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# Line 44 | Line 44 | Sum. I. Taylor-shifted and Gradient-shifted electrosta
44   %\preprint{AIP/123-QED}
45  
46   \title{Real space alternatives to the Ewald
47 < Sum. I. Taylor-shifted and Gradient-shifted electrostatics for multipoles}
47 > Sum. I. Shifted electrostatics for multipoles}
48  
49   \author{Madan Lamichhane}
50   \affiliation{Department of Physics, University
# Line 1446 | Line 1446 | and the damping parameter, $\alpha$ in Figs.  \ref{fig
1446   self-neutralization schemes, the primary quantity of interest is the
1447   analytic energy constant for the perfect arrays.  Convergence to these
1448   constants are shown as a function of both the cutoff radius, $r_c$,
1449 < and the damping parameter, $\alpha$ in Figs.  \ref{fig:Dipoles_rCut}
1449 > and the damping parameter, $\alpha$ in Figs.\ref{fig:Dipoles_rCut}
1450   and \ref{fig:Dipoles_alpha}. We have simultaneously tested a hard
1451   cutoff (where the kernel is simply truncated at the cutoff radius), as
1452   well as a shifted potential (SP) form which includes a
# Line 1454 | Line 1454 | The Hard cutoff exhibits oscillations around the analy
1454   forces and torques smoothly at the cutoff radius.  The SP method is
1455   essentially an extension of the original Wolf method for multipoles.
1456  
1457 < The Hard cutoff exhibits oscillations around the analytic energy
1457 > The hard cutoff exhibits oscillations around the analytic energy
1458   constants, and converges to incorrect energies when the complementary
1459   error function damping kernel is used.  The shifted potential (SP) and
1460   gradient-shifted force (GSF) approximations converge to the correct
1461 < energy smoothly by $r_c / 6 a$ even for the undamped case.  This
1461 > energy smoothly by $r_c = 6 a$ even for the undamped case.  This
1462   indicates that the correction provided by the self term is required
1463   for obtaining accurate energies.  The Taylor-shifted force (TSF)
1464   approximation appears to perturb the potential too much inside the
1465   cutoff region to provide accurate measures of the energy constants.
1466 +
1467   {\it Quadrupolar} analogues to the Madelung constants were first
1468   worked out by Nagai and Nakamura who computed the energies of selected
1469   quadrupole arrays based on extensions to the Luttinger and Tisza
1470 < approach.\cite{Nagai01081960,Nagai01091963} We have compared the
1470 < energy constants for the lowest energy configurations for linear
1471 < quadrupoles.  
1470 > approach.\cite{Nagai01081960,Nagai01091963}
1471  
1472   In analogy to the dipolar arrays, the total electrostatic energy for
1473   the quadrupolar arrays is:
# Line 1484 | Line 1483 | the effective moment, $\bar{Q}^2 = \frac{2}{3} \Theta
1483   (For the traceless quadrupole tensor, $\Theta = 3 Q - \text{Tr} Q$,
1484   the effective moment, $\bar{Q}^2 = \frac{2}{3} \Theta : \Theta$.)
1485  
1486 + To test the new electrostatic methods for quadrupoles, we have
1487 + constructed very large, $N=$ 8,000~(sc), 16,000~(bcc), and
1488 + 32,000~(fcc) arrays of linear quadrupoles in the orientations
1489 + described in Ref. \onlinecite{Nagai01081960}.  We have compared the
1490 + energy constants for the lowest energy configurations for these linear
1491 + quadrupoles. Convergence to these constants are shown as a function
1492 + of both the cutoff radius, $r_c$, and the damping parameter, $\alpha$
1493 + in Figs.~\ref{fig:Quadrupoles_rCut} and \ref{fig:Quadrupoles_alpha}.
1494 +
1495   \begin{figure}
1496   \includegraphics[width=\linewidth]{Quadrupoles_rcutConvergence.pdf}
1497   \caption{Convergence of the lattice energy constants as a function of
# Line 1493 | Line 1501 | the effective moment, $\bar{Q}^2 = \frac{2}{3} \Theta
1501    are indicated with grey dashed lines.  The left panel shows results
1502    for the undamped kernel ($1/r$), while the damped error function
1503    kernel, $B_0(r)$ was used in the right panel.}
1504 < \label{fig:QuadrupolesrcutCovergence}
1504 > \label{fig:Quadrupoles_rCut}
1505   \end{figure}
1506  
1507  
1508   \begin{figure}[!htbp]  
1509 < \includegraphics[width=3.5in]{Quadrupoles_alphaConvergence-crop.pdf}
1510 < \caption{Convergence to the analytic energy constants as a function of
1511 <  cutoff damping alpha for the different
1512 <  real-space methods for (a) dipolar and (b) quadrupolar crystals.The energy constants for hard, SP, GSF, TSF, and analytic methods are represented by the black sold-circle, red solid-square, green solid-diamond, and grey dashed line respectively.
1513 < The left panel shows results for the undamped kernel ($1/r$), while the damped
1514 <  error function kernel, $B_0(r)$ was used in the right panel. }
1515 < \label{fig:Quadrupoles_alphaCovergence-crop.pdf}
1509 > \includegraphics[width=\linewidth]{Quadrupoles_newAlpha.pdf}
1510 > \caption{Convergence to the lattice energy constants as a function of
1511 >  the reduced damping parameter ($\alpha^* = \alpha a$) for the
1512 >  different real-space methods in the same three quadrupolar crystals
1513 >  in Figure \ref{fig:Quadrupoles_rCut}.  The left panel shows
1514 >  results for a relatively small cutoff radius ($r_c = 4.5 a$) while a
1515 >  larger cutoff radius ($r_c = 6 a$) was used in the right panel.  }
1516 > \label{fig:Quadrupoles_alpha}
1517   \end{figure}
1518  
1519 + Again, we find that the hard cutoff exhibits oscillations around the
1520 + analytic energy constants.  The shifted potential (SP) and
1521 + gradient-shifted force (GSF) approximations converge to the correct
1522 + energy smoothly by $r_c = 4 a$ even for the undamped case.  The
1523 + Taylor-shifted force (TSF) approximation again appears to perturb the
1524 + potential too much inside the cutoff region to provide accurate
1525 + measures of the energy constants.
1526  
1527 +
1528   \section{Conclusion}
1529 < We have presented two efficient real-space methods for computing the
1529 > We have presented three efficient real-space methods for computing the
1530   interactions between point multipoles.  These methods have the benefit
1531   of smoothly truncating the energies, forces, and torques at the cutoff
1532   radius, making them attractive for both molecular dynamics (MD) and
# Line 1517 | Line 1534 | provide accurate convergence to lattice energies.  
1534   (GSF) and the Shifted-Potential (SP) methods converge rapidly to the
1535   correct lattice energies for ordered dipolar and quadrupolar arrays,
1536   while the Taylor-Shifted Force (TSF) is too severe an approximation to
1537 < provide accurate convergence to lattice energies.  
1537 > provide accurate convergence to lattice energies.
1538  
1539   In most cases, GSF can obtain nearly quantitative agreement with the
1540   lattice energy constants with reasonably small cutoff radii.  The only

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