10.03.2015 Views

Assignment 5: EOSC 352

Assignment 5: EOSC 352

Assignment 5: EOSC 352

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

<strong>Assignment</strong> 5: <strong>EOSC</strong> <strong>352</strong><br />

due Friday, November 9th, 2012<br />

1. In class, we have looked at diffusion of heat away from an initially hot thin layer,<br />

using the model<br />

∫ ∞<br />

−∞<br />

∂T<br />

∂t − k ∂ 2 T<br />

= 0<br />

ρc ∂x2 for t > 0 (1a)<br />

T (x, 0) = T ∞ for x ≠ 0 (1b)<br />

−k ∂T → 0<br />

∂x<br />

as x → ∞ at all times t > 0 (1c)<br />

ρc [T (x, t) − T ∞ ] dx = E 0 for all times t > 0 (1d)<br />

We then proceeded to find a solution of the form<br />

( x<br />

)<br />

T = T ∞ + t −α θ<br />

t β<br />

simply by trying to see if such a solution could be made to work. In this question,<br />

we will see that scaling the equations (1) leads to the conclusion that the solution<br />

T must be of the form (2), with specific choices of the exponents α and β dictated<br />

by the scaling procedure.<br />

(a) Define dimensionless variables x ∗ , t ∗ and T ∗ through<br />

x ∗ = x<br />

[x] ,<br />

t∗ = t<br />

[t] ,<br />

T ∗ = T − T ∞<br />

.<br />

[T ]<br />

Substitute these into the equations (1). Find two relationships between the<br />

three scales [x], [t] and [T ] that must be satisfied in order to give the following<br />

dimensionless version of (1)<br />

∫ ∞<br />

−∞<br />

∂T ∗<br />

∂t ∗<br />

− ∂2 T ∗<br />

∂x ∗2 = 0 for t∗ > 0 (3a)<br />

T ∗ (x ∗ , 0) = 0 for x ∗ ≠ 0 (3b)<br />

− ∂T ∗<br />

∂x → 0 ∗ as x∗ → ∞ at all times t ∗ > 0 (3c)<br />

T ∗ (x ∗ , t ∗ ) dx ∗ = 1 for all times t ∗ > 0 (3d)<br />

1<br />

(2)


Is it possible to define [x], [t] and [T ] uniquely in terms of the model parameters<br />

E 0 , k, ρ and c?<br />

(b) Let γ be a positive number, and let<br />

t ∗∗ = γt ∗ , x ∗∗ = γ β x ∗ , T ∗∗ = γ −α T ∗<br />

where α and β are exponents to be determined. Substitute the new variables<br />

into (3). Show that one can find α and β such that, for any γ > 0, the system<br />

of equations (3) is transformed into<br />

∫ ∞<br />

−∞<br />

∂T ∗∗<br />

∂t − ∂2 T ∗∗<br />

∗∗ ∂x = 0 for ∗2 t∗∗ > 0 (4a)<br />

T ∗∗ (x ∗∗ , 0) = 0 for x ∗∗ ≠ 0 (4b)<br />

∂T<br />

∗∗<br />

−<br />

∂x → 0 as ∗∗ x∗∗ → ∞ at all times t ∗∗ > 0 (4c)<br />

T ∗∗ (x ∗∗ , t ∗∗ ) dx ∗∗ = 1 for all times t ∗∗ > 0 (4d)<br />

Give the relevant values of α and β.<br />

(c) It is clear that (4) is the same as (3) except that T ∗ has been replaced by T ∗∗ ,<br />

x ∗ by x ∗∗ and t ∗ by t ∗∗ . This is known as a scale invariance of the equations<br />

(3). In essence, we see that the equations stay the same if we stretch our<br />

length, time and temperature scales in a particular way. What this means is<br />

that the physics of the problem actually looks ‘the same’ at different scales,<br />

and hence the solution will also look ‘the same’. We will show that this<br />

implies a self-similar solution of the form (2). If the set of equations (3)<br />

has a unique solution, then it is clear that the dependent variable T ∗∗ must<br />

therefore depend on the independent variables x ∗∗ and t ∗∗ in the same way<br />

as the dependent variable T ∗ depends on the independent variables x ∗ and<br />

t ∗ . In other words, if T ∗ can be written as a function of x ∗ and t ∗ in the<br />

form<br />

T ∗ = f(x ∗ , t ∗ )<br />

then<br />

T ∗∗ = f(x ∗∗ , t ∗∗ )<br />

with the same function f in both equations. Use the definition of T ∗∗ , x ∗∗<br />

and t ∗∗ to show that this means that<br />

f(x ∗ , t ∗ ) = γ α f(γ β x ∗ , γt ∗ ).<br />

But γ is arbitrary, so for any given t ∗ , we can choose γ = t ∗−1 . Show that it<br />

therefore follows that<br />

( ) x<br />

T ∗ = t ∗−α ∗<br />

f<br />

t , 1 .<br />

∗β<br />

Choosing ξ ∗ = x ∗ /t ∗β , θ ∗ (ξ ∗ ) = f(ξ ∗ , 1) then leads to the similarity solution<br />

form (2).<br />

Page 2


2. In class, we derived the similarity solution<br />

to the problem (1).<br />

T (x, t) = t −1/2 C exp<br />

(<br />

− ρc<br />

4k<br />

)<br />

x 2<br />

+ T ∞<br />

t<br />

(a) Sketch the form of T (x, t) as a function of x for some fixed time t > 0.<br />

(b) Compute heat flux as a function of x for fixed t > 0. Sketch the form of heat<br />

flux as a function of x on the same graph as above.<br />

(c) Compute the divergence of heat flux as a function of x for fixed t > 0.<br />

Sketch this on the same graph as above. Where is temperature increasing,<br />

and where is it decreasing?<br />

(d) Next, take a fixed position x > 0, and (on a separate graph) sketch how<br />

T (x, t) evolves over time at that fixed position x.<br />

(e) For any fixed x > 0, temperature reaches a maximum. Compute the time at<br />

which this maximum occurs as a function of x (as well as ρ, c and k), and<br />

compute the maximum temperature reached in terms of x, ρ, c, k and C.<br />

(f) To get a full solution, we still need to relate C to E 0 . We have<br />

∫ ∞<br />

−∞<br />

ρc [T (x, t) − T ∞ ] dx = E 0 .<br />

To use this to compute C in terms of E 0 , we need to be able to compute<br />

∫ ∞<br />

−∞<br />

exp ( −x 2) dx.<br />

There is a trick to doing this: consider<br />

[∫ ∞<br />

exp ( −x 2) 2 [∫ ∞<br />

dx]<br />

= exp ( −x 2) ] [∫ ∞<br />

dx × exp ( −y 2) ]<br />

dy<br />

−∞<br />

−∞<br />

−∞<br />

=<br />

∫ ∞ ∫ ∞<br />

−∞<br />

−∞<br />

exp ( −(x 2 + y 2) dx dy<br />

But, if we define r 2 = x 2 + y 2 , this is simply the integral of exp(−r 2 ) over<br />

the entire xy-plane, which can be done in polar coordinates:<br />

∫ ∞ ∫ ∞<br />

exp ( −(x 2 + y 2) ∫ 2π<br />

[∫ ∞<br />

]<br />

dx dy = exp(−r 2 )r dr dθ.<br />

−∞<br />

−∞<br />

By evaluating the integral in polar coordinates, show that<br />

∫ ∞<br />

−∞<br />

exp ( −x 2) dx = √ π<br />

0<br />

0<br />

Page 3


(g) Suppose that E 0 represents the excess heat (beyond the amount of heat<br />

associated with the background temperature T ∞ ) contained in a dyke of<br />

narrow width d filled with hot rock (of the same density ρ and heat capacity<br />

c as the surrounding rock) at an initial temperature T 0 , find C in terms of<br />

T 0 , T ∞ and d.<br />

(h) Suppose the dyke has a width of d = 2 cm, and the initial temperature of the<br />

rock in the dyke is T 0 = 2000 K. Suppose also that the rock surrounding the<br />

dyke has ρ = 2700 kg m −3 , c = 10 3 J kg −1 K −1 and k = 2 W m −1 K −1 , and<br />

that it has a background temperature of T ∞ = 600 K. You are told that the<br />

rock surrounding the dyke is chemically altered if raised to a temperature<br />

T > 1000 K. Once the heat in the dyke has been completely conducted away,<br />

how far do you have to be away from the rock to find chemically unaltered<br />

rock?<br />

Page 4

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!