I'm studying geometrical approaches to locomotion at low Reynolds number by reading the article Geometry of self-propulsion at low Reynolds number by Alfred Shapere and Frank Wilczek and found a situation I'm not understanding from a mathematical point of view what is being done.
The idea itself is not that hard and I shall present it first to make things clear: we consider that a body inside a fluid is a three-dimensional subset of the fluid region and we consider the body's shape as a parametrization of its boundary by means of a function S:U⊂R2→R3.
In that case, the idea as I understand is to consider a sequence of such shapes t↦St parametrized by time (that is a curve of shapes) which just contain deformations with the shape "held fixed" and try to find a curve of rigid motions resulting from the deformations.
If one considers M the space of all shapes, this is a space of functions. A sequence of shapes will be one curve γ:I⊂R→M. Considering then the euclidean group in three-dimensions (that is, the group of rigid motions in R3) which we denote E(3) there is a natural right action of E(3) in M in which a shape is translated and rotated by some element g∈E(3). Indeed, if S∈M then S⋅g will be the function
(S⋅g)(u,v)=S(u,v)⋅g
Where the right action on the right side is the natural action of E(3) in R3. Given the space M then we can also consider the quotient M/E(3) where shapes related by rigid motions are considered equivalent.
If π:M→M/E(3) is the natural projection, (M,π,M/E(3)) has the structure of a principle bundle with structure group E(3) and the problem at hand becomes the problem of finding a connection which allows the horizontal lift of sequence of unlocated shapes (just deformations) into sequences of deformations and movements.
In page 7 of the document, the author considers infinitesimal deformations, from which he will describe a way to obtain the connection (which he calls the gauge potential). He defines then one infinitesimal deformation by parametrizing a sequence of unlocated shapes by
S0(t)=S0+s(t),
where S0 is one initial shape and s(t) is infinitesimal. He then says we can expand s(t) as
s(t)=∑iαiwi
where wi is a "fixed basis of vector fields on S0". From one intuitive point of view I imagine that a tangent vector to M is equivalent to a vector field defined on the shape, so this makes sense.
Now, he considers the gauge potential as a vector field A with the property that denoting A˙S0(t)[S0(t)] the component of A at the point S(t) in the direction of ˙S0(t) this object belongs to the lie algebra of E(3), that is e(3) and we can find the curve of rigid motions R(t) by solving the equation
dRdt=RA˙S0(t)[S0(t)].
My doubt is then in what he does next: he considers this infinitesimal deformations S0(t) I gave and then he "expands the gauge potential" to second order in this way
A˙S0(t)[S(t)]=Av(t)[S0]+∑i∂Av∂wi˙αi≈∑jAwj˙αj+∑i∂Av∂wiαi˙αj
where this v(t)=S′0(t). Now what is going on here? I simply cannot understand where this equation came from and what does it means. What is really happening here?
This post imported from StackExchange Physics at 2015-04-09 12:10 (UTC), posted by SE-user user1620696