PSI - Issue 18
Plekhov O. et al. / Procedia Structural Integrity 18 (2019) 711–718 Author name / Structural Integrity Procedia 00 (2019) 000 – 000
713
3
Furthermore, by following common practice we can write a decomposition:
.
( , ) e
( ) e
( ) e
( ) T F T Ts
E
2
2
If we suggest that the specific heat is a constant value at room temperature ( ) c T c const , then we can obtain an expression for the function ( ) F T in the form 0 0 ( ) ln ( ) F T c T T T T T . If we also suppose that in the reference configuration 0 and 0 e at 0 T T , we can write:
2
(3)
,
( ) ln e S s p c T T E .
( ) ( / 2 ( e
) ) e
( F c T T T T T E p Ts p E ) ln ( )
T T
1
0
0
0
1
1
0
The energy balance equation has the following form:
(4)
q r ,
e
x
where x q - heat flux. Substitution of (3) into (4):
1 x x cT TE W E p q r W E p p q r , 1 ( ) '( ) e p p
(5)
where p W p - the plastic work rate. Here, we take into account the assumption that the full strain rate can be represented as the sum of three components: elastic e , plastic p and structural p strain rates. The equation defining the fraction of the plastic work rate converted into heating ( (1 ) ) is function characterizes the energy storage rate) can be expressed in the form: ( ) p
(6)
,
p
1 (
) p Tp F p TF p W
where
1 '( ) p F E p Ts p and 1 '( ) Tp F s p . If we can neglect entropy associated with a structural parameter equation (6) can be written as 1 '( )
1 1 '( )
. p E p p W
It allows us to determine '( )
(1 ) p E p p W and, consequently, estimate equation (3), describing the free energy of
system under consideration. To derive a constitutive equations for multidimensional case, we suppose that considered process of inelastic deformation is described in terms of two internal variables - p and r . An additional scalar parameter r characterizes isotropic hardening of the material. The second law of thermodynamics under isothermal conditions has the form:
F
F r r
.
: σ ε σ p
(
) :
0
p
p
We introduce the following notations: R F r ,
F P σ p . Vectors of thermodynamic forces X and
fluxes J can be defined as , , p = r J p . We will postulate the existence of a convex function Ψ , which defines thermodynamic fluxes J by the relation: , , = R X σ P ,
(7)
X ,
J
=
Ψ
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