Also the thickness, the loads and stresses are axisymmetric during forming... Chapter X: Sheet Forming Membrane Theory 3Examples Examples: q z C r0 0, sin R φ , sin r φ Surface BC: Surfa
Trang 1Chapter X: Sheet Forming (Membrane Theory) 1
Content of Membrane Analysis
• Basic Assumptions
• Static Equilibrium Equations
• Strain State
• Application 1: Hole Expansion
• Application 2: Drawing
• Application 3: Flaring
P
C
z
Surface Normal
r
f f
Basic Assumption 1
The sheet metal part is a surface of revolution, so that it is symmetric about a
central axis Also the thickness, the loads and stresses are axisymmetric during
forming
q
P
C
z
Principal radii of curvature:
,
r rθ φ
meridian
curve C
center of curvatures
sin
hoop plane
Trang 2Chapter X: Sheet Forming (Membrane Theory) 3
Examples Examples:
q
z
C
r0
0,
sin
R
φ
, sin
r
φ
Surface BC:
Surface AB:
q
z
dq
sf
sq
Basic Assumption 2
For thin plastically deforming shells, the bending moments are negligible and
because of axial symmetry the hoop (σθ) and tangential (σφ) stresses are
principal stresses The stress normal to the surface can be neglected, so that
the resulting stress state is the one of plane stress
1
2
3 0
θ
φ
σ
=
=
=
Normal pressure is assumed small enough
as compared to the flow stress of the material
Trang 3Chapter X: Sheet Forming (Membrane Theory) 5
P
Normal
f
dr
P’
90o
f
P
Normal
f
df
rfdf f
dr
Surface Normal
P’
A Useful Relation
A useful geometric
relationship: cos
dr
r dφ φ
φ =
PP ′ = r dφ φ
cos
dr PP
φ
′ =
Basic Assumption 3
Friction forces are neglected Only uniform pressure loads normal to the
surface (although small enough wrt the flow stress) and uniform edge tensions
tangential to the surface are allowed:
Pressure Load Edge Tension Load
( sf)0
z
Trang 4Chapter X: Sheet Forming (Membrane Theory) 7
Basic Assumptions 4 & 5
Assumption 4: (Not used to derive equilibrium equations)
Work hardening is compensated by thinning of the sheet, so that the product of
flow stress times current thickness is constant: σf ⋅ = t Tf= constant
Assumption 5:
The Tresca flow condition is assumed to be applicable:
sf
sq
sf0
wo
rk-hard
Tf= sft
Tf = sf0 0t = sft
Tq= sqt
Tf= sft
Tf = sf0 0t = sft
Tq= sqt
I
VI V
IV
III
II
The Flow Criterion
Region Stress State Flow Condition
f f f f f f
T T T T T
T T T T
T T T T
T T T T T
φ θ φ θ
φ θ θ
θ φ φ
θ φ θ φ
> > − =
> > = −
> > = −
> > − =
: Force per meridian-width in hoop direction : Force per hoop-width in meridian direction
T T
θ φ
The entity T is also called
a force-resultant
max min
f
Recall:
Trang 5Chapter X: Sheet Forming (Membrane Theory) 9
Static Equilibrium Equations (1)
A typical infinitesimal
membrane element
as a free-body
dq
r
T rq fdf
( +d )( +d ) Tf Tf r r dq
T rq fdf
T rf dq
z
p
r
dq hoop-plane T rq fdf
T rq fdf dq/2
meridian plane
dq/2
Static Equilibrium Equations (2)
( T r dθ φ ) d 2 θ ( T r dθ φ ) d 2 θ
T r d dθ φ φ θ
=
Normal resultant of hoop-forces:
Radial resultant in hoop-plane of hoop-forces
(in normal direction)
meridian-plane
T rq fd d f q df
surface normal
z
f
T rq fd d sin f q f
rf
Trang 6Chapter X: Sheet Forming (Membrane Theory) 11
Static Equilibrium Equations (3)
Tφ dTφ r dr d φ T r dθ φ
Normal resultant of meridian-forces:
T rd dθ φ θ
=
T rdφ φ dT rdφ φ
2
d
T drdφ φ θ +
2
d
dT drdφ φ θ
+
2
d
T rdφ φ θ
Static Equilibrium Equations (4)
Equilibrium in normal direction:
p ⋅ rφ ⋅ d φ ⋅ r d ⋅ θ − Tθ ⋅ rφ ⋅ d φ ⋅ d θ ⋅ φ − Tφ ⋅ r d ⋅ θ ⋅ d φ =
Cancelling out the term dφ dθ and pulling pout yields:
sin
T T
p
φ θ φ
φ
T T p
φ θ
θ φ
Or, using the geometric relation given
in Slide 02.002:
Trang 7Chapter X: Sheet Forming (Membrane Theory) 13
Static Equilibrium Equations (5)
Equilibrium of forces in the tangential plane to the shell surface yields:
( Tφ + dTφ) ( r + dr d ) θ − Tφ⋅ ⋅ r d θ − Tθ ⋅ ( rφ ⋅ d φ ) ⋅ d θ ⋅ cos φ = 0
T r dφ⋅ ⋅ θ dT r d T dr d dT dr d
T r d
φ
θ
+ ⋅ ⋅ + ⋅ ⋅ + ⋅ ⋅
− ⋅ ⋅ − Tθ⋅ ( r dφ⋅ φ ) ⋅ d θ ⋅ cos φ = 0
dTφ⋅ + r Tφ⋅ dr + dTφ⋅ dr − Tθ ⋅ r dφ ⋅ φ ⋅ φ =
Expanding:
Deleting dθ and cancelling terms:
cos
dr
r dφ φ
φ = Using from Slide 02.005
Static Equilibrium Equations (6)
0
dTφ⋅ + r Tφ⋅ dr + dTφ⋅ dr − Tθ ⋅ dr =
Yields:
0
dT
Hence:
REMARKS:
1) As seen from the last equilibrium equation the stress distribution is a
function of radius ronly and is independent of the shape (rφ) of the shell
2) The external axial force F delivers the boundary stress as:
( )0
0 0
2 sin
F T
r
Trang 8Chapter X: Sheet Forming (Membrane Theory) 15
Review of Membrane Model
The generalized stress distribution can be obtained from the Tresca flow
condition and the static equilibrium equation in the tangential direction:
0
dT
The tool pressure can be found from the static equilibrium equation in normal
direction: T T
p
φ θ
Remark: No dependency
on shape of shell!
Remark: Dependency on shape of shell!
0 0 0 0
0
0
f f f f f f
T T T T
T T T T
T T T T T
T T T T
T T T T
T T T T T
φ θ φ θ
φ θ θ
θ φ φ
θ φ θ φ
> > =
> > =
> > − =
> > = −
> > = −
> > − =
Strain State (1)
2 1
σ α σ
=
Defining the plane stress by the
three principal stress components: σ σ1; 2 and σ3 = 0
We can introduce a stress ratio α:
The hydrostatic stress is found by: 1 2 3
3
h
σ σ σ
1 1 3
h
σ = + α σ
The deviatoric stress components are: 1 1 ( ) 1
1 2 3
h
σ ′ = σ − σ = − α σ
1
3
h
σ ′ = σ − σ = α − σ
1 1 3
h
σ ′ = σ − σ = − + α σ
Trang 9Chapter X: Sheet Forming (Membrane Theory) 17
Strain State (2)
The strain increments are given as: d ε1; d ε2 and d ε3 = − ( d ε1+ d ε2)
Introducing the strain ratio β: 2
1
d d
ε β ε
= d ε3 = − ( 1 + β ) d ε1
From the flow rule:
1 2 3
1 2 3
d
λ
σ ′ = σ ′ = σ ′ =
1 2
1 2
σ ′ = σ ′
or:
d ε β d ε
⋅
=
2
α β
α
−
=
− and
2
β α
β
+
= +
by volume constancy
Strain State (3)
Hence having found Tθand Tφ, the stress-ratio α can be determined as: α = T Tθ φ
and using this stress-ratio, the strain-ratio β can be determined So, knowing
one of the strain components, the other components can be derived Also the
equivalent strain and equivalent stress (flow stress) can be determined:
( )2 ( )2 ( )2 1 2 2 3 3 1
1 2
σ =σ = σ −σ + σ −σ + σ −σ
f
σ =σ −α α+ =σ +β +β +β
Similarly, the equivalent plastic strain
increment can be determined as: 12 22 32
2 3
d ε = d ε + d ε + d ε
d ε = d ε + β + β = d ε − α α + − α
Trang 10Chapter X: Sheet Forming (Membrane Theory) 19
Application 1: Hole Expansion (1)
Note:
1) Both Tθand Tφare tensile
2) At the hole rim we have Tφ= 0
and Tθ>0, from which we can
conclude that Tθ> Τφ >0
3) Hence: Tθ = T f
4) From tangential equilibrium we find:
0
dT
0
f
dT
φ
f
φ φ
=
− − ln ( Tf − Tφ) = ln r + C
with Tφ= 0 at r = r i: Tφ = Tf − 1 ( r ri )
f
Tθ = T
Application 1: Hole Expansion (2)
Remark 1: The stress state varies from uniaxial tension at the edge of the hole
towards equal biaxial tension at the periphery for large radii
Remark 2: As the hole radius approaches zero r i 0, almost the entire shell
is in a state of uniform biaxial tension in which
f
Tθ = T ≈ Tφ
Trang 11Chapter X: Sheet Forming (Membrane Theory) 21
Application 1: Hole Expansion (3)
Remark 3: The case of r i= 0 provides an approximate solution for hydraulic bulging:
Since α= 1 we obtain β= 1 Hence:
f θ φ
2 t
ε =ε = − ε
2 θ t
ε = ε = −ε But by definition:
( 0)
ln
ε =
So: t = t e0 εt = t e0 −ε
0
n
f
Application 1: Hole Expansion (4)
Checking the assumption of constant T f:
ε
Trang 12Chapter X: Sheet Forming (Membrane Theory) 23
Application 2: Drawing (1)
Note:
1) At the outer rim we have Tφ= 0
and Tθ< 0, from which we can
conclude that Tφ> Tθ
2) Hence: Tφ– Tθ= T f
3) Tθ< 0 always 4) From tangential equilibrium we find:
0
dT
dr r
φ
+ =
f
φ
= − − Tφ = Tf ln r + C
with Tφ = 0 at r = r 0: Tφ = Tf ln ( r r0 ) Tθ = Tf ln ( r r0 ) − 1
Application 2: Drawing (2)
Remark 1: The given relations are valid if and only if Tφ> 0 > Tθ.
Remark 2: The stress resultant at the inner boundary is:
i
Tφ = T r r
( 0 )
f
Tθ = T r r − ≤ ln(r r0 )≤1 (r e0 )≤ ≤r r0
( 0 )
i
r ≥ r e
Remark 3: Note again that these results are independent of the shape of the die!
Trang 13Chapter X: Sheet Forming (Membrane Theory) 25
Application 3:
Flaring
Note the following:
1) At the bottom outer rim we have Tφ = 0 and Tθ>
0, from which we can conclude that Tθ> 0 > Tφ
2) Hence: Tθ – Tφ = T f
3) Tθ> 0 and Tφ≤0 always!
4) From tangential equilibrium we find:
0
dT
dr r
φ
− =
f
φ
= Tφ = Tf ln r + C
( 0)
ln
f
Tφ = T r r Tθ = Tf ln ( r r0) + 1
with Tφ = 0 at r = r 0: