The Principle Bundle Structure of Continuum Mechanics

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arXiv:2210.11537v1 [physics.flu-dyn] 20 Oct 2022
The Principle Bundle Structure
of
Continuum Mechanics
Stefano Stramigioli,
University of Twente, The Netherlands
Abstract
In this paper it is shown that the structure of the configuration space of any
continua is what is called in differential geometry a principle bundle Frankel
(2011). A principal bundle is a structure in which all points of the manifold
(each configuration in this case) can be naturally projected to a manifold
called the base manifold, which in our case represents pure deformations.
All configurations projecting to the same point on the base manifold (same
deformation) are called fibers. Each of these fibers is then isomorphic to
the Lie group se(3) representing pure rigid body motions. Furthermore,
it is possible to define what is called a connection and this allows to split
any continua motion in a rigid body sub-motion and a deformable one in a
completely coordinate free way. As a consequence of that it is then possible
to properly define a pure deformation space on which an elastic energy can
be defined. This will be shown using screw theory Ball (1900), which is vastly
used in the analysis of rigid body mechanisms but is not normally used to
analyse continua. Beside the just mentioned result, screw theory will also be
used to relate concepts like helicity and enstrophy to screw theory concepts.
Preprint submitted to Journal of Geometry and Physics October 24, 2022
1. Introduction
The study of continuous matter is of fundamental importance in all
branches of engineering mechanics Abraham and Marsden (1994), spanning
from solid deformations Jerrold E. Marsden (1983) to fluids Chorin and Marsden
(1993). A lot of interest is present also about proper coordinate free anal-
ysis descriptions of continua, like for example the excellent recent work of
Kolev and Desmorat (2021).
On the other hand in rigid body mechanics, the theory of screws, Ball
(1900) is vastly used to describe the motion of mechanisms of interconnected
rigid bodies. A nice example of its use can for example be found in the
analysis of dynamic balance by de Jong et al. (2019). The theory of screws is
based on two theorems: Mozzi’s theorem, for which an hystorical perspective
can be found in Ceccarelli (2000)1and Poinsot’s theorem. Mozzi’s theorem
states that any instantaneous rigid body motion can be interpreted as the
action of a rotation around an axis in space superimposed to a possible motion
along the same axis, proportional to a scalar called the pitch which indicates
the length traveled along the line for a full rotation along the line, like the
pitch of a “workshop” screw. Poinsot’s theorem is a dual theorem which
basically says that any systems of forces applied to a rigid body, would have
the same effect of a single force applied along a line in space and superimposed
to a possible torque around the same line, also relating the two by a scalar
pitch. These two theorems where then used in Ball (1900) to create a theory
based on the geometry of lines, or better screws, for the analysis of rigid
body kinematics. An extensive nice treatment of the mathematics and its
relation to Lie groups and Clifford’s algebras can be found in Selig (2005),
and specifically to Lie algebras in Stramigioli et al. (2002). In this work it
will be shown that it is possible to associate to each velocity and vorticity in
a certain point of a continua, an infinitesimal (associated to the infinitesimal
volume at the point) screw describing them at the same time. Such an
infinitesimal screw (relating to the infinitesimal volume element with velocity
vand vorticity dv), as in the rigid body case, will be characterised by an axis
and a pitch, but in this case the motion of the point will be considered
acted upon by the infinitesimal screw. It will be shown that the concepts of
helicity and enstrophy, well known in fluid dynamics, will get a very geometric
1In the literature of screw theory Chasles theory (1830) is often cited but Mozzi’s
presented the same result in 1763.
2
interpretation in the context of infinitesimal screws.
Considering that each of these screws are equivalent to elements of a Lie
algebra Stramigioli et al. (2002), they can be summed or integrated. Such an
operation will reveal the superimposed motion that each point will generate:
if all motions would follow the same rigid body motion, the resultant would
be such a motion, but in case of non rigid motions, the resultant will show
the “main rigid body motion” of the continuum. This construction will
be presented precisely and it will be shown that, thanks to this, it will be
possible to uniquely decompose, in a completely coordinate free way, the rigid
component of a continuum motion and the resting pure deformation. This
will be done by the introduction of what is called a differential geometric
connection Frankel (2011) in the principal bundle of motions.
During the paper, to stress the coordinate invariance of the approach,
different terms will be used as synonymous like geometric or intrinsic.
The paper will start in Sec.2 with the general framework formulation of
the analysis of a continua. In Sec.3 it will be shown that the configuration
space of a continuum has indeed a principle bundle structure whose fibers
are isomorphic to SE(3). In Sec. 4 the geometry and basics of screws theory
will be reviewed to then in Sec.5 use this insight to define the connection on
the principle bundle introduced in Sec.3. Finally, in Sec.6 the results will be
framed in the context of a geometric description of potential energy of the
deformation, only using an energy formulation to then draw some concluding
remarks in Sec.7.
Notation. A compact, orientable, n-dimensional Riemannian manifold M
with (possibly empty) boundary M models the spatial container of a non
relativistic continuum mechanical system. It possesses a metric field gand
induced Levi-Civita connection . The space of vector fields on Mis de-
fined as the space of sections of the tangent bundle T M, that will be de-
noted by Γ(T M). The space of differential p-forms is denoted by Ωp(M)
and we also refer to 0-forms as functions, 1-forms as co-vector fields and
n-forms as top-forms. For any vΓ(T M), we use the standard definitions
for the interior product by ιv: Ωp(M)p1(M) and the Lie derivative
operator Lvacting on tensor fields of any valence. The Hodge star operator
: Ωp(M)np(M), the volume form µ=1, as well as the ”musical” op-
erators : Γ(T M)1(M) and # : Ω1(M)Γ(T M), which respectively
transform vector fields to 1-forms and vice versa, are all uniquely induced
by the Riemannian metric in the standard way. To complement a purely
3
coordinate-free notation, we will represent tensorial quantities of interest in
local coordinates, denoted by x, when considered insightful, using Einstein
summation convention.
2. The Continuum Mechanics Setting
The goal of this paper is to show the intrinsic structures which appear in
the description of the kinematics of a continua. For this reason, there will be
no use of coordinates. The setting which will be used, using the approach of
Noll (1978) is the one of a continua moving in space and the various entities
of the problem will be introduced next.
2.1. Matter and Space
We consider the motion of matter in space where matter is mathematically
modeled as a manifold Mof dimension nto which some properties may be
associated via sections of a proper bundle. For example, in the case of a
purely mechanical description, we can consider µmn(M) as the mass top
form describing the mass distribution, where we have indicated with n(M)
the sections of the nalternating bundle to which n-forms on Mbelong. Any
other property could be defined in the same way. What is important to
realise is that such properties are all those properties which are conserved
for physical reasons and will be advected by the motion because strictly
connected to the matter and matter only, independently of any motion it
takes in the space. This could be for example also electrical charge. On the
other hand the scalar density ρis a quantity which is not conserved/advected
because its definition does not depend only on the matter, but on the relation
between the mass topform µmand a representation of the volume form of
the space.
We consider space as an ndimensional Riemannian manifold (S, g) where
with gsym+(T0
2S) we indicate the positive definite symmetric metric field
on Swith induced volume form µn(S).
2.2. The configuration space
We can now put matter into space with an embedding of the form:
e:M → S
4
摘要:

arXiv:2210.11537v1[physics.flu-dyn]20Oct2022ThePrincipleBundleStructureofContinuumMechanicsStefanoStramigioli,UniversityofTwente,TheNetherlandsAbstractInthispaperitisshownthatthestructureoftheconfigurationspaceofanycontinuaiswhatiscalledindifferentialgeometryaprinciplebundleFrankel(2011).Aprincipalbun...

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