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Grassmann Algebra

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TheComplement.nb 37<br />

Graphic of a vector bound through the origin perpendicular to a bivector x�y.<br />

S � � � x � y � ��������� � x � y<br />

One of the interesting properties of such an entity is that it is equal to its own complement. We<br />

can show this by simple transformations using the formulae derived in the sections above. The<br />

complement of each term turns into the other term.<br />

����� ���������������<br />

S � � � x<br />

���������<br />

� y<br />

�<br />

�<br />

���������<br />

x � y<br />

� x � y � ����������<br />

��������� � ��1� 2 �� � x � y � ���������<br />

� x � y � � � x � y � ��������� � S<br />

We can verify this by expressing x and y in basis form and using <strong>Grassmann</strong>Simplify.<br />

�3; x� CreateVector�a�; y� CreateVector�b�;<br />

��S � S<br />

����� �<br />

True<br />

This entity is a simple case of a screw. We shall explore its properties further in Chapter 7:<br />

Exploring Screw <strong>Algebra</strong>, and see applications to mechanics in Chapter 8: Exploring Mechanics.<br />

5.11 Reciprocal Bases<br />

Contravariant and covariant bases<br />

Up to this point we have only considered one basis for �, which we now call the contravariant<br />

1<br />

basis. Introducing a second basis called the covariant basis enables us to write the formulae for<br />

complements in a more symmetric way. Contravariant basis elements were denoted with<br />

subscripted indices, for example ei . Following standard practice, we denote covariant basis<br />

elements with superscripts, for example ei . The two bases are said to be reciprocal.<br />

This section will summarize formulae relating basis elements and their cobases and<br />

complements in terms of reciprocal bases. For simplicity, we adopt the Einstein summation<br />

convention.<br />

In � 1 the metric tensor gij forms the relationship between the reciprocal bases.<br />

ei � gij�e j<br />

This relationship induces a metric tensor g m<br />

i,j on � m .<br />

2001 4 5<br />

5.48

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