In abstract algebra, a coquaternion is an idea put forward by James Cockle in 1849. Like the 1843 quaternions of Hamilton, they form a four dimensional real vector space equipped with a multiplicative operation. Unlike the quaternion algebra, coquaternions may be zero divisors or nilpotent. They are isomorphic to hyperbolic quaternions from the hypernumbers program.
The set forms a basis. The coquaternion products of these elements are
-
-
With these products the set
is
isomorphic to the
dihedral group of a square.
A coquaternion
-
has conjugate
- and modulus
-
When the modulus is non-zero, then q has a multiplicative inverse.
-
is the set of units. The set P of all coquaternions forms a ring (P, +, •) with group of units (U, •).
Let
-
where u and v are ordinary complex numbers. Then the complex matrix
-
where
and
(
complex conjugates of
u and
v),
represents q in the ring
of matrices in the sense that multiplication of coquaternions behaves the same way as the
matrix multiplication.
For example, the
determinant of this matrix
; the appearance of this minus sign where there is a plus in
H leads to the alternative name
split-quaternion for a coquaternion.
Historically coquaternions preceded
Cayley's matrix algebra; coquaternions (along with quaternions and
tessarines) evoked the broader
linear algebra.
Profile
Let
- r(θ) = j cos θ + k sin θ (here θ is as fundamental as azimuth)
- p(a,r) = i sinh a + r cosh a
- v(a,r) = i cosh a + r sinh a
- E = { r ∈ P : r = r(θ), 0 ≤ θ < 2 π }
- J = {p(a,r) ∈ P : a ∈ R, r ∈ E } catenoid
- I = {v(a,r) ∈ P : a ∈ R, r ∈ E } hyperboloid of two sheets
Now it is easy to verify that
- {q ∈ P : q2 = + 1 } = J ∪ {1,-1}
and that
- {q ∈ P : q2 = -1 } = I .
These set equalities mean that when p ∈ J then the plane
- { x + yp : x,y ∈ R } = Dp
is a subring of P that is isomorphic to the plane of split-complex numbers just as when v is in I then
{x + y v : x,y ∈ R } = Cv
is a planar subring of P that is isomorphic to the ordinary complex plane C.
Note that for every r ∈ E, (r + i)2 = 0 = (r - i)2 so that r + i and r - i are nilpotents. The plane N = {x + y(r + i) : x,y ∈ R} is a subring of P that is isomorphic to the dual numbers. Since every coquaternion must lie in a Dp, a Cv, or an N plane, these planes profile P. For example, the unit sphere
- SU(1,1) = { q ∈ P : q q* = 1 }
consists of the "
unit circles" in the constituent planes of
P. In D
p this is an
hyperbola, in N the unit circle is a pair of parallel lines, while in C
v it is indeed a circle (though it appears elliptical due to v-stretching).
Pan-orthogonality
When coquaternion q = w + xi + yj + zk, then the
real part of q is w.
Definition: For non-zero coquaternions q and t we write
q ⊥ t when the real part of the product qt* is zero.
- For every v ∈ I, if q,t ∈ Cv, then q ⊥ t means the rays from 0 to q and t are perpendicular.
- For every p ∈ J, if q,t ∈ Dp, then q ⊥ t means these two points are hyperbolic-orthogonal.
- For every r ∈ E and every a ∈ R, p = p(a,r) and v = v(a,r) satisfy p ⊥ v .
- If u is a unit in the coquaternion ring, then q ⊥ t implies qu ⊥ tu.
- proof: (qu)(tu)* = (uu*)qt* follows from (tu)* = u*t*, a fact based on anti-commutativity of vectors.
Counter-sphere geometry
Take m = x + y i + z r where r = j cos θ + k sin θ. Fix theta (θ) and suppose
- m m* = − 1 = x2 + y2 − z2 .
Since points on the counter-sphere must line on a counter-circle in some plane
Dp ⊂ P , m can be written, for some p ∈ J
- m = p exp(b p) = sinh b + p cosh b = sinh b + i sinh a cosh b + r cosh a cosh b .
Let φ be the angle between the hyperbolas from r to p and m. This angle can be
viewed, in the plane
tangent to the counter-sphere at r , by projection :
- tan φ = x/y = sinh b / (sinh a cosh b) = tanh b / sinh a .
As b gets large, tanh b nears one. Then tan φ = 1/ sinh a . This appearance of the
angle of parallelism in a meridian θ inclines one to expect to see the counter-
sphere unfold as
metric space S
1 × HP where HP is the
hyperbolic plane.
Application to kinematics
By using the foundations given above, one can show that the mapping
- q → u−1 q u
is an ordinary or hyperbolic rotation according as
- u = exp(a v), p ∈ I or u = exp(a p), v ∈ J .
These mappings are projectivities in the
inversive ring geometry of coquaternions.The
collection of these mappings bears some relation to the
Lorentz group since it is also
composed of ordinary and hyperbolic rotations.Among the peculiarities of this approach
to relativistic kinematic is the
anisotropic profile, say as compared to
Hyperbolic quaternions.
Reticence to use coquaternions for kinematic models may stem from the (2,2) signature when spacetime is presumed to have signature (1,3) or
(3,1).Neverless, a transparently relativistic kinematics appears when a point of the
counter-sphere is used to represent an inertial frame of reference.Indeed, if t t* =
−1 , then there is a p ∈ J such that t ∈ Dp , and an a ∈
R such that t = p exp(a p).The if u = exp(a p) and s = i r , the set {t, u, v, s } is a
pan-orthogonal basis stemming from t, and the orthogonalities persist through applications of
the ordinary or hyperbolic rotations.
Historical notes and references
The coquaternions were initially identified and named in the
London-Edinburgh-Dublin Philosophical Magazine, series 3, volume 35, pp.434,5 in 1849 by James Cockle under the title "On Systems of Algebra involving more than one Imaginary". At the 1900
Paris meeting of the
International Congress of Mathematicians Alexander MacFarlane called the algebra the
exspherical quaternion system as he described its profile. MacFarlane examined a differential element of the submanifold {q ∈
P : q q* = - 1 } (the counter-sphere).
The sphere itself was considered in German by Hans Beck in 1910 (
Transactions of the American Mathematical Society, v.28; e.g. the dihedral group appears on page 419.)In 1942 and 1947 there were two brief mentions of the coquaternion structure in the
Annals of Mathematics:
- A.A. Albert "Quadratic Forms permitting Composition" 43:161-177
- V. Bargmann "Representations of the Lorentz Group" 48:568-640 .
See also
abstract algebra | quaternions | hyperbolic geometry | special relativity