Franz J. Vesely > Square Well Lines
 
 





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The Square Well Lines (SWL) model



Consider two lines of finite length $L = 2h$ containing a homogeneous density of square well centers. Let $\vec{r}_{1,2}$ and $\vec{e}_{1,2}$ be the position and direction vectors, respectively, of the two line centers, and write $\vec{r}_{12}$ for the vector between the centers; let $\lambda, \, \mu$ be the parameters giving the positions of the interacting points along $1$ and $2$. The squared distance between any two such points is given by $r^{2}= \left | r_{12}+\mu \cdot \vec{e}_{2}-\lambda \cdot \vec{e}_{1} \right|^{2} $. The total interaction energy between the two lines is then

$ u(1,2) \equiv u(\vec{r}_{12},\vec{e}_{1},\vec{e}_{2}) = \frac{\textstyle 1}{\textstyle L^{2}} \int \limits_{\textstyle -h}^{\textstyle h} d \lambda \int \limits_{\textstyle -h}^{\textstyle h} d \mu \, \, u_{SW}\left[ r(\lambda,\mu) \right] $

with $u_{SW}(r)= \infty $ if $r < s_{1}$, $= - \varepsilon $ if $s_{1} < r < s_{2}$, and $=0$ for $r > s_{2}$. Typically, $s_{1}=1.0$ and $s_{2}=1.5 - 2.0$. The elementary distance $r(\lambda,\mu)$ is $r^{2}= \lambda^{2}+\mu^{2} + 2 \mu b - 2 \lambda c - 2 \lambda \mu d + r_{12}^{2}$, where $b=\vec{r}_{12} \cdot \vec{e}_{2}$, $c=\vec{r}_{12} \cdot \vec{e}_{1}$, and $d=\vec{e}_{1} \cdot \vec{e}_{2}$. Note that we can always enforce $d > 0$ by simply turning $\vec{e}_{2}$ around; all parameters remain the same, except $b$ which changes sign.

In the $(\lambda, \mu )$ plane the integration region is represented by a square $S$ of side length $L$ around $(0,0)$. However, the integrand is non-zero, and constant, only for $ r^{2}(\lambda, \mu ) < s_{2}^{2}$. In other words, the integral gives the area shared by the square $S$ and an ellipse $E$ described by $\lambda^{2}+\mu^{2} + 2 \mu b - 2 \lambda c - 2 \lambda \mu d - a^{2} =0$ where $a^{2}=s_{2}^{2}-r_{12}^{2}$.

The potential between two SWL particles is given by the area of the overlap region between the square $S: \{ \lambda, \mu \, \epsilon \, [-h,h] \}$ and the ellipse $E: \lambda^{2}+\mu^{2} + 2 \mu b - 2 \lambda c - 2 \lambda \mu d - a^{2}=0$.


Since this overlap region must be within the smallest rectangle $R$ containing the ellipse, only the - generally rectangular - section $S \cap R$ needs to be considered; see Fig. 1.





Figure 1: Square well lines in 2D: $L=2$, $s_{2}=1.5$. The inset shows the configuration represented in the $\lambda, \mu$ plane. The potential is given by the overlap area of square and ellipse. The figure refers to the pair $\vec{r}_{12} = (0.1 | 1.4), \vec{e}_{1} = (1 | 0), \vec{e}_{2} = (0.95 | 0.312)$; the potential is $u=-1.5822/4= -0.39566$; numerical integration yields $-0.39554$.

2 or 3 dimensions?
We have not made any reference to the dimension in which the SW lines reside, even if Fig. 1 shows a 2D example. In fact, the procedure of calculating the pair potential is the same for coplanar (2D) and skew (3D) lines.

Here is a lengthy explanation how to compute the potential
A short recipe follows below.

The task of computing the common area of an ellipse and a rectangle may seem trivial, but we have to define a procedure that comprises all possible configurations of the interacting sticks, and thus of $E$ and $R$.

First we make sure that the SW particles have no overlap, i.e. contain no points with a mutual distance below $s_{1}$. In other words, the rectangle must not intersect the smaller concentric ellipse. A proven method for assessing the minimum distance btw two sticks is due to Allen et al., Adv. Chem. Phys. Vol. LXXXVI, 1993, p.1.; see also here.

Next, we find the points of minimum distance along the two carrier lines. (For coplanar lines these points coincide in the intersection, if any, of the two lines.) Assuming that the lines are not parallel, i.e. $d^{2} \neq 1$, these "proxy points" have the line parameters $\lambda_{0} = (c-bd)/(1-d^{2})$, $\mu_{0}=(cd-b)/(1-d^{2})$. If $d^{2}=1$, the sticks may be either in an end-to-end configuration, meaning that the carrier lines 1 and 2 are identical, or they are on parallel lines. In both such cases the parameters $\lambda_{0},\mu_{0},$ cannot, and need not, be calculated (see below.)

Since $d \equiv \vec{e}_{1} \cdot \vec{e}_{2} \geq 0$ the long axis of the ellipse is oriented along the main diagonal. The ellipse center is at
$\lambda_{0} = (c-bd)/(1-d^{2})$ $\mu_{0}=(cd-b)/(1-d^{2})$. Symmetry helps us to bring $E$ into a well-defined position: we require that the center of $E$ be in the lower quadrant, meaning that

if $\lambda_{0} \geq 0$ and $\mu_{0}^{2} \leq \lambda_{0}^{2}$ (right quadrant), let $b \leftrightarrow c$, which makes $(\lambda_{0},\mu_{0}) \rightarrow (-\mu_{0},-\lambda_{0})$
if $\lambda_{0} < 0$ and $\mu_{0}^{2} \leq \lambda_{0}^{2}$ (left quadrant), let $b \rightarrow -c$, $c \rightarrow -b$, making $(\lambda_{0},\mu_{0}) \rightarrow (\mu_{0},\lambda_{0})$
if $\mu_{0} > 0$ and $\lambda_{0}^{2} \leq \mu_{0}^{2}$ (upper quadrant), let $b \rightarrow -b$, $c \rightarrow -c$, resulting in $(\lambda_{0},\mu_{0}) \rightarrow (-\lambda_{0},-\mu_{0})$

The resulting configuration is in the lower quadrant and has the same overlap integral as the given pair.

Note: To avoid the spurious singularity at $d^{2}=1$ we do not compute the full $\lambda_{0}, \mu_{0}$ but only their numerators $c-bd$ and $cd-b$, which is sufficient to determine the quadrant.

For later reference we write the explicit form of $E$ as

$ \mu^{\pm}(\lambda) = \lambda d - b \pm \sqrt{A \lambda^{2} + 2B \lambda +C} $

where $A = - (1-d^{2})$, $B = c-bd$, $C = a^{2}+b^{2}$, and where the signs $\pm$ denote the upper and lower branches, respectively, of the ellipse. Alternatively, $E$ may be written as

$ \lambda^{\pm}(\mu) = \mu d + c \pm \sqrt{F \mu^{2} + 2G \mu +H} $

where $F=A = - (1-d^{2})$, $G = cd-b$, $H = a^{2}+c^{2}$, and where the signs $\pm$ denote the right and left branches, respectively, of the ellipse.

To find the container rectangle $R$ we have to determine the left- and rightmost points $N$ and $P$, as well as the lowest and uppermost points $O$ and $Q$ of the ellipse. Now, since $\lambda_{N,P}= (B \mp \sqrt{B^{2}-AC})/(1-d^{2})$ and $\mu_{O,Q}=(G \mp \sqrt{G^{2}-FH})/(1-d^{2})$ there is again the danger of a singularity. But actually we need the points $N,O,P,Q$ only if they are within the square $S$, and thus finite, meaning that in the case $d^{2}=1$ these points need not be determined at all. All we have to do is compare $\lambda_{P}(1-d^{2})$ to $h(1-d^{2})$, $\mu_{Q} (1-d^{2})$ to $h(1-d^{2})$, and similar for points $N$ and $O$. In this way we find the limits of the container rectangle according to $\lambda_{l}'=\max (-h \, , \, \lambda_{N})$, $\lambda_{u}'=\min (h \, , \, \lambda_{P})$, $\mu_{l}=\max (-h \, , \, \mu_{O})$, $\mu_{u}=\min (h \, , \, \mu_{Q})$.

Actually, the relevant integration limits $\lambda_{l,u}'$ may be reduced even further, which is why we have adorned them with an apostrophe. Consider the intersection points $1$ and $2$ of the lower rectangle side with the ellipse $E$ (see Figure 1.): let $\lambda_{1},\lambda_{2}$ be the left/right intersection of the lower side $\mu=\mu_{l}$ of $S \cap R$ with $E$; if such an intersection point is outside the limits ($\lambda_{l}, \lambda_{u}$), it is placed at the near end of that side:

$ \begin{eqnarray} \lambda_{1,2} &=& \min \left(\lambda_{u}',\max \left( \lambda_{l}',(\mu_{l}d+c) \mp \sqrt{F \mu_{l}^{2}+2G \mu_{l}+H} \right) \right) \end{eqnarray} $

Similarly, we find the intersections between the upper rectangle side and $E$: let $\lambda_{3,4}$ be the left/right intersection of the upper side ($\mu=\mu_{u}$) of $S \cap R$ with $E$; if such an intersection point is outside the limits ($\lambda_{l}, \lambda_{u}$), it is placed at the near end of that side:

$ \begin{eqnarray} \lambda_{3,4}= \min \left(\lambda_{u}',\max \left(\lambda_{l}',(\mu_{u}d+c) \mp \sqrt{F\mu_{u}^{2}+2G\mu_{u}+H} \right) \right) \end{eqnarray} $

Obviously, the portion of $E$ lying between $\lambda_{1}$ and $\lambda_{2}$ has a bottom part that extends below the limits of $R$ and will therefore be cut away. Now, in case $\mu_{l} > \mu_{P}$, with $\mu_{P} (1-d^{2}) = G + d \sqrt{B^{2}-AC}$, the point $2$ is on the upper branch of $E$, meaning that any point right of $2$ is also below $\mu_{l}$ and thus outside the interaction area. In other words, if $\mu_{l} > \mu_{P}$, the rectangle may be clipped down to $\lambda_{u}=\lambda_{2}$. A similar argument holds for point $1$ which may be lower than $\mu_{N} = (G - d \sqrt{B^{2}-AC})/ (1-d^{2})$, thus leading to a new lower integration limit $\lambda_{l}=\lambda_{1}$. Pursuing the same idea for the intersection points $3$ and $4$ of the upper rectangle side with $E$ we finally have

if $\mu_{l} > \mu_{P} \; \Rightarrow \; \lambda_{u}=\lambda_{2}$,    if $\mu_{u} < \mu_{P} \; \Rightarrow \; \lambda_{u}=\lambda_{4}$,
if $\mu_{l} > \mu_{N} \; \Rightarrow \; \lambda_{l}=\lambda_{1}$,    if $\mu_{u} < \mu_{N} \; \Rightarrow \; \lambda_{l}=\lambda_{3}$

which completes the clipping of the container rectangle.

The rest is easy: integrate the ellipse $E$ between the lower and upper limits, then clip off what is sticking out above and below, thus:

$ A = \int \limits_{\textstyle \lambda_{l}}^{\textstyle \lambda_{u}} (\mu^{+}(\lambda)-\mu^{-}(\lambda) ) + \int \limits_{\textstyle \lambda_{1}}^{\textstyle \lambda_{2}} (\mu^{-}(\lambda)-\mu_{l} ) - \int \limits_{\textstyle \lambda_{3}}^{\textstyle \lambda_{4}} (\mu^{+}(\lambda)-\mu_{u} ) \equiv I_{0} + I_{12}^{-} - I_{34}^{+} $


For the individual integrals we have
$ \begin{eqnarray} I_{0} & \equiv & 2 \, \int \limits_{\textstyle \lambda_{l}}^{\textstyle \lambda_{u}} d \lambda \, \sqrt{A \lambda^{2}+2 B \lambda + C } = J_{lu} \\ I_{12}^{-} & \equiv & \int \limits_{\textstyle \lambda_{1}}^{\textstyle \lambda_{2}} d \lambda \, \left[ \left( \lambda d - b - \mu_{l} \right) - \sqrt{A \lambda^{2}+2 B \lambda + C } \right] = \frac{\textstyle d}{\textstyle 2 } \left( \lambda_{2}^{2}-\lambda_{1}^{2} \right) - \left( b + \mu_{l} \right) \left(\lambda_{2}-\lambda_{1} \right) - J_{12} \\ I_{34}^{+} & \equiv & \int \limits_{\textstyle \lambda_{3}}^{\textstyle \lambda_{4}} d \lambda \, \left[ \left( \lambda d - b - \mu_{u} \right) + \sqrt{A \lambda^{2}+2 B \lambda + C } \right] = \frac{\textstyle d}{\textstyle 2 } \left( \lambda_{4}^{2}-\lambda_{3}^{} \right) - \left( b + \mu_{u} \right) \left(\lambda_{4}-\lambda_{3} \right) + J_{34} \\ {\rm with} && \\ J_{ab} & = & \frac{\textstyle 1}{\textstyle 2 A} \left[ \left( A \lambda + B \right) \sqrt{A \lambda^{2}+2 B \lambda + C } + \frac{ \textstyle B^{2} - AC }{\textstyle \sqrt{-A}} \arcsin \frac{\textstyle B + A \lambda}{\sqrt{B^{2}-AC}} \right]_{\textstyle \lambda_{a}}^{\textstyle \lambda_{b}} \end{eqnarray} $


Here is the procedure in short form:

Let $\vec{r}_{1,2}$ and $\vec{e}_{1,2}$ be given, as well as the length $L \equiv 2h$ and the square well limits $s_{1}$ and $s_{2}$.

Make sure that $d \equiv \vec{e}_{1} \cdot \vec{e}_{2} > 0$, if need be by $\vec{e}_{2} \rightarrow -\vec{e}_{2} $. Determine the parameters $b=\vec{r}_{12} \cdot \vec{e}_{2}$, $c=\vec{r}_{12} \cdot \vec{e}_{1}$, and $a^{2}=s_{2}^{2}-r_{12}^{2}$.

We assume that there is no hard body overlap between the two spherocylinders defined by the repulsive part of the SW interaction; this may be ascertained in the usual way, see here.

  • For computational convenience, apply symmetry transformations to move the ellipse center to the lower quadrant of the $\lambda, \mu$ plane:
    if $\lambda_{0} \geq 0$ and $\mu_{0}^{2} \leq \lambda_{0}^{2}$ let $b \leftrightarrow c$
    if $\lambda_{0} < 0$ and $\mu_{0}^{2} \leq \lambda_{0}^{2}$ let $b \rightarrow -c$, $c \rightarrow -b$
    if $\mu_{0} > 0$ and $\lambda_{0}^{2} \leq \mu_{0}^{2}$ let $b \rightarrow -b$, $c \rightarrow -c$

    Using these values of $b$ and $c$ as well as $a^{2}$ as defined before, compute the coefficients of the interaction ellipse, $A = - (1-d^{2})$, $B = c-bd$, $C = a^{2}+b^{2}$, and $F=A = - (1-d^{2})$, $G = cd-b$, $H = a^{2}+c^{2}$.

  • Determine the actual lower and upper rectangle sides $\mu_{l}=\max (-h , \mu_{O})$, $\mu_{u}=\min (h , \mu_{Q})$, where $\mu_{O,Q}=(G \mp \sqrt{G^{2}-FH})/(1-d^{2})$. Also, determine preliminary lower and upper integration limits according to $\lambda_{l}'=\max (-h \, , \, \lambda_{N})$, $\lambda_{u}'=\min (h \, , \, \lambda_{P})$, where $\lambda_{N,P}= (B \mp \sqrt{B^{2}-AC})/(1-d^{2})$. (Note that $\lambda_{N,P}$ and $\mu_{O,Q}$ need to be calculated only if they are within $\pm h$, meaning that the $d^{2} = 1$ singularity does not occur.)

  • Compute the intersection points of the lower/upper rectangle sides with $E$:

    $ \begin{eqnarray} \lambda_{1,2} &=& \min \left(\lambda_{u}',\max \left( \lambda_{l}',(\mu_{l}d+c) \mp \sqrt{F \mu_{l}^{2}+2G \mu_{l}+H} \right) \right) \\ \lambda_{3,4} &=& \min \left(\lambda_{u}',\max \left(\lambda_{l}',(\mu_{u}d+c) \mp \sqrt{F\mu_{u}^{2}+2G\mu_{u}+H} \right) \right) \end{eqnarray} $

    Depending on the relative heights of points $N$ and $P$ with respect to the rectangle bottom and top sides we now find the definitive integration limits:

    if $\mu_{l} > \mu_{P} \; \Rightarrow \; \lambda_{u}=\lambda_{2}$,    if $\mu_{u} < \mu_{P} \; \Rightarrow \; \lambda_{u}=\lambda_{4}$,
    if $\mu_{l} > \mu_{N} \; \Rightarrow \; \lambda_{l}=\lambda_{1}$,    if $\mu_{u} < \mu_{N} \; \Rightarrow \; \lambda_{l}=\lambda_{3}$

    where $\mu_{N,P} (1-d^{2}) = G \mp d \sqrt{B^{2}-AC}$.

  • The potential is then $u=-A \varepsilon/L^{2}$, where the overlap area $A$ is given by

    $ A = \int \limits_{\textstyle \lambda_{l}}^{\textstyle \lambda_{u}} (\mu^{+}(\lambda)-\mu^{-}(\lambda) ) + \int \limits_{\textstyle \lambda_{1}}^{\textstyle \lambda_{2}} (\mu^{-}(\lambda)-\mu_{l} ) - \int \limits_{\textstyle \lambda_{3}}^{\textstyle \lambda_{4}} (\mu^{+}(\lambda)-\mu_{u} ) \equiv I_{0} + I_{12}^{-} - I_{34}^{+} $

    with
    $ \begin{eqnarray} I_{0} & = & 2 \, J_{lu} \; , \;\;\;\;\;\; I_{ij}^{\mp} = \frac{\textstyle d}{\textstyle 2 } \left( \lambda_{j}^{2}-\lambda_{i}^{2} \right) - \left( b + \mu_{l,u} \right) \left(\lambda_{j}-\lambda_{i} \right) \mp J_{ij} \end{eqnarray} $
    where
    $ \begin{eqnarray} J_{ij} & = & \frac{\textstyle 1}{\textstyle 2 A} \left[ \left( A \lambda + B \right) \sqrt{A \lambda^{2}+2 B \lambda + C } + \frac{ \textstyle B^{2} - AC }{\textstyle \sqrt{-A}} \arcsin \frac{\textstyle B + A \lambda}{\sqrt{B^{2}-AC}} \right]_{\textstyle \lambda_{i}}^{\textstyle \lambda_{j}} \end{eqnarray} $




A Java Applet (under construction, apr-09) is here.



Franz Vesely, Jan 21, 2009