Skip to article frontmatterSkip to article content
Site not loading correctly?

This may be due to an incorrect BASE_URL configuration. See the MyST Documentation for reference.

2 Force and stress

The deformation, described in the previous chapter, may be the result of a variety of causes, e.g. change of temperature, change of chemical composition of the environment, electromagnetic forces, mechanical forces. In this chapter, attention is focused on the mechanical forces as the cause of deformation. Upon application of a mechanical force, a continuum will deform until the internal forces, resulting from the deformation, are in equilibrium with the external forces. The internal forces are most conveniently described in terms of stress.

2.1Forces

2.1.1Body forces

We consider a three-dimensional body with volume VV and outer surface AA.

Body forces \V{q} and surface forces \V{p}, acting on a body.

Figure 2.1:Body forces q⃗\V{q} and surface forces p⃗\V{p}, acting on a body.

Next we consider two types of forces that act on the body: body forces[1] and surface forces[2] also called surface traction. Body forces act on all material points in the body. Examples are gravitational forces. Body forces are usually reckoned per unit of mass, and denoted by q⃗\V{q}. In general, they may depend on the position in the body x⃗\V{x}:

q⃗  =  q⃗(x⃗)[N⋅kg−1]\V{q} \;=\; \V{q}(\V{x}) \quad [{\mathrm N}\inp{\mathrm kg}^{-1}]

The force per unit of volume is given by ρq⃗\rho \V{q}, where ρ\rho represents the momentary density of the material in kg⋅\inpm−3^{-3}.

2.1.2Surface forces

Surface forces are forces that are exerted on the body by the part of the environment that is in contact with the surface of the body. Thus surface forces are exerted on the material points at the boundary of the body. Surface forces are reckoned per unit area of the surface, and denoted by p⃗\V{p}. In general, they may also depend on the position x⃗b\V{x}_b of the boundary of the body:

p⃗  =  p⃗(x⃗b)[N⋅m−2]\V{p} \;=\; \V{p}(\V{x}_b) \quad [{\mathrm N}\inp{\mathrm m}^{-2}]

2.2The true stress or Cauchy stress tensor

2.2.1Definition

Let us again consider a three-dimensional body in its current configuration with volume VV and a surface AA. We assume that the body is in mechanical equilibrium, i.e. we assume that sum of the forces acting on the body equals zero. This means that the body will neither accelerate, nor deform.

A imaginary division of a body in two parts, and the stress vector \V{p},
acting in a point on the cutting plane.

Figure 2.2:A imaginary division of a body in two parts, and the stress vector p⃗\V{p}, acting in a point on the cutting plane.

Now we imaginary divide the body in two parts. To prevent deformation of the separate parts, we replace the forces, previously exerted by the parts upon each other, by a suitable surface force. In general, this surface force will vary with the location in the cutting plane. We consider a small part of the cutting plane with centre PP. The part has an area ΔA\Delta A, and the sum of the surface forces acting on it equals Δf⃗\Delta \V{f}. Then the traction vector or stress vector[3] in point PP is defined as:

p⃗  =  lim⁡ΔA→0Δf⃗ΔA  =  df⃗dA\V{p} \;=\; \lim_{\Delta A \rightarrow 0} \tfrac{\Delta \V{f}}{\Delta A} \;=\; \frac{d\V{f}}{dA}

We now postulate that, for any point in the body, there exists a tensor, the Cauchy stress tensor σ\T{\sigma}, that relates the normal unit vector n⃗\V{n} on an arbitrary surface element in that point (in the current configuration) to the stress vector p⃗\V{p} on that surface (in the current configuration) according to:

p⃗  =  σ⋅n⃗\V{p} \;=\; \T{\sigma} \inp \V{n}

The Cauchy stress tensor is fully defined on the current configuration. It is therefore often called the true stress tensor, since it is the only stress tensor which is physically meaningful. With respect to an orthonormal basis {e⃗1,e⃗2,e⃗3}\{\V{e}_1,\V{e}_2,\V{e}_3\}, the components of the tensor σ\T{\sigma}, arranged in the matrix σ‾\M{\sigma}, equal:

σ‾=e⃗∼⋅σ⋅e⃗∼T=[σ11σ12σ13σ21σ22σ23σ31σ32σ33]\begin{aligned} \M{\sigma} &= \C{\V{e}} \inp \T{\sigma} \inp \C{\V{e}}^T \\ &= \begin{bmatrix} \sigma_{11} & \sigma_{12} & \sigma_{13} \\ \sigma_{21} & \sigma_{22} & \sigma_{23} \\ \sigma_{31} & \sigma_{32} & \sigma_{33} \end{bmatrix} \end{aligned}

To interpret the meaning of the components σij\sigma_{ij}, we consider the stress vector p⃗\V{p} on a surface with unit normal vector n⃗=e⃗1\V{n}=\V{e}_1:

p⃗∣e⃗1  =  σ⋅e⃗1  =  (σ11e⃗1e⃗1+σ12e⃗1e⃗2+⋯+σ33e⃗3e⃗3)⋅e⃗1  =  σ11e⃗1+σ21e⃗2+σ31e⃗3\begin{aligned} \V{p}|_{\V{e}_1} \;&=\; \T{\sigma} \inp \V{e}_1 \\ \;&=\; (\sigma_{11}\V{e}_1\V{e}_1 + \sigma_{12}\V{e}_1\V{e}_2 + \dots + \sigma_{33}\V{e}_3\V{e}_3 )\inp \V{e}_1 \\ \;&=\; \sigma_{11}\V{e}_1 + \sigma_{21}\V{e}_2 + \sigma_{31}\V{e}_3 \end{aligned}

Thus, for example the component σ21\sigma_{21} represents the component in the e⃗2\V{e}_2- direction of the stress vector on the surface with normal unit vector e⃗1\V{e}_1. In general, the component σij\sigma_{ij} represents the component in the e⃗i\V{e}_i- direction of the stress vector on the surface with normal unit vector e⃗j\V{e}_j.

Components \sigma_{ij} of the Cauchy stress tensor.

Figure 2.3:Components σij\sigma_{ij} of the Cauchy stress tensor.

2.2.2Normal and shear stress

The stress vector on a surface through a material point can be written as the sum of two vectors, a vector p⃗n\V{p}_n perpendicular to the surface and a vector p⃗s\V{p}_s in the surface:

p⃗  =  p⃗n+p⃗s\V{p} \;=\; \V{p}_n + \V{p}_s

The vector p⃗n\V{p}_n is called the normal stress vector[4], and its magnitude pnp_n is called the normal stress[5]:

p⃗n  =  pnn⃗\V{p}_n \;=\; p_n \V{n}

with:

pn=p⃗⋅n⃗=(σ⋅n⃗)⋅n⃗=n⃗⋅σ⋅n⃗\begin{aligned} p_n &= \V{p} \inp \V{n} \\ &= (\T{\sigma} \inp \V{n}) \inp \V{n} \\ &= \V{n} \inp \T{\sigma} \inp \V{n} \end{aligned}
Decomposition of the stress vector \V{p} in a normal stress vector
\V{p}_n and a shear stress vector \V{p}_s.

Figure 2.4:Decomposition of the stress vector p⃗\V{p} in a normal stress vector p⃗n\V{p}_n and a shear stress vector p⃗s\V{p}_s.

If pnp_n is positive, i.e. if p⃗n\V{p}_n is directed along n⃗\V{n}, then pnp_n is called a tensile stress[6]. If pnp_n is negative, i.e. if p⃗n\V{p}_n is directed opposite to n⃗\V{n}, then pnp_n is called a compressive stress[7].

The vector p⃗s\V{p}_s is called the shear stress vector[8], and its magnitude psp_s is called the shear stress[9]:

p⃗s=p⃗−p⃗n\V{p}_s = \V{p} - \V{p}_n

and:

ps=∥p⃗s∥=∥p⃗∥2−pn2\begin{aligned} p_s &= \|\V{p}_s\| \\ &= \sqrt{ \|\V{p}\|^2 - p_n^2 } \end{aligned}

2.2.3Principal stresses

In the next chapter, Section 3.3, it will be shown that the Cauchy stress tensor is symmetric:

σ  =  σT\T{\sigma} \;=\; \T{\sigma}^T

Thus the Cauchy stress tensor possesses three real eigenvalues σ1\sigma_1, σ2\sigma_2 and σ3\sigma_3. The corresponding eigenvectors n⃗1\V{n}_1, n⃗2\V{n}_2 and n⃗3\V{n}_3 are (or can be chosen so that they are) mutually orthogonal. We can write σ\T{\sigma} in the following spectral form:

σ=σ1n⃗1n⃗1+σ2n⃗2n⃗2+σ3n⃗3n⃗3\T{\sigma} = \sigma_1 \V{n}_1\V{n}_1 + \sigma_2 \V{n}_2\V{n}_2 + \sigma_3 \V{n}_3\V{n}_3

Calculation of the stress vector p⃗\V{p} on a special surface with n⃗=n⃗i\V{n} = \V{n}_i yields:

p⃗  =  σ⋅n⃗i=σin⃗i\V{p} \;=\; \T{\sigma} \inp \V{n}_i = \sigma_i \V{n}_i

Thus, the stress vector on these special surfaces is aligned with the normal vector, i.e. only a normal stress is exerted on these special surfaces. Therefore the eigenvalues σ1\sigma_1, σ2\sigma_2 and σ3\sigma_3 and the eigenvectors n⃗1\V{n}_1, n⃗2\V{n}_2 and n⃗3\V{n}_3 are called principal stresses[10] and principal stress directions[11], respectively.

Footnotes
  1. volumekrachten

  2. oppervlaktekrachten

  3. spanningsvector

  4. normaalspanningsvector

  5. drukspanning

  6. trekspanning

  7. drukspanning

  8. schuifspanningsvector

  9. schuifspanning

  10. hoofdspanningen

  11. hoofdspanningsrichtingen