Bi-Yang–Mills equations explained

In differential geometry, the Bi-Yang–Mills equations (or Bi-YM equations) are a modification of the Yang–Mills equations. Its solutions are called Bi-Yang–Mills connections (or Bi-YM connections). Simply put, Bi-Yang–Mills connections are to Yang–Mills connections what they are to flat connections. This stems from the fact, that Yang–Mills connections are not necessarily flat, but are at least a local extremum of curvature, while Bi-Yang–Mills connections are not necessarily Yang–Mills connections, but are at least a local extremum of the left side of the Yang–Mills equations. While Yang–Mills connections can be viewed as a non-linear generalization of harmonic maps, Bi-Yang–Mills connections can be viewed as a non-linear generalization of biharmonic maps.

Bi-Yang–Mills action functional

Let

G

be a compact Lie group with Lie algebra

ak{g}

and

E\twoheadrightarrowB

be a principal

G

-bundle
with a compact orientable Riemannian manifold

B

having a metric

g

and a volume form

\operatorname{vol}g

. Let

\operatorname{Ad}(E) :=E x Gak{g}\twoheadrightarrowB

be its adjoint bundle.

\Omega\operatorname{Ad

}^1(E,\mathfrak)\cong\Omega^1(B,\operatorname(E)) is the space of connections,[1] which are either under the adjoint representation

\operatorname{Ad}

invariant Lie algebra–valued or vector bundle–valued differential forms. Since the Hodge star operator

\star

is defined on the base manifold

B

as it requires the metric

g

and the volume form

\operatorname{vol}g

, the second space is usually used.

The Bi-Yang–Mills action functional is given by:[2]

1(B,\operatorname{Ad}(E))R, \operatorname{BiYM}
\operatorname{BiYM}\colon \Omega
F(A) :=\int

B\|\deltaAF

2d\operatorname{vol}
g.

Bi-Yang–Mills connections and equation

A connection

A\in\Omega1(B,\operatorname{Ad}(E))

is called Bi-Yang–Mills connection, if it is a critical point of the Bi-Yang–Mills action functional, hence if:[3]
d
dt

\operatorname{BiYM}(A(t))\vertt=0=0

for every smooth family

A\colon (-\varepsilon,\varepsilon)\Omega1(B,\operatorname{Ad}(E))

with

A(0)=A

. This is the case iff the Bi-Yang–Mills equations are fulfilled:[4]

(\deltaAdA+l{R}A)(\deltaAFA) =0.

For a Bi-Yang–Mills connection

A\in\Omega1(B,\operatorname{Ad}(E))

, its curvature
2(B,\operatorname{Ad}(E))
F
A\in\Omega
is called Bi-Yang–Mills field.

Stable Bi-Yang–Mills connections

Analogous to (weakly) stable Yang–Mills connections, one can define (weakly) stable Bi-Yang–Mills connections. A Bi-Yang–Mills connection

A\in\Omega1(B,\operatorname{Ad}(E))

is called stable if:
d2
dt2

\operatorname{BiYM}(A(t))\vertt=0>0

for every smooth family

A\colon (-\varepsilon,\varepsilon)\Omega1(B,\operatorname{Ad}(E))

with

A(0)=A

. It is called weakly stable if only

\geq0

holds.[5] A Bi-Yang–Mills connection, which is not weakly stable, is called unstable. For a (weakly) stable or unstable Bi-Yang–Mills connection

A\in\Omega1(B,\operatorname{Ad}(E))

, its curvature
2(B,\operatorname{Ad}(E))
F
A\in\Omega
is furthermore called a (weakly) stable or unstable Bi-Yang–Mills field.

Properties

See also

Literature

External links

Notes and References

  1. Web site: de los Ríos . Santiago Quintero . 2020-12-16 . Connections on principal bundles . 2024-11-09 . homotopico.com . Theorem 3.7 . en.
  2. Chiang 2013, Eq. (9)
  3. Chiang 2013, Eq. (5.1) and (6.1)
  4. Chiang 2013, Eq. (10), (5.2) and (6.3)
  5. Chiang 2013, Definition 6.3.2
  6. Chiang 2013, Proposition 6.3.3.