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HAL Id: jpa-00246695

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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�

(2)

Classification

Physics

Abstracts

02.40 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 Klinowski

Department of

Chemistry, University

of

Cambridge,

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 of

tetragonal

axes, and

can be

fully

describd in terms of a

single

free parameter. We offer a choice of three such parameters, all related to surface geometry, and derive analytical

expressions

for their

relationships

to the axes ratio and the normalization factor. The latter is crucial for the

matching

of

specific

surfaces to real structures. Parametric

equations

for normalized tD surfaces make it possible, for the first time, to find the surface

corresponding

to any

given

value of the cla ratio, and to compare it with actual structural data.

Straightforward physical applications

of tD surfaces are therefore

possible.

We discuss the

geometric

consequences of this result and show that the z coordinate of any tD surface can be

approximated using elementary

functions. A rational

approximation

for the

relationship

between the free parameter and the cla ratio is also found. We list exact coordinates of tD surfaces

corresponding

to several

prescribed

values of the cla ratio.

Introduction.

Approximately

40

triply periodic

embedded minimal surfaces

(TPEMS)

derived

by

various methods

(now mainly by

group

theory),

have been described

[1-3].

Over the last 20 years TPEMS have been

applied

in many areas of the

physical

and

biological

sciences

[4]. They

are a useful

crystallographic concept

for the

description

of condensed matter, as advocated

by

Scriven

[5], Mackay [6-7], Hyde

and Andersson

[8], Mackay

and Klinowski

[9]

and Sadoc

and Charvolin

[10].

In

principle,

the translation

symmetry

of TPEMS makes it

possible

to

match them to actual structures, I,e, to compare surface coordinates with

spatial

pattems of atoms, and to establish

relationships

between surface

properties,

such as curvature and the volume-to-surface

ratio,

and

relationships

between structural

properties, especially

those

provided by X-ray

diffraction and solid-state NMR.

Modelling

of structures also suggests a

method of

quantifying

structural

changes by relating

them to transformations

(such

as the Bonnet and Goursat

transformations)

of minimal surfaces.

Finally,

studies of

interpenetrating crystalline

structures with

large

unit cells and

complicated

networks of cages and channels

exposed

the limitations of classical

crystallography, showing

the need for more

appropriate

concepts. Since TPEMS have

labyrinthine

structures,

they

are

likely

to lead to

simple

structural

descriptions

of such systems. A

rigorous

classification of all known and

hypothetical

TPEMS will be of great

importance

to materials science in

general.

(3)

Unfortunately,

mathematical arguments

linking

TPEMS and

physical

structures are often far from

rigorous.

The main obstacle to a wider

application

of minimal surfaces in

experimental

science is that most of them have been described

empirically,

without the

precise

mathematical

specification.

It is therefore essential to

quantify

all known

TPEMS,

to establish which

geometric properties

are related to the

properties

of

physical systems,

and to find a reliable method of

computing

their coordinates. In

particular,

it is

imperative

that

approximate computation

of TPEMS to a

prescribed degree

of accuracy be

systematically investigated.

A TPEMS is described

by giving

its

parametric representation

or the

Enneper-Weierstrass representation,

or

by specifying

the

boundary

conditions of a

partial

differential

equation [I1- l3].

In

general,

any surface in three-dimensional space is

completely

described

by

the

parametric 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 a

parametric representation

of such surfaces cannot be

expressed

in terms of

elementary

functions alone.

For

example, parametric representation

of surfaces of the T and CLP

family

involves

special

functions

[14].

Any

minimal surface is described

by

the

following

three

complex integrals

iw

x = Re

R(r) (I r~)

dr

w~

y =

Re

i~ iR(r) (I

+

r~)

dr

(i)

w~

z = Re

j~

2

R(r)

r dr

w~

known as the

Enneper-Weierstrass representation.

The

problem

of

finding

a minimal surface is thus reduced to

solving

these

integrals.

For this to be

possible,

the

complex

Weierstrass

»)

function R

(r )

must be known. Since a new method for the construction of R

(r )

for a

specific

TPEMS has been

developed [15, 30],

20 different surfaces have been so described. In

theory,

it seems

possible

to construct the function

R(r)

for any

TPEMS,

but this may involve

considerable

practical

difficulties

[16].

Coordinates of any minimal surface can be found

by solving partial

differential

equations

of the second order, known as the minimal surface

equations,

but this method is not easy and is

rarely

used. As

rule, computational

difficulties increase in the order :

parametric

represen-

tation, Enneper-Weierstrass representation

and

partial

differential

equations.

Our

primary objective

is the

application

of

triply periodic

embedded minimal surfaces to solid-state

chemistry.

We are therefore interested in

developing straightforward procedures

to compare such surfaces with actual structures. We will demonstrate that

parametric equations

for normalized tD surfaces achieve this

objective.

The tD

family

of TPEMS.

Following

Koch and Fischer

[17]

we use the

symbol

tD to refer to the oldest known

family

of

triply periodic

embedded minimal surfaces. The first tD surface was described

by Gergonne

as

one his famous

problems conceming

a free

boundary [18],

which was

subsequently

solved

by

Schwarz

[19].

The tD surfaces are

variously

known as T

surfaces,

D~

surfaces,

superman

(4)

surfaces and

Gergonne

surfaces. Because of their

tetragonal symmetry, they

can be

thought

of

as a «

tetragonal

deformation of the D surface » ; thus the abbreviation tD.

There are four

types

of tD surfaces with different

symmetries

which could be

generated

in six different ways

by using

various skew

straight-edged polygons [17]. Among

them is the skew

straight-edged 8-gon

obtained

by taking eight

of the twelve

edges

of a

tetragonal parallelepiped (right tetragonal prism)

with

edges

a, a and c. The solution of the Plateau Problem for such

8-gon

is a finite minimal surface

piece

of the tD

surface,

which will henceforth be referred to as the tD saddle surface

(see Fig.

I

).

It is

composed

of

eight

congruent parts related

by

four axes of symmetry and mirror

planes.

The tD saddle surface contains two

straight

line segments, which divide it into four congruent parts bounded

by straight

line segments

only.

A tD saddle surface can be used as a

building

block for

constructing

an infinite minimal surface : individual saddle surfaces assembled in such a way are related to their

neighbours by

twofold axes.

Fig.

I. The tD saddle surface (a finite minimal surface

piece

of the tD surface

spanning eight

of the twelve

edges

of a

right tetragonal prism) corresponding

to ~

=

~

a 2

Since there are

denumerably

many skew

straight-edged 8-gons which, prior

to

scaling,

can

differ for different cla

ratios,

tD surfaces are one-parameter surfaces. This means that the different surfaces of the tD

family 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 the

eight

flat

points

of tD saddle surface. We shall

also,

for the first

time,

derive

analytical

(5)

expression

for their

relationships

to the cla ratio. The

parameter

E with 0 ~ E ~

l,

determines coordinates on the unit

sphere

of the

images

of the flat

points

(± /$, 0,

±

E), (0,

±

/$,

±

E)

which are obtained

by

the Gauss map of a

specific

tD saddle surface. The parameter

fl (0

~

fl

~ l occurs in the standard

stereographic projection

of the

image 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 roots

given 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)

and

limiting

cases

A - ~x~

(E

-

I, fl

-

0)

and A

- 2

(E

-

0,

fl

-

1).

Table I.

-Relationships

between the

free

parameters which

fully

describe the tD

surfaces.

The parameter domains

of E, fl

and are

(0, 1), (0, 1)

and

(-

~x~, 2

), respectively.

E

p

A

I

p

2 ~

l

p

2 2

~'~

~/-

A ~

~

j~

~2

+

~~

~~~~

IA +fi

I -E

p8-1

2+A

fi fl4

Two surfaces

corresponding

to the same value of the free

parameter (I.e.

with the same cla

ratio)

differ

only by

the

multiplication

constant, known as the « normalization factor » and

denoted

by

K. For the same value of the free parameter, but different values of

K, a

multiplicity

of surfaces are

produced,

the coordinates of which differ

by

the factor

K. The normalization

factor,

so far

unknown,

is crucial to

matching

of a

specific

tD surface to

a real structure, and enables a

comparison

of different surfaces. We will show that

K is a function of the free

parameter,

and derive an

analytical expression

for it.

The

parametric representation

of the

family

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 and

w is

complex

w = u +

iv,

with

w « I

(see Fig. 2a),

All components of

equations (4) depend

on the value

(6)

Table II.

a) Multiplication

constants g~ and g~ and the moduli k~ and k~ used in

parametric

the

equations for

the tD

su~fiaces expressed

in terms

of JFee

parameters

E, p

and A

(see text).

b)

The

amplitudes

q~~ and

q~~ in

parametric equations for

the tD

su~fiaces

can be

expressed

in various ways. g~ and g~ are

defined

in table IIa.

I-E~

2

fl~ /~$~

gx

~~2 fi I+fl~

~

l-E

~

/

~ ~~~

~ ~/-A

+ 4

~2

E~ i~ p~ I_

~

l+E~

2

1+fl~

2

fi

~ ~~+~~~ ~~ ~~/_A~ 1~

a)

I cos 2

q~~

cos~

q~~

sin~

q~~

w~ 6(w/g~)~

+ l

w

~

2(w/g~)~

+ l

4(w/g~)~

x

~ ~ ~ ~

w +

2(w/g~)

+ I

w~

+

2(w/g~)~

+ l w +

2(w/g~)

+ I

z 2

(

w ~/g~)~ l

(w

~/g~ )~

(

w

9g~

)~

b)

of the same free real parameter, and the

relationship

between them and either of

E,

p and A, is

given

in tables

IIa,

b. Re in

(4)

stand for real part of

incomplete elliptic integrals

of the first kind F

(q~, k),

defined in its traditional

Legendre-Jacobi

normal form as

~

~~~ ~~ i~ ~/(I ~~~l

k~

t~)

~ ~

where we assume that the variable

k,

the

modulus,

is real and lies in the interval

[0, 1]

and the variable q~, the

amplitude,

is a

complex

number. We will often use various

properties

of

F(q~, k)

which are

explained

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 free

parameter (Tab. IIa),

and lie the interval

(0,1). Further, simple trigonometric

transformations allow us to express the

amplitudes

q~~ and

q~~ in number of

equivalent

ways in terms of

complex

inverse

trigonometric

functions

(Tab. IIb).

We shall use

complex

inverse sine

functions,

which differ for different values of the free parameter.

Quantitative

characteristics of the tD

family.

In order to match actual structural data

describing

a

tetragonal

system to a tD

surface,

it is necessary that the

following problem

be solved

given

the a and c dimensions of a

right

(7)

tetragonal prism,

find the coordinates of the

appropriate

tD saddle surface. To do that we must

examine closer the normalization factor K, and establish the

relationship

between the

cla ratio and other

properties

of the surface.

Our

parametric equations (4)

show

(Fig. 2b) that,

for any value of free parameter, the

point

A on the real axis of the

complex plane

with coordinates

(p, 0) (where p

is defined in Tab.

IIa)

is

mapped

into

point

A with coordinates

(a/2, 0, c/2)

of the tD saddle surface. This the basis of the derivation of an

analytical expression

for the ratio of

tetragonal

axes

cla

(which

we

designate by x),

which cannot be derived from the

Enneper-Weierstrass representation (Eqs. (I)

and

(3)

alone.

Thus,

from

(4)

we obtain

where

ll'~(fl

and

ll'~(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 first

kind, K(k)

=

F

(w/2, k), expressions (5)

are

a = Kg~

K(k~)

c = 2 Kg~

K(k~)

~~~

ant the

tetragonal

axis ratio is therefore

g~

K(k~)

x = 2

(8)

gx

K(k~)

where g~, g~, k~ and k~ are defined in table

IIa,

and

depend

on the value of the free

parameter

alone.

Using

table

IIa,

the ratio

(8)

can be

easily expressed

in terms of either of the parameters

E, p

or

A,

so that

expressions

for x

= x

(E),

x

= x

(p )

and x

= x

(A

are

readily

available.

We see therefore that the

tetragonal

axis ratio x is

independent

of the normalization factor, and

only depends (in

a continuous

manner)

on the free parameter. It follows that x is

uniquely

characteristic

(an invariant)

of a

specific

surface

belonging

to the tD

family.

We

verify (8) by

ap

fling

it to the tD surface with A = 14 which has the

only

known value

of the cla ratio

(x

=

2/2

) [22]

and

limiting

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's

descending

transformation which

gives [21]

K(k~)

I +

/~

K(k~)

2

(8)

(a)

~' 1°~~ z y

Re (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 surface

piece spanning

an

8-gon by projecting

a closed unit disc in the

complex plane using

parametric

equations

(I I).

Shading

indicates that

integration

(I I) is carried out over

the entire unit disc

including

the

boundary.

(b) and (c) construction of characteristic parts of the tD surface

by projecting

thick lines on the unit disc.

Since k~ = 1/2 and

g~/g~

=

/(2 /),

the

required

ratio

(8)

is x

=

l12.

The

limiting

behaviour of x

(Tab. III)

can be

explained by using only

the concept of

tetragonal

distortion as follows. Normalized tD surfaces span the

edges

of

right tetragonal prisms

with the same base

edge

a

(which

is

conveniently

used as a

unit)

but different

edges

c. In other

words,

the surfaces

(9)

Table III.

Limiting

values

of

the various constants

for

E

- 0

(corresponding

to

p

- I and

A -

2)

and

for

E

- I

(corresponding

to

fl

- 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. When

approaching

a limit of the free parameter

(A

- ~x~

)

the

length

of the

edge

c decreases

(hence

x

-

0),

and with

increasing c(A

-

2),

the ratio x increases towards

infinity.

It is

important

to be able to determine a tD surface for any

prescribed

value of xo. The

equation

x = xo, where x is

given by (8)

is transcendental, and can be solved

only numerically.

We have

adopted

the

following procedure.

To shorten the

root-searching

interval,

we express x in terms of either E or fl. Since there is

only

one real root and the interval is

known,

it is not necessary to

employ root-finding

methods which involve derivatives. Brent's

algorithm [23]

is

probably

the best numerical method of

solving

the

equation

x

= xo.

However,

in most

applications,

it is sufficient to

approximate

x

by

a rational function. We use

a rational

approximation

of the form

4

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 and

4)

need to be determined.

By employing

the standard method of rational

interpolation [23]

we have found rational

approximations

for x

(see

Tab.

IV)

with a numerical accuracy better than 7

significant figures.

Thus, for a

given

xo, the determination of free parameter is reduced to a

numerical solution of the

quartic

£

4 ~Pi xo qi E~

= o

(9b)

, o

with coefficients

given

in table IV.

Table IV. Three rational

approximations of

the

form (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

(10)

We note that A

=

14 has been

wrongly

attributed to the tD surface

spanning

an

8-gon

formed

by eight

of the twelve

edges

of a cube

(so

that xo =

I). By solving

the above

equation 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

for

given

a and c and if

parametric representation

of surface is considered as dimensional

equations,

then that K should be

given

units of inverse

length.

Further

simplification gives

the

following expression

for the normalization factor K in the

parametric equations (4)

for tD saddle surfaces

K = a

( IO)

~x

K(kx)

where g~ and k~ are defined in table

IIa,

and both

depend

on the value of free

parameter

alone.

Equation (10)

and

expressions

in table IIa

give

an

analytical expression

for K in terms of the free parameter.

Therefore,

for a

specific

value of the

length

of the

edge

a, K

depends only

on

the value of free parameter and

changes continuously

with

it,

with

limiting

values listed in table III. Until now

only

for tD surface with A

=

14 has been known normalization factor

(K

= 0.8389223 in Ref.

[24])

which can be

easily

obtained from

(lo)

as

K =

~~~~

a =

0.8389223 a

Parametric

equations

for normalized tD surfaces.

For the

parametric equations (4)

with the

amplitudes

q~~ and

q~~

given

in terms of

complex

inverse sine functions to be

practically useful,

it is necessary to examine the

complex

square

root function of the

complex

variable

w = u + iv with

w w

I,

which appears in

equations

for the coordinates x and y

(see

Tab.

IIb).

It is

clearly

desirable to choose the same branch of the

complex

square root for both coordinates on the entire unit disc. In what follows we

consider

only

that branch of the square root which is I at I. In this way, the

equation (4)

for the

x coordinate

correctly represents

the tD

tetragonal

surface for u m

0,

I.e. on

imaginary

axis and

right-hand

half of the unit disc. In order to

represent correctly

the surface on the left-hand part of the unit

disc,

it is sufficient to

change

the

sign

of the

expression

for x.

Symmetry

considerations

require

that for the calculation of the y coordinate the surface be

correctly represented

on the upper

(I

and II

quadrant)

or lower

(III

and IV

quadrant) parts

of the unit disc. Were it the

only requirement,

it could be satisfied

by

a

simple change

of

sign, just

as

was done for the x coordinate.

However,

the

expression (4)

for the y coordinate

gives

a correct

representation

in the I and the IV

quadrant

of the

complex plane,

instead of the I and II

quadrant.

To resolve this

problem,

we must «rotate» the solution function counter-

clockwise

by

w/2. The

required

function for y is found

using

the

procedure

described in

[14].

The new

equation

for y, obtained from

integral

231.00 in reference

[20],

which satisfies the convention

conceming

the branch of the square root is

y

(u,

v

)

=

KgxRe iF

(q~y,

kx)i

where the

expression

for

q~~ is derived from that for q~~ in the first row of table IIb

by changing signs

of all

quadratic

terms. In other

words,

the

relationship

between

q~~ and

q~~ is

~y(W )

" ~x

(I

W

).

(11)

Further,

it is convenient to use

polar

coordinates instead of the Cartesian. Hence, for

given lengths

a and c of the

edges

of a

right tetragonal prism

it is necessary to find the value of the free parameter

(conveniently

chosen from among

E, fl

and

A),

from

(8). According (4)

and

( lo),

the coordinates of the

appropriate

tD saddle surface

spanning eight

of the twelve

edges

of

a

right tetragonal prism

are

x(r,

0

= ±

~ Re

[F (arcsin ll'~(w ), k~)]

2

K(k~)

y

(r,

0

= ±

£

' Re

IF (arcsin

~l~~ (< w

), k~) I1)

2

K(k~)

z(r,

0

=

£

' Re

iF (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, the

plus sign

relates to

right

half and the minus

sign

to left half of the

complex plane.

In the

expression

for y, the

plus sign

relates to upper half and the minus

sign

to lower half. In this way, we arrive at

parametric equations

of the normalized tD

family.

Unfortunately,

there is no true addition formula for F

(q~, k)

with a

complex amplitude,

so

that F

(u

+ iv,

k)

cannot be

expressed

in terms of F

(u, k)

and F

(iv, k) only.

It is therefore

impossible

to separate the real and

imaginary

parts, and

parametric equations (11)

cannot be

simplified

further.

Consider the

limiting

behaviour of the

parametric equations

when the free parameter

approaches

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)

the

moduli k~ and k~ in

equations (4)

are 0 and I

respectively,

and therefore the

appropriate

functions F (q~,

k)

reduce to

elementary

functions. Since the

multiplication

constants are finite, the

equations

are

expressed

in terms of

elementary

functions

only,

and describe surface with the cla ratio

approaching 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 that

equations (4)

derived with the

assumption

A

~ 2 can be extended to the

limiting

case of A

= 2.

The

elliptic integrals

in II are finite in the entire

complex plane,

even at

points

defined

by

(2).

This means that F

(q~, k)

is finite at

singular points

of the Weierstrass function

(3).

This is

particularly important,

in view of the fact that numerical estimation of

integrals

fails close to the

singularities.

No

expressions

for the

approximate computations

of tD surfaces are known. It is clear that

they

can be deduced from

equations (11) by

an

appropriate approximation

of the

incomplete elliptic integrals

of the first kind

by elementary

functions. This

procedure

deserves additional

analysis,

but an

approximation

for z

immediately

suggests itself. Thus for A ~ 2 the values of the modulus k~ in the

expression

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 of

elementary

functions with a

high

numerical accuracy. Since

F(q~, k)

m q~ for small

k,

we have

z m

~ Re arcsin I

2

K(k~) g/

(12)

With w = r cos 0 + ir sin 0 the real

part

is

explicitly

found as

z 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 7

significant figures

on the entire unit

disc,

and for A « 000 to as many as 15

significant figures.

It is even

possible

to

approximate

the coordinate, albeit less

accurately, using only

the

quadratic

function

c ~

w~

~ 2

K(k~)

~

fi

and hence

~

~K~k~)fi~~~~~~~

Computation

of tD surfaces.

Since sketches

[26]

and

photographs

of models

[27]

of tD surfaces cannot be

regarded

as

quantitative, drawings [15]

obtained

using

the

Enneper-Weierstrass representation

are the

only

known case of their

computation.

Reference

[15] gives

the Cartesian coordinates for

A

=

2.01, 3,

14 and 50 obtained

by taking

the real

parts

of

complex integrals (our Eqs. (I)

and

(3))

defined on the unit disc.

Computation

of a tD surface

using

the

Enneper-Weierstrass representation requires

numerical

integration

to evaluate

hyperelliptic integrals,

and cannot be carried out without

prior analysis

of the behaviour of the

integrands

and the choice of an

appropriate

numerical

method from among a number which are available. For direct

comparison,

we have

performed

such

computations

for tD surfaces described below. These

computations

are

quite

cumbersome and

require

a careful

interpretation

of data in the

vicinity

of

singularities

of the Weierstrass

function,

since

large portions

of the surfaces are

generated by

small

regions surrounding

these

singularities. However,

the main weakness of

using

the

Enneper-Weierstrass representation directly

is that surfaces

corresponding

to a

specific

value of A

computed

from them cannot be

applied,

In other

words,

without the

knowledge

of

K and x

(neither

of which can be deduced from

it),

the

Enneper-Weierstrass representation

does not tell us how to

generate

a surface to match

prescribed

data.

Also,

it is

impossible

to compare different tD surfaces without

normalization.

By

contrast,

parametric equations (11) require

the evaluation of functions F

(q~, k)

and

K(k)

which is much

easier,

and

yield

all information

required

for

matching,

thus

making straightforward physical applications possible.

We use them to

compute

tD saddle surfaces for several

prescribed

values of the axes ratio.

The evaluation of the functions

F(q~, k)

and

K(k),

is now

usually

based on the Gauss

algorithm

of the

arithmetic-geometric

mean and Landen's transformation

[21, 23, 28]

and Carlson's

algorithm [29].

The latter is

implemented

in

NAG,

SLATEC and IMSL numerical

libraries.

However,

we use the Gauss

algorithm

because its use for the evaluation of

F(q~,

k) for

complex

values of

amplitude

is well documented. In order to demonstrate the

simplicity

of this

algorithm,

we outline it below. The

arithmetic-geometric

mean of two

numbers ao and

bo (where bo

is any

complex

number different from 0 and from

JOURNAL DEPHYSIQUE i T 2, N' 12, DECEMBER <992 79

(13)

ao),

is denoted

by AG(ao,bo),

and defined as the common limit of the arithmetic

(a,)

and

geometric (b;)

sequences

~< ~

~' '

j

~~ '

~i

~

~i

with I

=

1, 2, 3,

Both sequences are convergent for any choice of ao and

bo.

After

reaching

the

prescribed

accuracy at the n-th iteration step

(I,e,

difference between a~ and b~ is less than the

required value), AG(ao, bo)

can be

approximated by

a~ m

b~.

To calculate

K(k)

for any

particular

value of k we start from

ao =

I

bo

=

/$.

After n iterations we have

~~~~

2 AG

ao, bo)

~j~

To calculate F

(q~, k)

for any

particular

values of q~ and k we start from

ao =

I

bo

=

k(

=

/$

q~o = q~

and

by using

Landen's

descending

sequence

k)

j

~ ~ ' ~ "~~~~

~~

' ~~' ~

'~

~~~~ ~~

l +

k)

_,

where I

=

1, 2,

..., n,

together

with the

arithmetic-geometric

mean

algorithm.

After

prescribed

accuracy is reached at n iterations we have

~

~~' ~~

2~

AG(ao, bo)

2~ a~

The

algorithm

is

simple

and very fast

(it

converges

quadratically)

so that numerical accuracy to 7 and 15

figures

is

usually

reached at the

4th,

and 8th iteration

step, respectively.

Its

only

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. The

length

of

edge

a is assumed to be I and all

quantities required

in the calculation are

given

in table V.

Table V. Constants used in the

computation of

the various saddle tD minimal

su~fiaces for different

values

of

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

(14)

Tables VIa-c list

only

the coordinates of one

eighth

of each saddle surface. These minimal surface

pieces

are

asymmetric 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 divided

using

a 8 x 5

grid

where the coordinates of

grid points

are

given 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 a

complete

tD saddle surface can be obtained

by symmetry

considerations alone. Coordinates of surfaces

corresponding

to the same value of x but different values of

a can b£ obtained

by multiplying

the coordinates in tables VIa-c

by

a.

Table VI. Cartesian

coordi~ates of

three

different

tD

su~fiaces.

The columns

differ

in

n~ 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)

(15)

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 discussions

conceming

the

properties

and

computation

of

elliptic integrals.

References

[I SCHWARz H. A., Gesammelte Mathematische

Abhandlungen (Verlag

Julius

Springer,

Berlin, 1890) vol.1.

[2] SCHOEN A. H., Infinite Periodic Minimal Surfaces Without Self-intersections, NASA Technical

Report

No. TN D-05541 (1970).

[3] FISCHER W. and KOCH E., J.

Phys.

Colloq. France 51 (1990) C7-131-147.

[4] ANDERSSON S., HYDE S. T., LARSSON K, and LIDIN S., Chem. Rev. 88 (1988) 221-242.

[5] SCRIVEN L. E., Nature 266 (1976) 123.

[6] MACKAY A. L., Nature 314 (1985) 604-606.

[7] MACKAY A. L.,

Physica

131B (1985) 300-305.

[8] HYDE S. T. and ANDERSSON S., z.

Kristallogr.

168 (1984) 221-254 170 (1985) 225-239.

[91 MACKAY A. L. and KLINOWSKI J.,

Computers

and Mathematics with Applications 12B (1986) 803- 824.

[10] SADOC J. F. and CHARVOLIN J., J.

Phys.

France 47 (1986) 683, 48 (1987) 1559.

[ll] DARBOUX G., Thdorie Gdndrale des Surfaces, vol. I (Gautier-Villars, Paris, 1887).

[12] DO CARMO M. P., Differential

Geometry

of Curves and Surfaces (Prentice-Hall,

Engelwood

Cliffs, NJ, 1976).

[13] NITSCHE J. C. C., Lectures on Minimal Surfaces, vol. I

(Cambridge University

Press, 1989).

[14] CviJovit D., KLINOWSKI J., J. Phys. J France 2 (1992) 137-147.

[lsl LIDiN S. and HYDE S. T., J. Phys. France 48 (1987) 1585-1590.

[16] FOGDEN A., Ph. D. Thesis,

Department

of

Applied

Mathematics, ANU, Canberra (1991).

[17] KOCH E. and FISCHER W., z. Krist. 183 (1988) 129-152.

[18] GERGONNE J. D., Ann. Mathem. p. appl. 7 (1816) 68, 99-100 and 156.

[19] SCHWARz H. A., Monatsch. Berlin Akademie 3-27

(11January

1872).

(16)

[20] BYRD P. F. and FRIEDMAN M. D., Handbook of

Elliptic Integrals

for

Engineers

and Scientists, 2nd Edition,

Springer-Verlag, Berlin-Heidelberg-New

York

(1971).

[21] MILNE-THOMPSON L. M., Handbook of Mathematical Functions, M. Abramowitz and I. A.

Stegun

Eds. (Dover Publications Inc., New York 1980) ch.17.

[22] Reference [13], p. 234 and

figure

25.

[23] PRESS W. H., FLANNERY B. P., TEUKOLSKY S. A. and VETTERLING W. T., Numerical

Recepies

The Art of Scientific

Computing (Cambridge University

Press, 1986).

[24] ANDERSON D. M., Ph. D. Thesis,

University

of Minnesota (1986).

[25] Reference [13], p. 128 and

equation

(80).

[26] Reference [I], p. 126 and

figure

4 reference [I I], p. 430 and

figure

21.

[27] Reference [2],

figure

6 reference [4],

figure

12(c).

[28] BULIRSCH R., Namer. Math. 7 (1965) 78-90.

[29] CARLSON B. C., SIAM J. Math. Anal. 8 (1977) 231-242.

[30] FOGDEN A. and HYDE S. T., Acta

Cryst.

A 48 (1992) 442 and 575.

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