In a loop (+dx,+dy,-dx,-dy) the phase increases by :
Ax dx + (Ay + ¶x Ay dx) dy - (Ax + ¶y Ax dy) dx - Ay dy
= (¶x Ay - ¶y Ax) dx dy
= Fxy dx dy
Kaluza-Klein theory
The vielbeins eam are the matrices of base changing between curved and
locally flat coordinates.
The metric tensor gmn in curved coordinates is :
gmn = hab eam ebn
where hab is the metric tensor of the flat space-time (1 -1 -1 -1 on
the diagonal, 0 elsewhere).
According to Kaluza-Klein theory, gauge fields are equivalent to gravitation (curvature of space-time according to general relativity) in compactified dimensions.
The vielbein is :
eam = ( e'a'm 0 ) ( e''a''n'' An''m e''a''m'' )
We can number the dimensions of space-time from 0 to 3 (0=t, 1=x, 2=y, 3=z)
and the compactified dimensions from 4 to d-1, and consider all the tensor defined
for indices varying from 0 to d-1, completed with zeros, for example :
Amm = ( 0 0 ) ( Amm 0 )
With this convention, we have :
eam = e'am + e''an Anm + e''am
= e'a'm + e''an (Anm + dnm)
= e'am + e''am + e''am Amm
Then the metric tensor in curved coordinates is :
gmn = hab eam ebn
= hab (e'am + e''am + e''am Amm)
(e'bn + e''bn + e''bn Ann)
= hab e'am e'bn
+ hab e'am e''bn
+ hab e'am e''bn Ann
+ hab e''am e'bn
+ hab e''am e''bn
+ hab e''am e''bn Ann
+ hab e''am Amm e'bn
+ hab e''am Amm e''bn
+ hab e''am Amm e''bn Ann
Since hab e'am e''bn = 0 because hab is not 0 only if a = b,
e'am is not zero only if a is in 0..3 and e''bn is not zero only if
b is in 4..d-1, and same for hab e''am e'bn we have :
gmn = hab e'am e'bn
+ hab e''am e''bn
+ hab e''am e''bn Ann
+ hab e''am Amm e''bn
+ hab e''am Amm e''bn Ann
= g'mn
+ g''mn
+ g''mn Ann
+ g''mn Amn
+ g''mn Amm Ann