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		<summary type="html">&lt;p&gt;84.133.101.35: /* Proof */&lt;/p&gt;
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&lt;div&gt;In [[abstract algebra]], the &#039;&#039;&#039;biquaternions&#039;&#039;&#039; are the numbers  {{nowrap|&#039;&#039;w&#039;&#039; + &#039;&#039;x&#039;&#039; i + &#039;&#039;y&#039;&#039; j + &#039;&#039;z&#039;&#039; k}}, where &#039;&#039;w&#039;&#039;, &#039;&#039;x&#039;&#039;, &#039;&#039;y&#039;&#039;, and &#039;&#039;z&#039;&#039; are complex numbers and the elements of {{nowrap|{1, i, j, k}&amp;lt;nowiki/&amp;gt;}} multiply as in the [[quaternion group]]. As there are three types of complex number, so there are three types of biquaternion:&lt;br /&gt;
* (Ordinary) biquaternions when the coefficients are (ordinary) [[complex number]]s&lt;br /&gt;
* [[Split-biquaternion]]s when  &#039;&#039;w&#039;&#039;, &#039;&#039;x&#039;&#039;, &#039;&#039;y&#039;&#039;, and &#039;&#039;z&#039;&#039; are [[split-complex number]]s&lt;br /&gt;
* [[Dual quaternion]]s when &#039;&#039;w&#039;&#039;, &#039;&#039;x&#039;&#039;, &#039;&#039;y&#039;&#039;, and &#039;&#039;z&#039;&#039; are [[dual numbers]].&lt;br /&gt;
&lt;br /&gt;
This article is about the ordinary biquaternions named by [[William Rowan Hamilton]] in 1844 (see Proceedings of Royal Irish Academy 1844 &amp;amp; 1850 page 388). Some of the more prominent proponents of these biquaternions include [[Alexander Macfarlane]], [[Arthur W. Conway]], [[Ludwik Silberstein]], and [[Cornelius Lanczos]]. As developed below, the [[Hyperboloid#Relation to the sphere|unit quasi-sphere]] of the biquaternions provides a presentation of the [[Lorentz group]], which is the foundation of [[special relativity]].&lt;br /&gt;
&lt;br /&gt;
The algebra of biquaternions can be considered as a [[tensor product of algebras|tensor product]] {{nowrap|&#039;&#039;&#039;C&#039;&#039;&#039; ⊗ &#039;&#039;&#039;H&#039;&#039;&#039;}} (taken over the reals) where &#039;&#039;&#039;C&#039;&#039;&#039; is the [[field (mathematics)|field]] of complex numbers and &#039;&#039;&#039;H&#039;&#039;&#039; is the algebra of (real) [[quaternions]]. In other words, the biquaternions are just the [[complexification]] of the (real) quaternions. Viewed as a complex algebra, the biquaternions are isomorphic to the algebra of 2×2 complex matrices &#039;&#039;M&#039;&#039;&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;(&#039;&#039;&#039;C&#039;&#039;&#039;). They can be classified as the [[Clifford algebra]] {{nowrap|1=Cℓ&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;(&#039;&#039;&#039;C&#039;&#039;&#039;) = Cℓ&amp;lt;sup&amp;gt;0&amp;lt;/sup&amp;gt;&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt;(&#039;&#039;&#039;C&#039;&#039;&#039;)}}. This is also isomorphic to the [[Pauli algebra]] Cℓ&amp;lt;sub&amp;gt;3,0&amp;lt;/sub&amp;gt;(&#039;&#039;&#039;R&#039;&#039;&#039;), and the even part of the [[spacetime algebra]] Cℓ&amp;lt;sup&amp;gt;0&amp;lt;/sup&amp;gt;&amp;lt;sub&amp;gt;1,3&amp;lt;/sub&amp;gt;(&#039;&#039;&#039;R&#039;&#039;&#039;).&lt;br /&gt;
&lt;br /&gt;
==Definition==&lt;br /&gt;
Let {1, &#039;&#039;i&#039;&#039;, &#039;&#039;j&#039;&#039;, &#039;&#039;k&#039;&#039;} be the basis for the (real) [[quaternion]]s, and let &#039;&#039;u&#039;&#039;, &#039;&#039;v&#039;&#039;, &#039;&#039;w&#039;&#039;, &#039;&#039;x&#039;&#039; be [[complex number]]s, then&lt;br /&gt;
:&#039;&#039;q&#039;&#039; = &#039;&#039;u&#039;&#039; 1 + &#039;&#039;v&#039;&#039; i + &#039;&#039;w&#039;&#039; j + &#039;&#039;x&#039;&#039; k&lt;br /&gt;
is a &#039;&#039;biquaternion&#039;&#039;.&amp;lt;ref&amp;gt;Hamilton (1853) page 639&amp;lt;/ref&amp;gt;&lt;br /&gt;
To distinguish square roots of minus one in the biquaternions, Hamilton&amp;lt;ref&amp;gt;Hamilton (1853) page 730&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;Hamilton (1899) &#039;&#039;Elements of Quaternions&#039;&#039;, 2nd edition, page 289&amp;lt;/ref&amp;gt; and [[Arthur W. Conway]] used the convention of representing the square root of minus one in the scalar field &#039;&#039;&#039;C&#039;&#039;&#039; by h since there is an i in the [[quaternion group]]. Then&lt;br /&gt;
: h i = i h, h j = j h, and h k = k h since h is a scalar.&lt;br /&gt;
Hamilton&#039;s primary exposition on biquaternions came in 1853 in his &#039;&#039;Lectures on Quaternions&#039;&#039;, now available in the &#039;&#039;Historical Mathematical Monographs&#039;&#039; of Cornell University. The two editions of &#039;&#039;Elements of Quaternions&#039;&#039; (1866 &amp;amp; 1899) reduced the biquaternion coverage in favor of the real quaternions. He introduced the terms [[bivector (complex)|bivector]], &#039;&#039;biconjugate, bitensor&#039;&#039;, and &#039;&#039;biversor&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
Considered with the operations of component-wise addition, and multiplication according to the quaternion group, this collection forms a 4-dimensional [[algebra over a field|algebra]] over the complex numbers. The algebra of biquaternions is [[associative]], but not [[commutative]]. A biquaternion is either a [[unit (ring theory)|unit]] or a [[zero divisor]].&lt;br /&gt;
&lt;br /&gt;
==Place in ring theory==&lt;br /&gt;
&lt;br /&gt;
===Linear representation===&lt;br /&gt;
Note the matrix product&lt;br /&gt;
:&amp;lt;math&amp;gt;\begin{pmatrix}h &amp;amp; 0\\0 &amp;amp; -h\end{pmatrix}\begin{pmatrix}0 &amp;amp; 1\\-1 &amp;amp; 0\end{pmatrix}&amp;lt;/math&amp;gt; = &amp;lt;math&amp;gt;\begin{pmatrix}0 &amp;amp; h\\h &amp;amp; 0\end{pmatrix}&amp;lt;/math&amp;gt;&lt;br /&gt;
where each of these three arrays has a square equal to the negative of the [[identity matrix]].&lt;br /&gt;
When this matrix product is interpreted as i j = k, then one obtains a [[subgroup]] of the matrix group that is [[isomorphism|isomorphic]] to the [[quaternion group]]. Consequently&lt;br /&gt;
:&amp;lt;math&amp;gt;\begin{pmatrix}u+hv &amp;amp; w+hx\\-w+hx &amp;amp; u-hv\end{pmatrix}&amp;lt;/math&amp;gt; represents biquaternion &#039;&#039;q&#039;&#039; = &#039;&#039;u&#039;&#039; 1 + &#039;&#039;v&#039;&#039; i + &#039;&#039;w&#039;&#039; j + &#039;&#039;x&#039;&#039; k.&lt;br /&gt;
Given any 2 × 2 complex matrix, there are complex values &#039;&#039;u&#039;&#039;, &#039;&#039;v&#039;&#039;, &#039;&#039;w&#039;&#039;, and &#039;&#039;x&#039;&#039; to put it in this form so that the [[matrix ring]] is isomorphic&amp;lt;ref&amp;gt;[[Leonard Dickson]] (1914) &#039;&#039;Linear Algebras&#039;&#039;, §13 &amp;quot;Equivalence of the complex quaternion and matric algebras&amp;quot;, page 13&amp;lt;/ref&amp;gt; to the biquaternion [[ring (mathematics)|ring]].&lt;br /&gt;
&lt;br /&gt;
===Subalgebras===&lt;br /&gt;
Considering the biquaternion algebra over the scalar field of real numbers &#039;&#039;&#039;R&#039;&#039;&#039;, the set&lt;br /&gt;
{1, h, i, hi, j, hj, k, hk } forms a [[basis (linear algebra)|basis]] so the algebra has eight real [[dimension]]s.&lt;br /&gt;
Note the squares of the elements  hi, hj, and hk are all plus one, for example,&lt;br /&gt;
:&amp;lt;math&amp;gt;(hi)^2 \ = \  h^2 i^2 \ = \ (-1) (-1) \ =\  +1 .&amp;lt;/math&amp;gt;&lt;br /&gt;
Then the [[subalgebra]] given by&lt;br /&gt;
&amp;lt;math&amp;gt;\lbrace x + y(hi) : x, y \in R \rbrace &amp;lt;/math&amp;gt; is [[ring isomorphism|ring isomorphic]] to the plane of [[split-complex number]]s, which has an algebraic structure built upon the [[unit hyperbola]]. The elements &#039;&#039;hj&#039;&#039; and &#039;&#039;hk&#039;&#039; also determine such subalgebras. Furthermore,&lt;br /&gt;
&amp;lt;math&amp;gt;\lbrace x + yj : x,y \in C \rbrace &amp;lt;/math&amp;gt; is a subalgebra isomorphic to the [[tessarine]]s.&lt;br /&gt;
&lt;br /&gt;
A third subalgebra called [[coquaternion]]s is generated by hj and hk. First note that&lt;br /&gt;
(hj)(hk) = (&amp;amp;minus;1) i, and that the square of this element is &amp;amp;minus;1. These elements generate the [[dihedral group]] of the square. The [[linear subspace]] with basis {1, i, hj, hk} thus is closed under multiplication, and forms the coquaternion algebra.&lt;br /&gt;
&lt;br /&gt;
In the context of [[quantum mechanics]] and [[spinor]] algebra, the biquaternions hi, hj, and hk (or their negatives), viewed in the M(2,C) representation, are called [[Pauli matrices]].&lt;br /&gt;
&lt;br /&gt;
==Algebraic properties==&lt;br /&gt;
The biquaternions have two &#039;&#039;conjugations&#039;&#039;:&lt;br /&gt;
* the &#039;&#039;&#039;biconjugate&#039;&#039;&#039; or biscalar minus [[bivector (complex)|bivector]] is &amp;lt;math&amp;gt;q^* = w - xi - yj - zk \!\ ,&amp;lt;/math&amp;gt; and&lt;br /&gt;
* the [[complex conjugation]] of biquaternion coefficients &amp;lt;math&amp;gt;q^{\star} = w^{\star} + x^{\star} i + y^{\star} j + z^{\star} k \!&amp;lt;/math&amp;gt;&lt;br /&gt;
where &amp;lt;math&amp;gt;z^{\star} = a - bh&amp;lt;/math&amp;gt; when &amp;lt;math&amp;gt;z = a + bh,\quad a,b \in R,\quad h^2 = -1.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Note that &amp;lt;math&amp;gt;(pq)^* = q^* p^*, \quad (pq)^{\star} = p^{\star} q^{\star} , \quad (q^*)^{\star} = (q^{\star})^*.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Clearly, if &amp;lt;math&amp;gt;q q^* = 0 \!&amp;lt;/math&amp;gt; then &#039;&#039;q&#039;&#039; is a zero divisor. Otherwise &amp;lt;math&amp;gt;\lbrace q q^* \rbrace^{-1} \!&amp;lt;/math&amp;gt; is defined over the complex numbers. Further, &amp;lt;math&amp;gt;q q^* = q^* q \!&amp;lt;/math&amp;gt; is easily verified. This allows an inverse to be defined as follows:&lt;br /&gt;
* &amp;lt;math&amp;gt;q^{-1} = q^* \lbrace q q^* \rbrace^{-1}\!&amp;lt;/math&amp;gt;, iff &amp;lt;math&amp;gt;qq^* \neq 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Relation to Lorentz transformations===&lt;br /&gt;
Consider now the linear subspace&lt;br /&gt;
&amp;lt;ref&amp;gt;Lanczos (1949) Equation 94.16 page 305. The following algebra compares to Lanczos, except he uses ~ to signify quaternion conjugation and * for complex conjugation&amp;lt;/ref&amp;gt;&lt;br /&gt;
:&amp;lt;math&amp;gt;M = \lbrace q : q^* = q^{\star} \rbrace = \lbrace t + x(hi) + y(hj) + z(hk) : t, x, y, z \in R \rbrace .&amp;lt;/math&amp;gt;&lt;br /&gt;
&#039;&#039;M&#039;&#039; is not a subalgebra since it is not [[closure (mathematics)|closed under products]]; for example &amp;lt;math&amp;gt;(hi)(hj) = h^2 ij = -k \notin M.&amp;lt;/math&amp;gt;. Indeed, &#039;&#039;M&#039;&#039; cannot form an algebra if it is not even a [[magma (algebra)|magma]].&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Proposition:&#039;&#039;&#039; If &#039;&#039;q&#039;&#039; is in &#039;&#039;M&#039;&#039;, then &amp;lt;math&amp;gt;q q^* = t^2 - x^2 - y^2 - z^2 \!&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
proof: &amp;lt;math&amp;gt;q q^* = (t+xhi+yhj+zhk)(t-xhi-yhj-zhk) \!&amp;lt;/math&amp;gt;&lt;br /&gt;
:&amp;lt;math&amp;gt; = t^2 - x^2(hi)^2 - y^2(hj)^2 - z^2(hk)^2 = t^2 - x^2 - y^2 - z^2. \!&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Definition:&#039;&#039;&#039; Let biquaternion &#039;&#039;g&#039;&#039; satisfy &#039;&#039;g g&#039;&#039; * = 1. Then the &#039;&#039;&#039;Lorentz transformation&#039;&#039;&#039; associated with &#039;&#039;g&#039;&#039; is given by&lt;br /&gt;
:&amp;lt;math&amp;gt;T(q) = g^* q g^{\star}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Proposition:&#039;&#039;&#039; If &#039;&#039;q&#039;&#039; is in &#039;&#039;M&#039;&#039;, then &#039;&#039;T(q)&#039;&#039; is also in &#039;&#039;M&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
proof: &amp;lt;math&amp;gt;(g^* q g^{\star})^* = (g^{\star})^* q^* g = (g^*)^{\star} q^{\star} g = (g^* q g^{\star})^{\star}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Proposition:&#039;&#039;&#039; &amp;lt;math&amp;gt;\quad T(q) (T(q))^* = q q^* \!&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
proof: Note first that &#039;&#039;g g&#039;&#039; * = 1 means that the sum of the squares of its four complex components is one. Then the sum of the squares of the &#039;&#039;complex conjugates&#039;&#039; of these components is also one. Therefore, &amp;lt;math&amp;gt;g^{\star} (g^{\star})^* = 1.&amp;lt;/math&amp;gt; Now&lt;br /&gt;
:&amp;lt;math&amp;gt;(g^* q g^{\star})(g^* q g^{\star})^* = g^* q g^{\star} (g^{\star})^* q^* g = g^* q q^* g = q q^*.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==Associated terminology==&lt;br /&gt;
As the biquaternions have been a fixture of [[linear algebra]] since the beginnings of [[mathematical physics]], there is an array of concepts that are illustrated or represented by biquaternion algebra. The [[transformation group]] &amp;lt;math&amp;gt;G = \lbrace g : g g^* = 1 \rbrace \!&amp;lt;/math&amp;gt; has two parts, &amp;lt;math&amp;gt;G \cap H&amp;lt;/math&amp;gt;  and &amp;lt;math&amp;gt;G \cap M.&amp;lt;/math&amp;gt; The first part is characterized by &amp;lt;math&amp;gt;g = g^{\star}&amp;lt;/math&amp;gt; ; then the Lorentz transformation corresponding to &#039;&#039;g&#039;&#039; is given by &amp;lt;math&amp;gt;T(q) = g^{-1} q g \!&amp;lt;/math&amp;gt; since &amp;lt;math&amp;gt;g^* = g^{-1}. \!&amp;lt;/math&amp;gt; Such a transformation is a [[quaternions and spatial rotation|rotation by quaternion multiplication]], and the collection of them is [[O(3)]] &amp;lt;math&amp;gt;\cong G \cap H .&amp;lt;/math&amp;gt; But this subgroup of &#039;&#039;G&#039;&#039; is not a [[normal subgroup]], so no [[quotient group]] can be formed.&lt;br /&gt;
&lt;br /&gt;
To view &amp;lt;math&amp;gt;G \cap M&amp;lt;/math&amp;gt; it is necessary to show some subalgebra structure in the biquaternions. Let &#039;&#039;r&#039;&#039; represent an element of the [[quaternion#Square roots of −1|sphere of square roots of minus one]] in the real quaternion subalgebra &#039;&#039;&#039;H&#039;&#039;&#039;. Then (&#039;&#039;hr&#039;&#039;)&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; = +1 and the plane of biquaternions given by &amp;lt;math&amp;gt;D_r = \lbrace z = x + yhr : x, y \in R \rbrace&amp;lt;/math&amp;gt; is a commutative subalgebra isomorphic to the plane of [[split-complex number]]s. Just as the ordinary complex plane has a unit circle, &amp;lt;math&amp;gt;D_r \!&amp;lt;/math&amp;gt; has a [[unit hyperbola]] given by&lt;br /&gt;
:&amp;lt;math&amp;gt;exp(ahr) = \cosh(a) + hr\ \sinh(a),\quad a \in R. \!&amp;lt;/math&amp;gt;&lt;br /&gt;
Just as the unit circle turns by multiplication through one of its elements, so the hyperbola turns because &amp;lt;math&amp;gt;\exp(ahr) \exp(bhr) = \exp((a+b)hr). \!&amp;lt;/math&amp;gt; Hence these algebraic operators on the hyperbola are called [[versor#Hyperbolic versor|hyperbolic versors]]. The unit circle in &#039;&#039;&#039;C&#039;&#039;&#039; and unit hyperbola in &#039;&#039;D&#039;&#039;&amp;lt;sub&amp;gt;&#039;&#039;r&#039;&#039;&amp;lt;/sub&amp;gt; are examples of [[one-parameter group]]s. For every square root &#039;&#039;r&#039;&#039; of minus one in &#039;&#039;&#039;H&#039;&#039;&#039;, there is a one-parameter group in the biquaternions given by &amp;lt;math&amp;gt;G \cap D_r.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The space of biquaternions has a natural [[topology]] through the [[Euclidean metric]] on 8-space. With respect to this topology, &#039;&#039;G&#039;&#039; is a [[topological group]]. Moreover, it has analytic structure making it a six-parameter [[Lie group]]. Consider the subspace of [[bivector (complex)|bivector]]s  &amp;lt;math&amp;gt;A = \lbrace q : q^* = -q \rbrace \!&amp;lt;/math&amp;gt;. Then the [[exponential map]]&lt;br /&gt;
&amp;lt;math&amp;gt;\exp:A \to G&amp;lt;/math&amp;gt;  takes the real vectors to &amp;lt;math&amp;gt;G \cap H&amp;lt;/math&amp;gt; and the &#039;&#039;h&#039;&#039;-vectors to &amp;lt;math&amp;gt;G \cap M.&amp;lt;/math&amp;gt; When equipped with the [[commutator]], &#039;&#039;A&#039;&#039; forms the [[Lie algebra]] of &#039;&#039;G&#039;&#039;. Thus this study of a [[six-dimensional space]] serves to introduce the general concepts of [[Lie theory]]. When viewed in the matrix representation, &#039;&#039;G&#039;&#039; is called the [[special linear group]] [[SL(2,C)]] in M(2,C).&lt;br /&gt;
&lt;br /&gt;
Many of the concepts of [[special relativity]] are illustrated through the biquaternion structures laid out. The subspace &#039;&#039;M&#039;&#039; corresponds to [[Minkowski space]], with the four coordinates giving the time and space locations of events in a resting [[frame of reference]]. Any hyperbolic versor exp(&#039;&#039;ahr&#039;&#039;) corresponds to a [[velocity]] in direction &#039;&#039;r&#039;&#039; of speed &#039;&#039;c&#039;&#039; tanh &#039;&#039;a&#039;&#039;  where &#039;&#039;c&#039;&#039; is the [[velocity of light]]. The inertial frame of reference of this velocity can be made the resting frame by applying the [[Lorentz boost]] &#039;&#039;T&#039;&#039; given by &#039;&#039;g&#039;&#039; = exp(0.5&#039;&#039;ahr&#039;&#039;) since then &amp;lt;math&amp;gt;g^{\star} = \exp(-0.5ahr) = g^*&amp;lt;/math&amp;gt; so that &amp;lt;math&amp;gt;T(\exp(ahr)) = 1 .&amp;lt;/math&amp;gt;&lt;br /&gt;
Naturally the [[hyperboloid]]&lt;br /&gt;
&amp;lt;math&amp;gt;G \cap M,&amp;lt;/math&amp;gt; which represents the range of velocities for sub-luminal motion, is of physical interest. There has been considerable work associating this &amp;quot;velocity space&amp;quot; with the [[hyperboloid model]] of [[hyperbolic geometry]].  In special relativity, the [[hyperbolic angle]] parameter of a hyperbolic versor is called [[rapidity]]. Thus we see the biquaternion group &#039;&#039;G&#039;&#039; provides a [[group representation]] for the [[Lorentz group]].&lt;br /&gt;
&lt;br /&gt;
After the introduction of [[spinor]] theory, particularly in the hands of [[Wolfgang Pauli]] and [[Élie Cartan]], the biquaternion representation of the Lorentz group was superseded. The new methods were founded on [[basis (linear algebra)|basis vectors]] in the set&lt;br /&gt;
:&amp;lt;math&amp;gt;\lbrace q \ :\  q q^* = 0 \rbrace = \lbrace w + xi + yj + zk \ :\ w^2 + x^2 + y^2 + z^2 = 0 \rbrace &amp;lt;/math&amp;gt;&lt;br /&gt;
which is called the &amp;quot;complex light cone&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
==See also==&lt;br /&gt;
&lt;br /&gt;
*[[Conic octonion]]s (isomorphism)&lt;br /&gt;
*[[Hyperbolic quaternion#MacFarlane&#039;s hyperbolic quaternion paper of 1900|MacFarlane&#039;s use]]&lt;br /&gt;
*[[Quotient ring#Quaternions and alternatives|Quotient ring]]&lt;br /&gt;
*[[Hypercomplex number]]&lt;br /&gt;
&lt;br /&gt;
==Notes==&lt;br /&gt;
{{reflist|2}}&lt;br /&gt;
&lt;br /&gt;
==References==&lt;br /&gt;
* Proceedings of the Royal Irish academy November 1844 (NA) and 1850 page 388 from google books [http://books.google.com/books?id=ggoFAAAAQAAJ&amp;amp;pg=PA388&amp;amp;dq=proceedings+of+royal+irish+academy+1844+Hamilton&amp;amp;hl=en&amp;amp;ei=WysiTPLwMcKRnwepmoDBDw&amp;amp;sa=X&amp;amp;oi=book_result&amp;amp;ct=result&amp;amp;resnum=5&amp;amp;ved=0CD4Q6AEwBA]&lt;br /&gt;
* Arthur Buchheim (1885) [http://www.jstor.org/stable/2369176  &amp;quot;A Memoir on biquaternions&amp;quot;], [[American Journal of Mathematics]] 7(4):293 to 326 from [[Jstor]] early  content. &lt;br /&gt;
*{{citation|first=Arthur W.|last=Conway|authorlink=Arthur W. Conway|year=1911|title=On the application of quaternions to some recent developments in electrical theory|journal=Proceedings of the Royal Irish Academy|volume=29A|pages=1–9}}.&lt;br /&gt;
* [[William Rowan Hamilton]] (1853) &#039;&#039;Lectures on Quaternions&#039;&#039;, Article 669. This historical mathematical text is available on-line courtesy of [http://historical.library.cornell.edu/math/ Cornell University].&lt;br /&gt;
*Hamilton (1866) &#039;&#039;[http://books.google.com/books?id=fIRAAAAAIAAJ Elements of Quaternions]&#039;&#039; [[University of Dublin]] Press. Edited by William Edwin Hamilton, son of the deceased author.&lt;br /&gt;
*Hamilton (1899) &#039;&#039;Elements of Quaternions&#039;&#039; volume I, (1901) volume II. Edited by [[Charles Jasper Joly]]; published by [[Longmans, Green &amp;amp; Co.]].&lt;br /&gt;
*Kravchenko, Vladislav (2003),  &#039;&#039;Applied Quaternionic Analysis&#039;&#039;, Heldermann Verlag ISBN 3-88538-228-8.&lt;br /&gt;
*{{citation|first=Cornelius|last=Lanczos|authorlink=Cornelius Lanczos|year=1949|title=The Variational Principles of Mechanics|publisher=University of Toronto Press|pages=304–312}}.&lt;br /&gt;
*{{citation|first=Ludwik|last=Silberstein|authorlink=Ludwik Silberstein|year=1912|title=Quaternionic form of relativity|journal=Philosophy Magazine|series=Series 6|volume=23|pages=790–809}}.&lt;br /&gt;
*{{citation|first=Ludwik|last=Silberstein|authorlink=Ludwik Silberstein|title=The Theory of Relativity|year=1914}}.&lt;br /&gt;
*{{citation|last=Synge|first=J. L.|year=1972|title=Quaternions, Lorentz transformations, and the Conway-Dirac-Eddington matrices|journal=Communications of the Dublin Institute for Advanced Studies|series=Series A|volume=21}}.&lt;br /&gt;
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&lt;br /&gt;
{{Number Systems}}&lt;br /&gt;
&lt;br /&gt;
[[Category:Quaternions]]&lt;br /&gt;
[[Category:Ring theory]]&lt;br /&gt;
[[Category:Special relativity]]&lt;br /&gt;
[[Category:Articles containing proofs]]&lt;br /&gt;
&lt;br /&gt;
[[de:Biquaternion#Hamilton Biquaternion]]&lt;/div&gt;</summary>
		<author><name>84.133.101.35</name></author>
	</entry>
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