Adiabatic Shear Localization || Shear Localization in Deep Geological Layers During Seismic Slip

10Shear Localization in DeepGeological Layers DuringSeismic Slip

Jean Sulem

CERMES, Laboratoire Navier, Ecole des Ponts Paris Tech, IFSTTAR,Universite Paris-Est, Marne-la-Vallee, France

Nomenclature

p pressure

T temperature

n porosity

ρ density of the porous medium

ρf density of the saturating fluid

σn normal stress

τ shear stress

p pore fluid pressure

ε volumetric strain

γ shear strain

εp plastic volumetric strain

γp plastic shear strain

ωc Cosserat rotation

R Cosserat internal length

G elastic shear modulus

Gc Cosserat elastic shear modulus

K elastic bulk modulus of the porous medium

Ks bulk modulus of the solid matrix

b Biot coefficient

H plastic hardening modulus

μ friction coefficient

β dilatancy coefficient

βf pore fluid compressibility

λf pore fluid thermal expansion coefficient

βn pore volume compressibility

βf pore volume thermal expansion

β�storage coefficient

Λ undrained thermo-elastic pressurization coefficient

kf permeability

Adiabatic Shear Localization. DOI: http://dx.doi.org/10.1016/B978-0-08-097781-2.00010-1

© 2012 Elsevier Ltd. All rights reserved.

http://dx.doi.org/10.1016/B978-0-08-097781-2.00010-1

chy hydraulic diffusivity

cth thermal diffusivity

ρC specific heat per unit volume of the material

ΔrH0T enthalpy change of the chemical reaction for calcite decomposition

Ea activation energy of the chemical reaction for calcite decomposition

10.1 Introduction

In the past 30 years, the study of earthquake mechanisms has emphasized the major

role of rock friction. Earthquakes appear to be the result of a frictional instability

and occur by sudden slippage along a pre-existing fault because the frictional resis-

tance to slip on the fault walls decreases with increasing slip, causing an accelera-

tion of sliding. Field observations of mature faults, i.e. faults that have experienced

a large slip, show a generally broad zone of damaged rock, but nevertheless suggest

that shear in individual earthquakes occurs in very narrow localized zones of a

few millimetres thick or even less. Field observations reveal that the fault material

inside the localized shear zone is a finely granulated gouge that has usually under-

gone mechano-chemical degradation (intense grain comminution, gelification,

decarbonation and dehydration reactions, melting) [1]. The actual thickness of the

zone over which the shear is localized is a key parameter for the evaluation of the

energy budget during earthquake rupture. It is generally estimated that more than

90% of the frictional work is converted into heat [2]. Thus, it is expected that

weakening mechanisms from thermal origin are of major importance. Fault zones

commonly exhibit the presence of fluid interacting with the rock. Recent theoretical

studies have emphasized the role of thermal pore fluid pressurization as an impor-

tant cause of slip weakening [3]. The principle of slip weakening by thermal pres-

surization is based on the fact that pore fluids trapped inside the fault zone are put

under pressure by shear heating, thus inducing a reduction of the effective mean

stress and of the shearing resistance of the fault plane [4�7]. This mechanism has

also been suggested for weakening in catastrophic landslides [8�15]. The presence

of clay material in fault zones also affects thermal pressurization as possible col-

lapse of the clay under thermal loading may activate fluid pressurization [7,16].

Thermo-poro-mechanical couplings due to shear heating can also be associated

with chemical effects such as dehydration of minerals or decomposition of carbo-

nates [17�20]. Such reactions induce two competing effects: a direct increase in

pore pressure because they release fluid in the system and a limit in temperature

increase because these reactions are endothermic so that part of the frictional heat

is actually absorbed in the chemical reactions.

In this chapter, we first present the thermo-poro-mechanical background used to

analyse the effect of pore fluid and temperature in the strain localization process as

the result of instability of undrained adiabatic shearing of a rock layer. In particu-

lar, we analyse the possibility of a selection of a preferred wavelength of the insta-

bility mode (i.e. the one corresponding to the fastest growth), which could control

the width of the localized zone. The undrained adiabatic limit is applicable as soon

400 Adiabatic Shear Localization

as the slip event is sufficiently rapid and the shear zone broad enough to effectively

preclude heat or fluid transfer as is the case during an earthquake. Then we will

consider a particular example of chemical couplings during seismic slip by taking

into account the possibility for some parts of the fault zone to reach the threshold

temperature at which mineral decomposition can be triggered.

10.2 Position of the Problem and Governing Equations

We consider a layer of saturated rock of thickness h that is sheared in plane strain

(Figure 10.1) in such a way that there is no extensional strain in the x-direction and dis-

placements ux, and uz of material points vary only with z (and time t). The stress state

in the layer is a shear stress τ and a normal stress σ in the y-direction. The only non-

zero strains, a shear strain γ and a normal strain ε, are related to the displacements by

γ5@ux@z

; ε5@uz@z

ð10:1Þ

Because the normal strains in the other directions are zero, the volumetric strain

is equal to ε.The equilibrium equations during quasi-static deformation reduce to

@τ@z

5 0;@σ@z

5 0 ð10:2Þ

so that the stresses must be spatially uniform and vary only with time during the

deformation.

10.2.1 Constitutive Equations

The rate thermo-poro elasto-plastic relationships for the rock layer are expressed as

_γ51

G_τ1 _γp; _ε5

1

Kð _σ2 b _pÞ2αs

_T 1 _εp ð10:3Þ

p,T

τ

σ

h

qhqf

z

x

uy(z,t)

ux(z,t)

Figure 10.1 Model of a deforming shear

band with heat and fluid fluxes.

401Shear Localization in Deep Geological Layers During Seismic Slip

where G and K are the elastic shear and bulk modulus, respectively, of the empty

porous solid, p is the pore pressure, T is the temperature, b is the Biot coefficient,

and αs is the thermal dilatation coefficient of the empty porous solid. The Biot

coefficient is related to the bulk modulus of the solid matrix Ks according to the

following equation:

b5 12K

Ks

ð10:4Þ

The rate of plastic deformation is written as [21]

_γp 51

Hð_τ2μð _σ2 _pÞÞ

_εp 5 β _γpð10:5Þ

where H(γp) is the plastic-hardening modulus and is related to the tangent modulus

Htan of the τ versus γ curve by (Figure 10.2)

Htan 5H

11H=Gð10:6Þ

and is either positive or negative according to whether τ versus γ curve is rising

(hardening) or falling (softening), although the falling portion may never be

observed as homogeneous deformation in a drained test. In Eq. (10.5), β is the

dilatancy coefficient.

1 + H/G

H

H + μβ/β*

1+ (H + μβ/β*)/G1

γ

τ

Drained

Undrained

1

Figure 10.2 Stress�strain curve for a

saturated rock in drained or undrained

conditions.


10.2.2 Mass Balance Equation

Conservation of fluid mass is expressed by

@mf

@t52

@qf@z

ð10:7Þ

where mf is the total fluid mass per unit volume of porous medium (in the reference

state) and qf is the flux of fluid. The total fluid mass per unit volume of porous

medium is written as mf5 ρfn, where n is the pore volume fraction (Lagrangian

porosity) and ρf is the density of the saturating fluid. The left-hand side of

Eq. (10.7) is obtained by differentiating this product:

@mf

@t5 n

@ρf@t

1 ρf@n

@tð10:8Þ

The derivatives of the right-hand side of Eq. (10.8) are given by

@ρf@t

5 ρfβf

@p

@t2 ρfλf

@T

@tð10:9Þ

and

@n

@t5 nβn

@p

@t1 nλn

@T

@t1

@np

@tð10:10Þ

where βf 51ρf

@ρf@p

� �Tis the pore fluid compressibility, λf 52 1

ρf@ρfT

� �Pp

is the pore

fluid thermal-expansion coefficient, βn 51n

@n@p

� �Tis the pore volume compressibility

and λn 51n

@n@T

� �Pp

is the elastic thermal-expansion coefficient of the pore volume,

which is equal to the elastic thermal-expansion coefficient of the solid fraction,

λn5αs.

The expression of the pore volume compressibility is obtained from poro-elasticity

theory and is given by [3,22]

βn 51

n

1

K2

11 n

Ks

� �ð10:11Þ

In Eq. (10.10), @np

@t is the rate of plastic porosity change.

Using Eqs (10.2)�(10.4), the left-hand side of Eq. (10.7) is thus evaluated as

@mf

@t5 nρfðβn 1βfÞ

@p

@t2 ρfnðλf 2λnÞ

@T

@t1 ρf

@np

@tð10:12Þ


The flux term in Eq. (10.7) is evaluated assuming Darcy’s law for fluid flow

with viscosity ηf through a material with permeability kf:

qf 52ρfηf

kf@p

@zð10:13Þ

Substituting Eqs (10.12) and (10.13) into Eq. (10.7) gives the equation that gov-

erns the pore fluid production and diffusion:

@p

@t5 chy

@2p

@z21Λ

@T

@t2

1

β�@np

@tð10:14Þ

where

Λ5λf 2λn

βn 1βf

ð10:15Þ

is the thermo-elastic pressurization coefficient under undrained conditions [3]. This

coefficient is pressure and temperature dependent because the compressibility and

the thermal-expansion coefficients of the fluid vary with pressure and temperature

and also because the compressibility of the pore space of the rock can change with

the effective stress [22]. In Eq. (10.14), β�5 n(βn1 βf) is the storage capacity of

the rock and chy5 kf/(βηf) is the hydraulic diffusivity. For incompressible solid

phase and fluid, β�5 1/K.

If we assume that the solid matrix is plastically incompressible,

@np

@t5

@εp

@tð10:16Þ

10.2.3 Energy Balance Equation

Let EF be the rate of frictional heat produced during shearing. The equation of con-

servation of energy is expressed as

ρC@T

@t5EF 2

@qh@z

ð10:17Þ

where ρC is the specific heat per unit volume of the material in its reference state and qhis the heat flux. It is assumed here that all of the plastic work is converted into heat and,

thus, EF 5 τ _γp: The heat flux is related to the temperature gradient by Fourier’s law:

qh 52kT@T

@zð10:18Þ


where kT is the thermal conductivity of the saturated material. Substituting

Eq. (10.18) into Eq. (10.19) gives the energy conservation equation

@T

@t5 cth

@2T

@z21

1

ρCτ _γp ð10:19Þ

where cth5 kT/ρC is the thermal diffusivity.

Undrained Adiabatic Limit

We assume that the drainage and the heat flux are prohibited at the boundaries of

the layer (qf5 0 and qh5 0). This corresponds to the situation when the slip event

is sufficiently rapid and the shear zone broad enough to effectively preclude heat or

fluid transfer as is the case during an earthquake or a landslide. We also assume

that the normal stress σ acting on the sheared layer is constant ( _σ5 0). From Eqs

(10.5), (10.14), (10.16) and (10.19), we obtain the following relationship between

the pore pressure rate and the shear stress rate:

_p5ΛτρC 2 β

β�

H2μ ΛτρC 2 β

β�

� � _τ ð10:20Þ

Substituting Eq. (10.20) into Eq. (10.3), we get

_γ51

G1

1

H1μβ=β� 2μΛτ=ρC

� �_τ ð10:21Þ

or

_τ5H1μβ=β� 2μΛτ=ρC

11ðH1μβ=β� 2μΛτ=ρCÞ=G

� �_γ ð10:22Þ

If we neglect the thermal effect (Λ5 0), the expression for dilatant hardening

effect as proposed by Rice [21] is retrieved (Figure 10.2):

_τ5H1μβ=β�

11ðH1μβ=β�Þ=G

� �_γ ð10:23Þ

Equation (10.22) has to be compared with the drained case for which

_τ5H

11H=G

� �_γ ð10:24Þ


For dilatant material (β. 0), we identify in Eq. (10.22) a hardening effect

due to dilatancy with the term μβ/β�and a thermal-softening effect with the

term 2μΛτ/ρC. When thermal softening prevails against strain hardening, plastic

localization in the form of adiabatic shear banding can occur.

10.3 Stability of Analysis of Undrained Adiabatic Shearingof a Rock Layer

We consider again the shearing of the layer while drainage and heat fluxes are pre-

vented at its boundaries. The pertinent variables are written in the form

γ5 γ0 1 ~γ; ε5 ε0 1 ~ε; σ5σ0 1 ~σ; τ5 τ0 1 ~τ; p5 p0 1 ~p; T 5 T0 1 ~T

ð10:25Þ

where the quantities γ0, τ0 and so on represent the solution of the last section for

homogeneous deformation, and ~γ; ~τ and so on are perturbation quantities.

Specifically, the layer is sheared by application of a monotonically increasing shear

stress τ05 τ0(t) to its boundary while the normal stress is held constant at σ0.From the equilibrium equation (10.2), the stress field is uniform within the layer,

and thus ~σ5 0 and ~τ5 0: This problem is similar to the one addressed by Rice

[21] with the introduction here of the thermal effect. From the conservation equa-

tions (10.14) and (10.19), and by keeping only the first-order terms, we get the

same type of rate equations for the perturbation terms

@ ~p

@t5 chy

@2 ~p

@z21Λ

@ ~T

@t2

1

β�@~εp

@t

@ ~T

@t5 cth

@2 ~T

@z21

1

ρCτ0

@ ~γp

@t

ð10:26Þ

with the following from the constitutive equation (10.5):

@ ~γp

@t5

μH

@ ~p

@t;

@~εp

@t5β

@ ~γp

@t5 β

μH

@ ~p

@tð10:27Þ

The spatial dependence of the perturbations is decomposed into Fourier modes

with wavelength λ. Perturbations of the form

~p5Pð0Þest cos 2πzλ

� �; ~T 5 Tð0Þest cos 2πz

λ

� �ð10:28Þ


with λ5 h/n and n equal to an integer satisfy the zero heat and fluid flux boundary

conditions at y5 0, h. In Eq. (10.28), s is the growth coefficient in time of the per-

turbation. By substituting the perturbations field (Eq. (10.28)) into Eq. (10.26), we

obtain a homogeneous algebraic system for the coefficients P(0) and T(0). Thus, a

non-zero solution is possible only if the determinant of the coefficients vanishes:

det

s 11βμβ�H

0@

1A1 chy

2πλ

0@

1A2

2Λs

μρCH

τ0s 2 cth2πλ

0@

1A2

1 s

0@

1A

0BBBBBBB@

1CCCCCCCA

5 0 ð10:29Þ

The preceding condition yields a quadratic equation for the growth coefficient s:

ΛμρC

τ0 2βμβ� 2H

� �λ4s2 2 ðcth 1 chyÞH1

βμβ�

� �λ2s2 cthchyH5 0 ð10:30Þ

If a solution of Eq. (10.30) has a positive real part, then the corresponding per-

turbation grows exponentially in time.

If we do not consider the thermal effect, i.e. Λ5 0, the condition for stability is

simply H. 0. Thus, the result of Rice [21] is retrieved that undrained shearing is

stable only in those circumstances for which the underlying drained deformation

would be stable. This problem has also been examined by Vardoulakis [23,24] who

proposed a regularization of the mathematically ill-posed problem in the softening

regime by resorting to a second-grade extension of plasticity theory.

If we now take into account the thermal effect (Λ. 0), we observe that if

H. 0, the stability condition is

ΛμρC

τ0 ,βμβ� 1H ð10:31Þ

Consequently, the condition of stability of undrained adiabatic shearing is

H. 0 andΛμρC

τ0 ,βμβ� 1H ð10:32Þ

and the system is always unstable in the softening regime.

Obviously, this condition is more restrictive than the one for undrained shearing.

This result demonstrates the destabilizing effect of thermal fluid pressurization:

undrained adiabatic shearing of a material with positive strain hardening is

stable only when the thermal pressurization is not too high.


10.4 Wavelength Selection and Thickness of theShear Band

The stability analysis performed as described earlier for a classical Cauchy contin-

uum does not reveal any wavelength selection of the instability mode because

the change of sign from negative to positive values of the growth coefficient s

occurs for the same value of the hardening modulus independent of the considered

particular wavelength λ. Consequently, the width of the localized zone is actually

indeterminate. Moreover, we observe that at the onset of the instability, i.e. forΛμρC τ0 5

βμβ� 1H; there is a sharp transition from infinitely stable to infinitely

unstable behaviour, which indicates that the solution of the considered initial-value

problem does not exist and consequently that the corresponding problem is mathe-

matically ill-posed. The origin of this undesirable situation can be traced back to the

fact that conventional constitutive models do not contain material parameters with

dimension of length, so that the shear-band thickness (i.e. the extent of the plasti-

cally softening region) is undetermined. Rudnicki [25] proposed an ad hoc regulari-

zation by introducing a zone of finite thickness corresponding to a layer that has

already weakened due to past faulting. In doing so, inhomogeneous deformation is

prohibited over scales shorter than some prescribed length. Vardoulakis [24,26,27]

showed that by introducing viscous effects combined with second-gradient depen-

dency of the friction in strain may alleviate the ill-posedness of the problem. More

generally, it appears necessary to resort to continuum models with microstructure to

describe correctly localization phenomena. These generalized continua usually con-

tain additional kinematical degrees of freedom (Cosserat continuum) and/or higher

deformation gradients (higher grade continuum). Cosserat continua and higher grade

continua belong to a general class of constitutive models, which account for the

materials microstructure. The contemporary formulation of these models is based on

the work of Mindlin [28] and Germain [29,30]. Rotation gradients and higher veloc-

ity gradients introduce a material length scale into the problem, which, as already

mentioned, is necessary for the correct modelling of localization phenomena. This

idea was widely publicized by the paper of Muhlhaus and Vardoulakis [31] who

have resorted to concepts from Cosserat continuum mechanics to determine the

thickness of the shear band. Thus, by allowing both particle displacements and parti-

cle rotations, they accounted for the angularities of the grains and enriched the clas-

sical continuum with additional kinematic and static fields. For dry sand, they

obtained the shear-band thickness of about 16d50, where d50 is the mean grain diam-

eter. Considering the non-cohesive character of the cataclastic fault gouge inside the

slip zone, we follow the same idea and allow for additional rotational degrees of

freedom for the fault material within the frame of the Cosserat continuum theory.

10.4.1 Constitutive Equations

The incremental constitutive equations for the considered 2D Cosserat continuum

are derived from the Muhlhaus�Vardoulakis plasticity model. The main feature of


the model is that a 2D flow theory of plasticity for granular media with Cosserat

microstructure can be derived by keeping the same definitions for the yield surface

and the plastic potential as in the classical theory and by generalizing appropriately

the stress and strain invariants involved in these definitions.

In a 2D Cosserat continuum, each material point has two translational degrees

of freedom (v1, v2) and one rotational degree of freedom ( _ωc). The four components

of the rate of the non-symmetric deformation tensor are given by

_ε11 5 @v1=@x1; _ε12 5 @v1=@x2 1 _ωc

_ε22 5 @v2=@x2; _ε21 5 @v2=@x1 1 _ωc ð10:33Þ

and the two components of the ‘curvature’ of the deformation rate (gradient of the

Cosserat rotation rate) are given by

_κ1 5 @ _ωc=@x1; _κ2 5 @ _ωc=@x2 ð10:34Þ

Besides the four components of the non-symmetric stress tensor σij, there are

two couple stresses, mk (k5 1,2). The convention used here for the stress tensor fol-

lows Vardoulakis and Sulem [32], i.e. the first index denotes the direction of the

force and the second index, the face with which a stress component is associated

(Figure 10.3).

As in classical small-strain plasticity theory, the deformation is decomposed into

elastic and plastic parts:

_εij 5 _εeij 1 _εpij; _κk 5 _κek 1 _κp

k ðk5 1; 2Þ ð10:35Þ

p,T

u1(x2, t)

u2(x2, t)m2

m1

ωc

σn

σ22σ21

σ12σ11

τ

x1

x2

qfqh

D

Figure 10.3 Cosserat stresses and couple stresses.


Moreover, the stress and the deformation are decomposed into spherical and

deviatoric parts:

σij 5 sij 1σkkδij=2_εij 5 _eij 1 _εkkδij=2

ð10:36Þ

where δij is the Kronecker delta.The generalized stress and strain invariants are utilized

σ5σii=2; τ5ffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffih1sijsij 1 h2sijsji 1 h3mkmk=R2

p_εp 5 _εpkk; _γp 5

ffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffig1 _e

pij _e

pij 1 g2 _e

pij _e

pji 1 g3R2 _κp

k _κpk

q ð10:37Þ

where {hi}5 {3/4,2 1/4,1} and {gi}5 {3/2,1/2,1} for the so-called static Cosserat

model, and R is the internal length of the material [32].

As in the previous section, we assume a Coulomb yield surface and plastic

potential

F5 τ2μðσ2 pÞ; Q5 τ2βðσ2 pÞ ð10:38Þ

where the mobilized friction and dilatancy coefficients μ and β, respectively, areonly functions of the accumulated plastic strain γp.

The strain-rate thermo-poro elasto-plastic relationships are formally unchanged and

are expressed by Eq. (10.3). The rate of plastic deformation is given by Eq. (10.5).

For the considered 2D Cosserat continuum and the configuration of Figure 10.3,

the local equilibrium equations are

@σ12

@x25 0

@σ22

@x25 0

@m

@x21σ21 2σ12 5 0

ð10:39Þ

with m5m2 and m1� 0. It is assumed that no couple stress is imposed at the

boundary. Prior to localization, the state of stress and strain is uniform and consid-

ering the couple-free boundary condition, the couple stress is identically zero in the


sheared layer. Therefore, the rock layer behaves as a classical Cauchy continuum

prior to localization.

10.4.2 Stability of Analysis of Undrained Adiabatic Shearingfor a Cosserat Layer

The detailed analysis of the stability analysis of a Cosserat layer under shear is

presented in Ref. [33]. The main steps are recalled in the following. The small per-

turbations considered herein are defined as follows:

u1ðx2; tÞ5 u01ðx2; tÞ1 ~u1ðx2; tÞu2ðx2; tÞ5 u02ðx2; tÞ1 ~u2ðx2; tÞωcðx2; tÞ5ω0

cðx2; tÞ1 ~ωcðx2; tÞTðx2; tÞ5 T0ðx2; tÞ1 ~Tðx2; tÞpðx2; tÞ5 p0ðx2; tÞ1 ~pðx2; tÞ

ð10:40Þ

Dimensionless quantities are defined as

x5x1

R; z5

x2

R; ui 5

ui

R; i5 1; 2

p5p

σn

; σij 5σij

σn

; t5cth

R2t; T 5

Λσn

Tð10:41Þ

To simplify the notations, in the following and in the rest of the text, the line

over the symbols for the dimensionless variables is omitted: t � t; p � p; etc:The dimensionless form of the fluid mass balance equation (10.14) and the

energy conservation (10.19) is

@p

@t2

@T

@t2 η

@2p

@z21 δ

@γp

@t5 0

@T

@t2

@2T

@z22α

@γp

@t5 0

ð10:42Þ

where the dimensionless parameters α, δ and η are given by

α5Λτ0ρCσn

; δ5β

β�σn

; η5chy

cthð10:43Þ


and

@γ@t

p

51

2H

@σ12

@t1

@σ21

@t1μ

@σ011

@t1

@σ022

@t

0@

1A

0@

1A

H5H

σn

5 hσ0

σn

ð10:44Þ

The dimensionless form of the balance of linear momentum with inertia and

micro-inertia terms is as follows:

@σ12

@z2 I

@2u1@t2

5 0

@σ022

@z2

@p

@z2 I

@2u2@t2

5 0

@m

@z1 σ21 2σ12 2

1

2I@2ωc

@t25 0

ð10:45Þ

where the dimensionless inertia parameter is I5c2thρR2σn

: The moment of inertia of

the considered Cosserat continuum is ρR2/2 [32].

For the considered simple shear initial state of stress, the (dimensionless) incre-

mental thermo-poro elasto-plastic constitutive equations are given by

Δσ011

Δσ022

Δσ012

Δσ021

Δm

8>>>>>><>>>>>>:

9>>>>>>=>>>>>>;

5

a b c c 0

b a c c 0

f f d e 0

f f e d 0

0 0 0 0 g

0BBBBBB@

1CCCCCCA

Δγ11Δγ22Δγ12Δγ21Δκ

8>>>>>><>>>>>>:

9>>>>>>=>>>>>>;

2αs

ða1 bÞ=2ða1 bÞ=20

0

0

8>>>>>><>>>>>>:

9>>>>>>=>>>>>>;ΔT ð10:46Þ

where Δσ0ij 5Δσij 2Δpδij is the increment of dimensionless (Terzaghi) effective

stress:

Δγ11 5@Δu1

@x5 0; Δγ22 5

@Δu2

@z;

Δγ12 5@Δu1

@z1Δωc; Δγ21 5

@Δu2

@x2Δωc 52Δωc

Δκ5@Δωc

@z

ð10:47Þ


and the dimensionless incremental constitutive coefficients are given by

a51

σn

K1G2βμK2

G1H1 βμK

0@

1A; b5

1

σn

K2G2βμK2

G1H1βμK

0@

1A

c51

σn

2GKβ

G1H1βμK

0@

1A; f 5

1

σn

2GKμ

G1H1βμK

0@

1A

d51

σn

G1Gc 2G2

G1H1βμK

0@

1A; e5

1

σn

G2Gc 2G2

G1H1βμK

0@

1A

g5G

σn

αs 5αs

σn

Λ

ð10:48Þ

Inserting the constitutive equations (10.46) in the governing equations (10.42)

and (10.45), we get

d@2 ~u1@z2

1 f@2 ~u2@z2

1ðd2 eÞ @ ~ωc

@z2 I

@2 ~u1@t2

5 0

c@2 ~u1@z2

1 a@2 ~u2@z2

2 I@2 ~u2@t2

2@ ~p

@z2αs

a1 b

2

@ ~T

@z5 0

ðd2 eÞ @ ~u1@z

1 g@2 ~ωc

@z21 2ðd2 eÞ @ ~ωc

@z2

1

2I@2ωc

@t25 0

δH

d1 e

21μc

0@

1A @2 ~u1

@z@t1

δH

f 1μa1 b

2

0@

1A @2 ~u2

@z@t2 η

@2 ~p

@z2

1@ ~p

@t2 11

δHμαs

a1 b

2

0@

1A @ ~T

@t5 0

2αH

d1 e

21μc

0@

1A @2 ~u1

@z@t2

αH

f 1μa1 b

2

0@

1A @2 ~u2

@z@t2

@2 ~T

@z2

1 11αHμαs

a1 b

2

0@

1A @ ~T

@t5 0

ð10:49Þ


The spatial dependence of the perturbations is again decomposed into Fourier

modes with wavelength λ. We consider perturbations of the form

~u1ðz; tÞ5U1 est sin

z

λ

0@1A

~u2ðz; tÞ5U2 est sin

z

λ

0@1A

~ωcðz; tÞ5Ω est cosz

λ

0@1A

~pðz; tÞ5Π est cosz

λ

0@1A

~T 5Θ est cosz

λ

0@1A

ð10:50Þ

By substituting the perturbation field (Eq. (10.50)) into the governing equations

(10.49), we obtain a homogeneous algebraic system for the coefficients {U1, U2, Ω,Θ, Π}. Thus, a non-zero solution is possible only if the determinant of the linear

system vanishes. The resulting characteristic polynomial equation is of degree 8 for

the growth coefficient s. As before, if a root has a positive real part, then the corre-

sponding perturbation grows exponentially in time.

10.4.3 Numerical Example

We refer here to a deep rock layer at a 7 km depth with the following values for

the initial state of stress and thermo-mechanical parameters:

ρ5 2500 kg=m3; σn 5 200 MPa; p5 66 MPa

μ5 0:5; β5 0 ðat great depthÞτ0 5μðσn 2 pÞ5 67 MPa

Λ5 0:5 MPa=�C; ρC5 2:8 MPa=�CG5 10; 000 MPa; K5 20; 000 MPa

Gc 5 5000 MPa; R5 0:01 mm

cth 5 1 mm2=s; chy 5 10 mm2=s; αs 5 2:53 1025=�C

ð10:51Þ

With these numerical values, it is obtained that there exists a critical value for

the hardening modulus hcr5 0.015 (i.e. in the hardening regime of the stress�strain

curve) such that for h$ hcr, all of the real roots of the polynomial equation are neg-

ative. For h, hcr, positive real roots exist. It is worth mentioning that from these

numerical computations, it is found that the root with the greatest positive real part


is real (Figure 10.4). In other words, the instability mode with the fastest growth

coefficient is not a so-called flutter instability.

For a given value of the hardening modulus h, hcr, it is possible to plot the

greatest root (i.e. corresponding to the instability mode with the fastest growth in

time) as a function of the wavelength λ. This curve exhibits a maximum for

λ5λm so that a wavelength with the fastest growth in time appears (Figure 10.4).

In Figure 10.5, the selected wavelength is plotted versus the hardening modulus.

We observe that the selected wavelength tends to infinity for h ! h2cr: This selectedwavelength decreases with decreasing hardening modulus and reaches a minimum

(for h5 0.007, λm5 186.7) and then increases again and tends to infinity for h!0

(maximum shear stress). Muhlhaus and Vardoulakis [31] similarly obtained that at

bifurcation state, the shear-band thickness for dry granular materials is infinite and

decreases beyond the bifurcation state as the strain localization process evolves.

With R5 10 μm, which is an average grain size for a highly finely granulated

(ultra-cataclastic) fault core, the obtained minimum selected wavelength is about

2 mm, which is compatible with field observations of localized shear zones in

broader damaged fault zones.

0.0000

100

200

300

400

500

600

0.002 0.004 0.006 0.008

h

λ

0.010 0.012 0.014

Figure 10.5 Wavelength

selection.

Source: After Ref. [33].

Real part of polynomial roots for h = 0.0148

0.1

0.0

–0.1

Re(

s)

λ

–0.2

–0.30 200 400 600 800 1000 1200 1400

Figure 10.4 Real part of the

roots of the characteristic

equation (growth coefficient)

for h, hcr. The red, dashed

curves represent the real part

of the roots that are complex

(non-zero imaginary part),

while the thick, black curves

depict the real roots (zero

imaginary part). (For

interpretation of the references

to color in this figure legend,

the reader is referred to the

web version of this book.)

Source: After Ref. [33].


It is important to emphasize that the wavelength selection is not obtained if

Cosserat microstructure is not considered in the analysis. The critical hardening

modulus for instability is unchanged (hcr5 0.015), but the growth coefficient tends

to infinity for the infinitely small wavelength limit, which indicates that the con-

sidered problem is mathematically ill-posed. Moreover, it should be mentioned

that even if a Cosserat microstructure is considered, the mathematical problem

remains ill-posed without the inertia terms. The main point is that the inertia

terms remedy the ill-posedness of the mathematical problem, resulting in a finite

growth coefficient for the instability.

10.5 Effect of Chemical Couplings During RapidFault Shearing

In the preceding analysis, we have emphasized the role of shear heating and

fluid pressurization. The underlying assumption was that no fluid is produced

or consumed during seismic slip. There is, however, growing evidence that

temperature-induced decomposition of minerals may be a significant source of

fluids in faulted rocks, which may enhance the generation of pore-pressure excess.

This production of fluid is in competition with the change of porosity induced

by the reduction of solid volume during mineral decomposition. Obviously, the

competing effects of temperature rise (due to shear heating), thermal fluid pressuri-

zation, mineral decomposition and porosity/permeability increase induce strong

non-linearities in the problem of pore pressure and temperature evolution of a rap-

idly sheared fault zone. The kinetics of the chemical reaction of mineral decompo-

sition is also a major factor that competes with heat- and fluid-diffusion processes.

The endothermic character of the mineral decomposition reactions also plays a role

in the energy balance of the system. Therefore, the effect of thermal mineral

decomposition brings a very interesting chemical coupling to the problem under

consideration.

As an example, in this section, we will focus on the kinetics of chemical decom-

position of calcite (decarbonation) CaCO3!CaO1CO2, which is triggered when

the temperature reaches about 700�C. Carbonates are present in every fault zone

from the ductile�brittle transition (B15 km) to the subsurface, and there is evi-

dence of CO2 release in several active crustal faults. In the Corinth rift (Greece),

e.g. chemical analysis of water springs near the seismogenic Heliki and Aegion

faults revealed an anomalously high content of dissolved CO2 compared with the

regional values [34]. The surface trace of the San Andreas Fault also displays a positive

anomaly of CO2 fluxes [35], and this CO2 comes from a shallow source, not from

the mantle [36]. Moreover, there is growing evidence that CO2 release coincides

with seismic slip in crustal faults, active and/or exhumed. In the vicinity of the

Nojima fault (Japan), Sato and Takahashi [37] reported that the HCO32 concentration

of springs increased by 30 wt% immediately after the 1995 Kobe earthquake. This

carbon discharge, together with other co-seismic geochemical anomalies, decreased


gradually to normal values in the following 10 months. A micro-infrared analysis of

exhumed pseudotachylites (i.e. friction-induced melts produced by seismic slip)

from the Nojima fault revealed that shear melting destroyed the carbonates within

the fault zone and released CO2, thus providing an explanation to the co-seismic

CO2 spikes in springs [38]. The quantity of CO2 released by friction melting during

the 1995 Kobe earthquake was evaluated as 1.8�3.43 103 tons. As for the San

Andreas Fault, the carbon isotopic signature of springs and fault rocks from Nojima

is consistent with a decomposition of biogenic carbonates, not from a mantle origin

[39,40]. In the Central Apennines, Italiano et al. [41] also reported enhanced fluxes

of crustal CO2 (i.e. not from the mantle) during the 1997�1998 seismic crisis of

major faults and proposed that co-seismic decarbonation was responsible for the

CO2 emission. Recent studies of the Chelungpu Fault (Taiwan) responsible for

the 1999 ChiChi earthquake also showed that the fault core was depleted in carbon

relative to the damage zone, and the depletion was attributed to decarbonation

induced by frictional heat [42,43]. In addition, recent high-velocity friction experi-

ments on Carrara marble have shown that thermal decomposition of calcite due

to frictional heating induces a pronounced fault weakening [44]. The production of

co-seismic CO2 is therefore attested by various field and experimental techniques,

thus making the thermal decomposition of carbonates an important additional

mechanism to be investigated among possible fault-weakening processes as recently

proposed by Sulem and Famin [19].

10.5.1 Modelling

The rate of emitted CO2 is evaluated using the kinetics of the chemical reaction of

calcite thermal decomposition:

CaCO3 ! CaO1CO2 ð10:52Þ

The reacted fraction, α (0#α# 1; α5 1 if the entire substance is reacted), is

expressed by the Arrhenius equation [45]:

@α@t

5 f ðαÞA exp 2Ea

RT

� �ð10:53Þ

where f(α) is a kinetic function determined by the reaction mechanism, A is a con-

stant (pre-exponential term of the Arrhenius law), Ea is the activation energy of the

reaction and R is the gas constant (8.31447 J/K/mol). For calcite decomposition,

Ea5 319,000 J/mol and A5 2.953 1015 s21 [46].

Thus, the mass of emitted CO2 (per unit volume) is expressed as

@md

@t5χρCaCO3

ð12 nÞA exp 2Ea

RT

� �ð10:54Þ


where χ is the ratio between the molar mass MCO2of CO2 (44 g/mol) and the molar

mass MCaCO3of calcite (100 g/mol) if we assume that the total amount of calcite

can be decomposed. The corresponding change of porosity due to the decomposi-

tion of the solid phase is expressed as

@nd@t

521

ρCaCO3

@mCaCO3

@t2

1

ρCaCO

@mCaO

@t5

1

ρCaCO3

MCaCO3

MCO2

21

ρCaCO

MCaO

MCO2

!@md

@t

ð10:55Þ

where ρCaCO3(resp. ρCaO) and MCaCO3

(resp. MCaO) are the density and the molar

mass of CaCO3 (resp. CaO). The heat for calcite decomposition is calculated by

EC 5ΔrH

0T

χMCaCO3

@md

@tð10:56Þ

where ΔrH0T is the enthalpy change of the reaction (i.e. the energy consumed by

the reaction), which for calcite decomposition is equal to the activation energy Ea

in the isobaric mode [19].

Thus, the coupled system of production/diffusion equations (Eqs (10.14) and

(10.19)) are modified as:

@p

@t5 chy

@2p

@z21Λ

@T

@t2

1

β�@np

@t1

12 ρfζ=ρCaCO3

β�ρf

@md

@t

@T

@t5 cth

@2T

@z21

1

ρCτ _γp 2

ð12 nÞρC

ΔrH0T

MCaCO3

ρCaCO3A exp 2

Ea

RT

0@

1A ð10:57Þ

where ζ5 MCaCO3

MCO2

2ρCaCO3ρCaCO

MCaO

MCO2

: With MCaCO35 100 g=mol; MCaO5 56 g/mol,

MCO25 44 g=mol; ρCaCO3

5 2:71 g=cm3 and ρCaO 5 3:35 g=cm3; ζ5 1.24.

10.5.2 Numerical Example

For the pore pressure and temperature range considered here for which the

decarbonation of CO2 is active (T. 700�C, Pp. 70 MPa), water and carbon

dioxide are in a supercritical state. They are miscible, and their compressibility,

viscosity, density and thermal-expansion coefficient are nearly equal. Thus, it is

assumed in the computations that the fault zone is saturated with a unique fluid

and with the thermodynamical properties of water.

The decomposition of carbonate can induce substantial change in the porosity of

the rock, which affects the permeability. It is known that there is no unique


relationship between porosity and permeability applicable to all porous media and that

the geological evolution process of the pore space influences the permeability�porosity relationship. The commonly used cubic Carman Kozeny permeability law

is assumed here to take into account the effect of porosity change due to mineral

decomposition on the permeability of the rock:

kf 5 kf012 n0

12n

� �2n

n0

� �3ð10:58Þ

where kf0 is the reference permeability corresponding to the reference porosity n0.

The assumed permeability law has a strong effect on the numerical results, and

there is a need for experimental data on permeability changes resulting from the

particular process of carbonate decomposition.

The initial porosity of the rock is taken to be equal to 0.03. The recent high-velocity

shear experiments on Carrara marble of Han et al. [44] have shown that the friction

coefficient f decreases rapidly to values as low as 0.06 due to the thermal decompo-

sition of calcite induced by frictional heating. Here, we take f5 0.1.

We assume here that the initial permeability of the intact medium is

kf5 10218 m2.

The computed results are presented in Figure 10.6. The evolution in time of the

temperature and the pore pressure in the centre of the band is plotted in

Figure 10.6A. Considering the constant slip velocity of 1 m/s, this graph can also

be seen as the evolution of temperature and pore pressure with accumulated slip.

The corresponding shear stress is plotted in Figure 10.6B. These results show the

coupling effect of heat, which induces first a pore pressure increase. When the

decomposition of the carbonate rock begins at about 700�C, the temperature

increase is drastically slowed due to the energy consumed in the endothermic

chemical reaction. Two competing effects act on the evolution of the pore pressure:

on the one hand, the production of CO2 induces an additional fluid mass and thus a

pressurization of the pore fluid; on the other hand, the increase of porosity due to

the solid decomposition induces an increase of the permeability of the medium,

which limits the pressurization. The pore pressure in the centre of the band exhibits

a maximum of about 145 MPa, which does not exceed the total normal stress acting

(180 MPa) on the band so full liquefaction is not reached. As mentioned earlier,

through the friction law, the shear stress is related to the mean effective stress

inside the band (Figure 10.6B). Consequently, the shear stress decreases rapidly

during initial pressurization and then increases again. Thus, the mineral decomposi-

tion of the rock can be seen as a mechanism of fault weakening in a first stage and

then fault re-strengthening in a second stage.

The accumulated mass per unit area of the fault plane of emitted CO2 is plotted

on Figure 10.6C. After 1 s, the temperature reaches a quasi-constant state, and the

production rate is almost constant. These results show that the mass of emitted CO2

after 2 s is about 0.018 g/cm2. The corresponding rate of emitted CO2 is about


180 t/s/km2 of the fault zone. The corresponding solid mass change is shown

through the evolution of the porosity in the centre of the shear band

(Figure 10.6D).

The temperature field around the centre of the band is shown in Figure 10.7 for

t5 2 s with the corresponding value of the porosity. These plots show that the tem-

perature increase is localized in the central zone of the band. The porosity is

affected only in zones where the temperature exceeds 700�C, which for the compu-

tation considered corresponds to a width of about 4 mm.

The effect of mineral decomposition is also shown in Figure 10.8 where the

results of the preceding computation are compared to the ones obtained without

CO2 emission. In this latter case, only thermal pressurization occurs. If no mineral

decomposition occurs, the pore pressure increase is slower, and for the parameters

considered, the maximum pore pressure is about 120 MPa. Consequently, the tem-

perature increase is much stronger, and melting of the rock can eventually occur

(the melting temperature is about 1600�C for calcite).

0 0.4 0.8 1.2 1.6 2

Time (s)

0 0.4 0.8 1.2 1.6 2

Time (s)

0 0.4 0.8 1.2 1.6 2

Time (s)

0 0.4 0.8 1.2 1.6 2

Time (s)

200

400

600

800

Tem

pera

ture

(°C

)

200

400

600

800

Tem

pera

ture

(°C

)

60

80

100

120

140

160

TPp Pp

τ

7 km depthf=0.1; kf0=10–18 m2

h=5mm

7 km depthf=0.1; kf0=10–18 m2

h=5mm

7 km depthf=0.1; kf0=10–18 m2

h=5mm

7 km depthf=0.1; kf0=10–18 m2

h=5mm

(A) (B)

(C) (D)

2

4

6

8

10

12

Shea

r st

ress

(M

Pa)

60

80

100

120

140

160

Pore pressure (MPa)

Pore pressure (MPa)

0

0.004

0.008

0.012

0.016

0.02M

ass of emitted C

O2 per unit area (g/cm

2)

Tmd

200

400

600

800T

empe

ratu

re (

°C)

0.02

0.04

0.06

0.08

0.1

Porosity

TPorosity

Figure 10.6 Fault at 7 km depth: (A) evolution of temperature and pore pressure in the

centre of the shear band, (B) evolution of the shear stress, (C) evolution of the mass of

emitted CO2 and (D) evolution of the porosity in the centre of the band.


10.5.3 Discussion

Thermal decomposition of rocks appears to be an important physical process in the

phenomenon of thermal heating and pore fluid pressurization during seismic slip.

The combined effects of frictional heating, temperature rise, endothermic mineral

decomposition, pore pressure rise, porosity and permeability increase result in

highly coupled and competing processes.

A first essential result of the preceding analysis is that the endothermic reaction

of calcite decomposition limits the co-seismic temperature increase to less than

B800�C (corresponding to the initiation of the chemical reaction) within a

0.02 0.04 0.06 0.08 0.1Porosity

0

4

8

12

16

Dis

tanc

e to

the

cent

re o

f th

e ba

nd (

mm

)

200 400 600 800Temperature (°C)

After 2 s of slipPorosityT

7 km depthf=0.1; h=5mm; kf =10–18 m2

Figure 10.7 Fault at 7 km depth: temperature

and porosity fields after 1.9 s.

0 0.4 0.8 1.2 1.6 2

Time (s)0 0.4 0.8 1.2 1.6 2

Time (s)

60

80

100

120

140

160

Pore

pre

ssur

e (M

Pa)

200

400

600

800

1000

1200

Tem

pera

ture

(°C

)

With CO2 emissionWithout CO2 emission

With CO2 emission

(A) (B)

Without CO2 emission

7 km depthf=0.1; h=5mm; kf0=10–18 m2

7 km depthf=0.1; h=5mm; kf0=10–18 m2

Figure 10.8 Fault at 7 km depth: effect of CO2 emission on the evolution of temperature

(A) and pore pressure (B) in the centre of the shear band.


carbonate shear band under rapid slip. Decarbonation is only one of the possible

thermal reactions of mineral decomposition. Phyllosilicates are common secondary

minerals in faults, and their thermal dehydration is also endothermic. Therefore, it

is likely that the reaction-induced temperature limitation obtained in our model

may apply qualitatively to most fault zones. In this case, mature faults with a long

history of slip and a large cumulated displacement are likely to be more prone to

reaction-induced temperature limitation than recent faults because of their larger

content of volatile-rich secondary minerals. This would provide another explana-

tion for the notorious absence of a positive heat flow anomaly on active crustal

faults such as San Andreas [47]: a large part of the heat produced by friction would

be consumed by endothermic reactions. Another consequence is that friction melt-

ing is hampered by endothermic calcite decomposition in carbonate fault rocks and

probably in other faults containing a sufficiently high proportion of volatile-rich

secondary minerals. This is consistent with the relative scarcity of pseudotachylytes

in mature faults.

The second essential implication of the preceding analysis is that decarbonation

is a source of CO2 that significantly increases the slip-weakening effect of thermal

pressurization. The pore fluid pressure exhibits an initial phase of increase due to

thermal pressurization, then a sudden acceleration of pore pressure generated when

solid decomposition is activated. However, the increase of permeability limits the

pore pressure so that it reaches a maximum and then decreases. The numerical

results reproduce this pore pressure pulse and the initial fault weakening followed

by a re-strengthening of the shear stress.

10.6 Conclusion

In the first part of this chapter, we have analysed the undrained adiabatic shearing

of a saturated rock layer and shown the destabilizing effect of shear heating.

Instability can occur even in the hardening regime of the underlying drained

stress�strain response if dilatant hardening cannot compensate for the thermal

pressurization of the pore fluid. This result confirms that thermal effects play a

major role in the formation and evolution of the localized zone. A remarkable

result is that if we do not take into account the effect of microstructure and micro-

inertia, the underlying mathematical problem is ill-posed, i.e. for a hardening mod-

ulus lower than the critical hardening modulus at instability, the growth coefficient

of the instability is infinite. The complete dynamic analysis for a Cosserat contin-

uum leads to a wavelength selection of the instability mode as the growth coeffi-

cient in time is maximum and finite for a particular wavelength. The selected

wavelength is compatible with observed shear-band thickness in fault zones.

In the second part of the chapter, we analysed the effect of temperature-induced

mineral decomposition as it is a major slip-weakening process. Such chemical reac-

tions induce two competing effects: a direct increase in pore pressure because they

release fluid and a limit to the temperature increase because part of the frictional


heat is absorbed in the endothermic reactions. The combined effects of frictional

heating, temperature rise, endothermic mineral decomposition, pore pressure rise,

porosity and permeability increase result in highly coupled and competing

processes.

In this chapter, we have emphasized the weakening effects of thermal pressuri-

zation and thermal decomposition of minerals. However, other important weaken-

ing mechanisms could also be included in the modelling. Flash heating and shear

weakening of frictional micro-asperity contacts is a mechanism that has been first

proposed for dry-metal friction and recently been applied to rock friction [3,48].

From the microscopic point of view, the contact between two rough surfaces is

effective on micro-asperities with an area that is much smaller than the nominal

contact area. The stresses supported by these asperities are much higher than the

macroscopic applied stresses so that the local rate of heat production and conse-

quently the local temperature rise during sliding is large and may be sufficient to

activate thermal weakening of the contacts. Other mechanisms responsible for fault

lubrication involve a number of physicochemical processes [1], such as the lubrica-

tion of the contact zone with the formation of silica gels [49] or the production of

very fine particles with nanometric size [50], and also the formation of a molten

layer along the sliding interface that also lubricates the contact zone and reduces

the friction resistance

Acknowledgements

The author wishes to recall the memory of Ioannis Vardoulakis as recognition for an inspir-

ing collaboration and a deep friendship. He gratefully acknowledges the fruitful collaboration

with N. Brantut, V. Famin, A. Schubnel, I. Stefanou and E. Veveakis. He also thanks J. Rice

for inspiring discussions.

References

1. Di Toro, G., Han, R., Hirose, T., De Paola, N., Nielsen, S., Mizoguchi, K., Ferri, F.,

Cocco, M., and Shimamoto, T. (2011). Fault lubrication during earthquakes, Nature 471,

494�498.

2. Cocco, M., Spudich, P., and Tinti, E. (2006). On the mechanical work absorbed on

faults during earthquake ruptures. In “Radiated Energy and the Physics of Faulting,” R.

Abercrombie et al. (Eds.), Geophysical Monograph Series, 170, pp. 237�254, AGU,

Washington, DC.

3. Rice, J. R. (2006). Heating and weakening of faults during earth-quake slip, Journal of

Geophysical Research 111, B05311.

4. Lachenbruch, A. H. (1980). Frictional heating, fluid pressure and the resistance to fault

motion, Journal of Geophysical Research 85, 6097�6112.

5. Mase, C. W. and Smith, L. (1985). Pore-fluid pressures and frictional heating on a fault

surface, Pure and Applied Geophysics 122, 583�607.


6. Sulem, J., Vardoulakis, I., Ouffroukh, H., and Perdikatsis, V. (2005). Thermo-poro-

mechanical properties of the Aigion fault clayey gouge � application to the analysis of

shear heating and fluid pressurization, Soils and Foundations 45(2), 97�108.

7. Sulem, J., Lazar, P., and Vardoulakis, I. (2007). Thermo-poro-mechanical properties

of clayey gouge and application to rapid fault shearing, International Journal of

Numerical and Analytical Methods in Geomechanics 31(3), 523�540.

8. Habib, P. (1967). Sur un mode de glissement des massifs rocheux, Comptes Rendus a

l’Academie des Sciences, Paris 264, 151�153.

9. Habib, P. (1976). Production of gaseous pore pressure during rock slides, Rock

Mechanics 7, 193�197.

10. Anderson, D. L. (1980). An earthquake induced heat mechanism to explain the loss of

strength of large rock and earth slides. In “Engineering for Protection from Natural

Disasters” P. Karasudhi et al. (Eds.), pp. 569�580, Wiley, New York, NY.

11. Voight, B. and Faust, C. (1982). Frictional heat and strength loss in some rapid

landslides, Geotechnique 32, 43�54.

12. Vardoulakis, I. (2002). Dynamic thermo-poro-mechanical analysis of catastrophic

landslides, Geotechnique 52(3), 157�171.

13. Goren, L. and Aharonov, E. (2007). Long runout landslides: the role of frictional

heating and hydraulic diffusivity, Geophysical Research Letters 34, L07301.

14. Veveakis, E., Vardoulakis, I., and Di Toro, G. (2007). Thermoporomechanics of

creeping landslides: the 1963 Vaiont slide, northern Italy, Journal of Geophysical

Research 112, F03026.

15. Pinyol, N. and Alonso, E. (2010). Criteria for rapid sliding. II. Thermo-hydro-mechanical

and scale effects in Vaiont case, Engineering Geology 114, 211�227.

16. Sulem, J., Vardoulakis, I., Ouffroukh, H., Boulon, M., and Hans, J. (2004).

Experimental characterization of the thermo-poro-mechanical properties of the Aegion

fault gouge, Comptes Rendus Geosciences 336(4�5), 455�466.

17. Brantut, N., Schubnel, A., Corvisier, J., and Sarout, J. (2010). Thermochemical pressurization

of faults during coseismic slip, Journal of Geophysical Research 115, B05314.

18. Brantut, N., Sulem, J., and Schubnel, A. (2011). Effect of dehydration reactions

on earthquake nucleation: stable sliding, slow transients and unstable slip, Journal of


19. Sulem, J. and Famin, V. (2009). Thermal decomposition of carbonates in fault zones:

slip-weakening and temperature-limiting effects, Journal of Geophysical Research 114,

B03309.

20. Veveakis, E., Alevizos, S., and Vardoulakis, I. (2010). Chemical reaction capping of

thermal instabilities during shear of frictional faults, Journal of Mechanics and Physics

of Solids 58, 1175�1194.

21. Rice, J. R. (1975). On the stability of dilatant hardening for saturated rock masses,

Journal of Geophysical Research 80(11), 1531�1536.

22. Ghabezloo, S. and Sulem, J. (2009). Stress dependent thermal pressurization of a fluid-

saturated rock, Rock Mechanics and Rock Engineering 42, 1�24.

23. Vardoulakis, I. (1996). Deformation of water-saturated sand. I. Uniform undrained

deformation and shear banding, Geotechnique 46(3), 441�456.

24. Vardoulakis, I. (1996). Deformation of water-saturated sand. II. Effect of pore water

flow and shear banding, Geotechnique 46(3), 457�472.

25. Rudnicki, J. W. (1984). Effects of dilatant hardening on the development of concen-

trated shear deformation in fissured rock masses, Journal of Geophysical Research 89

(B11), 9259�9270.


26. Vardoulakis, I. (1985). Stability and bifurcation of undrained, plane rectilinear deforma-

tions on water-saturated granular soils, International Journal of Numerical and

Analytical Methods in Geomechanics 9, 339�414.

27. Vardoulakis, I. (1986). Dynamic stability of undrained simple shear on water-saturated

granular soils, International Journal of Numerical and Analytical Methods in

Geomechanics 10, 177�190.

28. Mindlin, R. (1964). Micro-structure in linear elasticity, Archive for Rational Mechanics

and Analysis 16, 51�78.

29. Germain, P. (1973). La methode des puissances virtuelle en mecanique des milieux conti-

nus. Premiere partie: theorie du second gradient, Journal de Mecanique 12, 235�274.

30. Germain, P. (1973). The method of virtual power in continuum mechanics. Part 2:

Microstructure, SIAM Journal of Applied Mathematics 25, 556�575.

31. Muhlhaus, H.-B., and Vardoulakis, I. (1987). The thickness of shear bands in granular

materials, Geotechnique 37, 271�283.

32. Vardoulakis, I. and Sulem, J. (1995). Bifurcation Analysis in Geomechanics, Blackie

Academic and Professional, Glasgow.

33. Sulem, J., Stefanou, I., and Veveakis, E. (2011). Stability analysis of undrained adiabatic

shearing of a rock layer with Cosserat microstructure, Granular Matter 13, 261�268.

34. Pizzino, L., Quattrochi, F., Cinti, D., and Galli, G. (2004). Fluid geochemistry along the

Eliki and Aigion seismogenic segments (Gulf of Corinth, Greece), Comptes Rendus

Geosciences 336(4�5), 367�374.

35. Lewicki, J. L. and Brantley, S. L. (2000). CO2 degassing along the San Andreas fault,

Parkfield, California, Geophysical Research Letters 27(1), 5�8.

36. Lewicki, J. L., Evans, W. C., Hilley, G. E., Sorey, M. L., Rogie, J. D., and Brantley,

S. L. (2003). Shallow soil CO2 flow along the San Andreas and Calaveras faults,

California, Journal of Geophysical Research 108(B4), 2187.

37. Sato, T. and Takahashi, M. (1997). Geochemical changes in anomalously discharged

groundwater in Awaji Island after the 1995 Kobe earthquake, Chikyukagaku 31, 89�98.

38. Famin, V., Nakashima, S., Boullier, A.-M., Fujimoto, K., and Hirono, T. (2008).

Earthquake produce carbon dioxide in crustal faults, Earth and Planetary Science

Letters 265(3�4), 487�497.

39. Arai, T., Tsukahara, H., and Morikiyo, T. (2003). Sealing process with calcite in the

Nojima active fault zone revealed from isotope analysis of calcite, Journal of

Geography 112(6), 915�925.

40. Lin, A., Tanaka, N., Ueda, S., and Satish-Kumar, M. (2003). Repeated coseismic

infiltration of meteoric and seawater into deep fault zones: a case study of the Nojima

fault zone, Japan, Chemical Geology 202(1�2), 139�153.

41. Italiano, F., Martinelli, G., and Plescia, P. (2008). CO2 degassing over seismic areas:

the role of mechano-chemical production at the study case of central Apennines, Pure

and Applied Geophysics 165, 75�94.

42. Hirono, T., Ikehara, M., Otsuki, K., Mishima, T., Sakaguchi, M., Soh, W., Omori, M.,

Lin, W., Yeh, E., Tanikawa, W., and Wang, C. Y. (2006). Evidence of frictional

melting from disk-shaped black material, discovered within the Taiwan Chelungpu fault

system, Geophysical Research Letters 33, L19311.

43. Hirono, T., Yokohama, T., Hamada, Y., Tanikawa, W., Mishima, T., Ikehara, M.,

Famin, V., Tanimizu, M., Lin, W., Soh, W., and Song, S.-R. (2007). A chemical kinetic

approach to estimate dynamic shear stress during the 1999 Taiwan Chi-Chi earthquake,

Geophysical Research Letters 34, L19308.


44. Han, R., Shimamoto, T., Hirose, T., Ree, J.-H., and Ando, J. (2007). Ultralow friction

of carbonate faults caused by thermal decomposition, Science 316, 878�881.

45. L’vov, B. V. (2002). Mechanism and kinetics of thermal decomposition of carbonates,

Thermochimica Acta 386, 1�16.

46. Dollimore, D., Tong, P., and Alexander, K. S. (1996). The kinetic interpretation of the

decomposition of calcium carbonate by use of relationships other than the Arrhenius

equation, Thermochimica Acta 282/283, 13�27.

47. Lachenbruch, A. H., and Sass, J. H. (1980). Heat flow and energetics of the San

Andreas fault zone, Journal of Geophysical Research 85, 6185�6223.

48. Noda, H. E., Dunham, M., and Rice, J. R. (2009). Earthquake ruptures with thermal

weakening and the operation of major faults at low overall stress levels, Journal of


49. Di Toro, G., Goldsby, D. L., and Tullis, T. E. (2004). Friction falls toward zero in

quartz rock as slip velocity approaches seismic rates, Nature 427, 436�439.

50. De Paola, N., Hirose, T., Mitchell, T., Di Toro, G., Togo, T., and Shimamoto, T.

(2011). Fault lubrication and earthquake propagation in thermally unstable rocks,

Geology 39, 35�38.


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