Application of vector integration
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Transcript of Application of vector integration
IS 2401 LINEAR ALGEBRA
AND
DIFFERENTIAL
EQUATIONS
ASSIGNMENT - 02
Contents GROUP MEMBERS .................................................................................................................................... 3
INTRODUCTION ........................................................................................................................................ 4
FUNDAMENTAL THEORIES OF VECTOR INTEGRATION ................................................................. 5
del (∇) operator ......................................................................................................................................... 5
The gradient .............................................................................................................................................. 5
Curl ........................................................................................................................................................... 6
Divergence ................................................................................................................................................ 6
Basic Vector integration theories. ............................................................................................................. 6
Theorem 1: ............................................................................................................................................ 6
Theorem 2 : ........................................................................................................................................... 6
Theorem 1.3: ......................................................................................................................................... 7
Theorem 1.4: ......................................................................................................................................... 7
Theorem 1.5: ......................................................................................................................................... 7
Application of vector integration in fluid dynamics ................................................................................... 10
To find the rate of change of the mass of a fluid flows. .......................................................................... 10
Stock theorem ......................................................................................................................................... 11
Calculate the circulation of the fluid about a closed curve. ................................................................ 11
To analyze the vorticity of the fluid body ........................................................................................... 11
Bjerknes Circulation Theorem ................................................................................................................ 13
To analysis sea breeze ......................................................................................................................... 13
Application of vector calculus in Electricity and Magnetism ..................................................................... 14
Theorem: ............................................................................................................................................. 17
GROUP MEMBERS
Name Registration number 1) Fernando W.T.V.S EG/2013/2191
2) Perera A.L.V.T.A EG/2013/2278
3) Ismail T.A EG/2013/2209
4) Kapuge A.K.V.S EG/2013/2224
5) SurendraC.K.B.B EG/2013/2318
INTRODUCTION
The objective of this report is to create a simple explanation on application of Vector
Integration. To do this we have analyzed concepts of vector calculus, fluid dynamics, and the
Navier-Stokes equation. Upon finding such useful and insightful information, this report
evolved into a study of how the Navier-Stokes equation was derived.
The Navier-Stokes equation is named after Claude-Louis Navier and George Gabriel Stokes.
This equation provides a mathematical model of the motion of a fluid. It is an important
equation in the study of fluid dynamics, and it uses many core aspects to vector calculus.
Before explaining the Navier-Stokes equation it is important to cover several aspects of
computational fluid dynamics. At the core of this is the notion of a vector field. A vector field
is defined as a mapping from each point in 2- or 3-dimensional real space to a vector. Each
such vector can be thought of as being composed of a directional unit vector and a scalar
multiplier. In the context of fluid dynamics, the value of a vector field at a point can be used
to indicate the velocity at that point. Vector fields are useful in the study of fluid dynamics,
since they make it possible to discern the approximated path of a fluid at any given point.
FUNDAMENTAL THEORIES OF VECTOR INTEGRATION
del (∇) operator
Del is defined as the partial derivatives of a vector. Letting i, k, and j denote the unit vectors
for the coordinate axes in real 3-space, the operator is defined.
∇= 𝑖𝜕
𝜕𝑥+ 𝑗
𝛿
𝛿𝑦+ 𝑘
𝜕
𝜕𝑧
Note that here it has indicated uppercase letters to denote vector fields, and lower case letters
to denote scalar fields.
The gradient
The gradient is defined as the measurement of the rate and direction of change in a scalar
field. The gradient maps a scalar field to a vector field. So, for a scalar field f,
𝑔𝑟𝑎𝑑(𝑓)=∇(𝑓)
As an example of gradient, consider the scalar field 𝑓=𝑥𝑦2+𝑧.We take the partial derivatives
with respect to x, y, and z.
𝑑/𝑑𝑥=𝑦2, 𝑑/𝑑𝑦=2𝑥 𝑑/𝑑𝑥=1
So, the gradient is:
(𝑓)=𝑦2𝑖+2𝑥𝑗+𝑘
Curl
Curl is defined as the measurement of the tendency to rotate about a point in a vector field.
The curl maps a vector field to another vector field. For vector F, we define
𝑐𝑢𝑟𝑙(𝐹)=∇ ×𝐹 .
Divergence
Divergence is models the magnitude of a source or sinks at a given point in a vector field.
Divergence maps a vector field to a scalar field. For a vector filed F,
𝑑𝑖𝑣(𝐹)=∇∙𝐹
Basic Vector integration theories.
Theorem 1:
Let γ be an oriented curve in R3 (R- Real) with initial and final points P0and p1,
respectively. Let h(x, y, z) be a scalar function. Then,
∫∇ℎ. 𝑑𝑟 = ℎ(𝑃1) − ℎ(𝑃0)𝛾
Theorem 2:
Let M be an oriented surface in R3 (R - Real) with boundary given by the closedcurve γ,
withorientation induced from that of M. Let F(x, y, z) be a vector field.Then,
∬ (∇ × 𝐹). 𝑛𝑀
𝑑𝑆 = ∮𝐹. 𝑑𝑟𝛾
Theorem 1.3:
Let E be a bounded solid region in R3(R- Real) with boundary given by theclosed surface M,
with theoutward pointing orientation. Let F(x, y, z) be a vectorfield. Then,
∭(∇. 𝐹) 𝑑𝑉 = ∯ 𝐹. 𝑛 𝑑𝑆𝑀𝐸
Theorem 1.4:
A vector field F in R3 is said to be conservative or irrational ifany of the following
equivalent conditions hold:
∇ × F = 0 At every point.
∫ 𝐹. 𝑑𝑟𝛾
Is independent of the path joining the same two endpoints.
∮ 𝐹. 𝑑𝑟 = 0𝛾
For any closed path γ.
F = ∇h For some scalar potential h.
In fact this theorem is true for vector fields defined in any region where all closedpaths can
be shrunk to a point without leaving the region.
Theorem 1.5:
A vector field F in R3 is said to be solenoidal or incompressible ifany of the following
equivalent conditions hold:
∇.F = 0 At every point.
∬ 𝐹. 𝑛 𝑑𝑆𝑀
Is independent of the surface M having the same boundary
curve.
∯ 𝐹. 𝑛 𝑑𝑆 = 0𝑀
For any closed surface M.
F = ∇ × A For some vector potential A.
Similarly, this theorem is actually true for vector fields defined in any regionwhere all closed
surfaces can be shrunk to a point without leaving the region. The above two theorems should
look very similar. Everything is shifted up byone dimension and the curl is replaced by the
divergence, but the theorems areidentical in form.
APPLICATION OF VECTOR INTEGRATION IN FLUID DYNAMICS
To find the rate of change of the mass of a fluid flows.
Since the fluids are not rigid like solid parts in the fluid body can move in different velocities
and fluid does not have the same density all over the body. We can fiend the total mass in the
fluid region by integrating the density over R.
∭ 𝜌(𝑥, 𝑦, 𝑧)𝑑𝑥𝑑𝑦𝑑𝑧𝑅
If the region R is not changing with the time (assume that R is a control volume or fixed
volume), only way that mass going to change is by the fluid entering and leaving the R
through its boundary surface M. If we let v(𝑥, 𝑦, 𝑧, 𝑡) be a time dependent vector field which
the v will give the velocity at any point we can say that the flux integral of 𝜌v over M will
give the rate of change of mass flow.
𝑑𝑚
𝑑𝑡= ∰ 𝜌𝒗 𝒏𝑑𝑆
𝑀
So we can see the vector integration is used to fiend the rate of change of the mass of a fluid
flow.
Stock theorem
Calculate the circulation of the fluid about a closed curve.
Stock theorem is used in this. The application is circulation of the fluid about a closed curve
γ. This is just the line integral of v over γ, which we can rewrite for any surface m which has
γboundary.
∬ ∇ × 𝒗𝑀
𝒏𝑑𝑆
To analyze the vorticity of the fluid body
As the Wikipedia says vorticity is a pseudo vector field that describes the local spinning
motion of a fluid near some point (the tendency of something to rotate), as would be seen by
an observer located at that point and traveling along with the fluid in fluid dynamics.
In hear the Stoke’s theorem is used in calculation. It states that the circulation about any
closed loop is equal to the integral of the normal component of velocity over the area
enclosed by the contour.
∮ 𝒗. 𝑑𝑙 = ∬(∇ × 𝒗)𝐴
. 𝒏𝑑𝐴
Bjerknes Circulation Theorem
To analysis sea breeze
In fluid dynamics, circulation is the line integral around a closed curve of the velocity field. It
is obtain by taking the line integral of Newton’s second law for a closed chain of fluid partial.
It is known as the Bjerknes Circulation Theorem.
∫(𝑑𝑣
𝑑𝑡= −2Ω × 𝒗 −
1
𝜌∇𝑝 × 𝒈 × 𝑭)𝑑𝑙
This theorem use vector integration. This theorem is used in analyzing the bartropic fluids.
The definition of the baratropic fluids is that they are useful model for fluid behavior in a
wide variety of scientific fields, from meteorology to astrophysics. Most liquids have a
density which varies weakly with pressure or temperature, which is the density of a liquid, is
nearly constant, so to first approximation liquids are barotropic.
The sea breeze analysis can be explain using the barotropic flow
Figure: Sea breeze illustration
The sea breeze will develop in which lighter fluid the warm land air is made to rise and
heavier fluid sea air is made to sink. So the air from see will come to land to fill the free place
this occurs sea breeze.
APPLICATION OF VECTOR CALCULUS IN ELECTRICITY AND
MAGNETISM
In this discussion we will discuss the mathematical consequences of theorems.Let us take
Electric and Magnetic field in space as E(x,y,z,t) and B(x,y,z,t) where (x,y,z) represents the
position in space and t represents the time. Further let ρ(x,y,z,t) be charge density and
J(x,y,z,t) the current density in space. Current density is a vector field since current is given
by both magnitude and direction.
The equations governing Electricity and Magnetism are;
∇ · E =𝜌
∈0 Gauss, law
∇ × E = −𝜕𝐁
𝜕𝑡 Faraday’s law
∇・B = 0
∇ × B = μ0J + μ0ϵ0𝜕𝐸
∂t Ampere-Maxwell Law
Where; ϵ0 = 8.85×10−12𝑐2
𝑁𝑚2is the permittivity of free space andμ0 = 4π×10−7
𝑁𝑠2
𝐶2 is the
permeability of free space.
Magnetic field B is always solenoidal, and can be written as the curl of a vector potential B =
∇×A. Thus we can show that magnetic flux through any closed surface is always zero by use
of following theorem.
Figure: Electricity and Magnetic field
Theorem:
A vector field F in 3 dimensional spaceis said to be solenoidal or incompressible if any of the
following equivalent conditions are true:
∇・F = 0 at every point
∬ 𝐅・𝐧𝑑𝑆𝑀
is independent of the surface M having the same boundary curve
∯ 𝐅・𝐧𝑑𝑆𝑀
= 0 for any closed surface M
F = ∇ × A for some vector potential A
Since the divergence of any curl is zero, we can write using Maxwell’s equation;
∇・ (∇ × E) = ∇・ (−∂𝐁
∂t) = −
∂
∂t(∇ ・𝐁) = 0
For the magnetic field we get;
∇・ (∇ × B) = ∇・ (μ0J + μ0ϵ0𝜕𝑬
∂t)
∇・ (∇ × B) = μ0∇・J + μ0ϵ0𝜕
∂t (∇・E)
∇・ (∇ × B) = μ0 (∇・J+∂ρ
∂t)
For the consistency of divergence of curl to be zero it is required that∇・J+∂ρ
∂tto be zero.
This is ideally the conservation of charge.
Now let us consider constant electric E and magnetic B fields. Then the two time derivatives
get drop out of Maxwell’s equation. In this case the curl of electric field is zero. Thus we can
write E = −∇ϕ. Where ϕ is some scalar potential function ϕ(x,y,z). The minus sign is used for
the easiness thus; we can represent the flow of positive charge from higher potential point to
lower potential. In this constant field, over a closed path the cyclic integral evaluates to zero.
Now we have;
∇・E = −∇・∇ ϕ = −∇2 ϕ =ρ
ϵ0
When the object is highly symmetric we can use Gauss’s Law and Ampere’s Law to calculate
electric and magnetic fields. Consider a uniformly charged solid sphere of radius R. since
there is no any preferred direction from symmetry we can say that electric charge outside the
sphere is radially directed which only depend on the radius r from the origin. So E· n = E(r)
because the electric field is parallel to the normal vector. Now we can integrate both side of
Gauss’s Law over a solid sphere Br of some constant radius
r > R and use the divergence theorem:
∭ (∇ ∙ 𝐄)𝑑𝑉𝐵𝑟
= ∭𝜌
ϵ0𝐵𝑟
𝑑𝑉 = 𝑄
ϵ0
∯ 𝐄 ∙ 𝐧𝑑𝑆 = 𝑀
∯ 𝐸(𝑟)𝑑𝑆 = 4𝜋𝑟2𝐸(𝑟)𝑀
Where, Q is the total charge of the sphere.
E(r) is a constant on the sphere of radius r since ρ is constant in the charged sphere and zero
outside it
We can do an analogous calculation for magnetic fields. Suppose we have an infinitely long
thick wire (an infinitely long cylinder) of some radius R. Current is flowing through this
cylinder with some uniform current density J. Now because the force on a moving charge due
to a magnetic field is perpendicular to both the direction of motion of the charge and the
direction of the field, symmetry tells us that the magnetic field due to this infinite wire must
be tangential to circles perpendicular to and centered on the wire. That is, if we point the
thumb of our right hand in the direction of the current, the field lines go around the wire in
the direction of our fingers. By symmetry, the magnitude of the magnetic field depends only
on the perpendicular distance r from the wire. Now we integrate both side of Ampere’s Law
over a solid disc Dr of some constant radius r > R and use Stokes’
Theorem:
∬ (∇ × 𝑩)𝑑𝑠 =𝐷𝑟
∬ μ0𝐉ds𝐷𝑟
=μ0𝑰
∮ 𝑩𝑑𝑥𝑟
= ∮ 𝐵(𝑟)𝑑𝑟 = 2𝜋𝑟
rB(r)
WhereIis the total current through the wire, since J is constant in the wire and zerooutside it,
and B(r) is a constant on the circle of radius r. Thus we see
B(r) = μ0I/2𝜋𝑟
Which is the same at the magnetic field due to an infinitely thin wire with current I Inside the
wire the field is slightly more complicated. As a final illustration of the use of vector calculus
to study electromagnetic theory, let us consider the case where the fields are time varying, but
we are in free space where the charge and current densities are both zero. We will need to
make use of the following identity for a vector field F, which can be easily proved by writing
down the definitions and checking each component:
∇ × (∇ × 𝐅) = ∇(∇ × 𝐅) − ∇2𝑭
We apply this identity to both the electric and magnetic fields, and use all of Maxwell’s
equations to simplify the results, remembering that both ρ and J are assumed to be zero:
∇ × (∇ × 𝐄) = ∇(∇. 𝐄) − ∇2𝑬 = −∇2𝑬
= ∇ (−𝜕𝑩
𝜕𝑡) = −
𝜕
𝜕𝑡(∇ × 𝑩) = −𝜇° ∈°
𝜕2𝑬
𝜕𝑡2
and similarly:
∇ × (∇ × 𝐁) = ∇(∇. 𝐁) − ∇2𝑩 = −∇2𝑩
= ∇ (𝜇° ∈°𝜕𝑬
𝜕𝑡) = 𝜇° ∈°
𝜕
𝜕𝑡(∇ × 𝑬) = −𝜇° ∈°
𝜕2𝑩
𝜕𝑡2
Thus we see that each of the three components of both the electric and magneticfields satisfy
the differential equation
𝜕2𝑓
𝜕𝑡2= 𝐶2∇2𝑓
Figure: Electric field and Magnetic field
Forc = 1
√(𝜇°∈°)
This equation represents the motion of a wave with speed c. Hence we see that in free space
the electric and magnetic fields propagate as waves with speed
1
√(𝜇°∈°)=
1
√(4𝜋×10−7𝑁82)(8.85×10−12 𝑐2
𝑁𝑚2)
= 2.99863 × 108 𝑚
𝑠
Figure: Gauss Figure: Faraday Figure: Maxwell Figure: Stokes
This is exactly the speed of light. Maxwell studied on electromagnetic waves and was able to
deduce that light is an electromagnetic wave upon the experimental information of speed of
light back in 1880.Allelectromagnetic waves: gamma rays, X-rays, ultraviolet rays, light,
infrared rays, microwaves, radio waves; are propagating electric and magnetic fields. The
only difference is the frequency from wave to wave is different. They All travel at the same
velocity. The energy of the wave is proportional to the frequency, which is why X-rays are
far more harmful to us than radio waves.
REFERENCE
http://en.wikipedia.org/wiki/Stokes'_theorem
http://wxmaps.org/jianlu/Lecture_6.pdf
http://www.math.ubc.ca/~cass/courses/m266-99a/ch8.pdf
http://www.cs.umd.edu/~mount/Indep/Steven_Dobek/dobek-stable-fluid-final-2012.pdf