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Addis Ababa Science and
Technology University
DEPARTMENT OF MPS
APPLIED MATHEMATICS IB(MATH 1041)
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Chapter One :
VECTORS AND VECTOR SPACES
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1. Scalar and Vectors
Definitions:
• A scalar is a physical quantity that is described by its magnitude alone.
For example, temperature, mass, length, time , work done and speed are
scalars because they are completely described by a number that tells
"how much"-say a temperature of 20°C, a length of 5 cm, or a speed of 10
m/s.
• A vector is a physical quantity that is described using both magnitude and
direction.
For instance, velocity, displacement, force and Torque are some examples
of vectors.
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(2)
Definitions (Cartesian product of two sets)
• Let A and B be two non empty set, then the Cartesian products of A and B defined as
Remarks:
1. Thus we have
• The set of ordered pairs of real numbers called Cartesian coordinate plane (Real plane) .
2. A vector in
(plane) represented by a point vector
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Cont.
3. Vectors in
 Thus, the vector in
(Space) represented by a point vector
Example 1. plot the following vectors in space P(1,3,2) and Q(-1,3,-2)
Solution :4. The distance b/n P(x,y,z)
(a) from xy-plane is
(b) from yz-plane is
(c) from xz-plane is
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5. The distance b/n the point
P(x,y,z) to
(a) X-axis is
(b) Y-axis is
(c) Z-axis is
6. The distance b/n the point P(x,y,z) to
is
6. The distance b/n the point P(x,y,z) to the
origin is
Example 2: Find the distance of the point
vector P(-1,2,4) from
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7) There is a one-to-one correspondence b/n points in a plane/space to
a vector in plane/space.(i.e Every point is a vector in Rectangular
representation)
8) Vector in n-dimensional space represented in rectangular form as
or
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Geometrical Vector representation
i) Position Vector: A vector in
(space ) is positioned so its initial
point is at the origin and terminal at a point P(x,y,z).i.e V = OP
z
P
V
O
y
x
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Definitions:
1. A located vector is a vector 𝐴𝐡 defined as an arrow whose initial point is at point A
and whose terminal point is at B.
Y
b2
B(b1,b2)
)
a2
A(a1,a2)
a1
b1
X
(b1 , b2 ) ο€½ (a1  (b1 ο€­ a1 )), (a 2  (b 2 ο€­a 2 ))
𝑏1 = π‘Ž1 + 𝑏1 − π‘Ž1
ο€½ (a1 , a 2 )  (b1 ο€­ a1 ,b 2 ο€­a 2 )
ο€½ (a1 , a 2 )  [(b1 ,b 2 ) ο€­ (a1 , a 2 )]
B ο€½ A  ( B ο€­ A)
𝑏2 = π‘Ž2 + 𝑏2 − π‘Ž2
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iii) EQUAL (OR EQUIVALENT) VECTORS
Example 3: Find the located vector
and B(6,-2,4).
Solution :-
where A(4,0,-2)
 Two vectors are said to be Equal/ Equivalent iff they have
the same magnitude and direction.
Let
, then
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3. Vector addition and Scalar multiplication
Definition: For any two vectors 𝑒 = 𝑒1 , 𝑒2 π‘Žπ‘›π‘‘ 𝑣 = 𝑣1 , 𝑣2 in ℝ2 , we define their sum to
be
𝑒 + 𝑣 = 𝑒1 + 𝑣1 , 𝑒2 + 𝑣2 .
Geometrically, if we represent the two vectors 𝑒 π‘Žπ‘›π‘‘ 𝑣 by 𝐴𝐡 π‘Žπ‘›π‘‘ 𝐡𝐢
respectively, then 𝑒 + 𝑣 is represented by 𝐴𝐢 , as shown in the diagram below:
C
U+V
V
A
B
U
AB  BC ο€½ AC
a) The Triangular Law
D
C
U+V = V+U
V
V
A
B
U
b) The Parallelogram Law
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Scalar Multiple of a Vector
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Addition of vectors on the coordinate plane
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Exercise:- Let A and B be points with position vectors a and b
respectively relative to a fixed origin “o”.
a) Find
in terms of a and b.
b) If P is the mid-point of AB, then find
c) Show that
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Properties of Vector addition & Scalar Multiplication
Let 𝑒, 𝑣 and 𝑀 be vectors in ℝ2 and 𝑐 & π‘š are scalars. Then:
a) 𝑒 + 𝑣 ∈ ℝ2
b) 𝑒 + 𝑣 = 𝑣 + 𝑒
c) 𝑒 + 0 = 0 + 𝑒 = 𝑒, π‘€β„Žπ‘’π‘Ÿπ‘’ 0 = 0,0 ∈ ℝ2 .
d) There exists 𝑀 ∈ ℝ2 such that 𝑒 + 𝑀 = 0 for every 𝑒 ∈ ℝ2 .
e) 𝑒 + 𝑣 + 𝑀 = 𝑒 + 𝑣 + 𝑀
f) 𝑐 π‘š 𝑒 = π‘π‘š 𝑒
g) 𝑐 + π‘š 𝑒 = 𝑐𝑒 + π‘šπ‘’
h) 1. 𝑒 = 𝑒
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Remark: The properties described above also hold true for vectors in ℝ3 , where
0 = 0,0,0 ∈ ℝ3 , replaces the zero vector 0 in ℝ2 .
SUMS OF THREE OR MORE VECTORS
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𝑣 2 = 𝑂𝑅 2 + 𝑃𝑅 2 = (𝑂𝑄)2 + (𝑄𝑅)2 + (𝑃𝑅)2
𝑣 = 𝑣12 + 𝑣22 + 𝑣32
Similarly, for a vector 𝑣 = 𝑣1 , 𝑣2 ∈ ℝ2 , its norm is given by
𝑣 = 𝑣12 + 𝑣22
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Examples: a) If 𝑣 = −1,4,3 , then find 𝑣 .
b) If 𝑒 = 6, 𝑓𝑖𝑛𝑑 π‘₯ such that𝑒 = −1, π‘₯, 5 .
Remarks: (i) 𝑣 ≠ 0 𝑖𝑓 𝑣 ≠ 0
(ii) 𝑣 = −𝑣 .
Theorem: If 𝑐 ∈ ℝ, then 𝑐 𝑣 = 𝑐
𝑣 .
Proof: suppose that 𝑣 ∈ 𝑅 𝑛 then
𝑐𝑣 =
𝑐𝑣1 2 + 𝑐𝑣2 2 + β‹― + π‘π‘£π‘˜ 2
=
𝑐 2 [ 𝑣1 2 + 𝑣2 2 + β‹― + π‘£π‘˜ 2 ]
= 𝑐
𝑣
Definition (Unit Vector)
Any vector 𝑒 satisfying 𝑒 = 1 is called a unit vector.
Examples: The vectors 0,1 , −1,0 ,
1
,
2
−1
2
, 1,0,0 are examples of unit vectors.
N.B: 1. All unit vectors in ℝ2 are of the form cos πœƒ , sin πœƒ , π‘€β„Žπ‘’π‘Ÿπ‘’ πœƒ ∈ ℝ.
2. For any non-zero vector 𝑣 , the unit vector 𝑒 corresponding to 𝑣 in the
direction of 𝑣 can be obtained as:
𝑒=
𝑉
𝑉
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Example:- Find the unit vector in the direction of u=2i-j-2k.
Solution:-
Example l:- let u and v be parallel vectors such that u=2i-j-2k and
IIvII=12, then find v.
Solution:-
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3. For two points 𝑃 𝑒1 , 𝑒2 π‘Žπ‘›π‘‘ 𝑄 𝑣1 , 𝑣2 on the plane ℝ2 , we
calculate the distance 𝑑 Ρ, 𝑄 between the two points, as :
𝑑 Ρ, 𝑄 = Ρ𝑄 =
𝑣1 − 𝑒1 2 + 𝑣2 − 𝑒2 2 , π‘€β„Žπ‘’π‘Ÿπ‘’ Ρ𝑄 is the vector with initial
point P and terminal point Q,
Ρ𝑄 = 𝑣1 − 𝑒1 , 𝑣2 − 𝑒2 .
4. Distance between two vectors can be viewed as the length of U -V where
π‘ˆ = 𝑒1 , 𝑒2 π‘Žπ‘›π‘‘ 𝑉 = 𝑣1 , 𝑣2
.
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The Dot Product (or Scalar Product)
Definition: Suppose that 𝑒 = 𝑒1 , 𝑒2 π‘Žπ‘›π‘‘ 𝑣 = 𝑣1 , 𝑣2 are vectors in ℝ2 , and that πœƒ ∈ 0, πœ‹
represents the angle between them. We define the dot product of 𝑒 π‘Žπ‘›π‘‘ 𝑉 denoted by 𝑒 βˆ™ 𝑣
by:
𝑒 βˆ™ 𝑣 = 𝑒1 𝑣1 + 𝑒2 𝑣2
Or alternatively, we write
π‘’βˆ™π‘£ =
Thus 𝑒
𝑒
𝑣 cos πœƒ, 𝑖𝑓 𝑒 ≠ 0 & 𝑣 ≠ 0
0
𝑖𝑓 𝑒 = 0 π‘œπ‘Ÿ 𝑣 = 0
𝑣 cos πœƒ = 𝑒1 𝑣1 + 𝑒2 𝑣2 , for non – zero vector 𝑒 π‘Žπ‘›π‘‘ 𝑣 𝑖𝑛 ℝ2 .
Similarly, if 𝑒 = 𝑒1 , 𝑒2 , 𝑒3 π‘Žπ‘›π‘‘ 𝑣 = 𝑣1 , 𝑣2 , 𝑣3 are vectors in ℝ3 , we define 𝑒 βˆ™ 𝑣 as bellow:
𝑒 βˆ™ 𝑣 = 𝑒1 𝑣1 + 𝑒2 𝑣2 + 𝑒3 𝑣3
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Remark: The dot product of two vectors is a scalar quantity,
and its value is maximum when πœƒ = 0° and minimum if πœƒ = 180° π‘œπ‘Ÿ πœ‹ radians.
Example: If 𝑒 = 𝑖 − 2𝑗 + 3π‘˜ π‘Žπ‘›π‘‘ 𝑣 = 0,1,−5 , then find:
a) 𝑒 βˆ™ 𝑣
b) 𝑒 βˆ™ 𝑒
c) 𝑒 + 𝑣 βˆ™ 𝑣
Properties of the dot product
If 𝑒,𝑣,π‘Žπ‘›π‘‘ 𝑀 are vectors in the same dimension, and 𝑐 ∈ ℜ, then:
1. 𝑒 βˆ™ 𝑒 = 𝑒 2
4. 0 βˆ™ 𝑒 = 0
2. 𝑒 βˆ™ 𝑣 = 𝑣 βˆ™ 𝑒
5. 𝑐 𝑒 βˆ™ 𝑣 = 𝑐 𝑒 βˆ™ 𝑣 = 𝑣 βˆ™ 𝑐 𝑒
3. 𝑒 βˆ™ 𝑣 + 𝑀 = 𝑒 βˆ™ 𝑣 + 𝑒 βˆ™ 𝑀
6. 𝑒 βˆ™ 𝑒 ≥ 0 π‘Žπ‘›π‘‘ 𝑒 βˆ™ 𝑒 = 0 𝑖𝑓𝑓 𝑒 = 0.
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Angle between two vectors
If πœƒ is the angle between two non – zero vectors 𝑒 π‘Žπ‘›π‘‘ 𝑣 , then,
the angle between the two vectors can be obtained by:
𝑒 βˆ™π‘£
cos πœƒ = 𝑒
⇒ πœƒ = π‘π‘œπ‘  −1
𝑣
𝑒 βˆ™π‘£
𝑒
𝑣
, π‘Žπ‘›π‘‘ πœƒ ∈ 0, πœ‹ .
Example: Find the angle between the vectors 𝑒 = 1,0, −1 π‘Žπ‘›π‘‘ 𝑣 = 1,1,0 .
Solution: Let πœƒ be the angle between the two vectors:
𝑒 βˆ™π‘£
Then cos πœƒ = 𝑒
𝑣
=
1
1
−1 1
= 2 ⇒ πœƒ = π‘π‘œπ‘ 
2βˆ™ 2
2
πœ‹
=3
Definition: Two non – zero 𝑒 π‘Žπ‘›π‘‘ 𝑣 are said to be orthogonal
πœ‹
(perpendicular) iff 𝑒 βˆ™ 𝑣 = 0, i.e, if πœƒ = .
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Example: Find the value (s) of x such that the vectors 𝐴 = 1 ,4, 3 π‘Žπ‘›π‘‘
Β = π‘₯, −1, 2 are orthogonal.
Definition: If P and Q are points in 2 or 3 spaces, the distance between P
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and Q, denoted by Ρ − 𝑄 is given by
Ρ−𝑄 =
Ρ−𝑄 . Ρ−𝑄
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Theorem: Given two vectors 𝑒 & 𝑣 in space, 𝑒 + 𝑣
=
𝑒−𝑣
iff
𝑒 π‘Žπ‘›π‘‘ 𝑣 are orthogonal vectors.
Proof : (‏) Given
WTS
2
𝑒+𝑣
2
2
𝑒−𝑣
𝑒 π‘Žπ‘›π‘‘ 𝑣 are orthogonal
+ 2𝑒. 𝑣 +
2
𝑣
= 𝑒 − 𝑣 βˆ™ (𝑒 − 𝑣)
= 𝑒
By hypothesis
𝑒
=
= 𝑒 + 𝑣 βˆ™ (𝑒 + 𝑣)
= 𝑒
𝑒−𝑣
𝑒+𝑣
2
2
− 2𝑒. 𝑣 +
𝑒+𝑣
+ 2𝑒. 𝑣 +
=
𝑣
2
𝑣
2
𝑒−𝑣
=
𝑒
2
− 2𝑒. 𝑣 +
𝑣
2
4𝑒. 𝑣 = 0
𝑒. 𝑣 = 0
Hence , 𝑒 π‘Žπ‘›π‘‘ 𝑣 are orthogonal
Proof :(‌) Given 𝑒 π‘Žπ‘›π‘‘ 𝑣 are orthogonal
WTS :
𝑒+𝑣
𝑒+𝑣
2
=
=
𝑒
= 𝑒
2
2
𝑒−𝑣
− 2𝑒. 𝑣 +
𝑣
2
And
𝑒−𝑣
2
− 2𝑒. 𝑣 +
𝑣
2
Since 𝑒 π‘Žπ‘›π‘‘ 𝑣 are orthogonal 𝑒 . 𝑣 = 0
Therefore,
𝑒+𝑣
=
𝑒−𝑣
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Example:- let u,v and w are vectors in space such that u+v+w=0, IIuII=3,
IIvII=5 and IIwII=7, then find the angle b/n u and v.
Solution:Example:- If u and v are unit vectors make an angle of
b/n them,
then find II3u+vII.
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Properties of NORMED Space
1.
2.
3.
4.
5.
6.
7.
…… Parallelogram Law
……………… Polarization identity
…….. Cauchy-Schwarz Inequality
…….. Triangle inequality
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Pythagoras Theorem:
If A and B are orthogonal vectors, then 𝐴 + 𝐡 2 = 𝐴 2 + 𝐡 2
Proof: 𝐴 + 𝐡 2 = 𝐴 + 𝐡 βˆ™ 𝐴 + 𝐡
= 𝐴 2 + 2𝐴 βˆ™ 𝐡 + 𝐡 2
= 𝐴 2 + 𝐡 2 𝑠𝑖𝑛𝑐𝑒 𝐴 βˆ™ 𝐡 = 0.
Note: If A is perpendicular to B, then it is also perpendicular to
any scalar multiple of B.
Orthogonal Projection
Definition: Suppose S is the foot of the perpendicular from R to
the line containing 𝑃𝑄 , then the vector with representation
𝑃𝑆 is called the vector projection of B on to A, and is denoted
by project𝐴𝐡 .
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R
R
B
B
A
S
A
Q
P
P
Proj AB
S
Q
projAB
π‘π‘Ÿπ‘œπ‘—π΄π΅ = 𝑃𝑆 = 𝑑𝐴
𝐡 − π‘π‘Ÿπ‘œπ‘—π΄π΅ = 𝑆𝑅
(𝐡 − π‘π‘Ÿπ‘œπ‘—π΄π΅ ).A=0
(B- t A).A =0
B.A –t A.A =0
π‘¨βˆ™π‘©
𝒕= 𝑨 𝟐
π‘¨βˆ™π‘©
π‘π‘Ÿπ‘œπ‘—π΄π΅ = 𝑃𝑆 = 𝒕. 𝑨 = 𝑨 𝟐 𝐴
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The scalar projection of B onto A (also called the component of B a long A)
is defined to be the length of project𝐴𝐡 , which is equal to 𝑩 𝐜𝐨𝐬 𝜽 and is
denoted by comp𝐴𝐡 . Thus:
𝒑𝒓𝒐𝒋𝑩𝑨 =
π’„π’π’Žπ’‘π‘©π‘¨ = 𝒑𝒓𝒐𝒋𝑩𝑨 =
π‘¨βˆ™π‘©
𝑨
𝑨
=
𝑨
π‘¨βˆ™π‘©
𝑨 =
𝑨 𝟐
π‘¨βˆ™π‘©
𝑨 𝟐
π‘¨βˆ™π‘©
𝑨 𝟐
𝑨
π‘¨βˆ™π‘©
𝑨 = 𝑨
Example: Let 𝐴 = −1,3,1 = −𝑖 + 3𝑗 + π‘˜ and 𝐡 = 2,4,3 = 2𝑖 + 4𝑗 + 3π‘˜
13
Then find (i) 𝒑𝒓𝒐𝒋𝑨𝑩 [π‘Žπ‘›π‘ . 29 2,4,3 ] ,
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(ii) 𝒑𝒓𝒐𝒋𝑩𝑨 [π‘Žπ‘›π‘ . 11 −1,3,1 ]
(iii) π’„π’π’Žπ’‘π‘©π‘¨
Directional angles and cosines
Let 𝐴 = π‘Ž1 𝑖 + π‘Ž2 𝑗 + π‘Ž3 π‘˜ be a vector positioned at the origin in ℝ3 , making an
angle of 𝛼 , 𝛽 π‘Žπ‘›π‘‘ 𝛾 with the positive π‘₯ , 𝑦 π‘Žπ‘›π‘‘ 𝑧 axes respectively. Then
the angles 𝛼 , 𝛽 π‘Žπ‘›π‘‘ 𝛾 are called the directional angles of A, and the quantities
cos 𝛼 , π‘π‘œπ‘  𝛽 π‘Žπ‘›π‘‘ cos 𝛾 are called the directional cosines of A, which can
be computed as follows:
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𝐴.𝑖
cos 𝛼 = 𝐴
π‘Ž
𝐴.𝑗
1
=
, cos 𝛽 = 𝐴
𝑖
𝐴
π‘Ž
𝑗
𝐴.π‘˜
= 𝐴2 and cos 𝛾 = 𝐴
π‘Ž
3
=
π‘˜
𝐴
From this relation we can deduce a unit vector
𝐴 = 𝐴 (π‘π‘œπ‘ π›Ό, π‘π‘œπ‘ π›½, π‘π‘œπ‘ π›Ύ)
𝐴
𝐴
= (π‘π‘œπ‘ π›Ό, π‘π‘œπ‘ π›½, π‘π‘œπ‘ π›Ύ) is a unit vector.
π‘Ž
cos 𝛼 = 𝐴1 , 𝛼 ∈ 0, πœ‹
π‘Ž
π‘Ž
, π‘π‘œπ‘  𝛽 = 𝐴2 , 𝛽 ∈ 0, πœ‹ , cos 𝛾 = 𝐴3 , 𝛾 ∈ 0, πœ‹
𝑍
A = a1 i + a2 j +a3k
𝛾
𝛼
𝛽
π‘Œ
𝑋
Remark: π‘π‘œπ‘  2 𝛼 + π‘π‘œπ‘  2 𝛽 + π‘π‘œπ‘  2 𝛾 = 1. (Verify!)
Solution
π‘Ž1
𝐴
2
+
π‘Ž2
𝐴
2
+
π‘Ž3
𝐴
2
=
π‘Ž1 2 + π‘Ž2 2 + π‘Ž3 2
𝐴 2
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𝐴 2
= 𝐴 2=1
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Solution:Solution:-
Solution:Exercise:- Use vector, Show that the altitudes of the triangle are concurrent.
Solution:-
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Definition: Suppose that 𝐴 =
𝐡 =
𝑏1 , 𝑏2 , 𝑏3
π‘Ž1 , π‘Ž2 , π‘Ž3
= π‘Ž1 𝑖 + π‘Ž2 𝑗 + π‘Ž3 π‘˜ and
= 𝑏1 𝑖 + 𝑏2 𝑗 + 𝑏3 π‘˜ be two vectors inℝ3 . Then the cross
product 𝐴 × π΅ of the two vectors is defined as:
𝑨×𝑩 =
Or
π’‚πŸ π’ƒπŸ‘ − π’‚πŸ‘ π’ƒπŸ π’Š + π’‚πŸ‘ π’ƒπŸ − π’‚πŸ π’ƒπŸ‘ 𝒋 + π’‚πŸ π’ƒπŸ − π’‚πŸ π’ƒπŸ π’Œ
𝐴𝑋𝐡 = 𝐷𝑒𝑑
Example: Let
𝑖
𝑗
π‘˜
π‘Ž1 π‘Ž2 π‘Ž3
𝑏1 𝑏2 𝑏3
𝐴 = 4𝑖 − 3𝑗 + 2π‘˜
𝐡 = 2𝑖 − 5𝑗 − π‘˜
Then find a) 𝐴 × π΅
b) 𝐡 × π΄
Remarks: For two non – zero vectors A & B,
1.
𝐴 × π΅ is a vector which is orthogonal to both A and B.
2.
𝐴 × π΅ is not defined for 𝐴, 𝐡 ∈ ℝ2 .
3.
𝑖 × π‘— = −𝑗 × π‘– = π‘˜
𝑗×π‘˜ = − π‘˜×𝑗
= 𝑖
π‘˜×𝑖 = − 𝑖×π‘˜
= 𝑗
A XB
B
A
Melak Mesfin
-A XB = B XA
37
Properties of Cross Product
Let A, B and C be vectors in ℝ3 and 𝛼 be any scalar. Then:
(1) 𝐴 × 0 = 0 × π΄ = 0, π‘€β„Žπ‘’π‘Ÿπ‘’ 0 = 0,0,0
(2) 𝐴 × π΅ = − 𝐡 × π΄
(3) 𝐴 × π΅ × πΆ
≠
𝐴×𝐡
(4) 𝛼𝐴 × π΅ = 𝐴 × π›Όπ΅
(5) 𝐴 ×
𝐡+𝐢
(6) 𝐴 βˆ™ 𝐴 × π΅
×𝐢
= 𝛼
𝐴×𝐡
= 𝐴×𝐡+ 𝐴×𝐢
= Ββˆ™ 𝐴×𝐡
= 0
(7) If A and B are parallel, then 𝐴 × π΅ = 0
(8) 𝐴 × Β
2
=
𝐴
(9) 𝐴 × Β
=
𝐴
(10)
2
𝐡
Β
𝐴×𝐡 = 𝑛
2
− π΄βˆ™Β 2
sin πœƒ , πœƒ ∈ 0, πœ‹ .
𝐴
𝐡
sin πœƒ, π‘€β„Žπ‘’π‘Ÿπ‘’ 𝑛 is the unit
vector in the direction of 𝐴 × π΅ π‘Žπ‘›π‘‘ πœƒ ∈ 0, πœ‹ is the
angle between A and B.
Example: If
𝐴
= 2,
A and B then find
Β
= 4 π‘Žπ‘›π‘‘ πœƒ = πœ‹ 4 for two vectors
𝐴×Β .
Note: The angle πœƒ between A and B can be obtained by
sin πœƒ =
𝐴×Β
𝐴
Β
, for two non – zero vectors A and B.
Melak Mesfin
38
Applications of cross Product:
(i)Area: The area of a parallelogram whose adjacent sides
coincides with the vectors A and B is given by 𝐴 × Β = 𝐴
d
B
Β
sin πœƒ
b
h
O
a
A
So, π‘Ž π‘œπ‘Žπ‘π‘ = π΅π‘Žπ‘ π‘’ π‘₯ β„Žπ‘’π‘–π‘”β„Žπ‘‘
= 𝐴
Β
sin πœƒ
N.B: The area of the triangle formed by A and B as its adjacent sides is given by
1
π‘Žπ‘Ÿπ‘’π‘Ž = 2 𝐴 × Β .
ii.Volume
The volume V of a parallelepiped with the three vectors A, B and C in ℝ3 as three of its
adjacent edges is given by:
𝑽= π‘¨βˆ™ 𝑩×π‘ͺ
π’‚πŸ
= 𝐝𝐞𝐭 π’ƒπŸ
π’„πŸ
π’‚πŸ
π’ƒπŸ
π’„πŸ
π’‚πŸ‘
π’ƒπŸ‘
π’„πŸ‘
Melak Mesfin
39
BXC
A
B
C
β„Ž=
π‘π‘Ÿπ‘œπ‘—
Hence,
𝐴
𝐡×𝐢
=
π΄βˆ™ 𝐡×𝐢
𝐡×𝐢 2
𝐡×𝐢
=
π΄βˆ™ 𝐡×𝐢
𝐡×𝐢
V =π΅π‘Ž β„Ž = 𝐴 βˆ™ 𝐡 × πΆ
Examples:
1. Find the area of a triangle whose vertices are 𝐴 1, −1,0 , 𝐡 2,1, −1
π‘Žπ‘›π‘‘ 𝐢 −1,1,2 .
Solution: The vectors on the sides of the
triangle βˆ† 𝐴Β𝐢 are 𝐴𝐡 = 𝐡 − 𝐴 = 1,2, −1 π‘Žπ‘›π‘‘ 𝐴𝐢 = −2,2,2 = 𝐢 − 𝐴.
So, π‘Ž βˆ† 𝐴Β𝐢 =
1
2
𝐴𝐡 × π΄πΆ
= 3 2 π‘ π‘žπ‘’π‘Žπ‘Ÿπ‘’ 𝑒𝑛𝑖𝑑𝑠.
1. Find the volume of the parallelepiped with edges
𝑒 = 𝑖 + π‘˜ , 𝑣 = 2𝑖 + 𝑗 + 4π‘˜ π‘Žπ‘›π‘‘ 𝑀 = 𝑗 + π‘˜.
Solution: V= 𝑒 βˆ™ 𝑣 × π‘€
= 1 𝑒3
Melak Mesfin
N.B: Three vectors 𝐴, 𝐡 π‘Žπ‘›π‘‘ 𝐢 are coplanar iff 𝐴 βˆ™ 𝐡 × πΆ = 0.
40
Lines and Planes in β„πŸ‘
Definition: A vector 𝑣 = π‘Ž, 𝑏, 𝑐 is said to be parallel to a line β„“ 𝑖𝑓 𝑣
is parallel to Ρ0 Ρ1 for any two distinct points Ρ0 π‘Žπ‘›π‘‘ Ρ1 π‘œπ‘› β„“.
A line β„“ 𝑖𝑛 ℝ3 is determined by a given point Ρ0 π‘₯0 , 𝑦0 , 𝑧0 on β„“
and a parallel vector 𝑣 (directional vector) 𝑣 = π‘Ž, 𝑏, 𝑐 π‘‘π‘œ β„“.
Equations of a line in space:
Let Ρ0 π‘₯0 , 𝑦0 , 𝑧0 be a given point on a line β„“ and 𝑃 π‘₯, 𝑦, 𝑧 be any
arbitrary point on β„“. If 𝑉 = π‘Ž, 𝑏, 𝑐 is the parallel vector to β„“, then
1) The parametric equation of β„“ is given by π‘₯ = π‘₯0 + π‘Žπ‘‘,
𝑦 = 𝑦0 + 𝑏𝑑 ,
𝑧 = 𝑧0 + 𝑐𝑑, 𝑑 ∈ ℜ, where t is called
the parameter.
2) The symmetric form of equation of β„“ is given by:
𝒙 − 𝒙 𝟎 π’š − π’šπŸŽ 𝒛 − 𝒛 𝟎
=
=
, 𝒇𝒐𝒓 𝒂, 𝒃, 𝒄 ≠ 𝟎.
𝒂
𝒃
𝒄
3) The vector equation of β„“ is written as 𝒓 − π’“πŸŽ = 𝒕𝒗, π‘€β„Žπ‘’π‘Ÿπ‘’ 𝑑 ∈ ℜ.
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41
Remarks:
1. The above equations of the line can be derived using vector
algebra as follows:
Z
p
P0
r0
r
Y
X
From vector addition, we have π‘Ÿ − π‘Ÿ0 = Ρ0 Ρ & π‘Ÿπ‘œ = π‘₯0 𝑖 + 𝑦0 𝑗 + 𝑧0 π‘˜,
π‘Ÿ = π‘₯𝑖 + 𝑦𝑗 + π‘§π‘˜. Since Ρ0 Ρ π‘£ , there exists 𝑑 ∈ ℜ such that
π‘Ÿ − π‘Ÿ0 = 𝑑𝑣 = Ρ0 Ρ
οƒž
π‘₯ − π‘₯0 , 𝑦 − 𝑦0 , 𝑧 − 𝑧0 = 𝑑 π‘Ž, 𝑏, 𝑐
 π‘₯ = π‘₯0 + π‘Žπ‘‘ , 𝑦 = 𝑦0 + 𝑏𝑑, 𝑧 = 𝑧0 + 𝑐𝑑.
2. If one of π‘Ž, 𝑏 π‘œπ‘Ÿ 𝑐 𝑖𝑠 0, (say for instance 𝑏 = 0),
the symmetric equation of β„“ is given as:
π‘₯ − π‘₯0
𝑧 − 𝑧0
Melak
= Mesfin
, 𝑦 = 𝑦0 .
π‘Ž
𝑐
42
Note that:- For two distinct lines
1)
Are intersecting lines iff
such that
2) Thus
3) Non-intersecting and non-parallel lines called skew line.
4)
Example: Find parametric equations and symmetric equations of the line l
containing the points P1 =(4, – 6, 5) and P2 = (2, –3, 0).
Solution:-
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43
Exercise:-1 Show that the lines and with parametric equations
are skew lines; that is, they do not intersect and are not parallel (and
therefore do not lie in the same plane).
Exercise:- 2 Find the point of intersection of the two lines
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44
Equation of a plane:
A plane in space is determined by a point Ρ0 π‘₯0 , 𝑦0 , 𝑧0 in the plane
and a vector 𝑛 that is orthogonal to the plane. This orthogonal
vector 𝑛 is called a normal vector. Suppose that 𝑃 π‘₯, 𝑦, 𝑧 be any
arbitrary point in the plane, and let π‘Ÿ π‘Žπ‘›π‘‘ π‘Ÿ0 be the position
vectors of 𝑃 π‘₯, 𝑦, 𝑧 and Ρ0 π‘₯0 , 𝑦0 , 𝑧0 . Then we have
𝑛 βˆ™ π‘Ÿ − π‘Ÿ0 = 0 (Since 𝑛 perpendicular to any vector in the plane).
 𝑛 βˆ™ π‘Ÿ = 𝑛 βˆ™ π‘Ÿπ‘œ ,which is called the vector equation of the plane.
If we let 𝑛 = π‘Ž, 𝑏, 𝑐 = π‘Žπ‘– + 𝑏𝑗 + π‘π‘˜, we get
π‘Ž, 𝑏, 𝑐 βˆ™ π‘₯ − π‘₯0 , 𝑦 − 𝑦0 , 𝑧 − 𝑧0 = 0
 π‘Ž π‘₯ − π‘₯0 + 𝑏 𝑦 − 𝑦0 + 𝑐 𝑧 − 𝑧0 = 0
(point - normal form of equation of a plane)
⟺ 𝒂𝒙 + π’ƒπ’š + 𝒄𝒛 + 𝒅 = 𝟎, π’˜π’‰π’†π’“π’† 𝒅 = − π’‚π’™πŸŽ + π’ƒπ’šπŸŽ + π’„π’›πŸŽ
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(general or standard form of the
equation of a plane).
45
Examples:
1. Find the equations of a line that contains the point 1,4, −1
and parallel to 𝑣 = −2𝑖 + 3𝑗.
Solution: let ΡΟ = 1 ,4, −1 = π‘₯0 , 𝑦0 , 𝑧0
Then the parametric form of the equation of the line is:
π‘₯ = 1 − 2𝑑
𝑦 = 4 + 3𝑑
𝑧 = −1
π‘₯−1
=
−2
𝑦−4
3
and its symmetric form is given as:
, 𝑧 = −1.
2. Find the equation of the plane through the points Ρ0 1,1,1 ,
Ρ1 2,2,0 π‘Žπ‘›π‘‘ Ρ2 4, −6,2 .
Solution: The vectors 𝐴 = Ρ0 Ρ1 = 1,1, −1 π‘Žπ‘›π‘‘
Β = Ρ1 Ρ2 = 3, −7,1
are parallel to the plane, and hence, their
cross product 𝑛 = 𝐴 × Β = −6, −4, −10 is normal to the plane.
Thus, the equation of the plane is given by:
−6 π‘₯ − 1 − 4 𝑦 − 1 − 10 𝑧 − 1 = 0
 3 × +2𝑦 + 5𝑧 − 10 = 0
Melak Mesfin
46
OR: The equation of the plane can be obtained by computing:
π‘₯−1
𝑑𝑒𝑑 π‘₯ − 2
π‘₯−4
𝑦−1
𝑦−2
𝑦+6
𝑧−1
𝑧−0
𝑧−2
=0
Distance in Space
a) Distance from a point to a line
The distance D from a point Ρ1 (not on β„“) to a line β„“ in space is given by:
𝒗 × πšΈπšΆ 𝚸𝟏
𝒗
𝑫=
, where 𝑣 is the directional vector of β„“ and ΡΟ is any point on β„“.
Proof:
Z
P1
L
D
πœƒ
P0
V
Y
X
sin πœƒ =
𝐷
ΡΟ Ρ1
⟹ 𝐷 = ΡΟ Ρ1 sin πœƒ
But since 𝑣 × ΡΟ Ρ1 = 𝑣
ΡΟ Ρ1
sinMelak
πœƒ , =Mesfin
𝑣 𝐷 , we have: 𝐷 =
𝑣 ×Ρ Ο Ρ 1
𝑣
.
47
a)
Distance from a point to a plane
The perpendicular distance D of a point Ρ0 π‘₯0 , 𝑦0 , 𝑧0
in space to the
plane with the equation π‘Žπ‘₯ + 𝑏𝑦 + 𝑐𝑧 + 𝑑 = 0 is given by:
𝐷 =
π‘Žπ‘₯ 0 +𝑏𝑦 0 +𝑐𝑧 0 +𝑑
π‘Ž 2 +𝑏 2 +𝑐 2
=
𝑛 βˆ™π‘œΡ
𝑛
, where o is the foot of 𝑛 within the plane.
Proof: Consider the diagram below:
P(x0,y0,z0)

O(x1,y1,z1)
𝐷 =
π‘π‘Ÿπ‘œπ‘—π‘›0Ρ
οƒž 𝐷 =
=
π‘œΡ βˆ™ 𝑛
𝑛 2
π‘Žπ‘₯ 0 +𝑏𝑦 0 +𝑐𝑧 0 +𝑑
π‘Ž 2 +𝑏 2 +𝑐 2
𝑛
=
π‘œΡ βˆ™ 𝑛
𝑛
, π‘€β„Žπ‘’π‘Ÿπ‘’ 𝑑 = − π‘Žπ‘₯1 + 𝑏𝑦1 + 𝑐𝑧1
P1(x1,y1,z1)
πœƒ

B
O
P0(x0,y0,z0)
Melak Mesfin
48
Melak Mesfin
49
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50
Distance between two parallel planes
Given two parallel planes πœ‹1 π‘Žπ‘›π‘‘ πœ‹2 . Then we can have normal vectors
with coefficients π‘Ž, 𝑏, 𝑐 to be the same such that:
πœ‹1 : π‘Žπ‘₯ + 𝑏𝑦 + 𝑐𝑧 = 𝑑1 and πœ‹2 : π‘Žπ‘₯ + 𝑏𝑦 + 𝑐𝑧 = 𝑑2.
Then the distance between πœ‹1 π‘Žπ‘›π‘‘ πœ‹2 is the same as the distance
from any arbitrary point 𝑃 π‘₯0 , 𝑦0 , 𝑧0
plane πœ‹2 . ⇒𝐷 =
Thus,
π‘Ž π‘₯ π‘œ +𝑏𝑦 π‘œ +π‘π‘§π‘œ −𝑑 2
π‘Ž 2 +𝑏 2 +𝑐 2
has been taken from πœ‹1 to the
. But π‘Žπ‘₯π‘œ + π‘π‘¦π‘œ + π‘π‘§π‘œ = 𝑑1
𝑑 1 −𝑑 2
𝐷=
π‘Ž 2 +𝑏 2 +𝑐 2
Example: Find the distance between the planes
πœ‹1 : π‘₯ + 2𝑦 − 2𝑧 = 3 π‘Žπ‘›π‘‘ πœ‹2 : 2π‘₯ + 4𝑦 − 4𝑧 = 7
Solution: We first rewrite the equations πœ‹1 π‘Žπ‘›π‘‘ πœ‹2 so that they
have the same 𝑛 = π‘Ž, 𝑏, 𝑐 . That is:
πœ‹1 : π‘₯ + 2𝑦 − 2𝑧 = 3
πœ‹2 : π‘₯ + 2𝑦 − 2𝑧 = 7 2 ⟹ 𝑑1 = 3& 𝑑2 = 7 2
Thus, 𝐷 =
=
𝑑 1 −𝑑 2
π‘Ž 2 +𝑏 2 +𝑐 2
7
2−3
1+4+4
=
, π‘€β„Žπ‘’π‘Ÿπ‘’ π‘Ž = 1, 𝑏 = 2, 𝑐 = −2
1
2
3
=1 6
Melak Mesfin
51
Remarks:1. Let
a) If two points of the line lies on the plane, the lies on .
b)
i.e.
c)
i.e.
2. Let
be two planes:
a)
i.e.
b)
i.e.
c) the angle b/n
is the angle b/n
thus, we have
Melak Mesfin
52
Example:- Find the equation of the plane passing through p(-2,3,5) and is
perpendicular to the line with parametric equation
Solution:Exercise:- 1. Find the point of intersection of the line with parametric
equations
intersect the plane
Exercise:-2 For two planes
a) Find the angle b/n
.
b) Find the symmetric equations for the line of intersection of the two
planes
.
Melak Mesfin
53
Vector Space
Definition(Vector Space)
A real vector space V is a set
of objects together with two
operations addition “+” and
Scalar multiple “.” satisfying
the following axioms:
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54
Note that :
i) R(the set of real number) is a vector space over a field R.
ii) any vector space contain at least one element(i.e. Nonempty)
Example:-1 The set of all vectors in a plane is a vector space over R
under the standard operation vector addition “+” and Scalar
Multiple.
Solution:iii) Under the standard operation
are real vector
space.
Example:- 2
together with the standard
operations Matrix addition and scalar Multiple form a real vector
spaces.
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55
Example:- 3
, the set of all polynomial of degree less than or
equal to 2 with standard operations is a real vector space.
iv) In order to show that V is not a vector space it is enough to show
that one axiom of the vector space doesn’t hold
Solution:Example:-4 Is
with standard operation is a vector space?
Solution:Example:-5
be the set of all vectors in a plane with defined
operations. Examine whether
is a vector space or not.
a)
b)
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56
Subspaces
Definition: Let V be a given vector space over a field F. Then a non-empty subset W of V is said
to be a subspace of V if W itself is a vector space over F under the operations of V.
Theorem: Suppose that V is a vector space over a field F.A non-empty subset W of V is a
subspace of V if it satisfies the following conditions:
i.
ii.
iii.
𝑒, 𝑣 ∈ π‘Š ⇒ 𝑒 + 𝑣 ∈ π‘Š.
∀𝑒 ∈ π‘Š π‘Žπ‘›π‘‘ 𝑐 ∈ 𝐹 ⇒ 𝑐𝑒 ∈ π‘Š.
0 ∈ π‘Š.
Examples
1. V and 0 are the trivial subspaces of any vector space V.
2. For the vector space 𝑉 = ℝ3 = { π‘₯, 𝑦, 𝑧 ; π‘₯, 𝑦, 𝑧 ∈ ℝ} over ℝ.Then the set π‘Š =
{ π‘₯, 𝑦, 0 ; π‘₯, 𝑦 ∈ ℝ} is a subspace of V. (verify!)
Solution
i) Let π‘ˆ = π‘₯1 , 𝑦1 , 0 and 𝑉 = π‘₯2 , 𝑦2 , 0
then π‘ˆ + 𝑉 = π‘₯1 + π‘₯2 , 𝑦1 + 𝑦2 , 0 ∈ π‘Š
ii) Let π‘ˆ = π‘₯1 , 𝑦1 , 0 and π‘π‘ˆ = {𝑐π‘₯1 , 𝑐𝑦1 , 0) ∈ π‘Š}
iii) (0,0,0)οƒŽW
Therefore W is the subspace of V Melak Mesfin
57
3. The set of all lines passing through the origin, 𝐿 = {π‘Žπ‘₯ + 𝑏𝑦 = 0, π‘Ž, 𝑏 ∈ ℝ} is a
subspace of the vector space 𝑉 = ℝ2 .
Solution
i) Let 𝐿1 = {π‘Žπ‘₯1 + 𝑏𝑦1 = 0, π‘Ž, 𝑏 ∈ ℝ} and 𝐿2 = {π‘Žπ‘₯2 + 𝑏𝑦2 = 0, π‘Ž, 𝑏 ∈ ℝ
the 𝐿1 + 𝐿2 = {π‘Ž π‘₯1 + π‘₯2 , 𝑏 𝑦1 + 𝑦2 = 0, π‘Ž, 𝑏 ∈ ℝ} ∈ 𝐿
ii)Let 𝐿1 = {π‘Žπ‘₯1 + 𝑏𝑦1 = 0, π‘Ž, 𝑏 ∈ ℝ} and 𝑐𝐿1 = {𝑐(π‘Žπ‘₯1 + 𝑏𝑦1 ) = 0, π‘Ž, 𝑏 ∈ ℝ} ∈ 𝐿
iii) 𝐿1 = {π‘Ž(0) + 𝑏(0) = 0, π‘Ž, 𝑏 ∈ ℝ} ∈ 𝐿 this implies that line L passes through the
origin.
Therefore L is the subspace of V
Exercise: 1.Is the set π‘Š = {π‘₯ − 4𝑦 = 1} a subspace of 𝑉 = ℝ2 ? Justify.
2. Which of the following is the subspace of 𝑉 = ℝ3 ?
a) π‘Š = { π‘₯1 , π‘₯2 , 1 ; π‘₯1 , π‘₯2 ∈ 𝑅
b) π‘Š = { π‘₯1 , π‘₯1 + π‘₯3 , π‘₯3 ; π‘₯1 , π‘₯Melak
3∈𝑅
Mesfin
58
Theorem2: A subset W of a vector space V is a subspace of v iff
Example:- Show that
of
.
Exercise:- Let V be a vector space
following are subspace or not.
a.
b.
c.
d.
Melak Mesfin
is the subspace
. Examine whether the
59
Definition 1.1.8 A vector w in Rn is said to be a linear combination.. of the vectors
V1, V2, … , Vk in Rn if w can be expressed in the form W = c1 v1 + c2v2 + . . . + ckvK
The scalars c1, c2, ... , ck are called the coefficients in the linear combination. In the case
where k = 1, Formula (14) becomes w = c1 v1, so to say that w is a linear combination of v1
is the same as saying that w is a scalar multiple of v1.
Example : Provided that X= (-1 , -2 , -2 ) , U = (0 ,1 ,4) , V = (-1 , 1 ,2) and W = (3 ,1 ,2) in
R3 find scalars a , b and c such that X = a U + b V + c W
SOLUTION (-1 , -2 , -2 ) = a (0, 1 ,4) + b ( -1 ,1 ,2 ) + c (3 , 1 ,2 )
= (-b +3c , a +b +c , 4a +2b +2c )
you can equate corresponding components so that they form the system of three linear
equations as shown below.
-b +3c = -1
a +b +c = - 2
,4a +2b +2c = -2
Answer a =1 ,b= - 2 and c = -1
Try using vector addition and scalar multiplication to check this result.
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Linear Dependence and Independence
Definition: Let 𝑣1 , 𝑣2, … , 𝑣𝑛 be elements of an arbitrary vector space V, and
𝛼1 , 𝛼2, … , 𝛼𝑛 be scalars. An expression of the form 𝛼1 𝑣1 + 𝛼2 𝑣2 + β‹― 𝛼𝑛 𝑣𝑛
is called linear combinations of the vectors 𝑣1 , 𝑣2, … , 𝑣𝑛 .
Examples:
1) For the set of vectors in ℝ3 , 𝑆 = { 1,3,1 , 0,1,2 , 1,0,5 }
Let 𝑣1 = 1,3,1 , 𝑣2 =
0,1,2 , π‘Žπ‘›π‘‘π‘£3 1,0,5
V1 is a linear combinations of v2 and v3 because
V1= c1 (0,1, 2) +c2 (1,0,5),
C1 =1 and
(1, 3, 1) = c1 (0, 1, 2) +c2 (1,0,5)
2c1 -5c2 =1, C2 =3
V1 =3 V2 + V3
This implies that S is linearly independent .
Exercise:
1) Write the vector W = (1,1,1) as a linear combination of vectors in the set S.
S = { (1,2,3),(0,1,2), (-1,0,1)}.
2) If possible, write the vector W = (1,-2, 2) as a linear combinations of vectors in the set
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S ={ (1,2,3),(0,1,2), (-1,0,1)}.
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Definition: Let 𝑣1 , 𝑣2, … , 𝑣𝑛 are vectors in a vector space V over ℝ.Then vectors are called:
1. linearly dependent if there exist scalars 𝛼1 , 𝛼2, … , 𝛼𝑛 not all zero such that
𝛼1 𝑣1 + 𝛼2 𝑣2 + β‹― 𝛼𝑛 𝑣𝑛 = 0.
2. Linearly independent if 𝛼1 𝑣1 + 𝛼2 𝑣2 + β‹― 𝛼𝑛 𝑣𝑛 = 0 implies
𝛼1 = 𝛼2 = … = 𝛼𝑛 = 0.
Linear dependence in the vector space V ¼ R3 can be described geometrically as follows:
(a) Any two vectors u and v in R3 are linearly dependent if and only if they lie on the same line
through the origin O, as shown in Fig. 4-3(a).
(b) Any three vectors u, v, w in R3 are linearly dependent if and only if they lie on the same
plane through the origin O, as shown in Fig. 4-3(b)Later, we will be able to show that any four
or more vectors in R3 are automatically linearly dependent.
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Examples:
1. Determine whether the following set of vectors in the vector space 𝑉 = ℝ3 are linearly
dependent or independent. a) 1, 0,0 , 0 , 1, 0 , (0, 0,3) b) 2, 6,0 , 2 , 4, 1 , (1 , 1, 1) .
c) {(1,2,3),(0,1,2),(-2,0,1)}
2. Let V be the vector space of all real valued functions of the variable t. Then which of the
following set of functions are LD/LI? Justify!
a) 𝑑, 𝑑 2 , 𝑠𝑖𝑛𝑑
b) π‘π‘œπ‘  2 𝑑, 𝑠𝑖𝑛 2 𝑑, 1
3. Determine whether the following set of vectors in the vector space 𝑉 = ℝ2 are linearly
dependent or independent a) {(1, 2), (2,4)} b) {(1, 0), (0,1),(-2,5)}
4 . Determine whether the following set of vectors in P2 are linearly dependent or
independent . S = {1+ x -2x2 , 2+5x –x2 , x+x2 }
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Basis of a vector space
Definitions: Let V be any vector space over a field F, and let the set 𝑆 = 𝑣1, 𝑣2 , … , 𝑣𝑛 be a set of
vectors in V. Then:
i)
ii)
iii)
S is said to spans (or generates) V if each element of V is a linear combinations of
elements of S.
S is called a basis for V if S is a linearly independent set and it spans V.
The dimension of V is said to be n (dim V=n) if V has basis consisting of n-elements.
Examples:
1. Show that the set 𝑆 = 1,0,0 , 0,1,0 , (0,0,5) form a basis of the vector spaceℜ3 .
Solution
I) we need to show that S is linearly independent
𝛼 1,0,0 + 𝛽 0,1,0 , + 𝛾 0,0,5 = (0,0,0)
𝛼=𝛽=𝛾=0
Hence S is linearly independent
ii) we need to show that S spans ℜ3
Let (x, y ,z) οƒŽℜ3 then (π‘₯, 𝑦, 𝑧) = 𝛼 1,0,0 + 𝛽 0,1,0 , + 𝛾 0,0,5
𝑧
𝛼 = π‘₯ , 𝛽 = 𝑦 π‘Žπ‘›π‘‘ 𝛾 =
5
𝑧
(π‘₯, 𝑦, 𝑧) = π‘₯ 1,0,0 + 𝑦 0,1,0 , + 5 0,0,5
Therefore , S Spans ℜ3
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1.8. Basis of a vector space.
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