Stress measures

The most commonly used measure of stress is the Cauchy stress tensor, often called simply the stress tensor or "true stress". However, several other measures of stress can be defined.[1][2][3] Some such stress measures that are widely used in continuum mechanics, particularly in the computational context, are:

1. The Kirchhoff stress (τ).
2. The Nominal stress (N).
3. The first Piola-Kirchhoff stress (P). This stress tensor is the transpose of the nominal stress (P=NT).
4. The second Piola-Kirchhoff stress or PK2 stress (S).
5. The Biot stress (T)

## Contents

* 1 Definitions of stress measures
* 1.1 Cauchy stress
* 1.2 Kirchhoff stress
* 1.3 Nominal stress/First Piola-Kirchhoff stress
* 1.4 Second Piola-Kirchhoff stress
* 1.5 Biot stress
* 2 Relations between stress measures
* 2.1 Relations between Cauchy stress and nominal stress
* 2.2 Relations between nominal stress and second P-K stress
* 2.3 Relations between Cauchy stress and second P-K stress
* 3 See also
* 4 Summary of relations between stress measures
* 5 References

## Definitions of stress measures

Consider the situation shown in the following figure. The following definitions use the notations shown in the figure.

Quantities used in the definition of stress measures

In the reference configuration Ω0, the outward normal to a surface element dΓ0 is 𝐍≡𝐧0 and the traction acting on that surface is 𝐭0 leading to a force vector d𝐟0. In the deformed configuration Ω, the surface element changes to dΓ with outward normal 𝐧 and traction vector 𝐭 leading to a force d𝐟. Note that this surface can either be a hypothetical cut inside the body or an actual surface. The quantity F is the deformation gradient tensor, J is its determinant.

### Cauchy stress

The Cauchy stress (or true stress) is a measure of the force acting on an element of area in the deformed configuration. This tensor is symmetric and is defined via

d𝐟=𝐭dΓ=σT⋅𝐧dΓ

𝐭=σT⋅𝐧

where 𝐭 is the traction and 𝐧 is the normal to the surface on which the traction acts.

### Kirchhoff stress

The quantity,

τ=Jσ

is called the Kirchhoff stress tensor, with J the determinant of F. It is used widely in numerical algorithms in metal plasticity (where there is no change in volume during plastic deformation). It can be called weighted Cauchy stress tensor as well.

### Nominal stress/First Piola-Kirchhoff stress

The nominal stress N=PT is the transpose of the first Piola-Kirchhoff stress (PK1 stress, also called engineering stress) P and is defined via

d𝐟=𝐭dΓ=NT⋅𝐧0dΓ0=P⋅𝐧0dΓ0

𝐭0=𝐭dΓdΓ0=NT⋅𝐧0=P⋅𝐧0

This stress is unsymmetric and is a two-point tensor like the deformation gradient.
The asymmetry derives from the fact that, as a tensor, it has one index attached to the reference configuration and one to the deformed configuration.[4]

### Second Piola-Kirchhoff stress

If we pull back d𝐟 to the reference configuration, we have

d𝐟0=F−1⋅d𝐟

or,

d𝐟0=F−1⋅NT⋅𝐧0dΓ0=F−1⋅𝐭0dΓ0

The PK2 stress (S) is symmetric and is defined via the relation

d𝐟0=ST⋅𝐧0dΓ0=F−1⋅𝐭0dΓ0

Therefore,

ST⋅𝐧0=F−1⋅𝐭0

### Biot stress

The Biot stress is useful because it is energy conjugate to the right stretch tensor U. The Biot stress is defined as the symmetric part of the tensor PT⋅R where R is the rotation tensor obtained from a polar decomposition of the deformation gradient. Therefore, the Biot stress tensor is defined as

T=12(RT⋅P+PT⋅R).

The Biot stress is also called the Jaumann stress.

The quantity T does not have any physical interpretation. However, the unsymmetrized Biot stress has the interpretation

RTd𝐟=(PT⋅R)T⋅𝐧0dΓ0

## Relations between stress measures

### Relations between Cauchy stress and nominal stress

From Nanson's formula relating areas in the reference and deformed configurations:

𝐧dΓ=JF−T⋅𝐧0dΓ0

Now,

σT⋅𝐧dΓ=d𝐟=NT⋅𝐧0dΓ0

Hence,

σT⋅(JF−T⋅𝐧0dΓ0)=NT⋅𝐧0dΓ0

or,

NT=J(F−1⋅σ)T=JσT⋅F−T

or,

N=JF−1⋅σandNT=P=JσT⋅F−T

In index notation,

NIj=JFIk−1σkjandPiJ=JσkiFJk−1

Therefore,

Jσ=F⋅N=F⋅PT.

Note that N and P are (generally) not symmetric because F is (generally) not symmetric.

### Relations between nominal stress and second P-K stress

Recall that

NT⋅𝐧0dΓ0=d𝐟

and

d𝐟=F⋅d𝐟0=F⋅(ST⋅𝐧0dΓ0)

Therefore,

NT⋅𝐧0=F⋅ST⋅𝐧0

or (using the symmetry of S),

N=S⋅FTandP=F⋅S

In index notation,

NIj=SIKFjKTandPiJ=FiKSKJ

Alternatively, we can write

S=N⋅F−TandS=F−1⋅P

### Relations between Cauchy stress and second P-K stress

Recall that

N=JF−1⋅σ

In terms of the 2nd PK stress, we have

S⋅FT=JF−1⋅σ

Therefore,

S=JF−1⋅σ⋅F−T=F−1⋅τ⋅F−T

In index notation,

SIJ=FIk−1τklFJl−1

Since the Cauchy stress (and hence the Kirchhoff stress) is symmetric, the 2nd PK stress is also symmetric.

Alternatively, we can write

σ=J−1F⋅S⋅FT

or,

τ=F⋅S⋅FT.

Clearly, from definition of the push-forward and pull-back operations, we have

S=φ*[τ]=F−1⋅τ⋅F−T

and

τ=φ*[S]=F⋅S⋅FT.

Therefore, S is the pull back of τ by F and τ is the push forward of S.

## See also

* Stress
* Finite strain theory
* Continuum mechanics
* Hyperelastic material
* Cauchy elastic material
* Critical plane analysis

## Summary of relations between stress measures

* v
* t
* e

Stress Tensor

* Cauchy stress tensor (σ)
* First Piola-Kirchhoff stress tensor (P)
* Second Piola-Kirchhoff stress tensor (S)
* Kirchhoff stress tensor (τ)
* Biot stress tensor (T)
* Mandel stress tensor (M)
* Rotation tensor(R)

Conversion formulae

| σ | P | S | τ | T | M
σ= | σ | J−1PFT | J−1FSFT | J−1τ | J−1RTFT | J−1RMRT
P= | JσF−T | P | FS | τF−T | RT | F−TM
S= | JF−1σF−T | F−1P | S | F−1τF−T | U−1T | C−1M
τ= | Jσ | PFT | FSFT | τ | RTFT | RMRT
T= | JRTσF−T | RTP | US | RTτF−T | T | U−1M
M= | JRTσR | FTP | CS | RTτR | UT | M
J=det⁡(F),C=FTF=U2,F=RU,RT=R−1
P=JσF−T,τ=Jσ,S=JF−1σF−T,T=RTP,M=CS

## References

1. ↑ J. Bonet and R. W. Wood, Nonlinear Continuum Mechanics for Finite Element Analysis, Cambridge University Press.
2. ↑ R. W. Ogden, 1984, Non-linear Elastic Deformations, Dover.
3. ↑ L. D. Landau, E. M. Lifshitz, Theory of Elasticity, third edition
4. ↑ Three-Dimensional Elasticity. Elsevier. 1 April 1988. ISBN 978-0-08-087541-5. https://books.google.com/books?id=tlGCC3w27iIC.

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