tokyo 04 dias
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Alain Bossavit
The question of forces
Laboratoire de Génie Électrique de Paris (CNRS)
Old controversies,
modern geometrical tools
http://www.lgep.supelec.fr/mse/perso/ab/bossavit.html
in ElectromagneticsOverlays, not part of
presented slides, contain
summary of oral comments
Overlays, not part of presented slides, contain
summary of oral comments
Tokyo,
Friday 11 June 2004
Thanks to organizers and
Prof. Takagi for support
Tokyo,
Friday 11 June 2004
Thanks to organizers and
Prof. Takagi for support
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Magnetoformingform
Conducting plate
Coil, with strong, shorttransient pulse
Countless problems require force computation in moving or deforming conductorsand/or magnets. Most often, the J × B formula suffices ...
Countless problems require force computation in moving or deforming conductorsand/or magnets. Most often, the J × B formula suffices ...
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Magnetoforming
J
sJ
B FJ × B, ↑
uCoenergy:Φ(u) ~ u |J |
s 2
Force: ∂ Φ > 0u
Force is, of course, upwards,
as more involved, but also more
general, rule based on derivation
of coenergy shows. (More on
that later.)
Force is, of course, upwards,
as more involved, but also more
general, rule based on derivation
of coenergy shows. (More on
that later.)
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Melting and stirring of liquid metals
σ > 0
µ >> µ0
J × B also OK for MHD applications, although Eulerian setup makes things more
difficult to handle (term v × B, with no obvious discrete form, to be included inOhm’ s law)
J × B also OK for MHD applications, although Eulerian setup makes things more
difficult to handle (term v × B, with no obvious discrete form, to be included in
Ohm’ s law)
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Rail
Mobile
µ >> µ0
µ >> µ0
B
Maglev
(manip)
In some situations, J × B definitely
not relevant. E.g., with magnets (be it
electromagnets, as here, or permanentones).
In some situations, J × B definitely
not relevant. E.g., with magnets (be it
electromagnets, as here, or permanentones).
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B
HB
– Hc
r B = µ (H + H )c
B = B + µ Hr
0 0
div B = 0
Hc
B = µ H0
rot H = rot H
div B = 0
rot H = 0c
~
~
B = µ (H + H )0c
F = (rot H ) × B
c
F
[1] Suppose hard magnet, with
simple affine constitutive law,
that can be expressed in twoequivalent ways, either this “
(with constant remanent
induction), or ...
[1] Suppose hard magnet, with
simple affine constitutive law,
that can be expressed in twoequivalent ways, either this “
(with constant remanent
induction), or ...
[2] … that “ (with
constant coercive field). If magnet alone in space,
equations are as shown
below, ” ...
[2] … that “ (with
constant coercive field). If magnet alone in space,
equations are as shown
below, ” ...
[3] … which is
equivalent to this “ ,
with amperian currents
as source, ...
[3] … which is
equivalent to this “ ,
with amperian currentsas source, ...
[4] … from which it would seem
that a plausible force formula’ would derive. But ….
[4] … from which it would seem
that a plausible force formula’ would derive. But ….
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B
HB
– Hc
r B = µ (H + H )c
B = B + µ Hr
0 0
div B = 0
Br
B = B + µ H0
rot H = 0
div B = div B
rot H = 0
~
B = µ H0
F = (div B ) H
r
Fr ~
r
– – ––––
+ ++
[5] … this alternative procedure
(take equivalent magnetic chargeas source) is just as reasonable, ...
[5] … this alternative procedure
(take equivalent magnetic chargeas source) is just as reasonable, ...
[6] … and gives a totally different
result for the force field.
[6] … and gives a totally different
result for the force field.
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Which for sure shatters confidence about naive approaches to the
force question.
All the more so that classical treatises are not of great help to the
programmer who is only looking for “some reliable formula to code”.
Indeed, here follows a sample of what the literature offers about
“the” analytical expression of force density:
Which for sure shatters confidence about naive approaches to the
force question.
All the more so that classical treatises are not of great help to the
programmer who is only looking for “some reliable formula to code”.Indeed, here follows a sample of what the literature offers about
“the” analytical expression of force density:
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F = M · ∇B + M × (∇ × B) – ∇B · (v × (M × v))/c 2
P. Penfield, Jr., H.A. Haus: Electrodynamics of Moving Media, The MIT Press (Cambridge, Ma.), 1967, p. 216
(electric field contribution neglected)
F = (J × B) – –– H ∇µ1
2
2
F.N.H. Robinson: Macroscopic Electromagnetism, Pergamon Press (Oxford), 1973
F = – ∇p – –– H ∇µ + –– J × H0
8π
1 2 µ
cL. Landau, E. Lifschitz: lectrodynamique des milieux continus, Mir (Moscou), 1965, p. 190
(for a fluid; p is pressure)0
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Numerical problems with J × B
H = ∑ h We
e ∈ E e => J = rot H
µ H · grad ϕ' = 0 ∀ ϕ'
edge elementB = µH
=> div B ~ 0 (weakly)
F = (rot H) × B
conformal non-conformal
Numerical methods are either
“h-oriented” (rot H = J exactly
enforced, but Faraday
satisfied in only “mesh-weak”form) or “b-oriented” (the other
way round). In both cases,
terms in the J x B formula are
not approximated with the
same accuracy.
Numerical methods are either
“h-oriented” (rot H = J exactly
enforced, but Faraday
satisfied in only “mesh-weak”
form) or “b-oriented” (the other
way round). In both cases,
terms in the J x B formula are
not approximated with the
same accuracy.
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And what about the Maxwell tensor
Ω F(Ω) = FΩ
F(Ω) = [(n · B) H – –– (B · H) n]1
2∂Ω
(flux of M = B H – –– B H δ )
ij i j 1
2
k kij ij
Main drawback of this popular device: it yields force integrals,
i.e., resultants and/or torques, not the force field .
Main drawback of this popular device: it yields force integrals,
i.e., resultants and/or torques, not the force field .
Besides, the expression of M is not a primitive result in
Maxwell’s theory. It is derived from that of local force.
Besides, the expression of M is not a primitive result in
Maxwell’s theory. It is derived from that of local force.
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1976Oxford
1989Tokyo
"Force" papers in the Compumag record 1978
Grenoble1981
Chicago1983Genoa
1985Ft-Collins
1987Graz
1991Sorrento
1993Miami
1995Berlin
1997Rio
1999Sapporo
2001Évian
Bizarre, bizarre.
Reichert
Aldefeld
WeissenburgerAldefeld Coulomb
Müller
Miya Miyata–Miya
Eastham
Reyne
Kabashima
Brauer
Matinescu
Morisue
Kabashima
Tani
Ito–Kanazawa
Kawase-Ito
Müller
Henneberger
Sattler, Shen
Liu, Freeman
Ren
Bossavit
Tsuchimoto
Arturi
Rodger
Kameari
Ren–Razek
Henrotte
JenkinsSmithHowe
Nishiguchi
Richard
NiikuraKameari
Takagi–Tani
Park KimS.-y. Hahn
Copeland KoppO'Handley
BartschWeiland
Ren
TegopoulosWiak
Tsukerman
Takahashi
Im–Kim
Tsuboi
Brauer
Besbes–Ren
Kurz FetzerLehner
TegopoulosWen Yao
McFee
Ito–Kawase
Richard
ReyneMeunier
Hur, Chun,Lee, Hyun
Vandevelde
Medeiros
Divoux, Reyne
SaviniDi BarbaPerugia
Fireteanu
Sebestyen
Hameyer
VandeveldeMelkebeek
Curiously, interest for forces in the Compumag
community has passed its peak, it seems. Yet,
theoretical problems discussed at the very first
Compumag conference (post-talk discussions were
opportunely recorded) seem still to be with us.
Curiously, interest for forces in the Compumag
community has passed its peak, it seems. Yet,
theoretical problems discussed at the very first
Compumag conference (post-talk discussions were
opportunely recorded) seem still to be with us.
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Rail
Mobile
µ >> µ0
µ >> µ0
B
Maglev
(manip)
Was presented, for instance,a 2D modelling of this model
problem for levitation
devices:
Was presented, for instance,
a 2D modelling of this model
problem for levitation
devices:
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The first Compumag paper on forcesK. Reichert, H. Freundl, W. Vogt: "The calculation of forcesand torques within numerical magnetic field calculationmethods", Proc. Compumag, Oxford (1976), pp. 64-73.
Integration
pathWinding
Rail
Core
Winding
Integration
surfaces
Magnetic levitation system
Note use of Maxwell’s tensor integrationNote use of Maxwell’s tensor integration
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Carpenter: "We need an operational definition of 'stress',
which is not a quantity which is directly observable." Authors: "A permanent magnet (...) can be modelled either by surfacecharges or by Ampère's currents. The total force in both cases is the
f = J × (B – M ) – H div M – grad µ H dH
With B = µH + M , they findp
p p0
H
Say "inadvisable" because of non-linearity, "magnetic history should
be known". Use surface integration with surface in µ = const (air).
Hammond: Can the surface traverse iron?
Authors: No, "artificial airgap not allowed",because "it may change the original fielddistribution", unless modification is slight.
Integration
paths
same but the stress inside is different." (We agree that) "the distinction between mag-
netic and mechanical forces inside is 'model depending' and therefore meaningless."
(Yet another expression of
local force field …)
(Yet another expression of
local force field …)
Discussion suggests basic disagreements about the very status of the “localforce” conce t. Some even seem to doubt its obective character.
Discussion suggests basic disagreements about the very status of the “local
force” concept. Some even seem to doubt its objective character.
As we saw← earlier
As we saw← earlier
Maxwell
tensor’s
integration
around a
node to getlocal force
Maxwell
tensor’s
integration
around a
node to getlocal force
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Carpenter : "there must be a definitive answer [to the questionof force density] in every case, and one could use strain gaugesto discover it. There ought, therefore, to be a mathematicalmethod which is physically more correct than the others."
Should we agreeinc(ε) = 0 σ = κε div(σ) =
strainstress force
*
*As quoted by G. Reyne, thesis, 1987.
Moon: "(...) the representation of the magnetic body forceis not unique (...). This raises serious questions regarding
the internal stress state in a magnetized body."
“ incompatibility
tensor
Elasticity equations
(here in simplified,symbolic form), say ε
should satisfy
compatibility conditions,
constitutive relationshould hold, and σ
should balance body
force.
Elasticity equations
(here in simplified,symbolic form), say ε
should satisfy
compatibility conditions,
constitutive relation
should hold, and σ
should balance body
force.
Strain ε is directly
observable, but notσ. Hence room for
disagreement. But i
constitutive law
known, then
cannot fail to beunique.
Strain ε is directly
observable, but notσ. Hence room for
disagreement. But if
constitutive law
known, then f
cannot fail to beunique.
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What I believe:
Force unambiguously derives, viathe virtual work principle, from
the material's constitutive law
Constitutive laws are mixed in magnetoelasticity:
both H and σ depend on both B and ε.Incomplete knowledge won't do.
Conflicting force formulas come from diverging,
unspoken assumptions about constitutive laws
Constitutive laws ought to be
measured, not theorized about
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Let’s proceed. The language of differential forms will be used. Here
follows a short reminder on the differential-geometric approach to
Maxwell’s equations, a dictionary of correspondences with the better
known vector-fields formalism, and a review of discretization
principles which underlie modern “mesh-based” computational
methods (FDM, FEM, FVM).
Let’s proceed. The language of differential forms will be used. Here
follows a short reminder on the differential-geometric approach to
Maxwell’s equations, a dictionary of correspondences with the better
known vector-fields formalism, and a review of discretization
principles which underlie modern “mesh-based” computational
methods (FDM, FEM, FVM).
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The electric field: a mappinge : ORIENTED CURVE → REAL
Unit charge pushedalong curve c ∫∫ ∫ ∫ e
cvolts
with additivity:
and continuity (w.r.t. variations of )c
∫∫ ∫ ∫
e = ∫∫ ∫ ∫
e + ∫∫ ∫ ∫
e,c + c 1 2 c2c1
Work involved:
Most economical
translation of observable
properties of e: as a map
(from curves to reals). This
is the very definition of a
differential form (of degree
1, the dimension of curves).
Most economicaltranslation of observable
properties of e: as a map
(from curves to reals). This
is the very definition of adifferential form (of degree
1, the dimension of
curves).
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E
(the vector field) e(the 1-form)as a proxy fo
Change " ", change E (and τ ), for same e
c
∫ e = Ec
∫ c
The observable is not E but e, the differential form
Standard representation
using vector field E ...
Standard representationusing vector field E ... … involves irrelevant metric
structure (dot product, length …)
… involves irrelevant metric structure (dot product, length …)
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Σ∀- ∂ ∫ d + ∫ h = ∫ jΣ ∂Σ Σt
S∀∂ ∫ b + ∫ e = 0S ∂St
–∂ d + dh = jt
∂ b + de = 0t
b = µh, d = εe source of field
New status for ε and µ, now operators,(Hodge) of type 1-FORM → 2-FORM :
Discretization strategy: Instead of all
S, Σ, enforce this for surfaces spanned
by faces of interlocked meshes:
rima
dua
outer oriented surfaceouter oriented surface
inner oriented surfaceinner oriented surface
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Correspondences: ∫ τ · E
c ∫ e
c
∫ n · JΣ ∫ jΣ
grad ϕ dϕ
rot E dediv J d j
J · E ∧ e ν |B|
2 ν b ∧ b
v × B i bv
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N → E → F → VG R D
grad rot div
here, R = – 1
fe
e, aat edges
h at dual edges(i.e., faces)
d, j at dual faces
h = h : f ∈ F f b = b : f ∈ F f
b at faces
e = e : e ∈ E e d = d : e ∈ E e
νν
εεεε
Set of nodesSet of nodes
Set of facesSet of faces
”
Incidence matrices”
” Incidence matrices ”
S uare matrices built as ex lained below and in com anion slideshowSquare matrices, built as explained below (and in companion slideshow)
Everything lives on the discrete structure (mesh + some dual mesh) from now onEverything lives on the discrete structure (mesh + some dual mesh) from now on
Dual mesh (n – p)-cells matched 1-to-1 with p-cells of primal meshDual mesh (n – p)-cells matched 1-to-1 with p-cells of primal mesh
G, analog of G, analog of R, analog of
R, analog of D, analog of
D, analog of
Di ti ti t lkit il bl ( l b b b t b R b t )
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Then, automatic spatial discretizationof Maxwell's equations:
–∂ d + R h = jt
t
∂ b + Re = 0th = bνννν d = eεεεε
hence a Yee-like scheme ("GFD"):
b – bk + 1/2 k – 1/2
+ Re = 0
k
δt
ε– e – ek + 1 k
δt
+ R b = jννννt k + 1/2k + 1/2
Discretization toolkit now available (replace b by b, rot by R, µ by µµµµ, etc.).Discretization toolkit now available (replace b by b, rot by R, µ by µµµµ, etc.).
More general than what we need. Term in ε (displacement currents) to be ignored, and j replaced by σe + js, (source current).More general than what we need. Term in ε (displacement currents) to be ignored, and j replaced by σe + js, (source current).
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Now, some motivation for “Lagrangian” approach to forces,
with “comoving” mesh.
Now, some motivation for “Lagrangian” approach to forces,
with “comoving” mesh.
Note that neglecting term ε ∂D/∂t amounts to ignore Coulomb
forces (as if ε were 0)
Note that neglecting term ε ∂D/∂t amounts to ignore Coulomb
forces (as if ε were 0)
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s
Bs
(AC)
(steady)
A standard benchmark (pbs. 12 &16 of the "TEAM workshop")
Strong short pulse in the coil
creates equivalent of “kicking blow”
to the clamped elastic plate, which
then deforms in complex (and well-
documented, by lab.measurements) manner.
Strong short pulse in the coilcreates equivalent of “kicking blow”
to the clamped elastic plate, which
then deforms in complex (and well-
documented, by lab.measurements) manner.
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u
Some air around
meshed, too
trajectory: t → u(t) (possibly virtual)
placement u
velocity field: v = ∂ ut (at t = 0, when u(0) = id)
Clearly, having mesh nodes, edges, etc., fixed
w.r.t. matter, has advantages. Hence
Lagrangian setup preferred.
Clearly, having mesh nodes, edges, etc., fixedw.r.t. matter, has advantages. Hence
Lagrangian setup preferred.
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Reference space Physical space
u
air
conductor,magnet, ...
State at time 0 State at time t
But thus having two distinct 3D manifolds mandates some care about which differential forms one speaks about. Centralnotion: placement u, i.e., mapping of material points (including fictitious “air points”) from left to right.
But thus having two distinct 3D manifolds mandates some care about which differential forms one speaks about. Centralnotion: placement u, i.e., mapping of material points (including fictitious “air points”) from left to right.
(or “material manifold”)(or “material manifold”)
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(rot H = σ(E + v × B) + J , ∂ B + rot E = 0)t
s
b = µh,
∫ h = ∫ j∂Σ Σ Σ∀
∂ ∫ b + ∫ e = 0S ∂St S∀
= σ(e – i b)v
dh = j
∂ b + dh = 0t
Equations with movement, in Eulerian
formulation, displacement currents ignored
Note v x B term, here in DF notation, “inner product”,or “contraction”, of 2-form b by velocity field v
Note v x B term, here in DF notation, “inner product”,or “contraction”, of 2-form b by velocity field v
Small case for “Eulerian” objectsSmall case for “Eulerian” objects
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Equations in so-called material form
(Lagrangian formulation):
material surface flux
B : S → ∫ b = ∫ u bu (S)t S t
*
"pull-back" of b
Same for H (m.m.f.), J (current through materialsurface), but E = u*(e – i b). Then,
b
ν
hu*
u*B
H
νu
∂ B + d E = 0, d H = J + Js
t
but now, H = ν B, and energy isu12 ν |B| ≡ νb ∧ b = ν B ∧ B
2u
12
12
t v
SMALL CAPITALS for
“Lagrangian” objects
SMALL CAPITALS for
“Lagrangian” objects
Definition of “material” flux
density B, and of pullback
Definition of “material” fluxdensity B, and of pullback
So B is pull-back
of b via u
So B is pull-back
of b via u
But E is not the pull-back
of e: E meant to represent e.m.f. in moving
conductor (as measured by comoving observer)
But E is not the pull-back of e: E meant to represent e.m.f. in moving
conductor (as measured by comoving observer)
Hodge map on material manifold, defined bycommutative dia ram de ends on lacement
Hodge map on material manifold, defined by
commutative diagram, depends on placement
Define two functionals (here quadratic but more generally conjugate convex functions) called energy and coenergy on material manifold
Define two functionals (here, quadratic, but more generally, conjugate convex functions), called energy and coenergy, on material manifold.
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Magnetic energy and co-energy
Ψ(u, B)
µ H ∧ Hu1
2ν B ∧ Bu1
2
Φ(u, H)
Theorem: Force = – ∂ Ψ ≡ ∂ Φu u
Proof: d [Ψ(u(t), B(t))] = <∂ Ψ, ∂ u> + ∫ H ∧ ∂ Bt ttu
d [energy] = – <F, ∂ u> – ∫ J ∧ Et
∂ B + d E = 0, d H = J => ∫ H ∧ ∂ B = – ∫ J ∧ Et t
t
Define two functionals (here, quadratic, but more generally, conjugate convex functions), called energy and coenergy, on material manifold.
See ICS News, 11, 1 (2004), pp. 4-12, for detailed proof. The point here is that this is a mathematical result, stemming from
an unassailable postulate (middle line)
See ICS News, 11, 1 (2004), pp. 4-12, for detailed proof. The point here is that this is a mathematical result, stemming from
an unassailable postulate (middle line)
Energy comes out as: work of forces exerted on rest of the world (1), plus Joule losses minus power tapped from supply network (2)Energy comes out as: work of forces exerted on rest of the world (1), plus Joule losses minus power tapped from supply network (2)
(1)(1)(2)
(2)
Algebraic consequences of the equations, plus differentiation of energy, using chain rule, then do the job. (Note that H = ∂BΨ is just the B–Hlaw.) Velocity v in tangent space, and force F in cotangent space at u of “configuration manifold” U, with < , > for duality pairing.
Algebraic consequences of the equations, plus differentiation of energy, using chain rule, then do the job. (Note that H =∂
BΨ
is just the B–Hlaw.) Velocity v in tangent space, and force F in cotangent space at u of “configuration manifold” U, with < , > for duality pairing.
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u
Coenergy: Φ(u, H) ~ u |J|2
Force: ∂ Φ > 0u
Example application. Eddy currents in plate make magnetic barrier, forcing a horizontal and uniform H in airgap. Assume mmf invariable
as u increases, thereby proportional to J, coil current. Then, coenergy proportional to u, hence force is upwards.
Example application. Eddy currents in plate make magnetic barrier, forcing a horizontal and uniform H in airgap. Assume mmf invariable
as u increases, thereby proportional to J, coil current. Then, coenergy proportional to u, hence force is upwards.
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Ψ(u, B) µ H ∧ Hu
1 2ν B ∧ Bu1 2
Φ(u, H) Force = – ∂ Ψ ≡ ∂ Φu u
Since ν u* = u* ν, boils down to differentiate u*u t
i.e., virtual power = lim t → 0 [ν – ν] B ∧ B12t u(t)
General computation, simple case when reluctivity uniform in physical space(all nonmagnetic materials). Then ν independent of u.
General computation, simple case when reluctivity uniform in physical space(all nonmagnetic materials). Then ν independent of u.
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. . . which is what the
Lie derivativeis about.
Coming: definitions of inner product and Lie derivativeComing: definitions of inner product and Lie derivative
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ext(c, v, t)
Extrusion (by the flow of a vector field v):
∫ i b = lim ∫ bvc1tt → 0 ext(c, v, t)
of a point:
c
v
of a p-manifold:
x
d u (x) = v(u (x))t
ext(x, v, t)
Inner product:
u (x)t
t tu (x) = x0
Yields 1-form ivb from 2-form bYields 1-form ivb from 2-form b
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Lie derivative of a differential form
b : S → bS
orientedsurface embracedflux
S
u (S)
ext(S, v, t)
tu*b : S → ∫ b
t u (S)t
L b = lim [ b – b]u (S)tSvS
L b = lim [u*b – b]t1tv
1t ≡ lim [ db – b]1t ext(S, v, t) ext(∂S, v, t)
L = i d + d
iv v vhence Cartan's "magic formula":
← definition← definition
Expression in terms of i and d, using StokesExpression in terms of i and d, using Stokes
← definition← definition
Si * * d d * L
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Since ν u* = u* ν and d u* = L ,t vu
t → 0 ν – ν] = L ν – νL1
t u(t)lim v v
so, when Ψ(u, b) = ∫ ν b ∧ b,u12
= ∫ L b ∧ νb – ∫ v vL h ∧ b = 2 ∫ L b ∧ h,v
virtual power = ∫
(νL – L ν)b ∧ b2
×v v
= 2 ∫ di b ∧ h = 2 ∫ i b ∧ dh ≡ 2 ∫ B × v · Jv v
= 2 ∫ J × B · v
Algebraic manipulations, based on
easy-to-prove integration by parts
formulas, yield expected result.
Algebraic manipulations, based on
easy-to-prove integration by parts
formulas, yield expected result.
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So one falls back on the familiar formula, by using dictionary of
correspondences. One should do that only after completion of the
differential-form calculus. Insistence on using vector notation in
dealing with Lie derivative may result in hopelessly awkward
computations. A sample (pU denotes p-form with proxy vector U):
So one falls back on the familiar formula, by using dictionary of
correspondences. One should do that only after completion of the
differential-form calculus. Insistence on using vector notation in
dealing with Lie derivative may result in hopelessly awkward
computations. A sample (pU denotes p-form with proxy vector U):
i f h bj fi ld
Th f d d h b f ld
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L B = [v div B + rot(B × v)]v2 2
L E = [– v × rot E + grad(v · E)]v1 1
Exists for other objects, e.g., vector fields.
But proxy of L ω is not L of ω's proxy:v v
L = i d + d iv v v
because d B = (div B), d E = (rot E),
i B = (B × v), i E = (v · E), i q = (q v)
2 2
2 1 0
13
1 3v v v
The notion of Lie derivative extends to other objects, e.g., vector fields
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Having thus verified the validity of the method, and gained familiarity
with manipulation of Lv, we turn to the permanent magnet problem,
to realize that considering the 1-form Hc or the 2-form Br as
invariable are two different assumptions, leading therefore todifferent force formulas.
Next slide: How approximations of “permanent” magnet, according
to either of these assumptions, can be realized. Imagine deformableputty peppered with either (1) small, rigid, hard magnets, or (2) small
coils, bearing constant intensity. Equivalent homogeneous material
behaves as described:
Having thus verified the validity of the method, and gained familiarity
with manipulation of Lv, we turn to the permanent magnet problem,
to realize that considering the 1-form Hc or the 2-form Br as
invariable are two different assumptions, leading therefore to
different force formulas.
Next slide: How approximations of “permanent” magnet, according
to either of these assumptions, can be realized. Imagine deformableputty peppered with either (1) small, rigid, hard magnets, or (2) small
coils, bearing constant intensity. Equivalent homogeneous material
behaves as described:
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Hard ("permanent") magnets
2-form b invariabler
b
hb
– hc
r
Two different ways to make one
small magnets small coils
1-form h invariablec(its flux through any materialsurface stays the same, whatever u)
(its m.m.f. across any material closed curvestays the same, whatever u)
Small magnets Small coils
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b
hb
– hc
rb = b + µ hr b = µ (h + h )c
(µν = 1)
Ψ(u, b) = / ∫ ν b ∧ b – ∫ ν b ∧ b
u1
2ru
u u
Ψ(u, b) = / ∫ ν b ∧ b
– ∫ b ∧ hu
12
cu
Φ(u, h) = / ∫ µ h ∧ h
+ ∫ b ∧ h + / ∫ ν b ∧ bu
12
r u1 2r r
Φ(u, h) = / ∫ µ (h + h) ∧ (h + h)u
1
2
c c
Derivatives ∂ Φ ≡ –∂ Ψ differ on left and rightu u
Non-equivalent ways to write down the
B–H law, because Lagrangian Hodgedepends on u.
Non-equivalent ways to write down the
B–H law, because Lagrangian Hodgedepends on u. Corresponding energy and coenergy,easy to write down, differ accordingly
Corresponding energy and coenergy,easy to write down, differ accordingly
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b
hb
– hc
rb = b + µ hr b = µ (h + h )c
(µν = 1)
u u
The bottom line:
F = (J + J ) × BcF = J × B – (H + H ) div B c r
– (J + J ) × Bc r
… which results in different force fields.… which results in different force fields.(Computation left as an exercise…)
(Computation left as an exercise…)
Jc defined as rot HcJc defined as rot Hc
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Now, which of the two is correct? Wrong question: What precedes only
shows that both “hc constant” and “br constant” (as 1- and 2-form,
respectively) are acceptable models for a permanent magnet. But the
latter’s real behavior (called “local law” in next slide) is a matter for
measurement, not speculation. In such measurements, one compares a
template constitutive law (for instance, some weighted mixture of the abovetwo) with the results of macroscopic readings (whose observed relations
form the “global law” of next slide), and one adjusts parameters till a good
match is achieved..
Now, which of the two is correct? Wrong question: What precedes only
shows that both “hc constant” and “br constant” (as 1- and 2-form,
respectively) are acceptable models for a permanent magnet. But the
latter’s real behavior (called “local law” in next slide) is a matter for
measurement, not speculation. In such measurements, one compares a
template constitutive law (for instance, some weighted mixture of the above
two) with the results of macroscopic readings (whose observed relations
form the “global law” of next slide), and one adjusts parameters till a good
match is achieved..
Constitutive laws ought to be
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gmeasured, not theorized about
I
F
L
Φ
macroscopic levelmicroscopic level
e.g., condensedmatter physics, etc.
B
H
1
2σ3
global lawslocal lawsquantum, etc., laws
B, H, ε, σ Φ, I, L, F ψ, etc.
mesoscopic level
measurementnum. simulationtheory
some lower levelof description,
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Such a process may require extensive numerical computation, and
so requires a good theory of forces (note that samples do deform, as
a rule, when measurements are taken, which makes what precedes
relevant) and a computational technique which go along well with this
theory. For identification of constitutive laws, static computations
(magnetostatics + elasticity) will suffice, as a rule.
But for applications exemplified by TEAM pbs. 12 & 16, one needs to
take eddy currents into account. So let us review the “generalized
finite differences” technique with that in mind:
Such a process may require extensive numerical computation, and
so requires a good theory of forces (note that samples do deform, as
a rule, when measurements are taken, which makes what precedes
relevant) and a computational technique which go along well with this
theory. For identification of constitutive laws, static computations
(magnetostatics + elasticity) will suffice, as a rule.
But for applications exemplified by TEAM pbs. 12 & 16, one needs to
take eddy currents into account. So let us review the “generalized
finite differences” technique with that in mind:
→ → →G R D
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N →
E →
F →
Vgrad rot div
here, R = – 1fe
e, a
at edges
h at dual edges(i.e., faces)
d, j at dual faces
h = h : f ∈ F f b = b : f ∈ F f
b at faces
e = e : e ∈ E e = j : e ∈ E e
fluxes
emf's
mmf's
currents As we saw, this discretization principle provides a toolkit, from which a discrete eddy-current model can be assembled. Neglecting
displacement currents, and taking as main unknown the time-integrals of edge electromotive forces (so-called “A* formulation”), one gets:
As we saw, this discretization principle provides a toolkit, from which a discrete eddy-current model can be assembled. Neglecting
displacement currents, and taking as main unknown the time-integrals of edge electromotive forces (so-called “A* formulation”), one gets:
ss
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σσσσ ∂ a + R ννννRa = j
s
t
t
νννν , σσσσ : square symmetric matriceswhich depend on placement u
= j – σσσσ ∂ a
h = νννν b
t
s
RRt
Two main ways to get them:Galerkin, with edge or face elements
∂ (µµµµ(h + h )) + R σσσσ Rh = jst
s –1t
FIT, or cell-method, with mutually orthogonal meshes
Bold smallcase for arrays of degrees of freedomb, h, etc., now attached to the comoving mesh
Bold smallcase for arrays of degrees of freedom
b, h, etc., now attached to the comoving mesh
( ( )) ( ( ))) W ( ) W ( ) df'1 1ff'
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ν = ν(u (x)) ; ε(u (x))) W (x) · W (x) dxu uf–1 –1
uff
intrinsic reluctivityof the material
material point
h = ν (ε)bu
Integration here is performed on
physical space. Since elements are
comoving, face elements depend
on u (the Jacobian of which is
therefore involved in the element-assembly process).
Integration here is performed on
physical space. Since elements are
comoving, face elements depend
on u (the Jacobian of which is
therefore involved in the element-assembly process).
Here, ν depends on the nature of
the material point that occupies
position x, but not on its state of strain.
Here, ν depends on the nature of
the material point that occupies
position x, but not on its state of strain.
Yet, the Lagrangian Hodge operator, and hence its discrete version νννν
u, dodepend on strain, via u. This is usually called the “shape effect”.
Yet, the Lagrangian Hodge operator, and hence its discrete version ννννu
, do
depend on strain, via u. This is usually called the “shape effect”.
First way to construct ννννu: Galerkin
method with face elements.
First way to construct ννννu: Galerkin
method with face elements.
[ ]
DoF arrays indexed by facets of comoving mesh
” ”
DoF arrays indexed by facets of comoving mesh
” ”
( ( )) ( ( ))) W ( ) W ( ) df'–1 1ff'
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ν = ν(u (x)) ; ε(u (x))) W (x) · W (x) dxu uf–1 –1
uff
intrinsic reluctivityof the material
material point
h = ν (ε)bu
Now, should ν also depend on strain or stress,
because the nature of the material changes with
its state of stress (think e.g. of terfenol), that
could be handled
Now, should ν also depend on strain or stress,
because the nature of the material changes with
its state of stress (think e.g. of terfenol), that
could be handled
The Hodge map then depends on u for two distinct reasons: shape effect,and (via the dependence onε) whatshould properly be called “magnetostrictive” effects. (Beware: meaning of “magnetostriction” is author-dependent.)
The Hodge map then depends on u for two distinct reasons: shape effect,and (via the dependence on ε) what
should properly be called “magnetostrictive” effects. (Beware: meaning of “magnetostriction” is author-dependent.)
Diagonal discrete HodgeSecond way
t t t νν
Second way
to construct νννν
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Diagonal discrete Hodge for FIT and cell-method
(vectorialarea)
f ~
f~
Here, f // f ~
ν = νf length(f )
area(f )
~depend on u
to construct ννννuto construct ννννu
As material deforms,
keep dual cells
orthogonal to primal
ones. (Not a problem if
deformations are small.)
As material deforms,
keep dual cells
orthogonal to primal
ones. (Not a problem if
deformations are small.)
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What it takes at the numerical level:
u : nodal positions un
Precompute the derivatives ∂ νννν
/ ∂u
ff'
n
at the assembly stage (cf. Coulomb 84)
Galerkin: cf. Z. Ren, 1991
J.L. Coulomb, IEEE Trans., MAG-
19, 6 (1983), pp. 2514-19.
J.L. Coulomb, IEEE Trans., MAG-19, 6 (1983), pp. 2514-19.
Z. Ren, A. Bossavit: "A New Approach to Eddy-Current Problems in Deformable Conductors, and some numericalevidence about its validity", Int. J. Applied Electromagnetics in Materials, 3, 1 (1992), pp. 39-46.
Z. Ren, A. Bossavit: "A New Approach to Eddy-Current Problems in Deformable Conductors, and some numerical
evidence about its validity", Int. J. Applied Electromagnetics in Materials, 3, 1 (1992), pp. 39-46.
Ren's calculations of 1991
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σσσσ ∂ a + R νννν R a = j
f 99
Hollow sphere in transient vertical field (TEAM #6)
iron
x
y
z
zy
x
z
air
iron
20 40 60 90
angle
100
200Normal force along meridian
h-method
a-methodanalytical
∂ (µµµµ (h + h ) + R σσσσ R h = 0uu
s tt
–1
uu
t
t
s
∂ Φ ≡ –∂ Ψu uJ × BRelative error4.97 %
7.17 %
2.12 %
2.10 %
Inferior erformance of J x B due to non-conformal a rox. of B see aboveInferior performance of J x B due to non-conformal approx. of B (see above)
Current challenge: how about FIT
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Current challenge: how about FIT and the cell method?
Only ∂ν / ∂u to care about
f
n
Circumcenters inside tetrahedra. Take Voronoi
cells. Deformed meshes still orthogonal
Not all meshes allow formation of dual with
cells orthogonal to primal ones, as this one does
Not all meshes allow formation of dual with
cells orthogonal to primal ones, as this one doesIn 3D, a convenient simplicial paving exists with this property:
In 3D, a convenient simplicial paving exists with this property:
… the “Sommerville mesh” (Voronoi construction on b.c.c. lattice)… the “Sommerville mesh” (Voronoi construction on b.c.c. lattice)
An exercise in plane geometry
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An exercise in plane geometry
θ
~
In "FIT", or the cell method,
ν = ν
Move A. What's ∂ ν / ∂θ ?
ff length(f )~
area(f )
A
ff
Proof:
Answer (in 2D): ∂ ν / ∂θ =ff
Coefficients vff depend on placement, but not in so complex a way. Here,
example where parameter u reduces to the sole angle θ.
Coefficients vff depend on placement, but not in so complex a way. Here,
example where parameter u reduces to the sole angle θ.
An exercise in plane geometry
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An exercise in plane geometry
θ
~
In "FIT", or the cell method,
ν = ν
Move A. What's ∂ ν / ∂θ ?
ff length(f )~
area(f )
A
ff
Proof: Rθ length(f )
~=
R cos θ
2R sin θ
Answer (in 2D): ∂ ν / ∂θ = – .ff
2 sin θ2
ν
length(f )3D analogue not too difficult3D analogue not too difficult
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"Genuine"
magnetostriction? Bs
b, ε = arginfΨ(u, b) + W(ε(u))
0 = – f + ∂ Wu
h = ν b σ = κ εu
Prospects: A full-fledged theory of magnetoelasticity, fully
accounting for non-linearities and possible dependence of B–H
law on local stress (beyond shape effects)
Prospects: A full-fledged theory of magnetoelasticity, fully
accounting for non-linearities and possible dependence of B–H
law on local stress (beyond shape effects)
Simple basic principle: Just minimize total energy. But ...Simple basic principle: Just minimize total energy. But ...
vector valued~
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h = ν b + c ε
σ = c' b + κ ε
1-formvector-valued
1-form
2-formcovector-valued2-form~
…which differential-geometric entity to use for
ε, still a matter for research.
…which differential-geometric entity to use for
ε, still a matter for research.