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Exam (elaborations)

Numerical Methods for Partial Differential Equations (1st Edition, 2015) – Solutions – Mazumder

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INSTANT PDF DOWNLOAD — Complete Solutions to Exercises for Numerical Methods for Partial Differential Equations: Finite Difference and Finite Volume Methods (1st Edition, 2015) by Sandip Mazumder. Covers all 8 chapters with detailed, step-by-step worked solutions for PDE discretization, stability, convergence, and computational algorithms. Perfect for engineering, physics, and applied math students. Numerical Methods for Partial Differential Equations solutions, Sandip Mazumder PDE exercises, finite difference method solutions, finite volume method solved problems, PDE textbook solutions manual, numerical analysis step-by-step answers, computational fluid dynamics PDE solutions, applied mathematics PDE manual, engineering numerical methods solved, Mazumder PDE solutions PDF, PDE discretization exercises, computational engineering solutions manual, stability and convergence problems solved, finite volume numerical techniques guide, numerical PDEs textbook answers, partial differential equations study guide, finite element comparison exercises, applied numerical methods workbook, engineering computation solutions manual, PDE problem solving with MATLAB

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ALL 8 CHAPTERS COVERED

,© Sandip Mazumder, 2015


Solution to Exercise Problems in Chapter 1
Exercise 1.1

Classify the following partial differential equations into the three canonical types or a
combination thereof. In each case, φ is the dependent variable.

∂φ
a) + U∇φ =0 , where U is a vector (such as velocity).
∂t
∂φ
b) + U∇φ = ∇(Γ∇φ ) , where Γ is a positive real number.
∂t
∂  ∂φ ∂φ  ∂  ∂φ ∂φ 
c)  Γ1 − Γ2  + Γ1 − Γ2 = 0 , where Γ1 and Γ 2 are real numbers,
∂x  ∂x ∂y  ∂y  ∂y ∂x 
either positive or negative.
∂φ 1 ∂  ∂φ 
d) − r = 0
∂t r ∂r  ∂r 
∂ 2φ ∂φ
e) + − ∇(Γ∇φ ) = φ , where Γ is a positive real number.
∂t 2 ∂t


Solution

Part 1(a)

Since U is a vector, in Cartesian coordinates, it may be written as
U = u ˆi + v ˆj + w kˆ .
Using Eq. (B.2a) and the above equation, we obtain
 ∂φ ∂φ ˆ ∂φ ˆ  ∂φ ∂φ ∂φ
( )
U∇φ= u ˆi + v ˆj + w kˆ  ˆi +
 ∂x ∂y
j + k = u
∂z  ∂x
+v
∂y
+w
∂z
.

Therefore, the governing PDE may be written as
∂φ ∂φ ∂φ ∂φ
+u +v +w = 0.
∂t ∂x ∂y ∂z
The above equation is the three-dimensional Euler equation [cf. Eq. (1.7)]. Since it has
no second derivatives, it cannot be compared to the standard PDE form shown in Eq.
(1.1). Therefore, we differentiate it with respect to time to yield
∂ 2φ ∂ 2φ ∂ 2φ ∂ 2φ ∂u ∂φ ∂v ∂φ ∂w ∂φ
+u +v +w + + + =0.
∂t 2 ∂t ∂x ∂t ∂y ∂t ∂z ∂t ∂x ∂t ∂y ∂t ∂z
Selecting t and one of x , y or z as the other independent variable, and comparing the
above equation with Eq. (1.1), we obtain A = 1 , B = u or v or w , and C = 0 , which yields
B 2 − 4 AC =
u 2 or v 2 or w2 . Thus, the PDE is hyperbolic.

1

,© Sandip Mazumder, 2015




Part 1(b)

Following the same procedure as Part 1(a), the PDE may be written in Cartesian
coordinates as
∂φ ∂φ ∂φ ∂φ ∂  ∂φ  ∂  ∂φ  ∂  ∂φ 
+u +v +w = Γ  + Γ  + Γ 
∂t ∂x ∂y ∂z ∂x  ∂x  ∂y  ∂y  ∂z  ∂z 
.
 ∂ 2φ ∂ 2φ ∂ 2φ  ∂Γ ∂φ ∂Γ ∂φ ∂Γ ∂φ
=
Γ 2 + 2 + 2  + + +
 ∂x ∂y ∂z  ∂x ∂x ∂y ∂y ∂z ∂z
Comparison with Eq. (1.1) yields A = Γ , B = 0 , and C = Γ . Thus, B 2 − 4 AC =−4Γ 2 , and
the PDE is elliptic.

Part 1(c)

Differentiating through, the governing PDE may be written as

∂ 2φ ∂ 2φ ∂ 2φ ∂φ ∂Γ1 ∂φ ∂Γ 2 ∂φ ∂Γ1 ∂φ ∂Γ 2
Γ1 − 2Γ + Γ + − + − =
0.
∂x 2 ∂x∂y ∂y 2 ∂x ∂x ∂y ∂x ∂y ∂y ∂x ∂y
2 1




Comparison with Eq. (1.1) yields A = Γ1 , B =−2Γ 2 , and C = Γ1 . Therefore,
B 2 − 4 AC = 4Γ 22 − 4Γ12 = 4(Γ 22 − Γ12 ) . Hence, the type of PDE is dictated by the relative
magnitudes of the coefficients Γ1 and Γ 2 .

If Γ1 =Γ 2 , the PDE is parabolic.

If Γ1 > Γ 2 , the PDE is hyperbolic.

If Γ1 < Γ 2 , the PDE is elliptic.


Part 1(d)
We first rewrite the governing equation as

∂φ 1 ∂  ∂φ  ∂φ ∂ 2φ 1 ∂φ
− r = − − =0
∂t r ∂r  ∂r  ∂t ∂r 2 r ∂r

Comparison with Eq. (1.1) yields A = −1 , B = 0 , and C = 0 . Therefore, B 2 − 4 AC =
0 , and
the PDE is parabolic.



2

, © Sandip Mazumder, 2015


Part 1(e)
Expanding in Cartesian coordinates, the governing PDE may be written as

∂ 2φ ∂φ ∂  ∂φ  ∂  ∂φ  ∂  ∂φ 
+ − Γ  − Γ  − Γ  = φ.
∂t 2 ∂t ∂x  ∂x  ∂y  ∂y  ∂z  ∂z 

Differentiating through, we obtain

∂ 2φ ∂φ ∂ 2φ ∂ 2φ ∂ 2φ ∂Γ ∂φ ∂Γ ∂φ ∂Γ ∂φ
+ − Γ − Γ − Γ − − − =φ .
∂t 2 ∂t ∂x 2 ∂y 2 ∂z 2 ∂x ∂x ∂y ∂y ∂z ∂z
In this case, we have 4 independent variables. Therefore, the type of PDE will depend on
which 2 of the 4 independent variables are considered for classification purposes.
If t and one of x , y or z is considered the other independent variable, then A = 1 ,
B = 0 , and C = −Γ . Hence, B 2 − 4 AC =
4Γ . Since Γ is a positive real number, the PDE is
hyperbolic.
If t is not considered as one of the independent variables, then A = −Γ , B = 0 , and
C = −Γ . Hence, B 2 − 4 AC =−4Γ 2 , which makes the PDE is elliptic.

To summarize, the PDE is hyperbolic in time, and elliptic in space.




3

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