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Thermodynamic Phase Transitions

and Shock Singularities

Giuseppe De Nittis

Joint work with: Antonio Moro

Proc. R. Soc. A (online) arXiv:1107.0394

(2)

Outline

1 Introduction to shock waves

2 Thermodynamic phase transitions vs Shocks

3 Equations of State

4 Singular Sector

(3)

Nonlinear Shock Waves: the simplest model

Burgers - Hopf equation

ut +uux =0 u=u(x,t)

The general solutionuis given (locally) by the following algebraic equation

x =ut+f(u) (Hodograph Equation)

(4)

Nonlinear Shock Waves: the simplest model

Burgers - Hopf equation

ut +uux =0 u=u(x,t)

The general solutionuis given (locally) by the following algebraic equation

x =ut+f(u) (Hodograph Equation)

(5)

Shocks

Burgers-Hopf equation+initial datum

ut +uux =0 u(x,0) =F(x)

t=0

-4 -2 0 2 4 0.0 0.2 0.4 0.6 0.8 1.0 1.2

tc

-2 0 2 4 6

0.0 0.2 0.4 0.6 0.8 1.0 1.2

t>tc

-2 0 2 4 6

0.0 0.2 0.4 0.6 0.8 1.0 1.2

t>tc

-2 0 2 4 6

(6)

Shocks

Burgers-Hopf equation+initial datum

ut +uux =0 u(x,0) =F(x)

t=0

-4 -2 0 2 4 0.0 0.2 0.4 0.6 0.8 1.0 1.2

tc

-2 0 2 4 6

0.0 0.2 0.4 0.6 0.8 1.0 1.2

t>tc

-2 0 2 4 6

0.0 0.2 0.4 0.6 0.8 1.0 1.2

t>tc

-2 0 2 4 6

(7)

Shocks

Burgers-Hopf equation+initial datum

ut +uux =0 u(x,0) =F(x)

t=0

-4 -2 0 2 4 0.0 0.2 0.4 0.6 0.8 1.0 1.2

tc

-2 0 2 4 6

0.0 0.2 0.4 0.6 0.8 1.0 1.2

t>tc

-2 0 2 4 6

0.0 0.2 0.4 0.6 0.8 1.0 1.2

t>tc

-2 0 2 4 6

(8)

Shocks

Burgers-Hopf equation+initial datum

ut +uux =0 u(x,0) =F(x)

t=0

-4 -2 0 2 4 0.0 0.2 0.4 0.6 0.8 1.0 1.2

tc

-2 0 2 4 6

0.0 0.2 0.4 0.6 0.8 1.0 1.2

t>tc

-2 0 2 4 6

0.0 0.2 0.4 0.6 0.8 1.0 1.2

t>tc

-2 0 2 4 6

(9)

Shocks

Burgers-Hopf equation+initial datum

ut +uux =0 u(x,0) =F(x)

t=0

-4 -2 0 2 4 0.0 0.2 0.4 0.6 0.8 1.0 1.2

tc

-2 0 2 4 6

0.0 0.2 0.4 0.6 0.8 1.0 1.2

t>tc

-2 0 2 4 6

0.0 0.2 0.4 0.6 0.8 1.0 1.2

t>tc

-2 0 2 4 6

(10)

Critical point

Thecritical point(xc,tc,uc), where thegradient catastropheoccurs is

determined by the following system

xc−uctc−f(uc) =0 tc+f0(uc) =0 f00(uc) =0.

wheref000(uc)<0.

Proof (easy!):Let us define

Ω(x,t,u(x,t)) :=x−ut−f(u) =0.

ComputingΩx =0 we obtain

ux =

1 t+f0(u).

At the gradient catastrophe pointux =∞i.e.

t+f0(u) =0

The solution displays the critical behaviour at theminimum time, such that

(11)

Critical point

Thecritical point(xc,tc,uc), where thegradient catastropheoccurs is

determined by the following system

xc−uctc−f(uc) =0 tc+f0(uc) =0 f00(uc) =0.

wheref000(uc)<0.

Proof (easy!):

Let us define

Ω(x,t,u(x,t)) :=x−ut−f(u) =0.

ComputingΩx =0 we obtain

ux =

1 t+f0(u).

At the gradient catastrophe pointux =∞i.e.

t+f0(u) =0

The solution displays the critical behaviour at theminimum time, such that

(12)

Critical point

Thecritical point(xc,tc,uc), where thegradient catastropheoccurs is

determined by the following system

xc−uctc−f(uc) =0 tc+f0(uc) =0 f00(uc) =0.

wheref000(uc)<0.

Proof (easy!):Let us define

Ω(x,t,u(x,t)) :=x−ut−f(u) =0.

ComputingΩx =0 we obtain

ux =

1 t+f0(u).

At the gradient catastrophe pointux =∞i.e.

t+f0(u) =0

The solution displays the critical behaviour at theminimum time, such that

(13)

Weak solutions

t>tc

-2 0 2 4 6

0.0 0.2 0.4 0.6 0.8 1.0

A measurable functionu :R×[0,T]→Ris aweak solutionto the

Burgers-Hopf equation ifu defines a continuous map

[0,T]3t 7−→u(·,t)∈L1loc(R)

such that

Z Z

(uφt +

u2

2 φx)dx dt =0

(14)

Weak solutions

t>tc

-2 0 2 4 6

0.0 0.2 0.4 0.6 0.8 1.0

A measurable functionu :R×[0,T]→Ris aweak solutionto the

Burgers-Hopf equation ifu defines a continuous map

[0,T]3t 7−→u(·,t)∈L1loc(R)

such that

Z Z

(uφt +

u2

2 φx)dx dt =0

(15)

Shock Fitting

In most of the cases a physical solution exists in a weak sense and one should allow discontinuous solutions.

Shock position

Equal Area Principle

Shock speed

Ushock =

u2

r

2 −

u2

l

2

ur −ul

= ul+ur

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Shock Fitting

In most of the cases a physical solution exists in a weak sense and one should allow discontinuous solutions.

Shock position

Equal Area Principle

Shock speed

Ushock =

u2

r

2 −

u2

l

2

ur −ul

= ul+ur

(17)

Shock Fitting

In most of the cases a physical solution exists in a weak sense and one should allow discontinuous solutions.

Shock position

Equal Area Principle

Shock speed

Ushock =

u2

r

2 −

u2

l

2

ur −ul

= ul+ur

(18)

Isothermal Curves vs Nonlinear Waves

A B

T<Tc

V P

T1>T2 T2>T3 T3

V P

Van der Waals gas Ideal Gas

T>Tc T=Tc

T<Tc

P V

(19)

Isothermal Curves vs Nonlinear Waves

A B

T<Tc

V P

T1>T2 T2>T3 T3

V P

Van der Waals gas Ideal Gas

T>Tc T=Tc

T<Tc

P V

(20)

Isothermal Curves vs Nonlinear Waves

A B

T<Tc

V P

T1>T2 T2>T3 T3

V P

Van der Waals gas Ideal Gas

T>Tc T=Tc

T<Tc

P V

(21)

Energy Balance Equation

dE =TdS−PdV +

m

X

j=1 Λjdτj

Introducing the Gibbs free energyΦ =E−TS+VP

dΦ =−SdT +VdP+

m

X

i=1 Λidτi

that is

S =−∂Φ

∂T, V =

∂Φ

∂P, Λi = ∂Φ

∂τi

i=1, . . . ,m

This system of equations is compatible if

∂V ∂T =−

∂S ∂P,

∂V ∂τi

= ∂Λi

(22)

Energy Balance Equation

dE =TdS−PdV +

m

X

j=1 Λjdτj

Introducing the Gibbs free energyΦ =E−TS+VP

dΦ =−SdT +VdP+

m

X

i=1 Λidτi

that is

S =−∂Φ

∂T, V =

∂Φ

∂P, Λi = ∂Φ

∂τi

i=1, . . . ,m

This system of equations is compatible if

∂V ∂T =−

∂S ∂P,

∂V ∂τi

= ∂Λi

(23)

Let us assume that the entropy functionSis of the form

S(T,P, τ1, . . . , τm) = ˜S V(T,P, τ1, . . . , τm),T, τ1, . . . , τm

Λi(T,P, τ1, . . . , τm) = ˜Λi V(T,P, τ1, . . . , τm),T, τ1, . . . , τm

Then, the system above can be written as follows

∂V

∂P = φ0(V,T, τ1, . . . , τm) ∂V ∂T ∂V

∂τi

= φi(V,T, τ1, . . . , τm)

∂V

∂T i =1, . . . ,m.

where

φ0(V,T, τ1, . . . , τm) :=−

∂S˜ ∂V

!−1

φi(V,T, τ1, . . . , τm) :=φ0(V,T, τ1, . . . , τm)

∂Λ˜i

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Let us assume that the entropy functionSis of the form

S(T,P, τ1, . . . , τm) = ˜S V(T,P, τ1, . . . , τm),T, τ1, . . . , τm

Λi(T,P, τ1, . . . , τm) = ˜Λi V(T,P, τ1, . . . , τm),T, τ1, . . . , τm

Then, the system above can be written as follows

∂V

∂P = φ0(V,T, τ1, . . . , τm) ∂V ∂T ∂V

∂τi

= φi(V,T, τ1, . . . , τm)

∂V

∂T i =1, . . . ,m.

where

φ0(V,T, τ1, . . . , τm) :=−

∂S˜ ∂V

!−1

φi(V,T, τ1, . . . , τm) :=φ0(V,T, τ1, . . . , τm)

∂Λ˜i

(25)

Under the extra assumptions

˜

S(V,T, τ1, . . . , τm) =σ0(V) +ψ0(T, τ1, . . . , τm),

Λi(V,T, τ1, . . . , τm) =σi(V) +ψi(T, τ1, . . . , τm)

the system takes the so-called hydrodynamic form

∂V

∂P = φ0(V) ∂V ∂T ∂V

∂τi

= φi(V)

∂V

∂T i=1, . . . ,m

The characteristic speedsφ0, . . . , φmdepend on the variableV only!

Remark :

(26)

Under the extra assumptions

˜

S(V,T, τ1, . . . , τm) =σ0(V) +ψ0(T, τ1, . . . , τm),

Λi(V,T, τ1, . . . , τm) =σi(V) +ψi(T, τ1, . . . , τm)

the system takes the so-called hydrodynamic form

∂V

∂P = φ0(V) ∂V ∂T ∂V

∂τi

= φi(V)

∂V

∂T i=1, . . . ,m

The characteristic speedsφ0, . . . , φmdepend on the variableV only!

Remark :

(27)

Equations of State

The general solution is locally given by the formula

T+φ0(V)P+

m

X

i=1

φi(V)τi =f(V) (Hodograph Equation)

Example 1 : Cauchy problem

Givenφ0js and the “initial datum”V0(P) :=V(T0,P, τ0,1, . . . , τ0,m)

f(V) =T0+φ0(V)P0(V) +

m

X

i=1

φi(V)τ0,i,

(28)

Equations of State

The general solution is locally given by the formula

T+φ0(V)P+

m

X

i=1

φi(V)τi =f(V) (Hodograph Equation)

Example 1 : Cauchy problem

Givenφ0js and the “initial datum”V0(P) :=V(T0,P, τ0,1, . . . , τ0,m)

f(V) =T0+φ0(V)P0(V) +

m

X

i=1

φi(V)τ0,i,

(29)

Example 2 : allφj(V)’s and f(V)unknown

Givenm+2 distinct isotherms

Vi(P) :=V(Ti,P, τi1, . . . , τim)

compute the set of inverse functionsP0=V0−1, . . . ,Pm=V

−1

m . Then

T0+φ0(V)P0(V) +

m

X

i=1

φi(V)τ0i =f(V)

T1+φ0(V)P1(V) +

m

X

i=1

φi(V)τ1i =f(V)

. . .

Tm+1+φ0(V)Pm(V) + m

X

i=1

φi(V)τmi =f(V)

(30)

Ideal Gas

Let us consider a monoatomic gas of constant number of particlesN and equation of state

T +φ0(V)P =f(V).

Assume we are given two particular isobaric curvesV1(T) =V(T,P1)

andV2(T) =V(T,P2)withP16=P2of the form

V1(T) =

T c1

, V2(T) =

T c2

, c1, c2 are consts

We get

φ0(V) =−

V

α f(V) =0, α=const

Then, we obtain thestate equation for the ideal gas

PV =αT (α=nR).

(31)

Ideal Gas

Let us consider a monoatomic gas of constant number of particlesN and equation of state

T +φ0(V)P =f(V).

Assume we are given two particular isobaric curvesV1(T) =V(T,P1)

andV2(T) =V(T,P2)withP16=P2of the form

V1(T) =

T c1

, V2(T) =

T c2

, c1, c2 are consts

We get

φ0(V) =−

V

α f(V) =0, α=const Then, we obtain thestate equation for the ideal gas

PV =αT (α=nR).

(32)

Real Gas (Virial Expansion)

Assumeτ’s=0 and consider two isotherms (j=1,2) atT16=T2

Pj(V) =

1 V −ν

k

X

n=0

αn(Tj)

Vn , ⇒ αn(Tj) =γnTj+cn

Then thesate equationisT +φ0(V)P =f(V)with

φ0(V) = (ν−V)

k

X

n=0

γn

Vn

!−1

, f(V) =−

Pk

n=0cnVk−n Pk

n=0γnVk−n

.

Particular case: (k=2)

P+n 2a

V2

(V −nb) =nRT (Van der Waals Equation).

This is a particular solution to the equation

∂V ∂P +

V −nb nR

∂V

(33)

Real Gas (Virial Expansion)

Assumeτ’s=0 and consider two isotherms (j=1,2) atT16=T2

Pj(V) =

1 V −ν

k

X

n=0

αn(Tj)

Vn , ⇒ αn(Tj) =γnTj+cn

Then thesate equationisT +φ0(V)P=f(V)with

φ0(V) = (ν−V)

k

X

n=0

γn

Vn

!−1

, f(V) =−

Pk

n=0cnVk−n Pk

n=0γnVk−n

.

Particular case: (k=2)

P+n 2a

V2

(V −nb) =nRT (Van der Waals Equation).

This is a particular solution to the equation

∂V ∂P +

V −nb nR

∂V

(34)

Real Gas (Virial Expansion)

Assumeτ’s=0 and consider two isotherms (j=1,2) atT16=T2

Pj(V) =

1 V −ν

k

X

n=0

αn(Tj)

Vn , ⇒ αn(Tj) =γnTj+cn

Then thesate equationisT +φ0(V)P=f(V)with

φ0(V) = (ν−V)

k

X

n=0

γn

Vn

!−1

, f(V) =−

Pk

n=0cnVk−n Pk

n=0γnVk−n

.

Particular case: (k=2)

P+n 2a

V2

(V−nb) =nRT (Van der Waals Equation).

This is a particular solution to the equation

∂V ∂P +

V −nb nR

∂V

(35)

Singular Sector and Phase Transitions

Let us introduce the function

Ω(V,T,P, τ1, . . . , τm) :=T +φ0(V)P+

m

X

i=1

φi(V)τi−f(V)

and denoteΩ(l)=∂lΩ/∂Vl.

Following Kodama-Konopelchenko (2002), let us introduce thesingular

sectorof codimensions≤m+2

Zs =

 

(T,P, τ1, . . . , τm)∈Rm+2 | V ∈ Uj such that s = m+2 X

j=1

j |Uj|

 

Uj :=nV >0|Ω(l)=0 ∀0≤l≤j and Ω(j+1)6=0o.

(36)

Singular Sector and Phase Transitions

Let us introduce the function

Ω(V,T,P, τ1, . . . , τm) :=T +φ0(V)P+

m

X

i=1

φi(V)τi−f(V)

and denoteΩ(l)=∂lΩ/∂Vl.

Following Kodama-Konopelchenko (2002), let us introduce thesingular

sectorof codimensions≤m+2

Zs =

 

(T,P, τ1, . . . , τm)∈Rm+2 | V ∈ Uj such that s = m+2 X

j=1

j |Uj|

 

Uj :=nV >0|Ω(l)=0 ∀0≤l≤j and Ω(j+1)6=0o.

(37)

Singular Sector and Phase Transitions

Let us introduce the function

Ω(V,T,P, τ1, . . . , τm) :=T +φ0(V)P+

m

X

i=1

φi(V)τi−f(V)

and denoteΩ(l)=∂lΩ/∂Vl.

Following Kodama-Konopelchenko (2002), let us introduce thesingular

sectorof codimensions≤m+2

Zs =

 

(T,P, τ1, . . . , τm)∈Rm+2 | V ∈ Uj such that s = m+2 X

j=1

j |Uj|

 

Uj :=nV >0|Ω(l)=0 ∀0≤l≤j and Ω(j+1)6=0o.

(38)

Singular Sector and Phase Transitions

Let us introduce the function

Ω(V,T,P, τ1, . . . , τm) :=T +φ0(V)P+

m

X

i=1

φi(V)τi−f(V)

and denoteΩ(l)=∂lΩ/∂Vl.

Following Kodama-Konopelchenko (2002), let us introduce thesingular

sectorof codimensions≤m+2

Zs =

 

(T,P, τ1, . . . , τm)∈Rm+2 | V ∈ Uj such that s = m+2 X

j=1

j |Uj|

 

Uj :=nV >0|Ω(l)=0 ∀0≤l≤j and Ω(j+1)6=0o.

(39)

The critical sector identifies the occurrence of thephase transitionas well as theshock formationof the solution to the hydrodynamic type system.

0 10 20 30 40

0 500 000 1.0´106

1.5´106

T P

0.05 0.10 0.15 0.20 0.25

0 1´106

2´106

3´106

4´106

5´106

V P

Left:Singular sectorZ1for the hydrogen using the Van der Waals model. The

intersection of the two lines is the critical sectorZ2={Tc =33.159K,

Pc =1.29508×106Pasc}.

Right:The bold line shows the critical isotherm. Below the critical isotherm there are two stationary points where the isotherm has a local maximum and minimum. As

(40)

The critical sector identifies the occurrence of thephase transitionas well as theshock formationof the solution to the hydrodynamic type system.

0 10 20 30 40

0 500 000 1.0´106

1.5´106

T P

0.05 0.10 0.15 0.20 0.25

0 1´106

2´106

3´106

4´106

5´106

V P

Left:Singular sectorZ1for the hydrogen using the Van der Waals model. The

intersection of the two lines is the critical sectorZ2={Tc =33.159K,

Pc =1.29508×106Pasc}.

Right:The bold line shows the critical isotherm. Below the critical isotherm there are two stationary points where the isotherm has a local maximum and minimum. As

(41)

The rôle of the unfolding

Locally, near the critical point, the Van der Waals equation is associated with theuniversal unfoldingof codimension 2 of a Riemann-Hugoniot catastrophe (power 4). More precisely, the universal unfolding gives the Gibbs free energy

Φ =F +PV

whereF =E−TS.

Virial expansions (for "τ-deformed" systems) can be considered

ashigher codimension unfoldingsof the Van der Waals model.

(42)

The rôle of the unfolding

Locally, near the critical point, the Van der Waals equation is associated with theuniversal unfoldingof codimension 2 of a Riemann-Hugoniot catastrophe (power 4). More precisely, the universal unfolding gives the Gibbs free energy

Φ =F +PV

whereF =E−TS.

Virial expansions (for "τ-deformed" systems) can be considered

ashigher codimension unfoldingsof the Van der Waals model.

(43)

The rôle of the unfolding

Locally, near the critical point, the Van der Waals equation is associated with theuniversal unfoldingof codimension 2 of a Riemann-Hugoniot catastrophe (power 4). More precisely, the universal unfolding gives the Gibbs free energy

Φ =F +PV

whereF =E−TS.

Virial expansions (for "τ-deformed" systems) can be considered

ashigher codimension unfoldingsof the Van der Waals model.

(44)

Separable entropy functions

Consider a system the state of which is completely specified by the set of thermodynamic variables(T,P,V).

S(T,P) = ˜S V(T,P),T= ∞

X

j=0

σj V(T,P)

∂ρj

∂T(T)

whereσj(V)andρj(T)are arbitrary functions of their argument.

Examples:

P= nRT

V −

c

V3/2√T (Classical Plasma);

P= nRT

V

Liα+1(z)

ζ(α)

T Tc

α

(45)

Separable entropy functions

Consider a system the state of which is completely specified by the set of thermodynamic variables(T,P,V).

S(T,P) = ˜S V(T,P),T= ∞

X

j=0

σj V(T,P)

∂ρj

∂T(T)

whereσj(V)andρj(T)are arbitrary functions of their argument.

Examples:

P = nRT

V −

c

V3/2√T (Classical Plasma);

P= nRT

V

Liα+1(z)

ζ(α)

T Tc

α

(46)

Summarizing

Equations of state→solutions to nonlinear hyperbolic PDEs;

Isothermal (isobaric) curves⇐⇒nonlinear waves;

Critical point of the phase transition⇐⇒gradient catastrophe.

Further Study

Stability of higher codimensional unfoldings;

Higher component hydrodynamic systems↔Composite thermodynamic systems↔Non-additive entropy;

Higher order effects:

→Phase transition as weak diffusive limit of the Burgers type eq?

(47)

Summarizing

Equations of state→solutions to nonlinear hyperbolic PDEs;

Isothermal (isobaric) curves⇐⇒nonlinear waves;

Critical point of the phase transition⇐⇒gradient catastrophe.

Further Study

Stability of higher codimensional unfoldings;

Higher component hydrodynamic systems↔Composite thermodynamic systems↔Non-additive entropy;

Higher order effects:

→Phase transition as weak diffusive limit of the Burgers type eq?

(48)

Summarizing

Equations of state→solutions to nonlinear hyperbolic PDEs;

Isothermal (isobaric) curves⇐⇒nonlinear waves;

Critical point of the phase transition⇐⇒gradient catastrophe.

Further Study

Stability of higher codimensional unfoldings;

Higher component hydrodynamic systems↔Composite thermodynamic systems↔Non-additive entropy;

Higher order effects:

→Phase transition as weak diffusive limit of the Burgers type eq?

(49)

Summarizing

Equations of state→solutions to nonlinear hyperbolic PDEs;

Isothermal (isobaric) curves⇐⇒nonlinear waves;

Critical point of the phase transition⇐⇒gradient catastrophe.

Further Study

Stability of higher codimensional unfoldings;

Higher component hydrodynamic systems↔Composite thermodynamic systems↔Non-additive entropy;

Higher order effects:

→Phase transition as weak diffusive limit of the Burgers type eq?

(50)

Summarizing

Equations of state→solutions to nonlinear hyperbolic PDEs;

Isothermal (isobaric) curves⇐⇒nonlinear waves;

Critical point of the phase transition⇐⇒gradient catastrophe.

Further Study

Stability of higher codimensional unfoldings;

Higher component hydrodynamic systems↔Composite thermodynamic systems↔Non-additive entropy;

Higher order effects:

→Phase transition as weak diffusive limit of the Burgers type eq?

(51)

Summarizing

Equations of state→solutions to nonlinear hyperbolic PDEs;

Isothermal (isobaric) curves⇐⇒nonlinear waves;

Critical point of the phase transition⇐⇒gradient catastrophe.

Further Study

Stability of higher codimensional unfoldings;

Higher component hydrodynamic systems↔Composite thermodynamic systems↔Non-additive entropy;

Higher order effects:

→Phase transition as weak diffusive limit of the Burgers type eq?

(52)

Summarizing

Equations of state→solutions to nonlinear hyperbolic PDEs;

Isothermal (isobaric) curves⇐⇒nonlinear waves;

Critical point of the phase transition⇐⇒gradient catastrophe.

Further Study

Stability of higher codimensional unfoldings;

Higher component hydrodynamic systems↔Composite thermodynamic systems↔Non-additive entropy;

Higher order effects:

→Phase transition as weak diffusive limit of the Burgers type eq?

(53)

Summarizing

Equations of state→solutions to nonlinear hyperbolic PDEs;

Isothermal (isobaric) curves⇐⇒nonlinear waves;

Critical point of the phase transition⇐⇒gradient catastrophe.

Further Study

Stability of higher codimensional unfoldings;

Higher component hydrodynamic systems↔Composite thermodynamic systems↔Non-additive entropy;

Higher order effects:

→Phase transition as weak diffusive limit of the Burgers type eq?

(54)

! Thank you for your attention !

Ackowledgements:

Grant no. ANR-08-BLAN-0261-01;

Grant of Istituto Nazionale di Alta Matematica - GNFM, Progetti Giovani 2011;

Referencias

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