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
Because we assume f to be bounded function, there exists a lower and upper bound on the interval [a,b]. 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.