+ t & 0 & 0 & + t \\
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0 & - t & + t & U \\
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\end{pmatrix},
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\end{equation}
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where $t$ is the hopping parameter and $U$ is the on-site Coulomb repulsion.}
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where $t$ is the hopping parameter and $U$ is the on-site Coulomb repulsion.
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We refer the interested reader to Refs.~\onlinecite{Carrascal_2015,Carrascal_2018} for more details about this system.
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\hugh{%
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To illustrate the formation of an exceptional points, we scale the off-diagonal coupling strength by introducing the complex parameter $\lambda$ through the transformation $t\rightarrow \lambda t$.
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When $\lambda$ is real, the Hamiltonian~\eqref{eq:H_FCI} is Hermitian with the distinct (real-valued) eigenvalues
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\begin{subequations}
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@ -233,10 +229,10 @@ E_{\text{T}} &= 0,
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E_{\text{S}} &= U.
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\end{align}
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\end{subequations}
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While the open-shell triplet ($E_{\text{T}}$) and singlet ($E_{\text{S}}$) are independent of $\lambda$, the closed-shell singlet ground state ($E_{-}$) and doubly-excited state ($E_{+}$) couple strongly to form an avoided crossing at $\lambda=0$ (see Figure~\ref{subfig:FCI_real}).
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While the open-shell triplet ($E_{\text{T}}$) and singlet ($E_{\text{S}}$) are independent of $\lambda$, the closed-shell singlet ground state ($E_{-}$) and doubly-excited state ($E_{+}$) couple strongly to form an avoided crossing at $\lambda=0$ (see Fig.~\ref{subfig:FCI_real}).
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At non-zero values of $U$ and $t$, these closed-shell singlets can only become degenerate at a pair of complex conjugate points in the complex $\lambda$ plane
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\begin{equation}
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\lambda_{\text{EP}} = \pm \frac{U}{4t} \i,
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\lambda_{\text{EP}} = \pm \i \frac{U}{4t},
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\end{equation}
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with energy
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\begin{equation}
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@ -247,9 +243,7 @@ These $\lambda$ values correspond to so-called EPs and connect the ground and ex
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Crucially, the energy surface becomes non-analytic at $\lambda_{\text{EP}}$ and a square-root singularity forms with two branch cuts running along the imaginary axis from $\lambda_{\text{EP}}$ to $\pm \i \infty$ (see Fig.~\ref{subfig:FCI_cplx}).
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On the real $\lambda$ axis, these EPs lead to the singlet avoided crossing at $\lambda = \Re(\lambda_{\text{EP}})$.
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The ``shape'' of this avoided crossing is related to the magnitude of $\Im(\lambda_{\text{EP}})$, with smaller values giving a ``sharper'' interaction.
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}
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\hugh{
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Remarkably, the existence of these square-root singularities means that following a complex contour around an EP in the complex $\lambda$ plane will interconvert the closed-shell ground and excited states.
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This behaviour can be seen by expanding the radicand in Eq.~\eqref{eq:singletE} as a Taylor series around $\lambda_{\text{EP}}$ to give
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\begin{equation}
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@ -259,7 +253,7 @@ Parametrising the complex contour as $\lambda(\theta) = \lambda_{\text{EP}} + R
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\begin{equation}
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E_{\pm} \qty(\theta) \approx E_{\text{EP}} \pm \sqrt{32t^2 \lambda_{\text{EP}} R}\, \exp(\i \theta/2)
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\end{equation}
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such that}
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such that
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\begin{align}
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E_{\pm}(2\pi) & = E_{\mp}(0),
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&
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@ -394,13 +388,28 @@ is the HF mean-field potential with
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\begin{subequations}
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\begin{gather}
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\label{eq:CoulOp}
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J_i(\vb{x})\phi_p(\vb{x})=\qty[\int\dd\vb{x}'\phi_i(\vb{x}')\frac{1}{\abs{\vb{r} - \vb{r}'}}\phi_i(\vb{x}') ] \phi_p(\vb{x})
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J_i(\vb{x})\phi_p(\vb{x})=\qty[\int \phi_i(\vb{x}')\frac{1}{\abs{\vb{r} - \vb{r}'}}\phi_i(\vb{x}') \dd\vb{x}' ] \phi_p(\vb{x})
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\\
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\label{eq:ExcOp}
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K_i(\vb{x})\phi_p(\vb{x})=\qty[\int\dd\vb{x}'\phi_i(\vb{x}')\frac{1}{\abs{\vb{r} - \vb{r}'}}\phi_p(\vb{x}') ] \phi_i(\vb{x})
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K_i(\vb{x})\phi_p(\vb{x})=\qty[\int \phi_i(\vb{x}')\frac{1}{\abs{\vb{r} - \vb{r}'}}\phi_p(\vb{x}') \dd\vb{x}'] \phi_i(\vb{x})
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\end{gather}
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\end{subequations}
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being the Coulomb and exchange operators (respectively) in the spin-orbital basis. \cite{SzaboBook}
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The HF energy is then defined as
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\begin{equation}
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\label{eq:E_HF}
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E_\text{HF} = \sum_i h_i + \frac{1}{2} \sum_{ij} \qty( J_{ij} - K_{ij} )
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\end{equation}
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with
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\begin{subequations}
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\begin{gather}
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h_i = \int \phi_i(\vb{x}) h(\vb{x}) \phi_i(\vb{x}) \dd\vb{x}
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\\
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J_{ij} = \int \phi_i(\vb{x}) J_j(\vb{x}) \phi_i(\vb{x}) \dd\vb{x}
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\\
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K_{ij} = \int \phi_i(\vb{x}) K_j(\vb{x}) \phi_i(\vb{x}) \dd\vb{x}
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\end{gather}
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\end{subequations}
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If the spatial part of the spin-orbitals are restricted to be the same for spin-up and spin-down electrons, one talks about restricted HF (RHF) theory, whereas if one does not enforce this constrain it leads to the so-called unrestricted HF (UHF) theory.
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From hereon, $i$ and $j$ are occupied orbitals, $a$ and $b$ are unoccupied (or virtual) orbitals, while $p$, $q$, $r$, and $s$ indicate arbitrary orbitals.
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@ -409,17 +418,17 @@ Rather than solving Eq.~\eqref{eq:SchrEq}, HF theory uses the variational princi
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\hH^{\text{HF}} = \sum_{i} f(\vb{x}_i).
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\end{equation}
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Coming back to the Hubbard dimer, the HF energy is
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Coming back to the Hubbard dimer, the HF energy is [see Eq.~\eqref{eq:E_HF}]
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\begin{equation}
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E_\text{HF} = -t \qty[ \sin \theta_\alpha + \sin \theta_\beta ] + \frac{U}{2} \qty[ 1 + \cos \theta_\alpha \cos \theta_\beta ]
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\end{equation}
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where
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\begin{align}
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\psi_{1\sigma} & = \cos(\frac{\theta_\sigma}{2}) s_1 - \sin(\frac{\theta_\sigma}{2})s_2
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\psi_{1\sigma} & = \cos(\frac{\theta_\sigma}{2}) \Lsi - \sin(\frac{\theta_\sigma}{2}) \Rsi
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\\
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\psi_{2\sigma} & = \sin(\frac{\theta_\sigma}{2}) s_1 + \cos(\frac{\theta_\sigma}{2})s_2
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\psi_{2\sigma} & = \sin(\frac{\theta_\sigma}{2}) \Lsi + \cos(\frac{\theta_\sigma}{2}) \Rsi
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\end{align}
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are the one-electron molecule orbitals for the spin-$\sigma$ electrons and the angles which makes the energy stationnary, \ie, $\pdv*{E_\text{HF}}{\theta_\sigma} = 0$ are given by
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\begin{align}
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\theta_\alpha & = \arctan (-\frac{\sqrt{U^2 - 4t^2}}{U},\frac{2t}{U})
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\\
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