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Grassmann Algebra

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GeometricInterpretations.nb 4<br />

Points<br />

In order to describe position in space it is necessary to have a reference point. This point is<br />

usually called the origin.<br />

Rather than the standard technique of implicitly assuming the origin and working only with<br />

vectors to describe position, we find it important for later applications to augment the vector<br />

space with the origin as a new element to create a new linear space with one more element in its<br />

basis. For reasons which will appear later, such a linear space will be called a bound vector<br />

space.<br />

The only difference between the origin element and the vector elements of the linear space is<br />

their interpretation. The origin element is interpreted as a point. We will denote it in<br />

<strong>Grassmann</strong><strong>Algebra</strong> by �, which we can access from the palette or type as �dsO� (doublestruck<br />

capital O). The bound vector space in addition to its vectors and its origin now possesses<br />

a new set of elements requiring interpretation: those formed from the sum of the origin and a<br />

vector.<br />

P � � � x<br />

It is these elements that will be used to describe position and that we will call points. The vector<br />

x is called the position vector of the point P.<br />

It follows immediately from this definition of a point that the difference of two points is a vector:<br />

P1 � P2 � �� � x1� � �� � x2� � x1 � x2<br />

Remember that the bound vector space does not yet have a metric. That is, the distance between<br />

two points (the measure of the vector equal to the point difference) is not meaningful.<br />

The sum of a point and a vector is another point.<br />

P � y � � � x � y � � � �x � y�<br />

and so a vector may be viewed as a carrier of points. That is, the addition of a vector to a point<br />

carries or transforms it to another point.<br />

A scalar multiple of a point (of the form a p or a�p) will be called a weighted point. Weighted<br />

points are summed just like a set of point masses is deemed equivalent to their total mass<br />

situated at their centre of mass. For example:<br />

� mi�Pi � � mi��� � xi� � �� mi�� � � mi�xi<br />

���<br />

�<br />

� ����������������� ��<br />

� � mi �<br />

This equation may be interpreted as saying that the sum of a number of mass-weighted points<br />

� mi�pi is equivalent to the centre of gravity � � � mi �xi ������������� weighted by the total mass � mi .<br />

As will be seen in Section 4.4 below, a weighted point may also be viewed as a bound scalar.<br />

Historical Note<br />

2001 4 5<br />

� mi

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