Mathematical Principles of Theoretical Physics

(Rick Simeone) #1

3.1. BASIC CONCEPTS 113


the inner product ofXandYis defined by


(3.1.18) 〈X,Y〉=gij(p)XiYj.


It is clear that the inner product (3.1.18) is an invariant. The angle betweenXandYis defined
as


cosθ=

〈X,Y〉


|X||Y|


, |Z|=



gijZiZj forZ=X,Y.


  1. The inverse of(gij), denoted by


(gij) = (gij)−^1 ,

is a second order contra-variant tensor. In fact, by (3.1.16) we have that


I= ( ̃gij)( ̃gij) =

(


∂ φ
∂x

)− 1


(gij)

[(


∂ φ
∂x

)T]− 1


(g ̃ij),

whereIis unit matrix. It follows that


(g ̃ij) =

(


∂ φ
∂x

)T


(gij)

(


∂ φ
∂x

)


.


Hence{gij}is a second-order contra-variant tensor.


3.1.2 Physical fields and vector bundles


LetMbe a manifold. A vector bundle onMis obtained by gluing anN-dimensional linear
spaceENat each pointp∈M, denoted by


(3.1.19) M⊗pEN
def



p∈M

{p} ×ENp,

whereEN=RN, orCN, or the Minkowski space.
In a vector bundle (3.1.19), the geometric position ofENp is related withp∈M. For
example, the set of all tangent spaces is a vector bundle onM, called the tangent bundle of
M, denoted by
TM=M⊗pTpM.


For (3.1.19), if the positions of bundle spacesENp(p∈M)are independent ofp, then it
is called a geometrically trivial vector bundle. Vector bundles on a flat manifold are always
geometrically trivial.
The physical background of vector bundles are very clear. Each physical field must be
a mapping from the base spaceMto a vector bundleM⊗pEN. Actually, all physical
events occur in the space-time universeM, and the physical fields describing these events
are defined on vector bundles. This point of view is well illustrated in the following examples.

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