A “right handed” (if you stand at the origin with your right arm along the positive x-axis and your left arm along the positive y-axis, your head will point in the direction of the positive z-axis) three-dimensional coordinate system has three perpendicular coordinate planes: the xy-, xz-, and yz-planes.
Equations of the coordinate planes in R3:
Plane
Equation
yz
x=0
xy
z=0
xz
y=0
In R3, the distance from the origin to (a,b,c) is d=a2+b2+c2.
We can summarize the distance formula for P1(x1,y1,z1) and P2(x2,y2,z2)
∥P1P2∥=Δx2+Δy2+Δx2
Graphs in R3
The graph of an equation in R3 is the collection of all points (x,y,z) whose coordinates satisfy a given equation. This graph is called the surface.
Planes
To graph a plane, find some ordered triples that satisfy the equation. The best ones to use are those that fall on a coordinate axis (intercepts).
Spheres
A sphere is defined as the collection of all points located a fixed distance (radius) from a fixed point (center).
Equation of a sphere: The graph of the equation
(x−a)2+(y−b)2+(z−c)2=r2
is a sphere with center (a,b,c) and radius r. This is the standard form of the equation of a sphere.
Solve given equations by rearranging to standard form and completing the square in the variables that require it.
Warning: Pay close attention to the signs when deriving the center coordinates from the equation since the coordinates are subtracted in the equation.
Cylinders
A cylindrical surface is a surface traced by a line moving parallel to a given fixed line and intersecting a given curve. A cylinder is defined with a generating curve (directrix) and a generating line (directrix). Lines running parallel to the directrix are called the rulings.
The curve is always in the plane containing the two variables in the equation. The rulings are parallel to the axis of the missing variable: e.g y=x2 has a generating curve in the xy-plane and rulings that run parallel to the z-axis. Any three variable equation missing one variable will be a cylindrical surface.
Vectors in R3
A vector in R3 is a directed line segment in space.
Representation and operations are analogous to the representation and operations defined in R2.
where r0 is a position vector (points to a point on the line) and v is a direction vector (a vector parallel to the vector).
Parametric Form of a Line in R3:
A line parallel to the vector v=⟨a,b,c⟩ that passes through the point (x1,y1,z1) is given by
x=x1+tay=y1+tbz=z1+tc
for some number t.
Symmetric Form of a Line in R3
The parameter t can be eliminated to obtain the symmetric form of a line
ax−x1=by−y1=cz−z1
Parametric Equations
Converting a parametric equation to a rectangular equation is called eliminating the parameter. General guidelines are:
Solve for t in one of the equations
Substitute into the second equation
Simplify
If the equation involve trigonometric functions, trigonometric identities may be needed
The domain may need to be adjusted based upon the original parametric equation
Determining if Two Lines are Parallel, Intersecting (or Perpendicular), or Skew
Test for parallel. If not, then
Test for intersecting
If intersecting, then test for perpendicular
If not intersecting, then is skew
For example, given ⟨3+2t,4−t,1+3t⟩ and ⟨1+4s,3−2s,4+5s⟩
Test for parallel: Take the ratio of each component’s direction numbers (coefficients on the parameters) and set them equal to each other. Does 42=−2−1=53? No, therefore the lines are not parallel.
Test for intersecting: Solve a system of simultaneous equations. If we can solve it, then the lines are intersecting. Solve
3+2t=1+4s4−t=3−2s1+3t=4+5s
Test for perpendicular: If the dot product of the two lines is 0, then the lines are perpendicular.
A common way to specify the direction of a plane is by means of a vector N (called a normal to the plane) that is orthogonal to every vector in the plane. The point-normal form comes from determining the dot product of all the points in the plane with the normal vector. The standard form then comes from distributing and simplifying.
A plane with normal N=⟨A,B,C⟩ containing the points (x0,y0,z0) has the following equations
Point-normal form: A(x−x0)+B(y−y0)+C(z−z0)=0
Standard form: Ax+By+Cz+D=0
Determine a Line’s Orthogonality/Collinearity With a Plane
A line is parallel to a plane if the direction vector of the line is orthogonal to the normal vector of the plane. Remember that two vectors are orthogonal if their dot product is zero.
A line is perpendicular to a plane if its direction vector is a scalar multiple of the normal vector of the plane. Remember that the normal vector is already perpendicular to the plane, so both being parallel means that their directions lie along the same line in R3.
Determine the Equation of a Plane Using a Normal Vector…
Orthogonal to a Given Plane:
Use the normal N of the given plane and the given point to construct the equation in point-normal form.
Containing Three Given Points:
Given the points P, Q, and R, a normal N to the required plane is orthogonal to the vectors PR and PQ and is, therefore, found by computing with the cross product.
N=PR×PQ
You can now find the equation of the plane using this normal vector and any point in the plane.
Parallel to the Intersection of Two Planes:
Because the required line is perpendicular to the normals N1 and N2 of the given planes, the aligned vector is found by computing with the cross product.
N1×N2
You can now find the equation of the plane using this normal vector and any point in the plane.
Vector Methods of Measuring Distances in R3
Distance from a Point to a Plane
The distance from the point P(x0,y0,z0) to the plane Ax+By+Cz+D=0 is given by
Where Q is any point in the given plane and N is a normal to the given plane.
Note that to determine QP, we will need to determine one point on the plane Q.
Obtain the Equation for a Sphere Tangent to a Given Plane
Given C(x0,y0,z0) and a plane, the radius r is the distance from the center C to the given plane (use the distance formula from above). Therefore the equation of the sphere is
(x−x0)2+(y−y0)2+(z−z0)2=r2
Distance from a Point to a Line
The distance from point %P% to the line L is given by
d=∥v∥∥v×QP∥
where v is a vector parallel to L and Q is any point on L.
Note that to determine QP, we will need to determine one point on the plane Q (set t=0).
9.7 Quadric Surfaces
A quadric surface is given by a degree two equation in the general form
Ax2+By2+Cz2+Dxy+Exz+Fyz+Gx+Hy+Iz+J=0
where A,…,J are constants.
Graphing Quadric Surfaces Using Traces
To graph a quadric surface, it is often helpful to graph the xy-trace, xz-trace, and yz-trace (the intersections of the surface with these three planes). To determine the xy-trace, sex z=0. To determine the xz-trace, set y=0. To determine the yz-trace, set x=0.
Common Quadric Surfaces
Ellipsoid
The general equation of an ellipsoid is
a2x2+b2y2+c2z2=1
If a=b=c then we will have a sphere.
Cylinder
The general equation of a cylinder is
a2x2+b2y2=1
If a=b we have a cylinder whose cross section is a circle. The cylinder will be centered on the axis corresponding to the variable that does not appear in the equation.
Hyperboloid of one sheet
The general equation of a hyperboloid of one sheet is
a2x2+b2y2−c2z2=1
The variable with the negative in front of it will give the axis along which the graph is centered.
Hyperboloid of two sheets
The general equation of a hyperboloid of two sheets is
−a2x2−b2y2+c2z2=1
The variable with the positive in front of it will give the axis along which the graph is centered.
Elliptic cone
The general equation of an elliptic cone is
a2x2+b2y2=c2z2
The variable that sits by itself on one side of the equal sign will determine the axis that the cone opens up along.
Elliptic paraboloid
The general equation of an elliptic paraboloid is
a2x2+b2y2=cz
The variable that isn’t squared determines the axis upon which the paraboloid opens up. The sign of c will determine the direction that the paraboloid opens. If c is positive then it opens up and if c is negative then it opens down.
Hyperbolic paraboloid
The general equation of a hyperbolic paraboloid is
a2x2−b2y2=cz
These graphs are vaguely saddle shaped and as with the elliptic paraboloid the sign of c will determine the direction in which the surface opens.
10 Vector-valued functions
10.1 Introduction to Vector Functions
Vector-valued Functions
A vector-valued function (or vector function) is a function where the domain is a subset of the real numbers and the range is a vector. It is given by
r(t)=f(t)i^+g(t)j^r(t)=⟨f(t),g(t)⟩
in R2.
r(t)=f(t)i^+g(t)j^+h(t)k^r(t)=⟨f(t),g(t),h(t)⟩
in R3.
The domain of a vector valued function is the intersection of the domain of its components.
Operations with Vector Functions
Let F and G be vector functions of the real variable t, and let f(t) be a scalar function.
Operation
Equation
Addition
(F+G)(t)=F(t)+G(t)
Subtraction
(F−G)(t)=F(t)−G(t)
Scalar multiplication
(fF)(t)=f(t)F(t)
Cross product
(F×G)(t)=F(t)×G(t)
Limits and Continuity of Vector Functions
Limit of a vector function
Suppose the components of the vector function F(t)=ai^+bj^+ck^ all have finite limits as t→t0, where t0 is any number or ∞ or −∞. Then
Let F and G be vector functions of the real variable t, and let h(t) be a scalar function so that all three functions have finite limits as t→t0, then
A vector function F(t) is said to be continuous at t0 if t0 is in the domain of F and t→t0limF(t)=F(t0)
10.2 Differentiation and Integration of Vector Functions
Vector Derivatives
The derivative of the vector function F is the vector function F′ determined by the limit.
F′(t)=Δt→0limΔtΔF
wherever the limit exists. We say that the vector function F is differentiable at t=t0 if F′(t) is defined at t0.
Derivative of a Vector Function
The vector function F(t) is differentiable whenever the components functions are each differentiable.
F′=f1′(t)i+f2′(t)j+f3′(t)k
Tangent Vectors
The vector derivative can be used to find tangent vectors to curves in space.
Smooth Curve
A vector function F is smooth on a given interval if F′(t)=0.
For example, if F(t)=⟨a,b,c⟩, then F′(t)=⟨0,0,0⟩.
Properties of Vector Derivatives
Higher-order derivatives of a vector function F are obtained by successively differentiating the components of F(t). For example, the second derivative of F is the derivative of F′(t), and so on.
Modeling the Motion of an Object in R3
An object that moves in such a way that its position at time t is given by the vector function R(t) is said to have
the position vector: R(t)
the velocity: V=R′(t)
At any time t,
the speed is the magnitude of the velocity: ∥V∥
the direction of motion is the unit vector: ∥V∥V
the acceleration vector is the derivative of the velocity: A=V′(t)=R′′(t)
Vector Integrals
Vector integration is performed per component.
The indefinite integral of F(t) is the vector function
∫F(t)dt=[∫f1(t)dt]i+[∫f2(t)dt]j+[∫f3(t)dt]k+C
where C=C1i+C2j+C3k is an arbitrary constant vector.
10.4 Unit Tangent and Principal Unit Normal Vectors; Curvature
11 Partial differentiation
This chapter extends the methods of single-variable differential calculus to functions of two of more independent variables.
11.1 Functions of Several Variables
Basic Concepts
A function of two variables is a rule f that assigns to each ordered pair (x,y) in a set D a unique number f(x,y). The set D is called the domain and the corresponding values of f(x,y) constitute the range.
When dealing with such functions, we may write z=f(x,y) and refer to x and y as the independent variables and to z as the dependent variable.
Level Curves and Surfaces
One way we can approach sketching the graph of a function of two variables, without the assistance of technology, is the same as graphing quadric surfaces in Section 9.7: Use the trace of of graph in a plane.
When the plane z=C intersects the surface z=f(x,y), the result is the trace, the equation f(x,y)=C. The set of points (x,y) in the xy-plane that satisfy this equation is called the level curve (or contour curve) of f at C. An entire family of level curves is generated as C varies over the range of f. Think of a trace as a “slice” of the surface at a particular location and a level curve as its projection onto the xy-plane.
Graphs of Functions of Two Variables
A more complete picture of a surface can be obtained by examining cross sections perpendicular to the other two principle directions as well.
If f is a function of three variables x, y, and z, then the solution set of the equation f(x,y,z)=C is a region of R3 called a level surface of f at C.
11.2 Limits and Continuity
Single variable functions have domains that can be expressed in terms of intervals. However, functions of two or more variables requires special terminology and notation introduced in this section followed by limits and continuity.
Open and Closed Sets in R2 and R3
An open disk in R2 centered at point C(a,b) with radius r is the set of all points P(x,y) such that (x−a)2+(y−b)2<r. If the boundary of the disk is included, it is said to be a closed disk. Open and closed disks are analogous to open and closed intervals on a coordinate line.
A point P0 is said to be an interior point of a set S in R2 if some open disk centered at P0 is contained entirely within S. If S is the empty set, or if every point of S is an interior point, then S is called an open set.
A point P0 is said to be a boundary point of a set S in R2 if every open disk centered at P0 contains both points that belong to S and points that do not. The collection of all boundary points of S is called the boundary of S. S is said to be closed if it contains its boundary.
The empty set ∅ is both open and closed in any topological space.
Similarly, an open ball centered at point C(a,b,c) in R3 is the set of all points P(x,y,z) such that (x−a)2+(y−b)2+(z−c)2<r. (etc. as above in R2).
Limit of a Function of Two Variables
For a function of two variables, the limit statement
(x,y)→(x0,y0)limf(x,y)=L
means that for each given number ϵ>0, there exists a number δ>0 such that for all (x,y)=(a,b), if (x,y) is in the open disk centered at (x0,y0) in the xy-plane with radius δ, then
∣f(x,y)−L∣<ϵ
What this says is that the function value of f(x,y) must lie in the interval (L−ϵ,L+ϵ) whenever (x,y) is a point in the domain of f other than P0(x0,y0) that lies inside the disk of radius δ centered at P0.
If the limit is not the same for all approaches within the domain of f, then the limit does not exist.
Evaluate:
Try direct substitution. If this results in an indeterminate form, then
Check if the equation is factorable and cancel the factored terms. If not, then
Take the limits (x,y)→(0,0) along the x-axis and y-axis or the lines y=x and y=−x.
Continuity
Using the definition of the limit of a function of two variables, we can define the continuity of a function of two variables analogously. The function f(x,y) is continuous at the point (x0,y0) if and only if
f(x0,y0) is defined
(x,y)→(x0,y0)limf(x,y) exists
(x,y)→(x0,y0)limf(x,y)=f(x0,y0)
The function f is continuous on a set S if it is continuous at each point in S.
Limits and Continuity for Functions of Three Variables
The concepts introduced for functions of two variables in R2 extend naturally to functions of three variables in R2.
The limit statement
(x,y,z)→(x0,y0,z0)limf(x,y,z)=L
means that for each number ϵ>0, there exists a number δ>0 such that
∣f(x,y,z)−L∣<ϵ
whenever (x,y,z) is a point in the domain of f such that
0<(x−x0)2+(y−y0)2+(z−z0)2
The function is continuous at the point P0(x0,y0,z0) if
f(x0,y0,z0) is defined
(x,y,z)→(x0,y0,z0)limf(x,y,z) exists
(x,y,z)→(x0,y0,z0)limf(x,y,z)=f(x0,y0,z0)
11.3 Partial Derivatives
Partial Differentiation
The process of differentiating a function of several variables with respect to one of its variables while keeping the other variable(s) fixed is called partial differentiation, and the resulting derivative is a partial derivative of the function.
If z=f(x,y), then the partial derivatives of f with respect to x and y are the functions fx and fy, respectively, defined by
fx(x,y)=Δx→0limΔxf(x+Δx,y)−f(x,y)
and
fy(x,y)=Δy→0limΔyf(x,y+Δy)−f(x,y)
provided the limits exist.
This means that we find the partial derivative with respect to x by regarding y as a constant while differentiating the function with respect to x. Similarly, the partial derivative with respect to y is found by regarding x as a constant while differentiating the function with respect to y.
Alternate notation for partial derivatives for z=f(x,y)
fx(x,y)=∂x∂f=∂x∂z=∂x∂f(x,y)=zx=Dx(f)
and
fy(x,y)=∂y∂f=∂y∂z=∂y∂f(x,y)=zy=Dy(f)
Calculate the partial derivative of an implicitly defined function
∂x∂z=fz−fx
where fx=0.
Higher-Order Partial Derivatives
The partial derivative of a function is a function, so it is possible to take the partial derivative of a partial derivative. If we take two consecutive partial derivatives with respect to the same variable, the resulting derivative is called the second-order partial. We can also take a second partial derivative with respect to a different variable,producing what is called a mixed second-order partial derivative.