<?xml version="1.0"?>
<!DOCTYPE html SYSTEM "mathml.dtd">
<html xmlns="http://www.w3.org/1999/xhtml"
xmlns:math="http://www.w3.org/1998/Math/MathML"
xmlns:xlink="http://www.w3.org/1999/xlink">
<head>
<meta name="generator" content="HTML Tidy, see www.w3.org" />
<title>University of Pittsburgh: Department of Mathematics</title>
</head>
<body bgcolor="#ffffff" leftmargin="0" marginwidth="0"
topmargin="0" marginheight="0" vlink="#b22222">
<table border="0" cellpadding="0" cellspacing="0" width="600">
<tbody>
<tr>
<td nowrap="nowrap" colspan="3"><img src="../images/bluedot.gif"
width="147" height="4" border="0" alt=" " /><br />
 <img src="../images/bluedot.gif" width="4" height="52"
border="0" /><a href="http://www.pitt.edu"><img
src="../images/pitt_01.gif" width="370" height="52" border="0"
alt="University of Pittsbrugh" /></a><a
href="http://www.pitt.edu"><img src="../images/pitt_02.gif"
width="77" height="52" border="0" alt="Pitt Home | " /></a><a
href="../contact.html"><img src="../images/pitt_03.gif" width="68"
height="52" border="0" alt="Contact Us | " /></a><a
href="http://accounts.pitt.edu/Public/"><img
src="../images/pitt_04.gif" width="85" height="52" border="0"
alt="Finding People | " /><br />
</a> <img src="../images/bluedot.gif" width="147" height="10"
border="0" alt=" " /></td>
</tr>

<tr>
<td width="147" align="Right" bgcolor="#99ccff"><img
src="../images/l2_02.jpg" width="129" height="51" alt=" " /></td>
<td colspan="2"><img src="../images/l2_03.jpg" width="252"
height="51" alt=" " /></td>
</tr>

<tr>
<td width="147" bgcolor="#99ccff" align="Right" valign="Top"><a
href="../index.html"><img src="../images/l2_07.gif" width="129"
height="41" vspace="15" alt="Department of Mathematics"
border="0" /></a><br />
</td>
<td valign="Bottom" width="287"><br />
 <a href="../fall2001.html"><img src="../images/mathzine.gif"
width="167" height="24" hspace="30" border="0" /></a><br />
 <img src="../images/spacer.gif" width="287" height="15"
border="0" /></td>
<td valign="Bottom" nowrap="nowrap" align="Right" width="170"><a
href="../fall2001.html"><font
face="Arial,Helvetica,Geneva,Swiss,SunSans-Regular" size="1"> Table
of Contents<br />
</font></a><br />
<br />
 <b><font face="Arial,Helvetica,Geneva,Swiss,SunSans-Regular"
size="2"> Fall 2001</font></b><br />
 <img src="../images/spacer.gif" width="170" height="15"
border="0" /><br />
</td>
</tr>

<tr>
<td align="Right" bgcolor="#99ccff"><a href="../index.html"> <img
src="../images/l2_09.gif" width="129" height="14" alt="HOME | "
border="0" /></a><br />
 <img src="../images/darkbluedot.gif" width="147" height="1"
border="0" /></td>
<td colspan="2" valign="Bottom"><img
src="../images/darkbluedot.gif" width="457" height="1"
border="0" /></td>
</tr>

<tr>
<td colspan="3" align="Center"><br />
 

<table border="0" cellpadding="3" cellspacing="0" width="100%">
<tbody>
<tr>
<td bgcolor="#003399"><img src="../images/spacer.gif" width="18"
height="8" border="0" /><font face="Verdana,Arial,Helvetica"
size="1" color="white"><b>Cannonballs and Honeycomb:</b> Fejes
Toth<b><br />
</b></font></td>
</tr>

<tr>
<td align="Center">
<table border="0" cellpadding="0" cellspacing="0" width="525">
<tbody>
<tr>
<td>
<p><br />
 <font face="Arial,Helvetica,Geneva,Swiss,SunSans-Regular"> Do
correction terms with the required properties exist? The evidence
suggests that they exist in abundance. The first correction term
was proposed by L. Fejes T\'oth in 1953, but his clusters were much
larger than than those used here. His clusters contain so many
balls that fcc-compatibility has never been established.
Nevertheless, his proposal represents a significance advance,
because it gave the first evidence that the Kepler conjecture could
be solved through an optimization problem in a finite number of
variables. He proposed in 1964 that computers might be used to
determine the minimum. Thus, the general strategy of a proof was
set.</font></p>

<p><font face="Arial,Helvetica,Geneva,Swiss,SunSans-Regular"> The
correction terms <math xmlns='http://www.w3.org/1998/Math/MathML'>
<mi>f</mi>

</math> are based on a careful study of the local
geometry of sphere packings. Fejes T\'oth's correction term <math xmlns='http://www.w3.org/1998/Math/MathML'>
<mi>f</mi>
<mo>(</mo><mi>p</mi><mo>)</mo>
</math>
has the form <math xmlns='http://www.w3.org/1998/Math/MathML' mode='display'>
<mo lspace="thinmathspace" rspace="thinmathspace">&Sum;</mo>
<mi>a</mi><mo>(</mo><mi>p</mi><mo>,</mo><mi>q</mi><mo>)</mo><mi>v</mi><mo>(</mo><mi>q</mi><mo>)</mo><mo>,</mo>
</math> with <math xmlns='http://www.w3.org/1998/Math/MathML'>
<mi>q</mi>

</math> running over all
centers of balls in the cluster <math xmlns='http://www.w3.org/1998/Math/MathML'>
<mi>p</mi>

</math> within a fixed distance of the
center of the cluster. The term <math xmlns='http://www.w3.org/1998/Math/MathML'>
<mi>v</mi>
<mo>(</mo><mi>q</mi><mo>)</mo>
</math> is the volume of a truncated
(a different truncation constant is used in this approach) Voronoi
cell centered at <math xmlns='http://www.w3.org/1998/Math/MathML'>
<mi>q</mi>

</math>. The constants <math xmlns='http://www.w3.org/1998/Math/MathML'>
<mi>a</mi>
<mo>(</mo><mi>p</mi><mo>,</mo><mi>q</mi><mo>)</mo>
</math> sum to zero, <math xmlns='http://www.w3.org/1998/Math/MathML'>
<msub><mo lspace="thinmathspace" rspace="thinmathspace">&Sum;</mo> <mi>q</mi></msub>
<mi>a</mi><mo>(</mo><mi>p</mi><mo>,</mo><mi>q</mi><mo>)</mo><mo>=</mo><mn>0</mn>
</math>, for all clusters <math xmlns='http://www.w3.org/1998/Math/MathML'>
<mi>p</mi>

</math> in a packing. This zero-sum
condition leads to a cancellation of the terms in <math xmlns='http://www.w3.org/1998/Math/MathML'>
<mo lspace="thinmathspace" rspace="thinmathspace">&Sum;</mo>
<mi>f</mi><mo>(</mo><mi>p</mi><mo>)</mo>
</math>, and
hence to the transience of <math xmlns='http://www.w3.org/1998/Math/MathML'>
<mi>f</mi>

</math>. This correction term illustrates
the general correction term strategy: <math xmlns='http://www.w3.org/1998/Math/MathML'>
<mi>f</mi>

</math> is constructed as sums of
volumes that are added at <math xmlns='http://www.w3.org/1998/Math/MathML'>
<mi>p</mi>

</math> and subtracted again at <math xmlns='http://www.w3.org/1998/Math/MathML'>
<mi>q</mi>

</math>. The sum
<math xmlns='http://www.w3.org/1998/Math/MathML'>
<mo lspace="thinmathspace" rspace="thinmathspace">&Sum;</mo>
<mi>f</mi><mo>(</mo><mi>p</mi><mo>)</mo>
</math> behaves like the telescoping series <math xmlns='http://www.w3.org/1998/Math/MathML'>
<mn>1</mn>
<mo>-</mo><mn>1</mn><mo>+</mo><mn>1</mn><mo>-</mo><mn>1</mn><mo>+</mo><mo>&sdot; &sdot; &sdot;</mo>
</math>,
and each term of the sum is swallowed by the next in its path.
Transience results from this cancellation of terms.</font></p>

<p><font face="Arial,Helvetica,Geneva,Swiss,SunSans-Regular"> Of
course, there is no need for the volumes that are shuffled between
<math xmlns='http://www.w3.org/1998/Math/MathML'>
<mi>p</mi>

</math> and <math xmlns='http://www.w3.org/1998/Math/MathML'>
<mi>q</mi>

</math> to be Voronoi cells. One of many other possibilities is
known as the Delaunay decomposition. In that decomposition, an edge
is drawn between two centers of balls if their Voronoi cells share
a face. These edges form simplices, known as Delaunay simplices,
and the simplices partition space.</font></p>

<p><font face="Arial,Helvetica,Geneva,Swiss,SunSans-Regular"> When
asked to name the most difficult part of the proof of the Kepler
conjecture, I answer without hesitation that it was the design of
the decomposition of space implicit in <math xmlns='http://www.w3.org/1998/Math/MathML'>
<mi>f</mi>

</math>. I had worked with
Voronoi cells without success and had also tried Delaunay
simplices. Both approaches became complicated beyond my ability to
understand them. My progress stopped. Finally, one day in November
1994, I realized how to combine the two approaches into a hybrid
decomposition that retained the best features of each. From that
day on, I never waivered in my confidence that the Kepler
conjecture would eventually be solved by the hybrid
approach.</font></p>

<p><font face="Arial,Helvetica,Geneva,Swiss,SunSans-Regular">
Hybrid correction terms are extremely flexible and easy to
construct, and soon Sam Ferguson and I realized that every time we
encountered difficulties in solving the minimization problem, we
could adjust <math xmlns='http://www.w3.org/1998/Math/MathML'>
<mi>f</mi>

</math> to skirt the difficulty. The function <math xmlns='http://www.w3.org/1998/Math/MathML'>
<mi>f</mi>

</math> became
more complicated, but with each change we cut months - or even
years - from our work. This incessant fiddling was unpopular with
my colleagues. Every time I presented my work in progress at a
conference, I was minimizing a different function. Even worse, the
correction function in my early papers differs from the one in the
final papers, and this required me to go back and patch the old
papers. The correction function did not become fixed until it came
time for Sam to defend his thesis, and we finally felt obligated to
stop tampering with it. However, if I were to revise the proof to
produce a simpler one, the first thing I would do would be to
change the correction function once again. It is the key to a
simple proof.</font></p>
</td>
</tr>

<tr>
<td align="right"><br />
<br />
 <a href="comb.xml"><font
face="Arial,Helvetica,Geneva,Swiss,SunSans-Regular" size="1">
More&gt; &gt; Combinatorial Structures</font></a></td>
</tr>

<tr>
<td align="Center"><br />
<br />
 <a href="../fall2001.html"><font
face="Arial,Helvetica,Geneva,Swiss,SunSans-Regular" size="1">
MathZine Table of Contents</font></a></td>
</tr>
</tbody>
</table>
</td>
</tr>
</tbody>
</table>
</td>
</tr>

<tr>
<td colspan="3" align="Center"><br />
<br />
 <font face="Arial,Helvetica,Geneva,Swiss,SunSans-Regular"
size="1"> <img src="../images/darkbluedot.gif" width="100%"
height="1" border="0" vspace="3" alt=" " /><br />
 <a href="../index.html">Mathematics Home</a>| <a
href="http://www.pitt.edu">Pitt Home</a>| <a
href="../contact.html">Contact Us</a>| <a
href="http://accounts.pitt.edu/Public/">Finding People</a>| <a
href="ftp://ftp.math.pitt.edu">FTP Site</a>| <a href="#top">Top of
Page</a></font><br />
</td>
</tr>
</tbody>
</table>

<br />
 <br />
 <br />
 <br />
</body>
</html>


