We can equip the (co)tangent bundle of a Riemannian manifold (B,g) with a Saski metric ˆg (see, for example, "On the geometry of tangent bundles" by Gudmunssun & Kappos) that looks like
ˆg=π∗g⊕gV
where
π:T(∗)B→B is the projection and
gV is the metric on the vertical directions of the fibration. In certain cases (i.e. when
B is affine), we can compactify by taking the quotient of
T(∗)B by a (dual) lattice
Γ(∗) to obtain the non-singular torus fibrations
T(∗)B/Γ(∗)→B.
In physics, there is a (I don't know how well-defined) notion of "time-compactification" by passing from a Riemannian manifold (M,ˆg+) to a pseudo-Riemannian manifold (M,ˆg−) via a "Wick rotation" (https://en.wikipedia.org/wiki/Wick_rotation). In flat coordinates, if
ˆg+=∑idx2i+∑jdy2j ,
then a Wick rotation is equivalent to the procedure of substituting
yj→√−1yj since
ˆg−=∑idx2i−∑jdy2j .
I would like to know whether this can be related to the procedure of taking the alternative metric
ˆg′=π∗g⊕(−1)gV
on
T(∗)B and whether this can somehow be seen as equivalent to compactification by taking the quoitient with respect to
Γ(∗).
This post imported from StackExchange MathOverflow at 2015-08-04 14:41 (UTC), posted by SE-user harry