\mathrm{SU}(1,1) = \left \{ \begin{pmatrix}u & v \\ v^* & u^* \end{pmatrix} \in M(2,\mathbb{C}): u u^* - v v^* = 1 \right \}, where ~u^*~ denotes the
complex conjugate of the complex number . This group is isomorphic to and where the numbers separated by a comma refer to the
signature of the
quadratic form preserved by the group. The expression u u^* - v v^* in the definition of is an
Hermitian form which becomes an
isotropic quadratic form when and are expanded with their real components. An early appearance of this group was as the "unit sphere" of
coquaternions (split-quaternions), introduced by
James Cockle in 1852. Let j = \begin{bmatrix} 0 & 1 \\ 1 & 0 \end{bmatrix}\,, \quad k = \begin{bmatrix} 1 & \;~0 \\ 0 & -1 \end{bmatrix}\,, \quad i = \begin{bmatrix} \;~0 & 1 \\ -1 & 0 \end{bmatrix}~. Then {{tmath|1= j\,k = \begin{bmatrix} 0 & -1 \\ 1 & \;~0 \end{bmatrix} = -i}}, {{tmath|1= i\,j\,k = I_2 \equiv \begin{bmatrix} 1 & 0 \\ 0 & 1 \end{bmatrix} }}, the identity matrix, , and , and the elements , , and all
anticommute, as in
quaternions. Also i is still a square root of (negative of the identity matrix), whereas are not, unlike in quaternions. For both quaternions and
coquaternions, all scalar quantities are treated as implicit multiples of and notated as . The coquaternion q = w + x\,i + y\,j + z\,k with scalar , has conjugate q = w - x\,i - y\,j - z\,k similar to Hamilton's quaternions. The quadratic form is q\,q^* = w^2 + x^2 - y^2 - z^2. Note that the 2-sheet
hyperboloid \left\{ x i + y j + z k : x^2 - y^2 - z^2 = 1 \right\} corresponds to the
imaginary units in the algebra so that any point on this hyperboloid can be used as a
pole of a sinusoidal wave according to
Euler's formula. The hyperboloid is stable under , illustrating the isomorphism with . The variability of the pole of a wave, as noted in studies of
polarization, might view
elliptical polarization as an exhibit of the elliptical shape of a wave with The
Poincaré sphere model used since 1892 has been compared to a 2-sheet hyperboloid model, and the practice of
interferometry has been introduced. When an element of is interpreted as a
Möbius transformation, it leaves the
unit disk stable, so this group represents the
motions of the
Poincaré disk model of hyperbolic plane geometry. Indeed, for a point in the
complex projective line, the action of is given by \bigl[\;z,\;1\;\bigr] \begin{pmatrix}u & v^* \\ v & u^* \end{pmatrix}\, = [\;u\,z + v, \, v^*\,z +u^*\;] \, = \, \left[\;\frac{uz + v}{v^*z +u^*}, \, 1 \;\right] since in
projective coordinates {{tmath| (\;u\,z + v, \; v^*\,z +u^*\;) \thicksim \left(\;\frac{\,u\,z + v\,}{v^*\,z +u^*}, \; 1 \;\right) }}. Writing {{tmath|1= suv + \overline{suv} = 2\,\Re\mathord\bigl(\,suv\,\bigr) }}, complex number arithmetic shows \bigl|u\,z + v\bigr|^2 = S + z\,z^* \quad \text{ and } \quad \bigl|v^*\,z + u^*\bigr|^2 = S + 1~, where . Therefore, z\,z^* so that their ratio lies in the open disk. == See also ==