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The T and CLP families of triply periodic minimal surfaces. Part 2. The properties and computation of T
surfaces
Djurdje Cvijović, Jacek Klinowski
To cite this version:
Djurdje Cvijović, Jacek Klinowski. The T and CLP families of triply periodic minimal surfaces. Part
2. The properties and computation of T surfaces. Journal de Physique I, EDP Sciences, 1992, 2 (12),
pp.2191-2205. �10.1051/jp1:1992276�. �jpa-00246695�
Classification
Physics
Abstracts02.40 61.30 68.00
The T and CLP families of triply periodic minimal surfaces.
Part 2. The properties and computation of T surfaces
Djurdje Cvijov16
and Jacek KlinowskiDepartment of
Chemistry, University
ofCambridge,
Lensfield Road,Cambridge
CB2 IEW, G-B-(Received 7 May J992, accepted in
final form 4August
J992)Abstract. The geometry of a tD minimal surface
depends
on the ratio cla oftetragonal
axes, andcan be
fully
describd in terms of asingle
free parameter. We offer a choice of three such parameters, all related to surface geometry, and derive analyticalexpressions
for theirrelationships
to the axes ratio and the normalization factor. The latter is crucial for the
matching
ofspecific
surfaces to real structures. Parametric
equations
for normalized tD surfaces make it possible, for the first time, to find the surfacecorresponding
to anygiven
value of the cla ratio, and to compare it with actual structural data.Straightforward physical applications
of tD surfaces are thereforepossible.
We discuss thegeometric
consequences of this result and show that the z coordinate of any tD surface can beapproximated using elementary
functions. A rationalapproximation
for therelationship
between the free parameter and the cla ratio is also found. We list exact coordinates of tD surfacescorresponding
to severalprescribed
values of the cla ratio.Introduction.
Approximately
40triply periodic
embedded minimal surfaces(TPEMS)
derivedby
various methods(now mainly by
grouptheory),
have been described[1-3].
Over the last 20 years TPEMS have beenapplied
in many areas of thephysical
andbiological
sciences[4]. They
are a usefulcrystallographic concept
for thedescription
of condensed matter, as advocatedby
Scriven
[5], Mackay [6-7], Hyde
and Andersson[8], Mackay
and Klinowski[9]
and Sadocand Charvolin
[10].
Inprinciple,
the translationsymmetry
of TPEMS makes itpossible
tomatch them to actual structures, I,e, to compare surface coordinates with
spatial
pattems of atoms, and to establishrelationships
between surfaceproperties,
such as curvature and the volume-to-surfaceratio,
andrelationships
between structuralproperties, especially
thoseprovided by X-ray
diffraction and solid-state NMR.Modelling
of structures also suggests amethod of
quantifying
structuralchanges by relating
them to transformations(such
as the Bonnet and Goursattransformations)
of minimal surfaces.Finally,
studies ofinterpenetrating crystalline
structures withlarge
unit cells andcomplicated
networks of cages and channelsexposed
the limitations of classicalcrystallography, showing
the need for moreappropriate
concepts. Since TPEMS havelabyrinthine
structures,they
arelikely
to lead tosimple
structural
descriptions
of such systems. Arigorous
classification of all known andhypothetical
TPEMS will be of great
importance
to materials science ingeneral.
Unfortunately,
mathematical argumentslinking
TPEMS andphysical
structures are often far fromrigorous.
The main obstacle to a widerapplication
of minimal surfaces inexperimental
science is that most of them have been described
empirically,
without theprecise
mathematicalspecification.
It is therefore essential toquantify
all knownTPEMS,
to establish whichgeometric properties
are related to theproperties
ofphysical systems,
and to find a reliable method ofcomputing
their coordinates. Inparticular,
it isimperative
thatapproximate computation
of TPEMS to aprescribed degree
of accuracy besystematically investigated.
A TPEMS is described
by giving
itsparametric representation
or theEnneper-Weierstrass representation,
orby specifying
theboundary
conditions of apartial
differentialequation [I1- l3].
Ingeneral,
any surface in three-dimensional space iscompletely
describedby
theparametric representation
of the form(X, y,
Z)
" IX(U,
V), Y(U, V), Z(U, V)j
where the coordinates are functions of two parameters, u and v. However, in most cases
analytical expressions
for the coordinates of TPEMS are unknown. Sometimes aparametric representation
of such surfaces cannot beexpressed
in terms ofelementary
functions alone.For
example, parametric representation
of surfaces of the T and CLPfamily
involvesspecial
functions
[14].
Any
minimal surface is describedby
thefollowing
threecomplex integrals
iw
x = Re
R(r) (I r~)
drw~
y =
Re
i~ iR(r) (I
+r~)
dr(i)
w~
z = Re
j~
2R(r)
r drw~
known as the
Enneper-Weierstrass representation.
Theproblem
offinding
a minimal surface is thus reduced tosolving
theseintegrals.
For this to bepossible,
thecomplex
(« Weierstrass»)
function R
(r )
must be known. Since a new method for the construction of R(r )
for aspecific
TPEMS has been
developed [15, 30],
20 different surfaces have been so described. Intheory,
it seems
possible
to construct the functionR(r)
for anyTPEMS,
but this may involveconsiderable
practical
difficulties[16].
Coordinates of any minimal surface can be found
by solving partial
differentialequations
of the second order, known as the minimal surfaceequations,
but this method is not easy and israrely
used. Asrule, computational
difficulties increase in the order :parametric
represen-tation, Enneper-Weierstrass representation
andpartial
differentialequations.
Our
primary objective
is theapplication
oftriply periodic
embedded minimal surfaces to solid-statechemistry.
We are therefore interested indeveloping straightforward procedures
to compare such surfaces with actual structures. We will demonstrate thatparametric equations
for normalized tD surfaces achieve this
objective.
The tD
family
of TPEMS.Following
Koch and Fischer[17]
we use thesymbol
tD to refer to the oldest knownfamily
oftriply periodic
embedded minimal surfaces. The first tD surface was describedby Gergonne
asone his famous
problems conceming
a freeboundary [18],
which wassubsequently
solvedby
Schwarz
[19].
The tD surfaces arevariously
known as Tsurfaces,
D~surfaces,
supermansurfaces and
Gergonne
surfaces. Because of theirtetragonal symmetry, they
can bethought
ofas a «
tetragonal
deformation of the D surface » ; thus the abbreviation tD.There are four
types
of tD surfaces with differentsymmetries
which could begenerated
in six different waysby using
various skewstraight-edged polygons [17]. Among
them is the skewstraight-edged 8-gon
obtainedby taking eight
of the twelveedges
of atetragonal parallelepiped (right tetragonal prism)
withedges
a, a and c. The solution of the Plateau Problem for such8-gon
is a finite minimal surfacepiece
of the tDsurface,
which will henceforth be referred to as the tD saddle surface(see Fig.
I).
It iscomposed
ofeight
congruent parts relatedby
four axes of symmetry and mirrorplanes.
The tD saddle surface contains twostraight
line segments, which divide it into four congruent parts boundedby straight
line segmentsonly.
A tD saddle surface can be used as abuilding
block forconstructing
an infinite minimal surface : individual saddle surfaces assembled in such a way are related to theirneighbours by
twofold axes.Fig.
I. The tD saddle surface (a finite minimal surfacepiece
of the tD surfacespanning eight
of the twelveedges
of aright tetragonal prism) corresponding
to ~=
~
a 2
Since there are
denumerably
many skewstraight-edged 8-gons which, prior
toscaling,
candiffer for different cla
ratios,
tD surfaces are one-parameter surfaces. This means that the different surfaces of the tDfamily correspond
to different values of the same free parameter.We offer a choice of one of three such parameters, all of them real and
closely
related to theeight
flatpoints
of tD saddle surface. We shallalso,
for the firsttime,
deriveanalytical
expression
for theirrelationships
to the cla ratio. Theparameter
E with 0 ~ E ~l,
determines coordinates on the unitsphere
of theimages
of the flatpoints
(± /$, 0,
±
E), (0,
±/$,
±
E)
which are obtained
by
the Gauss map of aspecific
tD saddle surface. The parameterfl (0
~
fl
~ l occurs in the standard
stereographic projection
of theimage points
onto the
complex plane.
The parameter A(with
A ~2)
appears in the Weierstrass function of tD saddle surfaces[15]
as a coefficient in the
polynomial
under square root with rootsgiven by (2).
Since all three parameters are related(see
Tab.I),
either of them can be used. We will often refer to the tD surface with A=
14
(corresponding
to E=
l13
and fl=
fi)
andlimiting
casesA - ~x~
(E
-
I, fl
-
0)
and A- 2
(E
-
0,
fl-
1).
Table I.
-Relationships
between thefree
parameters whichfully
describe the tDsurfaces.
The parameter domains
of E, fl
and are(0, 1), (0, 1)
and(-
~x~, 2), respectively.
E
p
AI
p
2 ~l
p
2 2~'~
~/-
A ~
~
j~~2
+
~~
~~~~
IA +fi
I -Ep8-1
2+A
fi fl4
Two surfaces
corresponding
to the same value of the freeparameter (I.e.
with the same claratio)
differonly by
themultiplication
constant, known as the « normalization factor » anddenoted
by
K. For the same value of the free parameter, but different values ofK, a
multiplicity
of surfaces areproduced,
the coordinates of which differby
the factorK. The normalization
factor,
so farunknown,
is crucial tomatching
of aspecific
tD surface toa real structure, and enables a
comparison
of different surfaces. We will show thatK is a function of the free
parameter,
and derive ananalytical expression
for it.The
parametric representation
of thefamily
of tD saddle surfaces is[14]
x(u, v)
= Kgx Re
iF
(q~x,kx)i y(u, v)
= Kgx Re
iF
(q~x,/fi)1 (4)
z(u, v)
= Kg~ Re
IF
(q~~,k~)j
where all components, except K, are defined in tables
IIa,
IIb andw is
complex
w = u +
iv,
withw « I
(see Fig. 2a),
All components ofequations (4) depend
on the valueTable II.
a) Multiplication
constants g~ and g~ and the moduli k~ and k~ used inparametric
the
equations for
the tDsu~fiaces expressed
in termsof JFee
parametersE, p
and A(see text).
b)
Theamplitudes
q~~ andq~~ in
parametric equations for
the tDsu~fiaces
can beexpressed
in various ways. g~ and g~ aredefined
in table IIa.I-E~
2fl~ /~$~
gx
~~2 fi I+fl~
~
l-E
~
/
~ ~~~
~ ~/-A
+ 4
~2
E~ i~ p~ I_
~
l+E~
21+fl~
2fi
~ ~~+~~~ ~~ ~~/_A~ 1~
a)
I cos 2
q~~
cos~
q~~
sin~
q~~
w~ 6(w/g~)~
+ lw
~
2(w/g~)~
+ l4(w/g~)~
x
~ ~ ~ ~
w +
2(w/g~)
+ Iw~
+
2(w/g~)~
+ l w +2(w/g~)
+ Iz 2
(
w ~/g~)~ l(w
~/g~ )~(
w9g~
)~b)
of the same free real parameter, and the
relationship
between them and either ofE,
p and A, isgiven
in tablesIIa,
b. Re in(4)
stand for real part ofincomplete elliptic integrals
of the first kind F
(q~, k),
defined in its traditionalLegendre-Jacobi
normal form as~
~~~ ~~ i~ ~/(I ~~~l
k~t~)
~ ~
where we assume that the variable
k,
themodulus,
is real and lies in the interval[0, 1]
and the variable q~, theamplitude,
is acomplex
number. We will often use variousproperties
ofF(q~, k)
which areexplained
in detail in standard texts[20-21].
The
multiplication
factors g~ and g~ and the moduli k~ and k~ in(4) depend only
on the value of freeparameter (Tab. IIa),
and lie the interval(0,1). Further, simple trigonometric
transformations allow us to express the
amplitudes
q~~ andq~~ in number of
equivalent
ways in terms ofcomplex
inversetrigonometric
functions(Tab. IIb).
We shall usecomplex
inverse sinefunctions,
which differ for different values of the free parameter.Quantitative
characteristics of the tDfamily.
In order to match actual structural data
describing
atetragonal
system to a tDsurface,
it is necessary that thefollowing problem
be solvedgiven
the a and c dimensions of aright
tetragonal prism,
find the coordinates of theappropriate
tD saddle surface. To do that we mustexamine closer the normalization factor K, and establish the
relationship
between thecla ratio and other
properties
of the surface.Our
parametric equations (4)
show(Fig. 2b) that,
for any value of free parameter, thepoint
A on the real axis of thecomplex plane
with coordinates(p, 0) (where p
is defined in Tab.IIa)
ismapped
intopoint
A with coordinates(a/2, 0, c/2)
of the tD saddle surface. This the basis of the derivation of ananalytical expression
for the ratio oftetragonal
axescla
(which
wedesignate by x),
which cannot be derived from theEnneper-Weierstrass representation (Eqs. (I)
and(3)
alone.Thus,
from(4)
we obtainwhere
ll'~(fl
andll'~(fl )
are~ 2
V'z
(P )
=
z
~ ~
~
j
4(w/g~)2
~~~~~~
W
~ + 2
(w/g~)2
+~ ~
Table IIa shows that
expressions (6) give ll'~(p
=
I and
ll'~(fl
=
I for any value of the free parameter. In terms of the
complete elliptic integral
of the firstkind, K(k)
=
F
(w/2, k), expressions (5)
area = Kg~
K(k~)
c = 2 Kg~
K(k~)
~~~ant the
tetragonal
axis ratio is thereforeg~
K(k~)
x = 2
(8)
gx
K(k~)
where g~, g~, k~ and k~ are defined in table
IIa,
anddepend
on the value of the freeparameter
alone.Using
tableIIa,
the ratio(8)
can beeasily expressed
in terms of either of the parametersE, p
orA,
so thatexpressions
for x= x
(E),
x= x
(p )
and x= x
(A
arereadily
available.We see therefore that the
tetragonal
axis ratio x isindependent
of the normalization factor, andonly depends (in
a continuousmanner)
on the free parameter. It follows that x isuniquely
characteristic
(an invariant)
of aspecific
surfacebelonging
to the tDfamily.
We
verify (8) by
apfling
it to the tD surface with A = 14 which has theonly
known valueof the cla ratio
(x
=
2/2
) [22]
andlimiting
cases(A
- ~x~ and A-
2).
It is easy to show that for A=
14
relationship
between k~ and k~ is~
l
/~
~ l +
/~
I.e, the moduli are related
by
Landen'sdescending
transformation whichgives [21]
K(k~)
I +/~
K(k~)
2(a)
~' 1°~~ z yRe (to) x
fi
~~
I m (w~
C A
B
,
~, A
' Re(to)
C
, '
D
B
m (to)
(c)
B A
,
A
,
Re (to)
D
~ ~
ifii
Fig.
2. (a) Construction of a tD surfacepiece spanning
an8-gon by projecting
a closed unit disc in thecomplex plane using
parametricequations
(I I).Shading
indicates thatintegration
(I I) is carried out overthe entire unit disc
including
theboundary.
(b) and (c) construction of characteristic parts of the tD surfaceby projecting
thick lines on the unit disc.Since k~ = 1/2 and
g~/g~
=/(2 /),
the
required
ratio(8)
is x=
l12.
Thelimiting
behaviour of x
(Tab. III)
can beexplained by using only
the concept oftetragonal
distortion as follows. Normalized tD surfaces span theedges
ofright tetragonal prisms
with the same baseedge
a(which
isconveniently
used as aunit)
but differentedges
c. In otherwords,
the surfacesTable III.
Limiting
valuesof
the various constantsfor
E- 0
(corresponding
top
- I and
A -
2)
andfor
E- I
(corresponding
tofl
- 0 and A- ~x~).
gx gz k~ k~ x K
E-o I 0 ~x~ 2/w
E-1 0 0
/
0 0 ~x~
2
are
tetragonally
distorted. Whenapproaching
a limit of the free parameter(A
- ~x~)
thelength
of theedge
c decreases(hence
x-
0),
and withincreasing c(A
-
2),
the ratio x increases towardsinfinity.
It is
important
to be able to determine a tD surface for anyprescribed
value of xo. Theequation
x = xo, where x isgiven by (8)
is transcendental, and can be solvedonly numerically.
We haveadopted
thefollowing procedure.
To shorten theroot-searching
interval,we express x in terms of either E or fl. Since there is
only
one real root and the interval isknown,
it is not necessary toemploy root-finding
methods which involve derivatives. Brent'salgorithm [23]
isprobably
the best numerical method ofsolving
theequation
x= xo.
However,
in mostapplications,
it is sufficient toapproximate
xby
a rational function. We usea rational
approximation
of the form4
p~ E' X #
' 4
(9a)
I
~, ~'i 0
where E is the free parameter with 0 ~ E ~ l, and the coefficients p~, q,
(I
=
0,
1,2,
3 and4)
need to be determined.
By employing
the standard method of rationalinterpolation [23]
we have found rationalapproximations
for x(see
Tab.IV)
with a numerical accuracy better than 7significant figures.
Thus, for agiven
xo, the determination of free parameter is reduced to anumerical solution of the
quartic
£
4 ~Pi xo qi E~= o
(9b)
, o
with coefficients
given
in table IV.Table IV. Three rational
approximations of
theform (9) for
ratio x(E) for different
intervals
of
the parameter E.0.05£ E £ 0,13 £L73 ) 0.13£E£0.50 0.50 £E£0.89
I
0 4.65nWWM2642 1 3.80339n64598255 2.7l697576312VM
1 95.016254824041 45.213715340127 1.051796760637337 5.37555S39100W09
2 %15.10224088421 4445.36501919f0& 1485%2176933356 213.073S84195259
3 15023.24273163% 10.97%3834344544
4 85.7994121752395 1.95526487007l338
We note that A
=
14 has been
wrongly
attributed to the tD surfacespanning
an8-gon
formed
by eight
of the twelveedges
of a cube(so
that xo =I). By solving
the aboveequation numerically
we find that the correct value is A= 5.3485782.
The
expressions (7)
and(8) give
~
x
~
2
g~K(k~)
so it is clear that the normalization factor K is related to the size of the
right tetragonal prism
forgiven
a and c and ifparametric representation
of surface is considered as dimensionalequations,
then that K should begiven
units of inverselength.
Furthersimplification gives
thefollowing expression
for the normalization factor K in theparametric equations (4)
for tD saddle surfacesK = a
( IO)
~x
K(kx)
where g~ and k~ are defined in table
IIa,
and bothdepend
on the value of freeparameter
alone.Equation (10)
andexpressions
in table IIagive
ananalytical expression
for K in terms of the free parameter.Therefore,
for aspecific
value of thelength
of theedge
a, Kdepends only
onthe value of free parameter and
changes continuously
withit,
withlimiting
values listed in table III. Until nowonly
for tD surface with A=
14 has been known normalization factor
(K
= 0.8389223 in Ref.[24])
which can beeasily
obtained from(lo)
asK =
~~~~
a =0.8389223 a
Parametric
equations
for normalized tD surfaces.For the
parametric equations (4)
with theamplitudes
q~~ andq~~
given
in terms ofcomplex
inverse sine functions to be
practically useful,
it is necessary to examine thecomplex
squareroot function of the
complex
variablew = u + iv with
w w
I,
which appears inequations
for the coordinates x and y
(see
Tab.IIb).
It isclearly
desirable to choose the same branch of thecomplex
square root for both coordinates on the entire unit disc. In what follows weconsider
only
that branch of the square root which is I at I. In this way, theequation (4)
for thex coordinate
correctly represents
the tDtetragonal
surface for u m0,
I.e. onimaginary
axis andright-hand
half of the unit disc. In order torepresent correctly
the surface on the left-hand part of the unitdisc,
it is sufficient tochange
thesign
of theexpression
for x.Symmetry
considerationsrequire
that for the calculation of the y coordinate the surface becorrectly represented
on the upper(I
and IIquadrant)
or lower(III
and IVquadrant) parts
of the unit disc. Were it theonly requirement,
it could be satisfiedby
asimple change
ofsign, just
aswas done for the x coordinate.
However,
theexpression (4)
for the y coordinategives
a correctrepresentation
in the I and the IVquadrant
of thecomplex plane,
instead of the I and IIquadrant.
To resolve thisproblem,
we must «rotate» the solution function counter-clockwise
by
w/2. Therequired
function for y is foundusing
theprocedure
described in[14].
The new
equation
for y, obtained fromintegral
231.00 in reference[20],
which satisfies the conventionconceming
the branch of the square root isy
(u,
v)
=
KgxRe iF
(q~y,kx)i
where the
expression
forq~~ is derived from that for q~~ in the first row of table IIb
by changing signs
of allquadratic
terms. In otherwords,
therelationship
betweenq~~ and
q~~ is
~y(W )
" ~x(I
W
).
Further,
it is convenient to usepolar
coordinates instead of the Cartesian. Hence, forgiven lengths
a and c of theedges
of aright tetragonal prism
it is necessary to find the value of the free parameter(conveniently
chosen from amongE, fl
andA),
from(8). According (4)
and( lo),
the coordinates of theappropriate
tD saddle surfacespanning eight
of the twelveedges
ofa
right tetragonal prism
arex(r,
0= ±
~ Re
[F (arcsin ll'~(w ), k~)]
2
K(k~)
y
(r,
0= ±
£
' ReIF (arcsin
~l~~ (< w), k~) I1)
2
K(k~)
z(r,
0=
£
' ReiF (arcsin
~l~~(w), k~)j
2 K(k~
where
~/
4(w/g~)~
'~'~~~°
w~
+2(w/g~)~
+ l~2 ll'~(w )
=gz
with w = r cos 0 + ir sin 0 and 0 « r « I and w
~ 0 w w, while k~, k~, g~ and g~ are
defined in table IIa. In the
equation
for x, theplus sign
relates toright
half and the minussign
to left half of thecomplex plane.
In theexpression
for y, theplus sign
relates to upper half and the minussign
to lower half. In this way, we arrive atparametric equations
of the normalized tDfamily.
Unfortunately,
there is no true addition formula for F(q~, k)
with acomplex amplitude,
sothat F
(u
+ iv,k)
cannot beexpressed
in terms of F(u, k)
and F(iv, k) only.
It is thereforeimpossible
to separate the real andimaginary
parts, andparametric equations (11)
cannot besimplified
further.Consider the
limiting
behaviour of theparametric equations
when the free parameterapproaches
its limits(see
Tab.III).
Close to one limit(A
- ~x~ we find that the
appropriate
F (q~,
k) exist,
but x= y = z =
0,
because g~ = g~ = 0. For the other limit (A =2)
themoduli k~ and k~ in
equations (4)
are 0 and Irespectively,
and therefore theappropriate
functions F (q~,
k)
reduce toelementary
functions. Since themultiplication
constants are finite, theequations
areexpressed
in terms ofelementary
functionsonly,
and describe surface with the cla ratioapproaching infinity.
It is easy to show that for A=
2 we obtain
parametric equations
of Scherk's surface z=
In
(cos y/cos x) [25],
so thatequations (4)
derived with theassumption
A~ 2 can be extended to the
limiting
case of A= 2.
The
elliptic integrals
in II are finite in the entirecomplex plane,
even atpoints
definedby
(2).
This means that F(q~, k)
is finite atsingular points
of the Weierstrass function(3).
This isparticularly important,
in view of the fact that numerical estimation ofintegrals
fails close to thesingularities.
No
expressions
for theapproximate computations
of tD surfaces are known. It is clear thatthey
can be deduced fromequations (11) by
anappropriate approximation
of theincomplete elliptic integrals
of the first kindby elementary
functions. Thisprocedure
deserves additionalanalysis,
but anapproximation
for zimmediately
suggests itself. Thus for A ~ 2 the values of the modulus k~ in theexpression
for z are between 0 and I, but for A~ 8 the value of
k~ is less than 0, I. This makes it
possible
to express the z coordinate in terms ofelementary
functions with ahigh
numerical accuracy. SinceF(q~, k)
m q~ for small
k,
we havez m
~ Re arcsin I
2
K(k~) g/
With w = r cos 0 + ir sin 0 the real
part
isexplicitly
found asz m
)
arcsin &K(k~)
where
&
=
~
[~/(r~
+ k~cos~
2 0)~ +kj sin~
2 0 +~/(r~
k~cos~
2 0)~ +k) sin~
2 0 2 k~For A « 50 this
approximation gives
numerical accuracy to 7significant figures
on the entire unitdisc,
and for A « 000 to as many as 15significant figures.
It is evenpossible
toapproximate
the coordinate, albeit lessaccurately, using only
thequadratic
functionc ~
w~
~ 2
K(k~)
~fi
and hence
~
~K~k~)fi~~~~~~~
Computation
of tD surfaces.Since sketches
[26]
andphotographs
of models[27]
of tD surfaces cannot beregarded
asquantitative, drawings [15]
obtainedusing
theEnneper-Weierstrass representation
are theonly
known case of their
computation.
Reference[15] gives
the Cartesian coordinates forA
=
2.01, 3,
14 and 50 obtainedby taking
the realparts
ofcomplex integrals (our Eqs. (I)
and(3))
defined on the unit disc.Computation
of a tD surfaceusing
theEnneper-Weierstrass representation requires
numerical
integration
to evaluatehyperelliptic integrals,
and cannot be carried out withoutprior analysis
of the behaviour of theintegrands
and the choice of anappropriate
numericalmethod from among a number which are available. For direct
comparison,
we haveperformed
such
computations
for tD surfaces described below. Thesecomputations
arequite
cumbersome andrequire
a carefulinterpretation
of data in thevicinity
ofsingularities
of the Weierstrassfunction,
sincelarge portions
of the surfaces aregenerated by
smallregions surrounding
thesesingularities. However,
the main weakness ofusing
theEnneper-Weierstrass representation directly
is that surfacescorresponding
to aspecific
value of Acomputed
from them cannot beapplied,
In otherwords,
without theknowledge
ofK and x
(neither
of which can be deduced fromit),
theEnneper-Weierstrass representation
does not tell us how togenerate
a surface to matchprescribed
data.Also,
it isimpossible
to compare different tD surfaces withoutnormalization.
By
contrast,parametric equations (11) require
the evaluation of functions F(q~, k)
andK(k)
which is mucheasier,
andyield
all informationrequired
formatching,
thusmaking straightforward physical applications possible.
We use them tocompute
tD saddle surfaces for severalprescribed
values of the axes ratio.The evaluation of the functions
F(q~, k)
andK(k),
is nowusually
based on the Gaussalgorithm
of thearithmetic-geometric
mean and Landen's transformation[21, 23, 28]
and Carlson'salgorithm [29].
The latter isimplemented
inNAG,
SLATEC and IMSL numericallibraries.
However,
we use the Gaussalgorithm
because its use for the evaluation ofF(q~,
k) forcomplex
values ofamplitude
is well documented. In order to demonstrate thesimplicity
of thisalgorithm,
we outline it below. Thearithmetic-geometric
mean of twonumbers ao and
bo (where bo
is anycomplex
number different from 0 and fromJOURNAL DEPHYSIQUE i T 2, N' 12, DECEMBER <992 79
ao),
is denotedby AG(ao,bo),
and defined as the common limit of the arithmetic(a,)
andgeometric (b;)
sequences~< ~
~' '
j
~~ '~i
~
~i
with I
=
1, 2, 3,
Both sequences are convergent for any choice of ao andbo.
Afterreaching
the
prescribed
accuracy at the n-th iteration step(I,e,
difference between a~ and b~ is less than therequired value), AG(ao, bo)
can beapproximated by
a~ mb~.
To calculate
K(k)
for anyparticular
value of k we start fromao =
I
bo
=
/$.
After n iterations we have
~~~~
2 AG
ao, bo)
~j~
To calculate F
(q~, k)
for anyparticular
values of q~ and k we start fromao =
I
bo
=k(
=
/$
q~o = q~
and
by using
Landen'sdescending
sequencek)
j~ ~ ' ~ "~~~~
~~
' ~~' ~
'~
~~~~ ~~l +
k)
_,
where I
=
1, 2,
..., n,
together
with thearithmetic-geometric
meanalgorithm.
Afterprescribed
accuracy is reached at n iterations we have
~
~~' ~~
2~
AG(ao, bo)
2~ a~The
algorithm
issimple
and very fast(it
convergesquadratically)
so that numerical accuracy to 7 and 15figures
isusually
reached at the4th,
and 8th iterationstep, respectively.
Itsonly
known
unsatisfactory
behaviour is for k- I and q~
- w/2, but these cases do not arise here.
We have
computed
the coordinates of tD saddle surfaces for x=
1,
0.5 and 0.25. Thelength
of
edge
a is assumed to be I and allquantities required
in the calculation aregiven
in table V.Table V. Constants used in the
computation of
the various saddle tD minimalsu~fiaces for different
valuesof
the axis ratio x.=1 =o.5
k 5.3485782 43.91463368 569.960o6523
K 0.71579938 1.054279364 1.899815152
0.85894265 0.543284378 0.289183541
0.44045702 0.15094129 0.041886923
0.36208944 0.593650606 0.676894704
0.19400238 0.022783273 0.00175451429
Tables VIa-c list
only
the coordinates of oneeighth
of each saddle surface. These minimal surfacepieces
areasymmetric units,
and for each the(r,
b) computational
domain is a sector of the unit disc with 0 « r w I and 0 w b « mm. The sector is dividedusing
a 8 x 5grid
where the coordinates ofgrid points
aregiven by
w
(n~,
no)
= n~ ro cos
(no Ho)
+in~
ro sin(no
Ho)
with ro =
1/8 and Ho = w/16
(n~
=1,
...,
8 and no =
0, 1,
...,
4).
It is clear that the coordinates of acomplete
tD saddle surface can be obtainedby symmetry
considerations alone. Coordinates of surfacescorresponding
to the same value of x but different values ofa can b£ obtained
by multiplying
the coordinates in tables VIa-cby
a.Table VI. Cartesian
coordi~ates of
threedifferent
tDsu~fiaces.
The columnsdiffer
inn~ and the rows in no,
a)
x = I,b)
x=
0.5,
c)
x = 0.25.I Z 3 4 5 6 7 8
o
1
2
3
4
a)
1 2 3 4 S 6 7 8
o
i
z
3
4
b)
Table VI
(continued).
1 2 3 4 5 6 7 8
o
i
z
3
4
C)
Acknowledgements.
We are
grateful
to Dr. C.Briggs
of the British Council for support, and to Professor B. C.Carlson of Iowa State
University
for discussionsconceming
theproperties
andcomputation
ofelliptic integrals.
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figure
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