P-wave modulus

From Wikipedia, the free encyclopedia
Jump to navigation Jump to search

There are two kinds of seismic body waves in solids, pressure waves (P-waves) and shear waves. In linear elasticity, the P-wave modulus M, also known as the longitudinal modulus, or the constrained modulus, is one of the elastic moduli available to describe isotropic homogeneous materials.

It is defined as the ratio of axial stress to axial strain in a uniaxial strain state. This occurs when expansion in the transverse direction is prevented by the inertia of neighboring material, such as in an earthquake, or underwater seismic blast.

σzz=Mϵzz

where all the other strains ϵ** are zero.

This is equivalent to stating that

Mx=ρxVP2,

where VP is the velocity of a P-wave and ρ is the density of the material through which the wave is propagating.


References

[edit | edit source]
  • G. Mavko, T. Mukerji, J. Dvorkin. The Rock Physics Handbook. Cambridge University Press 2003 (paperback). Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
Homogeneous isotropic linear elastic materials have their elastic properties uniquely determined by any two quantities among these; thus, given any two, any other of the elastic moduli can be calculated according to these formulas, provided both for 3D materials (first part of the table) and for 2D materials (second part).
3D Formulae
Knowns Bulk modulus (K) Young's modulus (E) Lamé's first parameter (λ) Shear modulus (G) Poisson's ratio (ν) P-wave modulus (M) Notes
(K, E) 3KE/3 − E/3K E/3 − E/3K 1/2E/6K 3K + E/3 − E/3K
(K, λ) 9K(K − λ)/3K − λ 3(K − λ)/2 λ/3K − λ 3K − 2λ
(K, G) 9KG/3K + G K2G/3 3K − 2G/6K + 2G K + 4G/3
(K, ν) 3K(1 − 2ν) 3/1 + ν 3K(1 − 2ν)/2(1 + ν) 3K(1 − ν)/1 + ν
(K, M) 9K(MK)/3K + M 3KM/2 3(MK)/4 3KM/3K + M
(E, λ) E + 3λ + R/6 E − 3λ + R/4 E + R/1/4 E − λ + R/2 R = ±(E2 + 9λ2 + 2Eλ)1/2
(E, G) EG/3(3GE) G(E − 2G)/3GE E/2G − 1 G(4GE)/3GE
(E, ν) E/3 − 6ν /(1 + ν)(1 − 2ν) E/2(1 + ν) E(1 − ν)/(1 + ν)(1 − 2ν)
(E, M) 3ME + S/6 ME + S/4 3M + ES/8 E + S/4M1/4 S = ±(E2 + 9M2 − 10EM)1/2
(λ, G) λ + 2G/3 G(3λ + 2G)/λ + G λ/2(λ + G) λ + 2G
(λ, ν) λ/3(1 + 1/v) λ(1/ν − 2ν − 1) λ(1/2ν − 1) λ(1/ν − 1)
(λ, M) M + 2λ/3 (M − λ)(M+2λ)/M + λ M − λ/2 λ/M + λ
(G, ν) 2G(1 + ν)/3 − 6ν 2G(1 + ν) 2 G ν/1 − 2ν 2G(1 − ν)/1 − 2ν
(G, M) M4G/3 G(3M − 4G)/MG M − 2G M − 2G/2M − 2G
(ν, M) M(1 + ν)/3(1 − ν) M(1 + ν)(1 − 2ν)/1 − ν M ν/1 − ν M(1 − 2ν)/2(1 − ν)
2D Formulae
Knowns (K) (E) (λ) (G) (ν) (M) Notes
(K2D, E2D) 2K2D(2K2DE2D)/4K2DE2D K2DE2D/4K2DE2D 2K2DE2D/2K2D 4K2D^2/4K2DE2D
(K2D, λ2D) 4K2D(K2D − λ2D)/2K2D − λ2D K2D − λ2D λ2D/2K2D − λ2D 2K2D − λ2D
(K2D, G2D) 4K2DG2D/K2D + G2D K2DG2D K2DG2D/K2D + G2D K2D + G2D
(K2D, ν2D) 2K2D(1 − ν2D) 2K2Dν2D/1 + ν2D K2D(1 − ν2D)/1 + ν2D 2K2D/1 + ν2D
(E2D, G2D) E2DG2D/4G2DE2D 2G2D(E2D − 2G2D)/4G2DE2D E2D/2G2D − 1 4G2D^2/4G2DE2D
(E2D, ν2D) E2D/2(1 − ν2D) E2Dν2D/(1 + ν2D)(1 − ν2D) E2D/2(1 + ν2D) E2D/(1 + ν2D)(1 − ν2D)
2D, G2D) λ2D + G2D 4G2D2D + G2D)/λ2D + 2G2D λ2D/λ2D + 2G2D λ2D + 2G2D
2D, ν2D) λ2D(1 + ν2D)/2ν2D λ2D(1 + ν2D)(1 − ν2D)/ν2D λ2D(1 − ν2D)/2ν2D λ2D/ν2D
(G2D, ν2D) G2D(1 + ν2D)/1 − ν2D 2G2D(1 + ν2D) 2 G2D ν2D/1 − ν2D 2G2D/1 − ν2D
(G2D, M2D) M2DG2D 4G2D(M2DG2D)/M2D M2D − 2G2D M2D − 2G2D/M2D