Corresponding to every zeta function there is a delta series. We make use of this fact to derive an explicit formula for Riemann Prime Counting Function.
laplace transform and inverse laplace, properties, Inverse Laplace Calculatio...Waqas Afzal
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-by identification
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This chapter provides complete solution of different circuits using Laplace transform method and also provides information about applications of Laplace transforms.
laplace transform and inverse laplace, properties, Inverse Laplace Calculatio...Waqas Afzal
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-Proof of common function
-properties
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Inverse Laplace Calculations
-by identification
-Partial fraction
Solution of Ordinary differential using Laplace and inverse Laplace
This chapter provides complete solution of different circuits using Laplace transform method and also provides information about applications of Laplace transforms.
MATH 200-004 Multivariate Calculus Winter 2014Chapter 12.docxandreecapon
MATH 200-004: Multivariate Calculus Winter 2014
Chapter 12: Vector-Valued Functions
Extra Credit Scribe: Charles Burnette
Disclaimer: These notes have not been subjected to the usual scrutiny reserved for formal publications.
They may be distributed outside this class only with my permission.
These notes cover some topics in addition to what you are expected to know about vector-valued functions.
You will not be tested on material from sections 12.3 – 12.6. An extra credit quiz on the content of these
notes is available at the end. Problems marked with a ? are ‘‘for your entertainment’’ and are not essential.
12.1 Introduction to Vector-Valued Functions
In general, a function is a rule that assigns to each element in the domain an element in the range. A
vector-valued function , or vector function , is simply a function whose domain is a set of real numbers
and whose range is a set of vectors. We are most interested in vector functions r whose values are three-
dimensional vectors. This means that for every t in the domain of r there is a unique vector denoted by r(t).
If f(t), g(t), and h(t) are the components of the vector r(t), then f, g, and h are real-valued functions called
the component functions of r and we can write
r(t) = 〈f(t), g(t), h(t)〉 = f(t)i + g(t)j + h(t)k.
We use the letter t to denote the independent variable, because it represents time in most applications of
vector functions.
Example 12.1 If
r(t) =
⟨
t3, ln(3− t),
√
t
⟩
,
then the component functions are
f(t) = t3 g(t) = ln(3− t) h(t) =
√
t.
By our usual convention, the domain of r consists of all values of t for which the expression r(t) is defined.
The expressions t3, ln(3− t), and
√
t are all defined when 3− t > 0 and t ≥ 0. Therefore, the domain of r is
the interval [0, 3).
We now wish to develop a notion of what it means for a vector function r in 2-space or 3-space to
approach a limiting vector L as t approaches a number a. That is, we want to define
12-1
12-2 Chapter 12: Vector-Valued Functions
Figure 12.1: Visualization of Limits for Vector Functions
lim
t→a
r(t) = L. (12.1)
One way to motivate a reasonable definition of (12.1) is to position r(t) and L with their initial points at the
origin and interpret this limit to mean that the terminal point of r(t) approaches the terminal point of L as t
approaches a or, equivalently, that the vector r(t) approaches the vector L in both length and direction as t
approaches a (Figure 12.1). Algebraically, this is equivalent to stating that
lim
t→a
||r(t)− L|| = 0 (12.2)
(Figure 12.1). Thus, we make the following definition.
Definition 12.2 Let r(t) be a vector function that is defined for all t in some open interval containing the
number a, except that r(t) need not be defined at a. We will write
lim
t→a
r(t) = L
if and only if
lim
t→a
||r(t)− L|| = 0.
Theorem 12.3 If r has a limit at a, then this limit is unique.
Proof: Suppose that r has limits L1 and L2 at a. Let � > 0 be given, but fixe ...
Contemporary communication systems 1st edition mesiya solutions manualto2001
Contemporary Communication Systems 1st Edition Mesiya Solutions Manual
Download:https://goo.gl/DmVRQ4
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contemporary communication systems mesiya download
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Digital Tools and AI for Teaching Learning and Research
Explicit Formula for Riemann Prime Counting Function
1. Zeta and Delta Function Pairs
and an explicit formula for the
Riemann Prime Counting Function
2. Zeta and delta function pairs
We start off with some definitions. Some names here are my
creation to facilitate communication.
Unit step function:
u(t) = 1, t ≥ 0
= 0, t < 0.
Unit delta function:
δ(t)
d
dt
u(t).
Since u(t) has no derivative at t = 0, mathematicians get over the
difficulty by calling δ(t), a generalized function.
3. Laplace transform of f(t):
L{f (t)}
∞
0
f (t)e−st
dt
where it is assumed that the integral is convergent in a right half
plane of s. It is easy to verify that
L{δ(t − a)} = e−as
and
L{u(t − a)} =
e−as
s
where a is a positive contant.
7. Secondary delta function:
Secδ(t; a)
∞
m=1
1
m
δ(t − ma)
where a is a positive constant.
Secondary zeta function:
Secζ(s; a) L{Secδ(t; a)} =
∞
m=1
1
m
e−mas
= − log(1 − e−as
)
8. Prime delta function:
Priδ(t)
∞
k=1
δ(t − log log pk)
where pk is the kth
prime number.
Prime zeta function:
Priζ(s) L{Priδ(t)}
=
∞
k=1
ak
−s
where ak = log pk.
9. Super delta function:
Supδ(t)
∞
k=1
Secδ(t; ak)
Super zeta function:
Supζ(s) L{Supδ(t)} =
∞
k=1
Secζ(s; ak)
log ζ(s) =
∞
k=1
− log(1 − p−s
k ) =
∞
k=1
Secζ(s; ak)
from which it follows that
Supζ(s) = log ζ(s).
11. Hyper zeta function:
Hypζ(s) L{Hypδ(t)}
=
∞
k=1
e−s log ak
∞
m=1
1
m
e−s log m
=
∞
k=1
a−s
k
∞
m=1
m−(s+1)
Using the previously defined symbols, we get
Hypζ(s) = Priζ(s)ζ(s + 1).
12. Derivation of prime counting formula
Rewriting the just derived equation gives us
Priζ(s) = Invζ(s + 1)Hypζ(s)
an explicit form for the prime counting formula. If we take the
inverse Laplace transform, we get
Priδ(t) = e−t
Invδ(t) ∗ Hypδ(t)
where ∗ represents the convolution product.