Riemann-Sums
Definition: Riemann Sum
Let be a real function, let be a closed interval and let .
A Riemann sum of over is any sum of the form
where and .
Note: Choice of
Different choices for yield different Riemann sums.
Definition: Left Riemann Sum
A left Riemann sum has for all .
Definition: Right Riemann Sum
A right Riemann sum has for all .
Definition: Left Riemann Sum
A middle Riemann sum has for all .
Definite Integrals
Definition: Riemann-Integrability
A real function is Riemann-integrable on the interval iff all of its Riemann sums on have the same limit as approaches .
Definition: Definite Integral
If the aforementioned limit exists, then we call it the definite integral of over .
NOTATION
The most common notation for the definite integral is
The upside of this notation is that it clearly shows where the integrand, i.e. the thing being integrated, begins and where it ends. This is not very useful when we are referring to by its name, but it helps to remove ambiguity when we substitute with an expression such as .
Its main downside is that it forces us to assign a symbol to the function’s argument which is redundant and can even be confusing in some contexts where we refer to by its name. In particular, it is irrelevant whether we write or or , hence we can shorten the notation to just
The main downside of this notation is that it implies that the order of and matters, which is not the case - what matters is the actual set which represents. To emphasise this, we can use the following notations:
In the latter case, we can also add to clarify where the integrand begins and ends, such as
All of these notations are useful in specific contexts and less so in others.
Notation: Definite Integrals with Special Bounds
A common convention is to define the notations
and
for each . This is merely notation which makes the formulation of many theorems easier and more natural.
Note: Definite Integrals over Non-Interval Domains
If is not an interval but can be represented as the union of finitely many closed intervals such that each interval overlaps with at most two other intervals and only at the endpoints, then we define the definite integral of over as the sum of ‘s definite integrals over :
Properties
Theorem: Linearity of the Definite Integral
The definite integral is linear - if and are real functions which are Riemann-integrable on , then for all
PROOF
TODO
Theorem: Integration by Parts
Let and are real functions which are defined on the closed interval and are continuously differentiable on the open interval , then they are Riemann-integrable on with
PROOF
TODO
Theorem: Substitution
Let and be real functions such that the image of is a subset of , i.e. .
If is continuous and is continuously differentiable, then the following definite Integral can be solved via substitution.
PROOF
TODO
Mean Value Theorem for Definite Integrals
Let be real functions on a closed interval .
If and are continuous and for all , then there exists some such that
PROOF
TODO
Tip:
In the case of for all , the mean value theorem simplifies to
Theorem: Integrability of the Absolute Value
Improper Integrals
Notation: Improper Integrals
An improper integral is a definite integral for a real function on an open or a semi-open interval :
- If where , the improper integral is defined through the left-sided limit
- If where , the improper integral is defined through the right-sided limit
- If where , the improper integral is defined through the limit
- If where , the improper integral is defined through the limit
- If , then for any choice of the improper integral is defined as
If the respective limit exists, then the improper integral is said to converge or simply exist. Otherwise, it diverges or does not exist.
Convergence Criteria
THEOREM
Let be Riemann-integrable on every closed interval where .
If for all and the integral converges, then also converges.
PROOF
TODO
THEOREM
Let be Riemann-integrable on every closed interval where .
If the integral converges, then also converges.
PROOF
TODO