In differential geometry, the curvature form describes curvature of a connection on a principal bundle. The Riemann curvature tensor in Riemannian geometry can be considered as a special case.
Definition
Let G be a Lie group with Lie algebra
g
{\displaystyle {\mathfrak {g}}}
, and P → B be a principal G-bundle. Let ω be an Ehresmann connection on P (which is a
g
{\displaystyle {\mathfrak {g}}}
-valued one-form on P).
Then the curvature form is the
g
{\displaystyle {\mathfrak {g}}}
-valued 2-form on P defined by
-
Ω
=
d
ω
+
1
2
[
ω
∧
ω
]
=
D
ω
.
{\displaystyle \Omega =d\omega +{1 \over 2}[\omega \wedge \omega ]=D\omega .}
(In another convention, 1/2 does not appear.) Here
d
{\displaystyle d}
stands for exterior derivative,
[
⋅
∧
⋅
]
{\displaystyle [\cdot \wedge \cdot ]}
is defined in the article "Lie algebra-valued form" and D denotes the exterior covariant derivative. In other terms,[1]
-
Ω
(
X
,
Y
)
=
d
ω
(
X
,
Y
)
+
1
2
[
ω
(
X
)
,
ω
(
Y
)
]
{\displaystyle \,\Omega (X,Y)=d\omega (X,Y)+{1 \over 2}[\omega (X),\omega (Y)]}
where X, Y are tangent vectors to P.
There is also another expression for Ω: if X, Y are horizontal vector fields on P, then[2]
-
σ
Ω
(
X
,
Y
)
=
−
ω
(
[
X
,
Y
]
)
=
−
[
X
,
Y
]
+
h
[
X
,
Y
]
{\displaystyle \sigma \Omega (X,Y)=-\omega ([X,Y])=-[X,Y]+h[X,Y]}
where hZ means the horizontal component of Z, on the right we identified a vertical vector field and a Lie algebra element generating it (fundamental vector field), and
σ
∈
{
1
,
2
}
{\displaystyle \sigma \in \{1,2\}}
is the inverse of the normalization factor used by convention in the formula for the exterior derivative.
A connection is said to be flat if its curvature vanishes: Ω = 0. Equivalently, a connection is flat if the structure group can be reduced to the same underlying group but with the discrete topology.
Curvature form in a vector bundle
If E → B is a vector bundle, then one can also think of ω as a matrix of 1-forms and the above formula becomes the structure equation of E. Cartan:
-
Ω
=
d
ω
+
ω
∧
ω
,
{\displaystyle \,\Omega =d\omega +\omega \wedge \omega ,}
where
∧
{\displaystyle \wedge }
is the wedge product. More precisely, if
ω
i
j
{\displaystyle {\omega ^{i}}_{j}}
and
Ω
i
j
{\displaystyle {\Omega ^{i}}_{j}}
denote components of ω and Ω correspondingly, (so each
ω
i
j
{\displaystyle {\omega ^{i}}_{j}}
is a usual 1-form and each
Ω
i
j
{\displaystyle {\Omega ^{i}}_{j}}
is a usual 2-form) then
-
Ω
j
i
=
d
ω
i
j
+
∑
k
ω
i
k
∧
ω
k
j
.
{\displaystyle \Omega _{j}^{i}=d{\omega ^{i}}_{j}+\sum _{k}{\omega ^{i}}_{k}\wedge {\omega ^{k}}_{j}.}
For example, for the tangent bundle of a Riemannian manifold, the structure group is O(n) and Ω is a 2-form with values in the Lie algebra of O(n), i.e. the antisymmetric matrices. In this case the form Ω is an alternative description of the curvature tensor, i.e.
-
R
(
X
,
Y
)
=
Ω
(
X
,
Y
)
,
{\displaystyle \,R(X,Y)=\Omega (X,Y),}
using the standard notation for the Riemannian curvature tensor.
Bianchi identities
If
θ
{\displaystyle \theta }
is the canonical vector-valued 1-form on the frame bundle, the torsion
Θ
{\displaystyle \Theta }
of the connection form
ω
{\displaystyle \omega }
is the vector-valued 2-form defined by the structure equation
-
Θ
=
d
θ
+
ω
∧
θ
=
D
θ
,
{\displaystyle \Theta =d\theta +\omega \wedge \theta =D\theta ,}
where as above D denotes the exterior covariant derivative.
The first Bianchi identity takes the form
-
D
Θ
=
Ω
∧
θ
.
{\displaystyle D\Theta =\Omega \wedge \theta .}
The second Bianchi identity takes the form
-
D
Ω
=
0
{\displaystyle \,D\Omega =0}
and is valid more generally for any connection in a principal bundle.
The Bianchi identities can be written in tensor notation as:
R
a
b
m
n
;
ℓ
+
R
a
b
ℓ
m
;
n
+
R
a
b
n
ℓ
;
m
=
0.
{\displaystyle R_{abmn;\ell }+R_{ab\ell m;n}+R_{abn\ell ;m}=0.}
The contracted Bianchi identities are used to derive the Einstein tensor in the Einstein field equations, a key component in the general theory of relativity.
Notes
- since
[
ω
∧
ω
]
(
X
,
Y
)
=
1
2
(
[
ω
(
X
)
,
ω
(
Y
)
]
−
[
ω
(
Y
)
,
ω
(
X
)
]
)
{\displaystyle [\omega \wedge \omega ](X,Y)={\frac {1}{2}}([\omega (X),\omega (Y)]-[\omega (Y),\omega (X)])}
. Here we use also the σ = 2 {\displaystyle \sigma =2}
Kobayashi convention for the exterior derivative of a one form which is then d ω ( X , Y ) = 1 2 ( X ω ( Y ) − Y ω ( X ) − ω ( [ X , Y ] ) ) {\displaystyle d\omega (X,Y)={\frac {1}{2}}(X\omega (Y)-Y\omega (X)-\omega ([X,Y]))}
- Proof:
σ
Ω
(
X
,
Y
)
=
σ
d
ω
(
X
,
Y
)
=
X
ω
(
Y
)
−
Y
ω
(
X
)
−
ω
(
[
X
,
Y
]
)
=
−
ω
(
[
X
,
Y
]
)
.
{\displaystyle \sigma \Omega (X,Y)=\sigma d\omega (X,Y)=X\omega (Y)-Y\omega (X)-\omega ([X,Y])=-\omega ([X,Y]).}
References
- Shoshichi Kobayashi and Katsumi Nomizu (1963) Foundations of Differential Geometry, Vol.I, Chapter 2.5 Curvature form and structure equation, p 75, Wiley Interscience.