Kluitenberg,
Physica
G. A.
28
2 17-232
1962
THERMODYNAMICAL ELASTICITY
THEORY
AND
OF
PLASTICITY
by G. A. KLUITENBERG Onderafdeling
der Wiskunde
van
de Technische
Hogeschool,
Eindhoven,
Nederland.
Synopsis h theory of elasticity of irreversible principle
and plasticity
processes.
and
degree
plastic
Onsager may
of freedom.
flow,
relations
exist
elasticity
be due
deformations
The entropy The
media,
hardening
of plasticity
The vanishing
In the theory
is derived.
in anisotropic
strain
the inelastic production,
phenomenological between
with
the help of the
of this principle strain tensor which
the temperature
plays
the role of an
is due to heat conduction
equations
are
given
and plastic
Phenomena
as, for instance,
in this theory.
is an approximation of the
is based on the thermodynamics is defined
heat conduction
are discussed. are included
of the rate of the plastic
to a property
which tensor
In the discussion
for the cross effect
and strain
Mises theory to
is given,
inelastic
of relaxability-in-the-small.
is also taken into account. internal
The
It is shown
to the theory
developed
tensor
the yield
strain
phcnomenological
within tensors.
and
the
flow, which thermo-
that the Von in this paper. surface
It is assumed
is seen that
the
are small.
5 1. Introduction. In this paper a theory of elasticity and plasticity is developed using the general theory of thermodynamics of irreversible processes in continuous medial) 2). In 5 2 - $5 the law of conservation of mass and the balance equations for momentum, total energy, kinetic energy and
internal energy are discussed. In 0 6 the tensor of total strain (which consists of two parts: the tensors of elastic and inelastic strain) is introduced. In the following section the inelastic strain tensor is defined with the help of the principle
of relaxability-in-the-small
and it is introduced
as an internal
degree of freedom in the Gibbs relation. In 9 8 and $ 9, according to the usual procedure of the thermodynamics of irreversible processes, the entropy balance, the phenomenological equations and the Onsager relations are given. In the last three sections plasticity is discussed and it is shown that theVonMises theory is an approximation to the theorydevelopedin this paper. We consider a medium consisting $ 2. The law of conservation of mass. of one chemical component and we shall assume that mass is conserved (i.e., such phenomena as nuclear reactions are excluded). Hence, one has aP -=
-
at -
217
div pv,
-
(2-l)
218
G. A. KLUITENBERG
where p is the density of mass, v is the velocity time. We now define the substantial
derivative
of the medium and t is the
with respect
to time by
where vy is the y-component of v and xy is the y-component vector x(y = 1, 2, 3). (A rectangular axis - frame is used.) From the two preceding equations it follows that dP -=
-p
dt
of the position
div v,
and dv pdt = divv, where 21= p-l
(2.5)
is called the specific volume (volume per unit of mass). Finally, if 4 is an arbitrary quantity (for instance a component of a tensor), one has
dq a(Pq) Pdt= ~ at +
(2.6)
Wpqv),
which follows from (2.2) and (2.3). 5 3. The equations of motion (balance equation for momentum). form for the equations of motion reads
’
dv, __ dt
ah
--I&L
__ax
u
The usual
(3.1)
+ pFa,
where F is the force per unit of mass and Pall is the mechanical pressure tensor. Since pv is the density of momentum one may call v the specific momentum (i.e., the momentum per unit of mass). Hence, Plvs may be considered as the tensor of the density of the conductive flow of momentum and pF as the source of momentum (per unit of volume and per unit of time). Using (2.6) one has dv,
Px==
a(pva)
at
+
a(Pv,vs)
Is:,“=, ax--’
(3.2)
u
and hence, one can write for (3.1) (pvavs
+ PM) +
pF,.
(3.3)
THERMODYNAMICAL
From this equation convective
THEORY
OF ELASTICITY
AND
PLASTICITY
it is clear that PV~ZJBis the tensor of the density
flow of momentum,
219 of the
while pvUa2/b + Pa,g is the tensor of the density
of the total flow of momentum. It will be assumed that Pa&9= PO&. This assumption
is equivalent
internal
momenta.
angular
(3.4)
to the assumption
that the medium
has no
5 4. The balance equation for the total energy. It will be assumed that the only source of energy is the newtonian work done by the external forces. (This means that for instance polarization and magnetization phenomena are not taken into consideration.) Hence, one has de pdt=
-divJ(@+pv*F,
(4-l)
where e is the specific total energy (i.e., the sum of the kinetic and internal energies) and J(e) is the density of the conductive flow of the total energy. 3 5. The balance equations for the kinetic and internal energies. On multiplying (3.1) by ua and summing over 6, one obtains
where (3.4) has been used. Since the quantity iv2 is the specific energy, (5.1) is a balance equation for the kinetic energy. On substracting
kinetic
(5.1) from (4.1) one obtains
c,“,,=, pas
pg=-divJtq)-+ where u is the specific internal
energy given by u = e -
and J(q) is the density
(54
9vz 2
of the conductive
flow of the internal
bY J$q’ = $’
-
cl=,
&Pa&
(5.3) energy given
(5.4)
J(q) is usually called the heat flow. The equation (5.2) is a balance equation for the internal energy and is usually called the first law of thermodynamics. From (5.1) and (5.2) it is seen that
220
G. A. KLUITENBEKG
is the amount of energy which transforms of time from kinetic to internal energy.
per unit of volume and per unit
9 6. The tensor of total stmin. Consider an arbitrary point P of the medium. Let the position of this point at the time t = to be given by the vector E,. At an arbitrary time t the point P will have the position x = X(E> t),
(6.1)
where ~(5, t) is a single valued function of g and t such, that x(E,, to) = g. On the other hand, if at the time t the point P has the position x then E,, the position of P at the time to, is uniquely determined by x and t and hence, also 5 = E(XJ t) (6.2) is a single valued function. The displacement vector of P with respect to the position of P at the time to is defined by u = x - 5 = u(C, t) = u(x, t), (6.3) and the velocity
of P at the time t is
v=
tug,
(6.4)
t).
The state of deformation of the medium in the surrounding of P at the time t with respect to the state of the medium in the surrounding of P at the time to is given by the tensor of total strain defined by
(6.5) It will be assumed in this paper that the deformations From the preceding $
equation
are small.
and (6.4) it follows that
I a W(S* t) = g 1% Q5,
t) + $
h
v/3(&t) . 1
(6.6)
From (6.3) one obtains 4
%%(F,t) = $
where day is the Kronecker
tensor.
%x(5‘ t) + Bay,
(6.7)
Using this equation
one gets from (6.6)
Y
THERMODYNAMICAL
If one assumes that
THEORY
OF ELASTICITY
the deformations
are small,
AND
PLASTICITY
the preceding
221 equation
becomes
Using (6.3), (6.4) mentioned above)
and
(2.2)
one has
(even
without
the
approximation
(6.10) From the two preceding
equations
one gets (6.11)
It should be remarked that in the following sections all quantities will be considered as functions of x and t (which has also been done in the preceding sections). From (6.5) one has (6.12) Eai3= Qor. In the following the state of the medium at the time to will be called the reference state. An assumption about this state will be made in the following section. If one defines the quantities &o and E by e = + c;=,
(6.13)
+Jy,
and SC@= El%/3 - Q&X, c;=,
eyy,
(6.14)
one has (6.15)
“CQ= gal3 + &s, and = 0.
(6.16)
zag = E&ga.
(6.17)
c,“=, I,, From
(6.12) and (6.14) it follows that
Using (2.4), (2.5),
(6.1 1) and (6.13) one obtains dv d& v-1 _ = 3 -. dt dt
Hence, v is a function
(6.18)
of E.
5 7. The Gibbs relation and the principle of relaxability-in-the-small. If one considers pure elastic processes in a solid, the Gibbs relation has the form T ds = du + v Z&i where T is the temperature
Pars dea,r,
and s is the specific entropy.
222
G. A. KLUITENBERG
If, however, the medium has internal degrees of freedom, terms must be added to the right hand side of the preceding equation. For instance, in a fluid
consisting
of one
chemical
component,
T ds = du + P dv, where P is the hydrostatic fluid consists
of several chemical
components,
the
Gibbs
pressure. one has
relation If, however,
reads the
T ds = du + P dv - & purdck, where ck is the concentration of the chemical component K. Meixnera) has added terms of this kind to the Gibbs relation for an elastic solid in order to discuss relaxation phenomena. We shall now assume that there exsists an internal degree of freedom characterized by a tensor .scrS. (O (The physical interpretation of this tensor will be discussed in the following.) Still other degrees of freedom may be present, but, as will be seen, for the explanation of plasticity phenomena it is sufficient to assume that there exists only a degree of freedom characterized by a tensor. For the Gibbs relation one then gets
T ds = du t_ v xc,“,+, Pfig dccrg -j- Z’&, Hence,
7:; d&r;.
one has ;
S(E~O, E$, u) = T-1,
a
a q-
(7.3)
s(eor5, E$, u) =
VT-~
7:;.
It follows from (7.1) that ds du T,,=dt+vC:,B=iP”~
dt
In order to give the physical meaning of .&$ we use the principle of relaxability-in-the-small introduced by EC kar t 4). We consider a small bit of matter (surrounding some point P of the medium), which is large from the microscopic point of view (Le., it contains still a great many molecules (or atoms)) and small from the macroscopic point of view (i.e., the variations within the bit of such quantities as the temperature and the strain tensor may be neglected). It will be assumed that the reference state mentioned in $ 6 has a uniform temperature To,Moreover, it will be assumed that if such a small bit is cut out of the medium while the medium is in the reference state, no changes will occur in the bit. If, when the medium is in an arbitrary state, a small bit is cut out, all strains will be relaxed, since on the surface
THERMODYNAMICAL
THEORY
OF ELASTICITY
AND
of the bit no forces work. In the relaxed state, however, deformation
left with respect to the reference
223
PLASTICITY
there may be some
state. For E$ we now take the
tensor describing the strain (with respect to the reference state) of the dissected bit after one has brought the bit to the temperature To*). One may call 8:; the inelastic strain tensor. From this definition and from (6.12) one gets and one may also assume that The elastic part tensor defined by
(i) EC@= &PA,
(7.6)
7:; = $2.
(7.7)
of the deformation
is described
&$ = E&OFrom
by the elastic
strain
Et;.
(7.8)
(6.12) and (7.6) one obtains (7.9)
e:eil = @)W state P a~ = 0 and hence, one has
In the relaxed
P”b(&&eS), E$, T) = 0 for ES = 0 and T = To,
(7.10)
on account of the definitions of E$’ and E$ given above. If one linearizes the function Pao(&$, E$, T) in E$ and T, one obtains with the help of (7.10) Pap = C;,,= i G,WC es) + aas(T -
(7.11)
To),
where the tensors a,g,,c and aao may still depend on E$. It should be remarked that E&B satisfies the compatibility equationss) on account of the definition (6.5). In general, however, neither E$ nor F$ will satisfy these equations. $ 8. The balance equation for the entrofiy. Using (7.5), (2.5), (5.2) and (6.11) one finds p
$ =-
div(T-1 J(4)) + T-1
T-1 J(P). grad T +
-
~~,s=1$
?!$!_. (8.1)
>
Hence, ds Px=
-
div J(8) + a(s),
(8.2)
where J(s) =
T-lJ(@,
(8.3)
and &9 *) Eckart account
=
T-1
-
4), in his discussion
the temperature.
a unique definition
of &$.
T + C&=1
T-VW*grad of the principle
The temperature,
r$j$
of relaxability-in-the-small,
however,
may not be neglected
.
(8.4)
does not take into if one wants to obtain
224
G. A. KLUITENBERG
From
these
equations
it follows
J(S) is the
that
density
of the
conductive
flow of entropy and G(S) is the entropy production per unit of volume and per unit of time. It is seen that the entropy production is due to the irreversible Since
phenomena the entropy
of heat conduction production must J(a) .grad
and inelastic deformation. be positive definite, it follows
that
T (
(8.5)
0,
and
(8.6) Using
(2.6) the equation
(8.2) may
w =__
div
also be written
in the form
(J(S) + ~SV) + CT(')
(8.7)
8t
Hence, psv is the density of the convective is the density of the total flow of entropy. We now give the following definitions ,(i) = 13 x3= -(i) Tab
_ -
(i) Tafl
1’
1
-
4
E(i) = Q c;=, -(i) = E$ &xP From
these
definitions
(0
&)
Further,
T-1
$)
PSV
(8.8)
i’/’
&x&s c;=,
(8.9)
+f;>
(8.10)
&$j, 4 &x/3c,“=, E!$.
(8.11)
= “$
+ T(i) SLY&
(8.12)
(i) = EC; + &W &.@, &3P
(8.13)
c,“=, ?!i) /y = 0 ’
(8.14)
x.3= : r E?31,)= 0 *
(8.15)
the four preceding zc
and J@) +
one finds rafl
Using
flow of entropy
-T-lJ(q)
one has from
equations
one can write
.grad
~~,8=1
(7.6),
T +
for a@) defined
+tjz
(7.7), (8.9) and
+ 3?-(i)$9.
by (8.4) (8.16)
(8.11)
-(i) = +“’ fin’ TUB
(8.17)
&i’ _ aB
(8.18)
and $0 8%’
THERMODYNAMICAL
THEORY
OF ELASTICITY
AND
PLASTICITY
225
We also have (8.19) and 7(6) de(*) __ 20, dt since the entropy
production
(8.20)
must be positive
definite.
9 9. The phenomenological equations and the Onsager relations. On account of the expression (8.4) for the entropy production, we have for the phenomenological equations in an anisotropic medium
(9.2) where
L$)“,“Q’, LDpB’,‘i), ,Tti$‘d
The Onsager
relations
and
L$,$) ,
are phenomenological
tensors.
read L$‘B)(Q)= LIp,“P’,
(9.3)
L$;i’
= pd,
(9.4)
L$$’
= Ly;’
(9.5)
On account of the symmetry of E$ and v$$ one may choose LDpsl’“‘,L$‘JQ) and L$$’ such that the following relations are satisfied6) 7) LC90 = LC$’
(9.6)
L(i)(q) = LpW”“‘: @Y L’W = LCg’ = L$g ‘%SYC Hence, we have from the five preceding LST’
= Ly;‘.
(9.7) (9.8)
equations
= LCQ0 == Lgj$) = L;WC?),
(9.9)
and L$$’
= LC#
= LC$’
= L?Ci&’= L;W;J = L$X$’ = L:iy’j, = LCi&‘. (9.10)
Due to symmetry in the crystal lattice the number of independent components of the phenomenological tensors may further be reduceda). In an isotropic substance one has the requirement that the phenomenological tensors must be invariant with respect to all rotations and to inversion of
226
G. A. KLUITENBERG
the axis-frame.
It can be shown that in this case one obtains
(9.2)
for (9.1) and (9.1 1)
J(Q) = -A grad T,
(9.12) d&(i) = #Z),(i). dt
(9.13)
Hence, in general, there may exist cross effects in anisotropic media between heat conduction and plastic flow (the second term on the right hand side of (9.1) and the first term on the right hand side of (9.2)). In an isotropic substance, however, such cross effects do not exist. From the positive definite character of the entropy production inequalities may be derived for the components of the phenomenological tensors. As an example we consider an isotropic substance. With the help of (9.1 I), (9.12) and (9.13) one obtains for (8.16) o(s) = T-i{LT-i(grad
T)s + ~(1) C&=,
(?$)2
+ 317@)(7(i))s}.
(9.14)
Hence,
If one considers $ 10. Discussion of plasticity. and u one obtains with the help of (7.8) ds = $
du + &+,
~
s as a function
as
as
a&)
(9.15)
Tj@) > - 0.
$1) 2 0,
120,
d&ao +
C:,,+
In the following s will always be considered Hence, one has from (7.1) and (10.1)
1 $J-as a function
a&$)
of F$, E$!
d+.
(10.1)
of e$‘, ~2, and U.
(10.2)
(10.3) 1
aS
T
at4
-=_
where also (2.5) has been used. With the help of (10.3) one gets for (9.2)
’
(10.4)
THERMODYNAMICAL
THEORY
and for (9.12) and (9.13) one obtains
OF ELASTICITY
AND
PLASTICITY
with the help of (10.3),
227
(8.8) and (8.9)
and d&(i) -=
5 P)
dt
PT
(10.7)
C;=,
In general the components of the phenomenological tensors still depend on E$, E$’ and u (or, for instance, on Paa, E$ and T). It is known from experiments that if a medium is in a state with a certain inelastic deformation no changes in E$! will occur if Pa0 is small enough. This means that there ,exists a function @ = @(P,o,
Et;,
T),
(10.8)
such that for @ < 0 the right hand sides of (10.5), (10.6) and (10.7) vanish. We shall now assume that this is due to the fact that L$fZ), L$$, ~(1) and q@) vanish for @ < 0 and get finite values if @ increases. The other possibility would be that 7:; and L$p) vanish, but it will be shown in 4 12 that this is less probable. It should be remarked that one can write for (9.1)
JF’ = -
T-1 I;&
L$)(‘J)
-& + c;,y=l
L$F’
pT
P
?-
aEg
_
PBV , >
(10.9)
where (10.3) has been used. In the case of isotropy this equation reduces to (9.11). Thermodynamical equilibrium is characterized by the vanishing of the entropy production. This is the case if the heat conduction and the plastic flow vanish. Hence, one must have grad T = 0 and CD< 0. It should be stressed, however, that it is not necessary that Pan, E$,’ or E$ vanish. This means that there is no relaxability-in-the-large. If there is mechanical
however,
6P,b is such that @(P,B
+ ~P,B, E$, T) > 0.
228
G.
A. KLUITENBERG
This effect (often called strain hardening)
can be explained
in the following
way. If one changes the pressure the irreversible process described by (9.2) (or by (9.12) and (9.13)) will start when the yield surface (the surface in P,D-space
for which @ = 0) is reached.
If the pressure
final value P&/3+ dP,o, it may occur that the inelastic
is brought deformation
to its tensor
reaches a value E$ + &$j such that @(P@
+ 6P,p, 8)=P+ BE$, T) < 0,
and, hence, the medium is again in a state of thermodynamical 9 11. Some approximations. In this section we mations of which the meaning will become clear I. The assumption 0 = 0. It is known that if plastic deformations occur in a medium, has a vanishing trace i.e.,
equilibrium.
shall discuss two approxiin the following. from experimental data, the inelastic strain tensor
&W = 0. From
(8.10),
(9.2) and the preceding c;=,
(11.1)
equation
it follows that
LZii”;’ = 0,
(11.2)
and c”= a
1
L(M) ‘Iw
and hence, using the Onsager relations
= 0
(11.3)
,
(9.4) and (9.5), one also has
c;=,
L$$
= 0,
(11.4)
c;=,
L$;i’
= 0.
(11.5)
and
With
the help of (8.12)
and the two preceding
equations
one then gets
for (9.1) and (9.2) (11.6)
For the case of isotropy
it follows from (I 1.1) and (9.13) that q(2) = 0.
II.
An assumption
about
the
entropy.
(1 1.8) If one assumes that (1 1.9)
THERMODYNAMICAL
one obtains
THEORY
for the equations
OF ELASTICITY
(10.5),
Jkp) = _ T-l'&
(10.9),
L$)(q)$
AND
PLASTICITY
229
(10.6) and (10.7)
_
c;,,=,
fl
L$!!i’ Pp,,
(11.11)
(11.12) and d&
= -
dt
$2) P,
(11.13)
where P’ns = P&L3-
(11.14)
4 Bap Lx,“=, P,,,
and P = g g_-,
(11.15)
P,,.
The equations (11.12) and (11.13) only hold in the case of isotropy. We remark that one has from (11.14) and (11.15) (11.16)
Pn$ = R%S + P Baa, c:=, and, finally,
P’,,
(11.17)
= 0,
one has (11.18)
Rx, = &,, from (3.4) and (11.14). III.
The
combination
of
the
(10.3), (11.9) and (11.14) one obtains
For the case of isotropy $2) zzz 0.
two
assumptions.
again the equation
We now define the quantities
Using
(8.9),
for (1 1.6) and (11.7)
(11.12)
holds and in (11.13)
&) and E$ by
&) = + z;=,
(11.21)
E$
and z$j = &$? -
g &-Qc;=,
&g!
(11.22)
230
G. A. KLUITENBERG
Hence, E% = E$) + &@)f&g,
(11.23)
c:= 1 SE Z=Z0.
(1 1.24)
and
Using (7.9) and (11.22)
one has g(e) = $a) a@
From
(11.25)
(7.8) it follows with the help of (6.13),
(8.10) and (1 1.21) that
E = &W + c(i) and using (6.14),
(8.1 1) and (11.22)
(1 1.26)
one finds from (7.8)
- = $e.$+ $j &aB
.
(1 1.27)
From (10.4) and (1 1.9) it follows that (11.28) and from (10.2),
(2.5) and (1 1.9) one obtains
+J(+p,, >= r_
(1 1.29)
0.
On account
of the two preceding Pn,c = v-lf$QJ),
equations
one has
u) = z+f$‘(&$),
T).
Since II = ‘U(E) (cf. the end of 4 6) one gets from (11 .I) and (1 1.26) u-1 = = f(3)(&)). Hence, Pas = fap (‘) (Q(e), T ), and if one linearizes this function one obtains Pas = z;,c= 1 %3yt $2 + Ga(T
-
To),
on account of (7.10). The tensors a,gyt and aao are constant. remark at the end of 4 7.) In the case of isotropy one gets Pa0 = asg + {b&) + c(T -
To)) da&
(11.30) (Cf. also the
(11.31)
where the scalars a, b and c are constants. The equation (11.31) is the Duhamel-Neumann law9) for thermoelasticity. If one assumes that c = 0 (or if T = To) (11.31) reduces to the law of Hooke for isotropic media. It should be noted that the theory developed in this paper is based on the thermodynamics of irreversible processes. In order to give a theory for plasticity, Ziegler lo), however, attempts to extend the thermodynamics by introducing non-linear relations among fluxes and affinities.
THERMODYNAMICAL
THEORY
OF ELASTICITY
AND
9 12. The Von Mises theory for the case of isotropy. theoryri) 1s) 13) 14) it is assumed that @ = $ z;,,=, where K is the yield stress in shearli) theory that
(&5)2
-
231
PLASTICITY
In the Von Mises (12.1)
k2,
14). Moreover,
it is assumed
in this
(12.2) where Y_P vanishes for @ < 012) 14). The latter equation is the so called Von Mises flow law. Using (12.1) and (11.14) one can also write for (12.2) de:; -_=dt
(12.3)
Yj(l) P&p,
a formula which has been proposed by Levy in 187015). In those cases in which the assumptions (11 .l) and (11.9) are correct, the theory developed in this paper also gives the flow law (12.3) (cf. (8.13), (1 1.12), (11.13) and (1 1.8)). In 5 10 we made an assumption about the phenomenological tensors in order to explain the plastic behaviour of a solid. It was remarked in that section that another possibility would be to assume that $i vanishes for @ < 0. In the latter case one would have on account of (10.3)
as = PT-S a&$ a&$)
Pa0 = pT -
for
@ < 0:
It seems, however, less probable that as/&$ = as/&&es).Moreover, to obtain the Von Mises theory (which gives a good description of plasticity), it was necessary to make the assumption (11.9). Hence, one would have P,b = 0 for @ < 0, which is absurd. Therefore, the fact that changes in the plastic deformation only occur if @ > 0 must be due to the vanishing of the phenomenological tensors for @ < 0. In a following paper Maxwell and Kelvin bodies will be considered. Received
10-7-61
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