Riemann Integral
The Riemann Integral was the first formal definition of an integral, defined by Bernhard Riemann in 1854. Gaston Darboux developed a simpler approach to the Riemann Integral in 1875 (source needed), that I’ll be using in this section.
Partitions
A partition serves to chop up our interval [a,b] into fintely many subintervals [x_{i-1},x_{i}]. We notate the length of the i^{th} sub-interval in our partition with \Delta x_i = x_i - x_{i-1}.
Darboux sums
The upper (lower) sums are defined as the sum of the product of the supremum (infimum) of each subinterval multiplied by the length of the subinterval.
Because we assume f to be bounded function, there exists a lower and upper bound of the function on the interval [a,b]. This also implies the existence of a supremum and infimum, so we know our upper and lower sums exist.
Call these bounds m,M respectively (No relation to m_i,M_i). For any partition P of [a,b] we have m(b-a) \leq L(f,p) \leq U(f,p) \leq M(b-a).
Thus we know the upper and lower sums for f exist, and form a bounded set.
Riemann Integral
If a function is Riemann integrable, then the value of the integral on [a,b] will be equal to the signed area between the function and the x-axis.
Essentially this Corollary states that every lower sum will be less than any upper sum.
Not every function is going to be Riemann integrable.