Physica 45 (1969) 33-66
0 North-Holland Publishing Co., Amsterdam
BRAVAIS TWO-DIMENSIONAL
CLASSES
OF
RELATIVISTIC
LATTICES
A. JANNER Instituut VOOY theoretische Fysica, Katholieke Universiteit, Nijmegen, Nederland and E. ASCHER Battelle Institute, Advanced Studies Center, Carouge-Genive, Suisse Received
14 February 1969
synopsis Repetition of motifs in space and time gives rise to regular patterns with syrnmetries described by relativistic crystallographic groups. This leads to natural generalizations of concepts familiar in Euclidean crystallography. Here only the twodimensional relativistic case is considered. Conditions are derived for a Lorentz transformation to be crystallographic, i.e. to leave invariant a lattice in the twodimensional Minkowskian space. The introduction of crystallographic transformations that change the sign of the indefinite metric tensor appears to be a necessary step in relativistic crystallography. The corresponding concepts of the theory of binary quadratic forms and of real quadratic fields are briefly discussed. A classification of all possible relativistic two-dimensional lattices is given and the corresponding Bravais classes are derived (at least in principle, as there are an infinite number of them). Isotropic lattices (i.e. with lattice points on the light cone) and incommensurable lattices (i.e. with incommensurable metric tensor) have as holohedry a point group of finite order. The other ones, which are described essentially by metric tensors g(B) = (a, b, c) with relatively prime rational integers a, b, c and discriminant d = b2 - 4ac not a square, always have a holohedry of infinite order. A number of lattice representatives of Bravais classes ordered according to the kinematical interpretation of the Lorentz transformation is given in the appendix. 1. Introduction. Periodic repetition of an arbitrary (finite) motif in space gives rise to patterns having crystallographic space groups as symmetry groupslls). H omo g eneity of empty space, or in other words, covariancy of physical laws with respect to the Euclidean translation group, is a necessary condition for the existence of crystals. This property, which makes possible the existence of the same motif of matter (e.g. molecule) at different places, is of course not sufficient for ensuring the existence of crystals, but makes this existence not at all surprising. 33
34
A. JANNER
AND
E. ASCHER
Actually physical laws are covariant with respect to the inhomogeneous Lorentz group, which includes the Euclidean translations as a subgroup. In the same way as above, this fundamental property makes very plausible the existence in nature of periodic repetition of some (finite) motif in space and time. We call such four-dimensional patterns space-time crystals, which then have the symmetry of relativistic space-time groups 3). Periodic motions on the one hand, and static (three-dimensional) crystals on the other, are degenerate cases of space-time crystals, as they give rise to infinite space-time unit cells. To get a finite unit cell, one may consider the combination of the two previous examples in the form of some crystal vibrating in a given mode, which then has the symmetry of a space-time group. From a general point of view, however, this example may represent too simple a case. Further analysis of the problem of finding out the possible physical manifestations of space-time crystals shows that one has to look into kinematic symmetries in distributions of matter (like e.g. those of conduction electrons in metals). It is then clear that if the typical velocities occurring in such distributions with respect to the centre of mass are small compared to the velocity of light, one has to consider the non-relativistic limit, i.e. what we call Galilean space-time groups. These groups have very peculiar features, and will form the subject of a subsequent paper. Our lack of a synthetic intuition of physical phenomena in space and time together, and the incredible richness of relativistic crystallography (as compared with the Euclidean one) make it advisable not to start thinking about possible space-time crystals before having some basic knowledge of space-time groups334). In our opinion this is also true if one is interested in another fundamental question, namely that of the existence of a fundamental length in nature. If such a length does exist and space-time is homogeneous no more, then one expects that some type of crystallographic description of matter in space-time is not only possible but even necessary. This is in fact what can be observed already in the current literature where a lattice is associated to the fundamental lengths-g). However, we should like to underline the fact that matter can very well be arranged according to the symmetry of space-time groups even if there is no fundamental length. We begin now to have a first view of relativistic crystallography and this paper is the first one devoted to the two-dimensional case (one timedimension, one space-dimension). In two dimensions everthing can be done explicitly. This is no more the case in higher dimensions, in which (for the moment) only some families of groups can be derived. The interesting point is that even in two dimensions and because of the richness of the indefinite metric case, it is much more easy to grasp general laws than in the positive definite case. More than that, a two-dimensional crystallography appears which may be formulated completely in terms of
TWO-DIMENSIONAL
RELATIVISTIC
LATTICES
35
arithmetic functions independently of the character of the metric. We consider this as a main result. Even the case where the determinant of the metric tensor vanishes, which arises in the limiting case of Galilean spacetime, is correctly described in such an approach. In this paper, however, we consider only the relativistic case. The comparison between the relativistic and the Euclidean case will be made elsewhere. Elsewhere also we hope to be able to discuss the interesting relations between relativistic crystallographic groups and Lie groups. In the Euclidean case such relations play an important role in the classification of complex semi-simple Lie algebras and in the representation theory of linear Lie groups lo-14). 2. Relativistic lattices and crystallographic Lorentz transformations. Given the two-dimensional Minkowskian vector space V with metric tensor 0
( >
g(B)= ;
__1
(we put for the velocity of light: c = l), and orthonormal We consider a basis B’ = (ei, ei) = BS defined by
4 =
we1
+
s2le2
eH = s12el + s22e2
basis B = (ei, es).
with
(2.1)
and the lattice generated by B’ A(B’)
= {zlei + zzee 1.~1,.z2 E Z}.
The lattice A(B’) is a set of vectors in V. If T is a unimodular transformation, T E GL(2, Z), then A(B’T) = A(B’). We shall write simply A when it is not necessary to specify the basis. GL(2, R) and GL(2, 2) are the groups of real and integer non-singular two-by-two matrices, respectively. The metric tensor corresponding to the basis B’ is given by g(B’) = Stg(B) S.
(2.2)
One finds:
a
2 Sll tw')
=
4
( SllS12 - SZlS22
SllS12 - s21.722 De* XI= 2 s12 - G2
ii) and of course det g(B’) -C 0, which means that d !?F?b2 -
4ac > 0.
The quantity d is called the discriminant of (a, b, c). Those Lorentz transformation are crystallographic
b 5
b z
c
!!Zf(a, b,c)
(2.3) (2.4)
that are unimodular
36
A. JANNER
with respect to a certain L’ = s-lL.s,
AND E. ASCHER
basis B’, i.e. :
with
L E O(l, l),
for some S E GL(2, R). Since by definition: L’tg(B’)
(2.5)
Ltg(B) L = g(B) it follows that
L’ = g(B’).
The unimodular generated
L’ E GL(2,Z)
(24
character
of L’ ensures
by B’ under this Lorentz
the invariance
transformation,
of the lattice
n
so that we may write:
L’A = A.
(2.7)
Any set of transformations (Li, LB, . . ., Li} satisfying the above three relations generates a relativistic point group K which is a subgroup of GL(2, 2) and leaves n invariant. The largest point group H leaving a given lattice invariant is called its holohedry. Two metric tensors g(Bi) and g(Bz) are arithmetically equivalent g(Bl) A g(Bz) and belong to the same arithmetic class if g(Bi)
= SWz)
S
whereas the arithmetic KIZKK~
if
for some equivalence S-lKIS
S E GL(2, Z),
(2.8)
of point groups is given by
= KZ
for some
S E GL(2, 2).
(2.9)
Relation (2.9) means that K1 and Kz are two conjugate subgroups of GL(2, 2). To a given lattice there corresponds the whole set {B’S /S E GL(2, 2)) of its possible bases, and thus an arithmetic class {g(B’)} of metric tensors and also an arithmetic class {K] of point groups. The concept of Bravais classes arises from the fact that whereas a lattice II determines the arithmetic class class determines a Bravais class of of its holohedry {H), an arithmetic latticesrs). Two lattices belong to the same Bravais class if they have arithmetically equivalent holohedries : n,E.&
if
HI & HZ.
As the dimension of the space is even, it is possible to consider lattices
(2.10) with
orientation, and oriented Bravais classes. In this case conjugation occurs with respect to an element of SL(2, Z), the subgroup of proper elements of GL(2, 2) 15). In this paper we shall consider oriented lattices. If the holohedry of such a lattice is a subgroup of SL(2, Z), then its arithmetic class splits into two proper arithmetic classes and two enantiomorphic lattices A and ,4’ belong to the same (non-oriented) Bravais class, where rl’ arises from n by changing orientation. If the holohedry of II is not a subgroup dSL(2,Z) then ,4 = II and the lattice is called ambiguous. Further on we shall discuss this in greater detail and in a more general frame. The holohedry H of a lattice is determined by the metric tensor of any
TWO-DIMENSIONAL
lattice
basis B’, because
L’@I’)
RELATIVISTIC
LATTICES
37
the relation with
L’ = g(B’)
L’ E GL(2,Z)
(2.11)
is a necessary and sufficient condition for L’ to belong to H. But a metric tensor does not determine a single lattice, because it simply fixes the length and the relative position of the two basis vectors. Thus bases Bi and Bz (and therefore lattices rli and As) obtained one from the other by a Lorentz transformation: Bz = BlL, g(Bz) = Ltg(B1) L = g(B1)
with
L E GL(2,Z)
(2.12)
determine the same metric tensor. One says that B1 and BB, and the respective lattices Ai and As, are relativistic-geometrically equivalent (B1 25 Bz; Al 25 A,). Two lattices then belong to the same relativistic geometric class if they differ simply in the frame of reference. From (2.11) and (2.12) one arrives at the conclusion that relativistic-geometrically equivalent lattices belong to the same Bravais class. Consider now any lattice. It contains a space-like vector which can be taken as first basis vector ei. Then &ills = a > 0. In other words a lattice determines an arithmetic class of metric tensors; in this class there is always a metric tensor g(B’) = (a, b, c) with a > 0. This means that if a is negative, one has to go over to an arithmetically equivalent metric tensor in order to meet the requirement. By taking another representative of the Bravais class of the lattice considered above, it is always possible to have the first basis vector ei in the space direction ei. This fixes the basis B’ (and the lattice A) according to: ei = Ja
er;
b 42 = z~d.
a +
d 2Ja
(2.13) e2.
By this procedure, to each lattice A a metric tensor (a, b, c) with a > 0 is associated. Henceforth (if nothing else is explicitly stated) we shall always adhere to the choice (2.13). The condition (2.5) for L’ to be a proper Lorentz transformation leaving A invariant becomes : S-_lLS
=
L’
=
0 au
w
where
L=&
cash x
sinh x
sinh x
cash x ’
-0.4
Hn + bu)>
s=
E GL(2, 2)
(2.14)
38
A. JANNER
AND E. ASCHER
with n = f2 cash x and u = f ,/{(ns - 4)/d} with sign u = sign x. This means that ti and u are solutions of the equation ns -
du2 = 4
(2.15)
expressing the condition det L’ = + 1. One easily verifies that in fact L’ of (2.14) leaves invariant g(R’) = (a, b, c). Let us remark that the only transformations L’ of finite order are those associated with the trivial solutions u = 0 and n = 12, i.e. the identity E and the total inversion Improper Lorentz transformations are of the form cash x
ikiT=* therefore
S-lMS
-sinh
x
sinh x -cash
traceless. Referred
=
n/irl
=
-E.
to the lattice basis B’ of (2.13), they become:
i Hn+ w \-CXU
x ’
-cu+$(n+bu) -&(n
+ bu)
J
Note that M’ is always of order two and can be written as:
(2.17)
with L’ as in (2.14). Therefore if a divides b and L’ leaves A invariant, then so does A!f’, and A is ambiguous. A metric tensor g(B’) = (a, b, c ) is called integral when a, b, c are rational integers. If furthermore a, b, c are relatively prime, then g(B’) is called primitive. The lattices corresponding by (2.13) to these tensors also are called integral or primitive lattices. We now formulate a property that is of fundamental importance in relativistic crystallography. Proposition 1. Each Bravais class of lattices that have holohedries of infinite order contains a primitive lattice; at most two primitive lattices are contained in such a class. Proof. We first show that there is a primitive lattice. According to the hypothesis, there is in the Bravais class a lattice II, with g(B’) = (a, b, c) with some a, b, c E R, left invariant by a L’, as in (2.14), with u # 0. We may suppose u > 0; otherwise we consider L’-1 instead of L’. Note that lattices differing only by a positive scaling factor are invariant with respect to the same point groups and belong to the same Bravais class. Therefore g(uB’) = (au, bu, cu) defines by (2.13) an integral lattice ZUI that is in the same Bravais class as A. Consider the greatest positive divisor k of au, bu and cu. Then uA/k is primitive and is in that same Bravais class. For g(uB’/k) we write again (a, b, c) but now a, b, c E 2 are relatively prime.
TWO-DIMENSIONAL We
show that class. Let
now
Bravais
L’ =
B
there
RELATIVISTIC
LATTICES
are at most two primitive
39
lattices
in a same
( > OL
6
ESL(2, -q
Y
be a proper Lorentz transformation of infinite order leaving primitive lattice with g(B) = (a, b, c). Then by (2.14) one has S -
y = au,
-p
01 = bu,
= cu
invariant
a! + 6 = n
and
a
(2.18)
implying /U/= gcd(y, 6 -
(Y, +3)
E2
i.e. u is the greatest common a > 0, one has to take:
(u # O),
(2.19)
divisor of y, S -
ill and -/3. In order to have
sign U = sign y.
(2.20)
By (2.18), (2.19) and (2.20), together with (2.13), a primitive lattice with metric tensor g(B) = (a, b, c) is uniquely determined. L’ leaves invariant also --g(B) = (- a, -b, -c) which defines an inverse lattice d of A (see section 4) and possibly A + A. Corollary 1.1. Every element L’ E SL(2,Z) crystallographic Lorentz transformation referred primitive lattice. Corollary transformation L,
=
1.2. The general is :
:(a -
w
with (tr L’I > 2 is a to the basis (2.13) of a
form of a proper crystallographic
-cu
a26
Lorentz
(2.21a)
3(n + bu) >
for any a, b, c E 2 such that gcd(a, b, c) = 1 and a > 0, and for (1z, U) any integral solution of the Pell (plus) equation: nz -
d~z = 4 9
where
d = b2 -
4ac > 0.
(2.21b)
In this way we arrive at the theory of indefinite binary quadratic forms and of real quadratic fields, which of course are nothing else than other aspects of the same thing. The formulation of this matter in crystallographic terms is precisely the aim of this paper. From the theory of binary forms and quadratic fields we therefore mention only a minimum number of essential points. Consider the indefinite quadratic form : f(x, y) = ax2 + bxy +
cy2 Ef
[a,b, cl,
VX,YEZ a, b, c E R
(2.22)
40
A. JANNER
AND
E. ASCHER
with discriminant d = b2 -
4ac > 0.
One says that
the real numbers
f(x, y) are represented
by the
quadratic
form [a, b, c]. Clearly, one may make a lattice rl in the hyperbolic plane associated with the metric tensor g(B’) = (a, b, c) correspond to the set of numbers represented by [a, b, c]. The number f(x, y) then expresses the distance between the origin and a lattice point P with coordinates x and y with respect to the basis B’ of (2.13). We may say that the lattice il is represented by the quadratic form [a, b, c]. One has the following properties. Proposition 2. equivalent quadratic forms (i.e. conjugated in 4 Two arithmetically GL(2, 2)) represent the same set of numbers. b) To quadratic forms that are conjugated in SL(2, 2) there corresponds one single (oriented) lattice. 4 To quadratic forms that are conjugated by an improper element of GL(2,Z) there correspond two lattices, one of which is the mirror image of the other (with respect to the first basisvector). The two enantiomorphic lattices may coincide (ambiguous case). Proof. See Bachmannle), pp. 100-l 17. Conjugate of quadratic forms occurs as for metric tensors after identification of [a, b, c] with (a, b, c). Suppose now a
At
b
5
b
z
a
A=
c
b
-5
i- 2
(2.23)
1,
b c
then any A E GL(2, R) satisfying (2.23) defines an automorphism of the quadratic form (a, b, c), and any A E GL(2, 2) satisfying (2.23) an automorph of the same form 17).Comparison with (2.12) and (2.11) shows that Lorentz transformations are automorphisms, and the crystallographic ones automorphs of the quadratic form defined by the metric of the basis vectors (and vice versa). Actually, in order to obtain the relativistic Bravais classes one needs a generalization of these concepts, as is done in section 3. But before doing this, we add a few remarks on real quadratic fieldsIs? 19). Consider the real quadratic field Q(,/D) generated by JD over the rationals Q, where D is a positive rational integer (D > 0). We assume D is not a square, but it may have square divisors. The square-free part is noted by Do. One has:
QW)
= Q(JDo)
where
D = q2Do,
q EZ.
(2.24)
TWO-DIMENSIONAL
Any element 1=
RELATIVISTIC
3, E Q(,/D) can be written
41
LATTICES
as
zl+zzJD
(2.25)
v.21, 22, 23 EL-.
> z3
The uniquely 1’ =
defined element :
21 -
ZdD
(2.26)
23
is called the conjugate of il. A norm N and a trace S are defined by N(A) !kf Lil’
and
(2.27)
s(n) !zf il + 2’
with properties N(ilIit2) = N(1r) N(jZ2) ;
N(A) = N(A’);
S(A1 + 12) = S(Al) + S(&);
S(M)
N(A) = 0 o ;z = 0
= kS(1)
for
k E Q.
(2.28)
Quadratic integers v are defined as those elements of Q(JD) which have rational integral norm and trace. One showsI*) that they form a ring and are of the form : v=
.a + a& a, 22 E.z-
2
where d is the discriminant d=
(2.29)
'
of Q(JD)
given by
40
if
D = 2 or 3 (mod 4) ;
i D
if
D = 1 (mod4).
(2.30)
The quadratic field Q(JD) will also be denoted by Q(Jd). The quadratic integers of Q(JD):that have an integer inverse are called units of the quadratic field. They have norm f 1 and form a group under multiplication, called the group of units. Accordingly units are given by &=
eu,ld
where m, u E 2 are solution 122 -
(2.31a)
2
dus = &4.
of the (plus, minus) Pell equation: (2.31b)
It is now possible to indicate the relation between quadratic fields and twodimensional relativistic crystallography. Relativistic Bravais lattices having holohedries of infinite order can be brought in correspondence with Z-modules J of quadratic integers. Consider the Bravais lattice II defined by the basis B’ of (2.13) with primitive metric d = b2 - 4ac > 0. The tensor g(X) = (a, b, c), a > 0 and discriminant correspondence is then indicated in the following table (2.32).
A. JANNER
42
AND E. ASCHER
TABLE (2.32) Correspondence between relativistic Bravais lattices and Z-modules in real quadratic fields Minkowskian vector space V basis
Real quadratic field Q(JD)
Discriminant
el, JD e2 2Ja A
1, w Dz,/D
d = 40
lattice or module
A! = [2a, b + co]
d = 4q2Do
basis
el, Hqel + JD es)
l,o%Afi(q+,/‘D)
d=D
lattice or module
Ju A
d = q2Do
In the case d = D one has a = b (mod 2) = q (mod 2). The correspondence is such that if I E Q(,/D) corresponds to I E V, then N(A) = 11Jl12;
S(n) = 2Z.ei.
(2.33)
Note that 2Ja rl, as well as Ju n are lattices in the same Bravais class as A. Comparison of (2.31) with (2.21) shows that for a given primitive lattice (a, 6, c), crystallographic proper Lorentz transformations L =
Q(n - ba) a24
-cu Hfl + bu) >
are in one-to-one correspondence Q( JO) given by : & = j&z -
with the positive
units
(N(E) = + 1) of
uJd).
In this way we see that proper crystallographic Lorentz transformations and relativistic Bravais lattices (in the primitive case) appear as elements of one and the same quadratic field. The interpretation of negative units (N(E) = - 1) will b e indicated in the following section. 3. The g-uutomor$hs. We first consider the case of real (a, b, c), later on that of primitive (a, b, c), and we identify quadratic forms with corresponding metric tensors. An automorphism X of a real indefinite c is an element of GL(2, R) such that g(B) = (a, b, ) Definition. XW)
X = g(B),
X E GL(2, R).
Definition. A negautomorphism X of a real indefinite g(B) is an element of GL(2, R) such that: XW)
X = -g(B),
metric
X E GL(2, R).
tensor (3.1)
metric
tensor (3.2)
TWO-DIMENSIONAL
If no distinction
RELATIVISTIC
is made between
43
LATTICES
automorphism
and negautomorphism
we
speak of generalized automorphisms (or simply of g-automorphisms). In the case of g(B) = (1, 0, - 1) we have the following possible general parametrization of g-automorphisms for I# E R: cash 4
(
zt L(4) = f f
M(4)
= +
*
A(&
=&
sinh
(
proper automorphism
sinh + cash I#>
d
cash 4 _ sinh #
sinh q5 -cash
r$>
transformation)
;
improper
automorphism
(Lorentz
mirror) ;
improper negautomorphism;
y;;)
:;;
(Lorentz
(3.3a) (3.3b) (3.3~)
( cash r$ -sinh
$>
proper negautomorphism.
(3.3d)
In what follows we shall use the letters L, Ikl, A, N, for the above gautomorphisms. One easily verifies the following relations : A(h)
A(42)
=
A(42)
A(h)
=
L(f$l +
52);
Wl)
L(42)
=
W2)
L(h)
=
q+1+
+2j;
M(h)
Jf(42)
=
W(#2)
Jf(41))-1
=
L($z
-
41);
N(h)
N(42)
=
W(42)
N(h))-1
=
--L($z
-
41);
A-l@)
=
A(-$),
M-W
=
J,f(#f
therefore
N-l(+)
= -IV($),
therefore
L-l($)
=
q-4);
AP(#
=
1;
W(4)
= -1.
(3.4)
The result of conjugation of a g-automorphism Xi by another g-automorphism X2, i.e. the element X;lXiX2 is indicated in the following table. TABLE (3.5) Conjugations of g-automorphisms conjugated by
We
I
LZ
A2
M2
N2
Ll
Ll
Ll
Lil
Lil
Al
Al
AI
-Ai1
-Ai1
MI
ML.;
-MIA;
MzMlMz
-Ml
NI
NIL:
-NlA;
-NI
- NzNlNz
metric
tensors.
g-automorphism
now go over to primitive
44
A. JANNER
AND
E. ASCHER
Definition. An automorph Y of a primitive metric tensor g(B) = (a, b, c) with a > 0, is an element of GL(2, 2) such that YW)
Y E GL(2, 2).
Y = g(B),
Definition.
A negautomorph
(3.6)
Y of a primitive
metric tensor g(B) as
above is an element of GL(2, 2) such that: Y%(B) Elements
Y E GL(2, 2).
Y = -g(B), of GL(2, 2) satisfying
(3.7)
(3.6) or (3.7) are called g-automorphs
g(B)* Before discussing the basic properties of automorphs we introduce metic functions pk(a) defined by the recurrence relation: fit+&)
=
qbc(fin) -
Vrt, kE.Z
Pk-l(fi),
of
arith-
(3.8a)
and the initial values:
$0(n) = 0, Furthermore A$&)
Pl(%) =
VrtEZ.
1,
(3.8b)
we define : =‘fifi+l(fi)
also obeying
-
the recurrence and
A$o(%) = 2
Vn, keZ
$,-I(@,
(3.9)
relation (3.8a) but now with the initial values: Afir
vnez.
= 1~7
(3.10)
The detailed properties of these functions will be discussed elsewhere. Let us here mention only a useful parametrization in term of trigonometric and hyperbolic functions. For any n E Z, consider + E R with + > 0 such that (sign n) 2 cash + 2 cos I#
if
InI 2 2;
if
lfil I 2.
(3.11)
Then 2 cos k+ = A$k(n);
for
In’ L 2 2 sin k$ = J(4 -
(3.12a)
ns) fik(n)
and 2 2 cash k+ = Apk(n);
n,
for
2 sinh k+ = J(d
-
with $k(-n)
= (-
-
l)k+rfik[n) and dfir(--~)
(3.12b)
4) p,(n), = (-
l)kdfk(n).
Note that Afik(n) and *k(n) are solutions of the Pell (plus) equation of discriminant d = ns - 4: A&n)
-
Proposition
(nz -
4) p:(n)
(3.13)
= 4.
3. A proper automorph
L of a primitive
g(B) = (a, b, c)
TWO-DIMENSIONAL
can always be written L=&L;=*
RELATIVISTIC
LATTICES
45
as: #zl-bul)
-cu
i&k--b%k)
-c%k
au1
&l+bw)
a%k
@k+b%)
>’
(3.14) where
(121, ur) is the least positive
discriminant
d = b2 -
ns -
dus = 4
nk
&k(Q),
solution
of the Pell (plus) equation
of
4ac > 0:
and =
uk =
(3.15)
fh$k@l).
We call LO the fundamental Lorentz transformation (of g(B)). Proof. For any given primitive g(B) = (a, b, c) there is a one-to-one correspondence between positive units E of the quadratic field Q(,/d), where d = b2 - 4ac, and the proper automorphs L of g(B) : L =
t@ au (
4
--GsfT 3(a + bg) >
0 E = $(n + uJd).
(3.16)
We now show that Lk is given by Lk =
&(nk
-
buk)
--cuk +k
auk
+
buk)
>
where nk
=
and
&k(n)
uk
=
f@k(fi).
For k = 1 the statement is trivially true. Suppose it is true for k for Lk one finds the above expression with %k
=
$(flk-1
n
uk
=
i(uk-ln
where, according ns -
uk-1
ud),
+
uk-1
+
flk-1%))
to the induction
dzG = 4,
n;_r
-
hypothesis: = 4,
du;_l
nk-1
=
A$k--l(B)
Zdpk-l(n).
=
Using the relations : +k,+d’d A#‘k,+k,(n)
= +&,(@
Ai’h(rt)
=
A+,@)
+ AZk(“d
=
i(A+k,(n)
A#k,(n)
+
(n2
=
+(bk,(n)
A#k,(n)
+
f’k,@)
which are a simple consequence nk
and
1, then
@k
of (3.12), =
@‘k(n).
#k,(n))t -
4) !‘k,(@ f’k,(fi)
@d),
one finds :
#k,(@))
=
and
A. JANNER
46
In exactly
AND E. ASCHER
the same way one proves that
&k = &(Yzk+ UkJd). It follows that Lk corresponds Any positive unit of Q(,/d)
to $. can be written as E = &.$, where ~1 is the
fundamental
obtained
(positive)
unit
(tir, nr) of the Pell equation morph of g(B) is given by:
from
the
least
positive
solution
(see e.g. ref. 18), so that any proper
auto-
L = fLt with LO the fundamental Lorentz transformation (of g(B)). Note that in our case lrtil > 2 if d is not a square. Lorentz transformations LO and Corollary 3.1. The crystallographic L = fLi of (a, b, c) are in correspondence uniquely to ~1 = +(+zr + ulJd) the fundamental (positive) unit of Q(Jd), and to E = &E!, respectively. Corollary 3.2. An improper automorph can always be written as &(fik +
M=+M,,L;=f
buk)
--auk
M of a primitive g(B) = (a, b, c)
--cuk
+
-&(fik
& +
(wk +
buk)
(3.17)
buk)
where
and ?&k,%&uk: as above. Proof. Consider (2.16) and (2.17). The negautomorphs can be treated in the same way, with an important restriction, however; we have to consider only those primitive g(B) for which there are negautomorphs. The explicit conditions therefore are discussed further on. Let us, for the time being, merely underline the fact that there are (oriented) lattices that admit proper negautomorphs but no improper ones. (See section 4.) We first introduce new arithmetic functions qk(??%)defined by the recurrent relation : qk+l(m)
=
mqk(m)
+
qk-l(m),
Vm,kcZ
(3.18a)
V9nE.z.
(3.18b)
and the initial values: 40(m) = 0, Furthermore &r(m)
41(m)
=
1,
we define sf qk+l(m)
+
qk-l(m),
Vk,mEZ
(3.19)
TWO-DIMENSIONAL
also obeying
RELATIVISTIC
LATTICES
47
the recurrent relation (3.18a) but with the initial values: and
Aqo(m) = 2
VW%EZ.
Aqr(m) = m,
(3.20)
Note that q&(l) are the numbers of Fibonacci and Aqk(l) those of Lucas. These arithmetic functions too can be parametrized in terms of hyperbolic functions. Consider for any m E Z a 4 E R such that 2 sinh 4 = m.
(3.21)
Then for any k E 2: 2 sinh 2k+ = J(m2 and
+ 4) 4sk(m),
i 2 cash 2k+ = A42+2) 2 sinh (2k + i 2 cash (2k +
(3.22)
1) 4 = A4sk+r(m), 1) + = ,/(m2 + 4)
42k+1(4
where Aqk(m) and qk(m) are solutions of the Pell equation discriminant d = ms + 4: A&m)
-
(m2 + ‘4) q;(m) = (-
(plus, minus) of
1)” 4.
(3.23)
Proposition 4. Suppose g(W) = (a, b, c), a > 0, a primitive metric tensor admitting as in (3.7) an improper negautomorph A. Then A can always be written as: *(ml---bvr)
A=*Af$=&
( au1
k
-c’or ii(ml+h)
>
=
* (
i(mk-bvk)
-cvk
@vk
i(mk+
bvk) >
(3.24) with k = 1 (mod 2) and (ml, VI) the least positive solution of the Pell (minus) equation of discriminant d = b2 - 4ac > 0: m2 -
dv2 = -4,
(3.25a)
furthermore mk
=
Aqk(ml),
vk =
"lqk(ml).
(3.25b)
Proof. One may regard an improper negautomorph A of g(W) as an improper negautomorphism of ( 1, 0, - I), which becomes unimodular when referred to the basis B’ of (2.13). Therefore, using (3.3~) one gets:
= f
+(7iz av
bv)
-cv i(m + bv) >
(3.26)
A. JANNER
48
AND
E. ASCHER
where m = 2 sinh x E 2, and v = J((ms solutions of the Pell (minus) equation: ms -
+ 4)/d) E 2.
(m, v) are integral
dvs = -4.
Therefore E = j--(m + vJd) is a negative unit of Q(Jd) and is uniquely determined by A. Let Aa be the improper negautomorph that corresponds to the fundamental (negative) unit ~1 of Q(Jd) given by: ~1 = *(ml + v~,/d). Then E = &E: for some k E 1 (mod 2) (see e.g. ref. 18, p. 303) and correspondingly A = &At. Defining now #I by : mr=2sinh+
(3.27)
it follows that 2 sinh k+ = rnk = Aqk(mr) and vk = vrqk(mr), then, is a simple consequence of (3.23). Corollary 4.1. The improper negautomorphs A = *.4ik+’ of g(B) = (a, b, c) are in one-to-one negative units E = &@+’ of Q(Jd), for k E 2.
of infinite order correspondence with the
Remark. The restriction in corrollary 4.1 to negautomorphs of infiniteorder, i.e. to the case ml > 0, is due to the fact that in the case of negautomorph of finite order the correspondence with negative units breaks down. Fo(m = 0 the Pell (minus) equation becomes dv2 = 4 with positive solutions : v=2
for
a=
v=l
for
d = 4.
1,
In both cases Q(Jd) = Q and the only units are & 1, thus positive. For d = 1, no primitive metric tensor is possible (see ref. 17 theorem 75, p. 1Ol), but for d = 4, the metric tensor g(B) = (1, 0, - 1) admits improper negautomorphs of finite order:
A=*&=*
0 1
I
( >
(3.28)
o.
Note also that the group of g-automorphs of a given primitive g(B), is in general not isomorphic with the group of units of Q(,,/d) for d being the discriminant of g(B). In fact, no correspondence has been formulated between units of Q(Jd) and improper automorphs or proper negautomorphs of g(B) * The one-to-one correspondence broadly summarized as follows :
between
units and g-automorphs
positive units t--tproper automorphs (also of finite order), negative units ts improper negautomorphs (only of infinite order).
can be
TWO-DIMENSIONAL
A table indicating
real quadratic
RELATIVISTIC
fields Q(,/De)
LATTICES
49
having negative units can
be found in ref. 19, pp. 271-274 for Da up to 97. We now go over to proper negautomorphs. In the same way as in (3.26) and using (3.13) and (3.3d) one sees that the general form of a proper negautomorph of a primitive g(B) = (a, b, c), if it exists, is given by:
(3.29)
with (m, V) solutions of the Pell (minus) equation (3.25a). Note that these solutions need be integral (and therefore of the form (3.25b)). Comparing with (2.16) and (2.17) one finds that N can be written as:
(3.30)
Me is an improper automorphism and A an improper negautomorphism as in (3.26). The point is that only if a divides b, i.e. if g(B) is ambiguous, are Me and A necessarily unimodular, i.e. (m, V) are integral solutions of (3.25). In general this is not the case. As an example let us consider the lattice defined by g(B) = (5, 11, -5). One verifies that g(B) is not ambiguous and does not admit improper negautomorphs. In fact the discriminant is d = D = 221 and the fundamental unit of Q(J221) is ~1 = a(15 + J221), thus of norm + 1. But g(B) d oes admit proper negautomorphs, namely, for example : No
=
(3.3 1)
which may indeed be obtained from (3.29) for m = 1 l/5 and v = l/5, a non-integral solution of m2 - 221~2 = -4. We think that in the case of enantiomorphic lattices, proper negautomorphs can always be put into the form (possibly after a suitable basis transformation) : N = NoL
(3.32)
where No is as in (3.31) and L is an arbitrary proper automorph of g(B). This is indeed the case in the example mentioned above, although in general, we have not been able to prove it. Clearly proper negautomorphs need further investigation. 4. Classification of primitive lattices. Let II be an oriented lattice defined by primitive g(B) = (a, 6, c ) , a > 0, according to (2.13). By rl’ we indicate
50
A.
the mirror lattice il’=X/l We know that
JANNER
AND
E.
ASCHER
X E GL(2, 2) -
SL(2,Z).
of n given by: with
if A’ = A, the lattice
form an enantiomorphic
(4.1)
is ambiguous,
otherwise
A and A’
pair.
We now define A, the inverse of lattice A, is the lattice of {-g(B)}+. Here we have to consider the proper arithmetic class of --g(B) = (-a, --b, -c), because of the convention (2.13). We have the following correspondences A 0
(g(B)}+
and
J + {-g(B))+.
(4.2)
In the case where A = d we speak of a stable are called unstable.
lattice,
otherwise
A and R
Proposition 5. A lattice A defined by primitive g(B) according (2.13) is stable if and only if it is left invariant by proper negautomorphs
to of
g(B). Proof. Suppose A = 3, this means that -g(B) E {g(B)}+; thus there is a N E SL(2,Z) such that Ntg(B) N = -g(B). Clearly N is a proper negautomorph. The converse is also true, as can be seen by reversing the arguments. Corollary 5.1. A lattice A of a primitive nant d > 0, which is ambiguous and stable TABLE Classification Transformations
(4.3)
of relativistic
leaving
n
g(B) # (1, 0, - 1) of discrimiis left invariant by improper
primitive
Characterization
invariant
of
Type
the lattice
negautomorphs improper
lattices
ambiguous
_4 = n’
stable negative
‘4=/I /I = -A’
ambiguous
A = A’
unstable
A#/i
positive
‘4 # ?i’
proper negautomorphs A==‘%
enantiomorphic
A # A’
stable positive
A=fi
improper negautomorphs A = 2’
enantiomorphic
A # A’
unstable
Afji A = A
A=ii
I
automorphs n = n’
automorphs
only
Aitd
no improper automorphs A # A’
proper automorphs only (no negautomorphs)
negative
A # ;i’
enantiomorphic
A # A’
unstable positive
A#A A # ;i’
II -. III ____ IV
V
TWO-DIMENSIONAL
negautomorphs
of g(B).
fundamental unit. We call such a lattice
The
RELATIVISTIC
real
quadratic
field
51
LATTICES
Q(,/d) has a negative
with (il)’ = (d’) = ?i’ a negative
lattice.
If ,4 # /I
the lattice
is said to be positive. In this case there are no improper negautomorphs of g(B) and the units of Q(,/d) are all positive. Using these various definitions relativistic primitive lattices can be divided into five different types as indicated in the table (4.3). Explicit examples are indicated in the appendix showing that lattices of the five different types effectively occur. There are infinitely many primitive lattices and it is therefore worthwhile to group some of them in families of lattices having some peculiar properties. Given a value d of the discriminant, there is always a principal quadratic form with this discriminant (see e.g. ref. 16, p. 119). Accordingly we call principal lattices Pa,those lattices which are defined by the correspondence pd
(l,l,G) o
(I,o,-G) I Principal lattices are always pd one finds:
if
dEl(mod4),
(4.4a)
if
d=O(mod4).
(4.4b)
ambiguous.
if if
For the inverse
principal
lattices
d = 1 (mod 4),
(4.5a)
d F 0 (mod4).
(4.5b)
The concept of natural lattice plays an important ralein crystallography, even if not yet generally recognized. The name “natural” has been suggested by W. Opechowski. In order to explain the idea, consider a g-automorph X of a lattice rl. One has VXEA Xx=yEfl. (4.6) In general (x, y) is not a basis of ,4 but only of a sublattice. Suppose now that there is an element ei E ~4 and a g-automorph X of n such that (ei, Xei) forms a basis of rl. In this case we speak of a natural lattice generated by X. If X is an improper negautomorph
Xf
0
1
1
0
( >
we speak of a negative
natural
lattice;
and if X is a proper automorph
52
A. JANNER
we speak of a positive
natural
AND
E. ASCHER
lattice.
Proposition 6. For any n E 2, there are two positive natural lattices, M, and its inverse ii?!,. The lattice M, is the principal lattice of discriminant d = 12s -
4. One has the following correspondences
Ms,
o(l,O,
MB+1
-3
M2Y
e(v2
M2v+1
0
-
1 -V2)
(1, 1, 1 - v(v+ 1)) -l,O,
-1)
vv E z
(4.7)
-
(v(v
+
1) -1,
1, -1).
Proof. Consider a primitive lattice corresponding general form of a proper automorph L being (2.21), a vector x = xiei + xse6 E A and its transformed with yi = &i(1z - bu) - X~CU and ys = X~UZC + lattice of index d in _4, where d = (&
by (2.13) to (a, b, c). The the lattice generated by y = Lx = ylei + yzei +xs(n. + bu) is a sub-
+ bxlx2 + cx;) U.
(4.8)
For II natural: d = f 1; consequently may suppose 24 = 1. Then for d = 1 ax; + bxlx2 + cx; =
1
and
u = & 1. Without d = ns -
restriction
we
4.
According to a theorem of Lagrange (see ref. 17, p. 111) there is in the proper arithmetic class of (a, b, c) a quadratic form (a’, b’, c’) with a’ = 1. For 1z = 2v + 1 (odd n), b’ is also odd and, indicating proper arithmetic equivalence by 2, one has: (a,b,c)~(l,b’,c’)~(l,l,c”)=
(l,l,
For even n, n = 2v, b’ is also even and, analogously,
now A = - 1 and
1)).
one finds:
(u,b,c)i(l,b’,c.)i(l,O,c”)-(1,0.-;)=(I,O,l Suppose
1 --y(v+
-v2).
ax; + bxlx2 + cxi = - 1. As above,
in the
proper arithmetic class there is an (a’, b’, c’) with c’ = - 1, and one finds the inverse lattices i@, in the same way. Corollary 6.1. For getting all positive natural to consider all integers n 2 0, since M_, = M,.
lattices
it is sufficient
Proposition 7. The value vz = 3 is the only one for which i@, = M,. The lattice MS is of type I. Proof. For 1z = 3 the discriminant of MS is d = 5 and the fundamental unit of Q(J5) is negativeia). Being ambiguous and negative, Ms is stable.
TWO-DIMENSIONAL
Quadratic
fields
RELATIVISTIC
of discriminant
d = ns -
LATTICES
4, for
53
InI > 3, have
positive units. To prove this, suppose that there are integral
only
solutions of the
corresponding Pell (minus) equation. Take the least positive one (ml, ~1). It follows that the least positive solution of the Pell (plus) equation for same discriminant is given by and
ni = m; + 2
Ui = mi211.
(4.9)
This can be seen by squaring the improper negautomorph Aa of (3.24). But for natural lattices, ztr = 1, and this implies ml = zli = 1, thus ni = 3, which is contrary to the hypothesis. Proposition 8. For any m E 2 there is a negative natural lattice which is the principal lattice of discriminant d = ~2 + 4. One has: Nzfi
+ (1, 0, -(l
+ p2))
Nzfi+l
0 (1, 1, 1 -
p(p +
Proof. The generated by with (m, v) = one arrives at
p # 0,
VllEZ,
proof is obtained exactly as in proposition 7. One finds Nm the improper negautomorph A (3.26) of a primitive (a, b, c) (m, l), so that d = ms + 4. Applying Lagrange’s theorem the desired results.
Corollary 8.1. For getting all negative natural to consider integral positive m (since N-, = N,). Corollary
(4. IO)
V/.&EZ.
1))
Nnz,
8.2.
Any negative
natural
lattice
lattices,
Nm is stable
it is sufficient
(Nm = fl,).
Corollary 8.3. The only case where negative and positive lattices coincide is for m = 1 and n = 3, i.e., Ni = Ma.
natural
We shall also mention two other properties that give a geometrical interpretation of the least positive solution of Pell’s equation. We shall omit the proof as it can be derived straightforwardly. Proposition 9. Suppose dE.Z a given positive discriminant (d E 2) and (ni, zdi) the least positive solution of the corresponding Pell (plus) equation. The positive natural lattice M,, is a sublattice of index ~1 in the principal lattice Pd. Proposition 10. Suppose d a given positive discriminant appearing in a Pell (minus) equation, which has non trivial solutions, and let (ml, vi) be the least positive one. The negative natural lattice Mm, is a sublattice of index zli in the principal lattice Pd. Quite generally, as all primitive lattices of same discriminant have equal surface of their elementary cell (d = -4 det g(B)), there is an obvious generalization of the last two propositions.
54
A. JANNER
AND
E. ASCHER
5. Some properties of ambiguous lattices. The language of quadratic forms is a very convenient one for the matter discussed in this section and for referring to the literature. Only primitive quadratic forms are considered here, and in this section by equivalency (2.8). We recall that a form (a, b, c) is ambiguous if a divides b. In this case the proper arithmetic class coincides with the arithmetic one (see ref. 17, p. 7 1) : the lattice represented by the forms of the class is ambiguous and vice versa. An ambiguous form is called rectangular if b/a is even and rhombic if b/a is odd. This nomenclature is understandable on the basis of the following proposition. Proposition 11. A rectangular form is equivalent a rhombic form to one with b = a. More explicitly: (a, 2ka, c) N (a, 0, c (a, (2k + 1) a, c) -
k2a)
to one with b = 0;
VkEZ,
(a, a, c -
k(k +
(5.1)
1) a).
Proof.
2k;
1 a
‘“;:
“)(:
-:)=i,
c_k(ki)J’
It is in general not easy to decide whether given a quadratic form (a, b, c) is equivalent to an ambiguous one or not, the number of equivalent forms being infinite. The standard approach is to go over to equivalent reduced forms (see ref. 18, p. 100). The conditions for a form (a, b, c) to be reduced are : 0 < Jd
-
b < 2 Ial -=c Jd
+ b
and
O
(5.2)
and imply also 0 < Jd
-
b < 2 ICI < ,/d + b.
(5.3)
The number of equivalent reduced forms is finite (ref. 17 theorem 79, p. 103). These can be ordered into a chain of equivalent reduced forms. Prop o sit i o n 12. A rectangular form is equivalent to a reduced rectangular form. The same is true if one replaces rectangular by rhombic. Proof. We show first that any primitive (A, 0, C) is equivalent to a reduced form (a, 2ka, c). Suppose IA / < (Cl and take for k the largest rational integer satisfying the inequality : 0 < J ]C j - lkl J IA / (d is not a
TWO-DIMENSIONAL
RELATIVISTIC
LATTICES
55
square). The form (A, 0, C) is equivalent to the reduced one (A, 2KA, C + @A), If /A1 > ICI the same can be proved by considering the (equivalent) form (C, 0, A), called the associate of (A, 0, C). In the case of a rhombic form, one verifies that any form (a, (a(, c) with -UC > 0 is reduced. Now a rhombic form can always be given as (&A, A, &C) with A, C > 0. The only non-reduced cases are (A, A, C) and (--A, A, -C). The first form is equivalent to (4C - A, A - 4C, C), the second one to (A - 4C, A - 4C, C) which are both reduced rhombic forms. We may distinguish between three sorts of ambiguous lattices: (i) A lattice is rectangular (R) if any ambiguous form representing it is rectangular. (ii) A lattice is rhombic (D) if any ambiguous form representing it is rhombic. (iii) A lattice is mixed (RD) if it is represented by rhombic as well as by rectangular forms. Corollary 12.1. In a chain of reduced equivalent forms representing an ambiguous lattice, there are always two ambiguous forms. If both of these are rectangular (or both rhombic) the lattice is rectangular (or rhombic). If one form is rectangular and the other is rhombic, the lattice is mixed (RD). Proof. See ref. 17, p. 116 and use proposition 12. Let us remark that this classification of ambiguous lattices has a deeper meaning than one might be tempted to think initially. One can e.g. show that a RD-lattice cannot be of type I. This result will be proved and discussed in a subsequent paper 21). 6. Isotropic lattices. A lattice is called isotropic if it contains isotropic lattice vectors. One may then always choose a lattice basis B’ = (ei, eh) with metric tensor g(B’) = (0, b, c) h aving a square discriminant d = b2 (6 E R). In particular if the lattice is primitive, then its discriminant is a squared integer. This property is characteristic for isotropic primitive lattices. Proposition 13. A primitive lattice is isotropic if and only if its discriminant is a squared integer. Proof. We may suppose the lattice given by a primitive g(B) = (a, b, c). The lattice is isotropic if and only if the corresponding quadratic form: f(x, y) = ax2 + bxy + cyz,
Vx,yeZ
(6.1)
represents zero over 2. The necessary and sufficient condition for (a, b, c) to represent zero over the rationals Q (i.e. for x, y E Q) is that the discriminant d be a squared integer (see ref. 20, p. 395, theorem 10) ; conversely, if d is a squared integer, than (a, b, c) also represents zero over 2.
A. JANNER
56
AND
E. ASCHER
Proposition 14. The only proper automorphs of an isotropic are E and -E. Proof. Consider the metric tensor g(B) = (0, b, c) of an isotropic and its automorph SE
a
B 6
( > Y
E .x(2,
lattice
Z).
Then (for b # 0, because
d > 0) : (YB= 1.
and
a!=6
p=y=o, Proposition
lattice
15. A primitive
isotropic
lattice
(6.2) given by g(B) = (0, b, c)
is: ambiguous
if b divides cs -
1,
(ii)
stable
if b divides ca +
1,
(iii)
negative
if b divides 2.
(i)
imply the third one.
Two of the three conditions Proof. Let
s= and g(B) = (0, b, c) with c # 0. If S is an improper then : ab + yc = 0,
a =
&j -
and
-8
automorph
of (0, b, c)
By = --I.
This means
s-i: y.
If S is a proper negautomorph, 01=
ab + yc = 0,
(6.3) then : -6
and
016 -
By=
016
-1,
giving
%*(-, ‘“j. If now S is an improper
y = 0,
negautomorph,
,9b = (a -
6) c
then and
:
1,
TWO-DIMENSIONAL
RELATIVISTIC
LATTICES
57
(6.5) As b and c are relatively prime, it follows that b divides 2. Clearly two of the three relations imply the third one. If now c = 0, we have for the primitive lattice g(B) = (0, 1, 0), and the isotropic
lattice is ambiguous,
stable and negative.
In fact we have in this
case : improper
automorphs :
proper negautomorphs
improper
:
negautomorphs
(6.6) :
As in table (4.3) one may distinguish between different types of primitive isotropic lattices. Note, however, that type IV lattice (enantiomorphic, unstable and negative) does not occur, because if b = 2, then c is odd and b divides c2 * 1; the same is trivially true for b = 1. The general situation is illustrated in the following table. TABLE (6.7) Classification of isotropic primitive lattices with metric tensor g(B) = (0, b, c) Lattice type
Characterization of the lattice A
Conditions on the metric tensor
ambiguous stable negative
A = A’ A=li A = /i’
b=l b=2 andc
II
ambiguous unstable positive
A = A’ A#/r A#z
b/,2-1 bfc”+ b # 192
III
enantiomorphic stable positive
A # A’ A=/i A #6’
bfc”b/cs+l b # 1,2
V
enantiomorphic unstable positive
A # A’ A#jl A #A’
bfc2bfc2+ b # 1,2
I
or -
1 (mod2)
1
Examples of g(B) (0, 1, 0) (0,2, -1)
and
2 (l,O, -1)
(0, 3, -4
1 (0, 5, -2)
1 1
(0, 7, -2)
The conditions for an ambiguous primitive isotropic lattice to be rhombic or rectangular are expressed by the following proposition.
A. JANNER
58
AND
E. ASCHER
Proposition 16. An ambiguous primitive isotropic lattice with metric tensor g(B) = (0, b, c) is rectangular if b is even and rhombic if b is odd. Proof. Let us first remark that an ambiguous isotropic lattice is either rhombic or rectangular, because it admits only two mirrors (&&I), which then belong to the same arithmetic class. Suppose the lattice rectangular;
(0, b, c) 2 (A, 0, C)
then:
by
giving the conditions : 2A6 = yb, 2(Sc -
-2Cy &)
= Sb,
2(yc + ,&A) = --LYb,
= -_Bb,
(6.8)
which implies b -O(mod2). Suppose the lattice rhombic, then by S as above (0, b, c) & (A, A, C), giving olb = A(2S however,
y),
db = A(6 -
2~);
(6.9)
B or y is odd, thus :
b = 1 (mod2). 7. Bravais classes. One has to distinguish between Bravais classes and relativistic Bravais classes. We have already defined the first concept by condition (2.10). The second arises only if one considers the identification of isomorphic space-time groups as discussed in ref. 3. In this section we consider only the subdivision of relativistic lattices into usual Bravais classes. Having these, it is very easy to go over to relativistic Bravais classes. A first and important distinction can be made between relativistic lattices with holohedry of finite order (the ametric case) and lattices with holohedry infinite order (the metric case). (a) Lattices with holohedries of finite order. In section 2 and 6 we have seen that lattices with metric tensors proportional to the integral ones, with discriminant not a squared integer, always have an infinite holohedry. Therefore only real incommensurable (a, b, c) and/or isotropic (0, b, c) give rise to lattices with finite holohedries. Proposition 17. The holohedry of a lattice is of finite order if and only if the lattice is isotropic and/or has an incommensurable metric tensor
TWO-DIMENSIONAL
RELATIVISTIC
LATTICES
59
g(B) = (a, b, c). Th is means that for no real positiv k are Ku, kb and kc rational integers. Any lattice is left invariant by the identity E and by the total inversion -E. Lattices that are invariant only with respect to these two elements have holohedries that belong to a single arithmetic class, which defines the oblique Bravais class. The corresponding holohedry is No = {-E} z Cz. In the relativistic case, mirrors M are the only other lattice symmetries of finite order. We therefore consider ambiguous lattices. The holohedry of isotropic and/or incommensurable ambiguous lattices is : H = {-E,
M} g Ds.
(7.1)
In fact, two mirrors Ml and Ms, where Mr f &Ma generate a proper Lorentz transformation of infinite order (cf. 3.4). We have now to find out the arithmetic classes of (7.1). These are the same as the arithmetic classes of crystallographic Lorentz mirrors. Proposition 18. There are two arithmetic classes of crystallographic class (MR} and the improper Lorentz transformations : the rectangular rhombic class {MD} where
,,=(A _i).
MR=(:, _y> Proof.
Any Lorentz
M& = f
mirror is of the form:
cash $
sinh C$
- sinh C$
M+ leaves invariant
the space-like
,u = k(cosh $4 ei with k real positive;
M*=fp
sinh #
C$ >* direction
es)
and M_ leaves invariant
p = k(sinh &rj ei with k real positive,
-cash
the time-like
direction
cash $4 es),
where as usual g(B) = (1, 0, - 1). One has and
M+ being crystallographic,
Mkp = +
(7.2)
there is a S E GL(2, R) and a basis
BS = B’ = (ei, eh), such that: M;
= S-lM*
S E GL(2,Z)
(7.3)
and there are lattice vectors in the ,u and p directions (for more details, see refs. 21 and 22). According to the results of section 2 of this paper, there is, in the relativistic geometric class of lattices having the same g(B’), a lattice (1 left invariant by M; which lattice has p as first basis vector (,u = e;). This
A. JANNER
60
AND
E. ASCHER
means that there is a basis B” = (e;, e; =) B’S’ of n such that: S’-rM;S’=MI;
=(i
_:>
with
7~2.
(7.4)
The same can be said for M_ taking el = p. By:
(:,
-:)(6
-:>(:,
Y) = (:
y ‘:“)j
\dLwE.z
(7.5)
one sees that: (;
_;)“(6
Furthermore MD. Finally
(7.6)
y-y).
one verifies that 44~ is not in the same arithmetic
MR,Z--_fi
and
MO & -
MD.
class as
(7.7)
To prove this, it is sufficient to interchange the role of p and ,u in the demonstration above. According to proposition 18, holohedries (7.1) belong to two arithmetic classes. Lattices having holohedries equivalent to the rectangular class belong to the rectangular Bravais class; those with holohedries equivalent to the rhombic class belong to the rhombic Bravais class. Note that invariance with respect to MR implies g(B) = (a, 0, c) ; invariance with respect to MD gives g(B) = (a, a, c). This explains the name of the class. To conclude, there are the following three Bravais classes of lattices in the ametric and isotropic cases. (i) The rectangular Bravais class. The lattices AR belonging to this class have either an incommensurable or an isotropic metric tensor g(B’) = (a’, b’, c’ ) such that there are real u, c with: a > 0.
(a’, b’, c’) 2L (a, 0, c), Their holohedry HR = {-E,
(7.8)
(with respect to a rectangular
basis) is:
MR} g Dz.
(7.9)
(ii) The rhombic class. The lattices AD belonging to this class have either an incommensurable or an isotropic metric tensor g(B’) = (a’, b’, c’) such that there are real a, c with
Their holohedry HD = {--E,
(with respect to a rhombic n/rD>s
(7.10)
a > 0.
(a’, b’, c’) r% (a, a, c),
D2.
basis) is: (7.11)
TWO-DIMENSIONAL
RELATIVISTIC
LATTICES
61
All incommensurable or isotropic (iii) The oblique Bravais class. lattices that are neither in the rectangular nor in the rhombic Bravais class belong to the oblique Ho = {-E} (b) Lattices
s
Bravais
class. Their holohedry
is: (7.12)
c2.
with
holohedries
of
infinite
order.
As we have
already seen in section 2, we may restrict our attention to primitive lattices whose discriminant is not a squared integer. In what follows by primitive lattices we mean non-isotropic primitive lattices. According to proposition 3 any proper automorph of a primitive lattice is given by (3.14) and is therefore generated by the total inversion -E and the fundamental Lorentz transformation LO, which leave the lattice invariant. The holohedry of an enantiomorphic primitive lattice is thus given by: H, = {-E,
Lo} E C,
x Cs.
(7.13)
Any improper automorph M of an ambiguous primitive lattice is the product of a particular mirror MO leaving the lattice invariant and a certain proper automorph. It follows that the holohedry of a primitive ambiguous lattice is : H, = {-E,
Lo, MO} cg D,
x Cz.
(7.14)
We do not have to investigate the arithmetic classes of (7.13) and of (7.14), for we know already the result: The proper arithmetic classes of primitive indefinite quadratic forms are in one-to-one correspondence with the Bravais classes of metric lattices. In each Bravais class we have singled out by (2.13) a primitive lattice. A list of chains of equivalent reduced quadratic forms corresponding to primitive lattices is given in the appendix for a number of discriminants. The table needs some comments. Usually reduced quadratic forms are tabulated according to the increasing value of the discriminant. It is well known that the number of different arithmetic classes for a given discriminant is finite (see ref. 17, theorem 79, p. 103). The least positive solutions of Pell’s equation are determined by a given discriminant. In our classification, however, we have adopted another ordering criterion that is based on the kinematical interpretation of the proper Lorentz transformations leaving a relativistic lattice invariant. To a proper Lorentz transformation of infinite order there corresponds the transformation from an inertial frame to one moving with relative velocity z, in the x direction (the only spatial dimension in two-dimensional Minkowskian space). The absolute value of z, is determined by the trace G E 2 of the Lorentz transformation
62
A. JANNER
considered.
AND
E. ASCHER
One has :
n=2cosh+=
(7.15) 2
giving :
(7.16)
We indicate below the correspondence
for low values of n.
TABLE (7.17) Kinematical interpretation of n n
-
v?z
3
4
5
6
7
8
Js 3
J3 2
J21 5
242 3
345 7
p_ 4
0.745
0.866
0.916
0.942
0.958
c 0.968
From the physical point of view we expect that the lowest values of n are the most interesting ones. Therefore we have ordered the Bravais classes of primitive lattice according to increasing value of 12. For a given n it is easy (by looking at the factor decomposition of 12s - 4) to determine all possible integral values of u and d in the Pell equation. Knowing the discriminant d, the corresponding arithmetic classes are derived by standard methods (see e.g. ref. 17). 8. Concluding remarks. By means of this paper we have laid down the foundation of a two-dimensional relativistic crystallography. The next step consists in determining of the arithmetic classes of relativistic point groups. These can then be used for the derivation of all two-dimensional space-time groups. Acknowledgements. The financial contribution accorded by the Curatoren of the Katholieke Universiteit Nijmegen is gratefully acknowledged. The authors wish to thank Professor W. Opechowski for critical remarks.
TWO-DIMENSIONAL
RELATIVISTIC
63
LATTICES
APPENDIX Bravais 1221
5 6
7
5 1 1
9 10
21 32
2
8
3 8
12
1
1
1
1 1
12
45 5 60
77 96
Type
Lattices Mg N1
[l, 2, --2x-2, 2, 11 [2, 2, - I][- 1, 2, 21
M4 -
r1, 3, -3x-3, [3, 3, -lx_-
3, 11 1, 3, 31
IID
[l> 4, -41[-4, [4, 4, -111-
4, 11 1, 4, 41
IIRD
MB M6
[l, 2, -1x-
1, 2, 11
IR
NB
[l, 5, -511-5, 5, I] [5, 5%- llC- 1, 5,51
IID
M, -
[l, 1, -ll[-1,
ID
N1
[l, 6, -6][-6, 6, 11 [6, 6, - I][-- 1, 6, 63
IIRD
M, Mg
[2, 6, -a][-3, [3, 6, -2][-2,
IIRD
M4
M7
1, 11
6, 21 6, 31
IID
[l, 8, -8][-8, 8, 1] [8, 8, - l][-- 1, 8, 81
IIRD
4, 4][4, 4, -5][-5, 6, 5][5, 4, -4][-4,
Mg M3
[l, 7, -71[-7, 7, 11 c7, 7, - lx,- 1, 7, 71
Mg Ms
6, 31 4, 5]
Mlg Mlo
IIRD
2
24
[l, 4, -2x-2, [2, 4, - ll[-
4, 11 1, 4, 21
IIR
1
117
[l, 9, -9][-9, [9, 9, - ll[-
9, I] 1, 9, 91
IID
Ml1 Ml1
3
13
Cl, 3, -1x-1,
3, 11
ID
N3
1
140
IIRD
Ml2 -
[l, 10, -lO][-10, [lo, 10, - 1x-1,
1
165
[l, 11, -ll][-11, [II, 11, -l][-1, [3. 9, -7x-7. [7? 9, -3x-3,
14
lattice (for n 5 25)
ID
1, 11
[2, 10, -5x-5, [S, 10, -2][-5, 13
relativistic
IIRD
[l, 1, -1x-1.
[3, 6, -5][-5, [5, 6, -3][--3,
11
(non-isotropic)
Chains of equivalent primitive reduced forms
d
31 4
classes of primitive
1
192
10, I] 10, lo]
M12
IIRD
10, 21 10, 21
IID
11, 1] 11, 111 5, 51[5, 5, --77[-7, 9, 7x7, 5, -5x-5,
p24 p24
M13 M13
9, 31 9, -31
IID
[1, 12, -12][-12, 12, 1] [- 1, 12, 12][12, 12, - 1]
IIRD
[3, 12, -4][-4, 12, 31 [-3, 12, 4![4, 12, -33
IIRD
Ml4 M14
A.
64
(A$$endix nu 14
AND
E.
ASCHER
continued) d
2
JANNER
Chains of equivalent
48
[l, 6, -3][-3,
primitive
reduced
forms
6, l]
Type
Lattice
IIR
P48
I-- 1, 6, 3][3, 6, -11 4
12
r1, 2, -2x-2, L--l,
15
1
221
2, 2x2,
[I, 13, c-1,
2, l] 2, -
13][-
[5> 11, -51r-5, 16
1
3 17
1
252
28 285
1
320
9, -7l[-7,
IIRD
14, 21 14, -21
80
19
20
20
8
5
IID
[3, 15, -5x-5,
15, 31
IID
1
357
1
3
396
44
M17 M17
IIRD
16, l] 16, -11 10,5][5,
10, -ll][-11,
12,4]
10, ll][ll,
12, -43
IIRD IIR
8, l]
1, 8, 4][4, 8, -11
[l, 4, -1x--1, l, -1x-I,
IR
N4
1, 11
ID
N1
IID
-ll][-11,
L-3,
7, 11][11,
7, -7][-7,
15,3]
18, 11 18, -11
IIRD IIRD
[5, 16, -7][-7, L-5, 16, 7][7,
12, 9][9, 6, -lo][-10, 12, -9][-9. 6, lO][lO,
14, 51 14, -51
L-7, 16, 5][5, [7, 16, -5][-5,
14, -lO][-10, 6, 9][9, 14, lO][lO, 6, -9][-9,
12, -71 12, 7J
6, l]
Mzo M20
18, 21 18, -21
1, 6, 2X2, 6, -11
IID
15, -31
[2, 18, -9][-9, [--2, 18, 9][9,
[1, 6, -2][-2,
Mrs =19
[3, 15, -1ll[-11.7,71[7,7, [1, 18, -18][-18, [-1, 18, 18][18,
PSO PSO
4, l]
[l, 17, -17l[-17, 17, l] [-- 1, 17, 17J[17, 17, -11
15, ll][ll,
Ml8 El8
12, 111[11, 10, -5][-5,
[l, 8, -4][-4,
[-
Pz8
15, 51[5, 15, -31
[1, 16, -16][-16, [-1, 16, 16][16,
[l,
Ml6 Ml6
p28
15, l] 15, -11
[4
IIRD
2, -3x-3, 4, 11 2, 3][3, 4, - 11
[l, 15, -15][-15, [--1, 15, 15][15,
[4, 12, -lll[-11, 2
III
9, 51
5, 71[7, 9, -51
[2, 14, -7x-7, L-2, 14, 7][7,
2, 2x2, 2, -2][-2,
M15 JQ15
IIRD
L-4, 18
IID
13, -11
[l, 14, - 14][- 14, 14, l] [- 1, 14, 14][14, 14, - 11
[l, 4, -31[-3, [- 1. 4, 3x3,
Me M4
9, 7][7, 5, -7][-7,
11, 5x5,
L-3, 18
11
13, 13, I]
13, 13x13,
c-5,
P48
IIRD
V
IIRD
P44 P44
TWO-DIMENSIONAL
RELATIVISTIC
65
LATTICES
(Appendix continzced) nu 21
Chains of equivalent
d 1
437
[l,
19, -19][-19,
[-1, 22
1
480
16, 7][7,
[3, 18, C-3, 2
120
[l,
12, 12][12,
1
525
8, 8][8, 8, -13][-13,
5 24
1
21 572
3, 11 -
1, 3, 3x3,3,
1
621
[l, 22, -22][-22,
69
15, -
21, 5H5, 19, -13x-13,
7, -13][-13, 11, 7, 13][13,
1l][-
7, ll][ll,
19, 13][13,
7, -ll][-11.
3, 3][3, 3, -5][-5,
1, 7, 51[5, 3, -31[-3,
M25 B25
15, ll][ll,
L-9,
[-
IID
23, l] 23, -11
21, 9][9,
[l, 7, -51[-5,
IIRD
22, 21
L-5,
[9, 21, -51[--5, 3
M24 M24
22, -21
1, 23, 23][23,
[5, 21, -9][-9,
IIRD
22, -11
22, ll][ll,
p21 61
22, l]
1, 22, 22][22,
[l, 23, -23][-23, [-
IID
11
[2, 22, -ll][-11, 25
M23 M23
IID
21, 31
[l, 3, -31[-3,
[-2,
IID
21, -31
[[-
IIR
8, 21
21, -11
c3, 21, -7x-7,
p120 p120
6, 71[7, 8, -21
21, l]
1, 21, 21][21,
21, 7x7,
IIR
6, 3X3, 6, -7][-7,
8, 7][7, 6, -3][-3,
r-3,
IIRD
18, 31
8, 13][13, 8, -31
10, l]
[l, 21, -21-j-21, [-
IIRD
16, 81 16, -81
10, --I]
[2, 8, --71[-7, 23
12, -7][-7, 12, 7][7,
8, -8][-8,
10, -5][-5,
C-2,
Mz2 M22
12, -12][-12,
13][-13,
10, 5][5,
M21 M21
IIRD
20, 41
18, 13][13,
c-1.
IIRD
11
Lattices
20, -43
[8, 16, --71[-7, [-8,
IID
20, l] 20, -
[4, 20, -5][-5, 20, 5x5,
Type
forms
19, -11
1, 20, 20][20,
[-4,
reduced
19, l]
19, 19x19,
[l, 20, -2O][-20, [-
primitive
19, 51 V
19, 51 15, -91 15, 91
7, l]
IID
3, 5][5, 7, -11
P69 p69
REFERENCES
1) 4
Buerger, M. J., Elementary Crystallography, Burckhardt, J. J., Die Bewegungsgruppen
3) 4)
Janssen, T., Janner, A. and Ascher, E., Physica 41 (1969) Fast, G. and Janssen, T., Non-equivalent four-dimensional
(Basel,
J. Wiley (New York, der Kristallographie,
1956). Birkhluser,
1947). 541; 42 (1969) 41, 71. generalized magnetic
TWO-DIMENSIONAL
66 space-time
groups,
Techn.
RELATIVISTIC
Rep.
Inst.
Theor.
LATTICES
Fysica,
Katholieke
Universiteit,
Nijmegen. 5)
Schild,
A., Phys.
6)
Schiff,
L., Phys.
7)
Hill, H., Phys.
8)
Redei,
9)
Bopp, Weyl,
73 (1948)
der Wiss.,
H., Math.
Math.
Zeit.
(Basel,
11)
Stiefel,
E., Commentarii
12)
Speiser, Summer
13)
Speiser,
14)
Antoine,
15)
Janner,
16) 17)
Naturwiss.
School
Math.
Bayrische
13.
328, 377. Selecta
Phys. Phys.
38 (1965)
H. Weyl,
39 (1966)
17 (1944-45)
Birk-
165.
to elementary
in elementary
Gordon
and Breach
particles.
parti-
Istambul
(New York,
1964).
73.
D., J. math.
Acta
350;
and applications
and methods
Physics,
Acta
P., Grundlehren Leipzig
14 (1941-42)
Lie groups
concepts
J. P. and Speiser,
Dickson,
24 (1926)
Helv.
in Theoretical
A., Helv.
Bachmann,
Kl. (1967)
271;
of compact
theoretical
D., Helv.
leger (Berlin,
999.
1956).
D., Theory
cles in Group
29.
117, 133, 142; 204 (1967) 311 and Sitzber.
23 (1925)
hPuser
1 (1949)
1780.
145 (1966)
200 (1967)
J. Math.
766.
100 (1955)
Rev.
F., Z. Phys.
414, Canad.
92 (1953)
Rev.
L., Phys.
Akademie 10)
Rev. Rev.
Phys.
5 (1964)
1226, 1560.
665.
der neueren
Zahlentheorie,
Vereinig.
Wissensch.
Ver-
192 1) .
L. E., Introduction
to the theory
of numbers,
Dover
Publ.
(New York,
1957). 18)
Hasse,
19)
Cohn, H., A second
H., Vorlesungen
20)
Borevich,
21)
York, 1965). Janner, A. and Ascher,
E., Physica
22)
Janner,
E., Crystallography
Z. I. and
in number
Shafarevich,
A. and Ascher,
be published
iiber Zahlentheorie,
course
in Z. kristalloprafie).
Springer
theory,
I. R.,
J. Wiley
Number
45 (1969)
(Berlin,
1964).
(New York,
theory,
London,
Academic
Press
1962). (New
67.
in two-dimensional
metric
spaces
(to