302 CHAPTER 13. THE GENERALIZED RIEMANN INTEGRAL

With this proposition and definition, it is time to define the generalized Riemann inte-gral. The functions being integrated typically have values inR orC but there is no reason torestrict to this situation and so in the following definition, X will denote the space in whichf has its values. For example, X could be Rp which becomes important in multivariablecalculus. For now, just think C. It will be assumed Cauchy sequences converge and thereis a norm although it is likely possible to generalize even further.

Definition 13.1.3 For a = xi−1 < · · · < xn = b, and F an increasing function, ∆Fiwill be defined as F (xi)−F (xi−1). Let X be a complete normed vector space. (For exam-ple, X = R or X = C or X = Rp.) Then f : [a,b]→ X is generalized Riemann integrable,written as f ∈ R∗ [a,b] if there exists R ∈ X such that for all ε > 0, there exists a gauge δ ,such that if P≡ {(Ii, ti)}n

i=1 is δ fine, then defining S (P, f ) by

S (P, f )≡n

∑i=1

f (ti)∆Fi,

it follows |S (P, f )−R|< ε. If such an R exists, then the integral is defined as follows.∫I

f dF ≡∫ b

af dF ≡ R.

Here |·| refers to the norm on X . For R, this is just the absolute value.

Note that if P is δ 1 fine and δ 1 ≤ δ then it follows P is also δ fine. Because of this, itfollows that the generalized integral is unique if it exists.

Proposition 13.1.4 If R, R̂ both work in the above definition of the generalized Rie-mann integral, then R̂ = R.

Proof: Let ε > 0 and let δ correspond to R and δ̂ correspond to R̂ in the above defini-tion. Then let δ 0 = min

(δ , δ̂

). Let P be δ 0 fine. Then P is both δ and δ̂ fine. Hence,∣∣R− R̂∣∣≤ |R−S (P, f )|+

∣∣S (P, f )− R̂∣∣< 2ε

Since ε is arbitrary, it follows that R = R̂.Is there a simple way to tell whether a given function is in R∗ [a,b]? The following

Cauchy criterion is useful to make this determination. It looks just like a similar conditionfor Riemann Stieltjes integration.

Proposition 13.1.5 A function f : [a,b]→ X is in R∗ [a,b] if and only if for every ε > 0,there exists a gauge function δ ε such that if P and Q are any two divisions which are δ ε

fine, then |S (P, f )−S (Q, f )|< ε.

Proof: Suppose first that f ∈ R∗ [a,b]. Then there exists a gauge, δ ε , and an element ofX , R, such that if P is δ ε fine, then |R−S (P, f )| < ε/2. Now let P,Q be two such δ ε finedivisions. Then

|S (P, f )−S (Q, f )| ≤ |S (P, f )−R|+ |R−S (Q, f )|< ε

2+

ε

2= ε.

Conversely, suppose the condition of the proposition holds. Let εn→ 0+ as n→∞ andlet δ εn denote the gauge which goes with εn. Without loss of generality, assume that δ εn

302 CHAPTER 13. THE GENERALIZED RIEMANN INTEGRALWith this proposition and definition, it is time to define the generalized Riemann inte-gral. The functions being integrated typically have values in R or C but there is no reason torestrict to this situation and so in the following definition, X will denote the space in whichf has its values. For example, X could be R? which becomes important in multivariablecalculus. For now, just think C. It will be assumed Cauchy sequences converge and thereis anorm although it is likely possible to generalize even further.Definition 13.1.3 fora= Xj] <+++ <X, = b, and F an increasing function, AF;will be defined as F (x;) — F (x;-1). Let X be a complete normed vector space. (For exam-ple, X =RorX =C or X =R?.) Then f : |a,b| > X is generalized Riemann integrable,written as f © R* [a,b] if there exists R € X such that for all € > 0, there exists a gauge 6,such that if P = {(Ij,t;) };_ is 6 fine, then defining S(P, f) bynS(PS)=Y f(t) AR,i=1it follows |S(P, f) —R| < €. If such an R exists, then the integral is defined as follows., »b[sar = | fdF =R.I aHere |-| refers to the norm on X. For R, this is just the absolute value.Note that if P is 6; fine and 6, < 6 then it follows P is also 6 fine. Because of this, itfollows that the generalized integral is unique if it exists.Proposition 13.1.4 if R,R both work in the above definition of the generalized Rie-mann integral, then R = R.Proof: Let € > 0 and let 6 correspond to R and 5 correspond to R in the above defini-tion. Then let 69 = min (6. 2) . Let P be 5g fine. Then P is both 6 and 6 fine. Hence,|R—R| <|R—S(P,f)|+|S(P,f) —R| < 2eSince € is arbitrary, it follows that R = R. |Is there a simple way to tell whether a given function is in R* [a,b]? The followingCauchy criterion is useful to make this determination. It looks just like a similar conditionfor Riemann Stieltjes integration.Proposition 13.1.5 A function f : |a,b| — X is in R* [a,b] if and only if for every € > 0,there exists a gauge function 6¢ such that if P and Q are any two divisions which are 6¢fine, then |S(P,f) S(O, f)| <.Proof: Suppose first that f € R* [a,b]. Then there exists a gauge, 5, and an element ofX, R, such that if P is d¢ fine, then |R—S(P, f)| < €/2. Now let P,Q be two such 6¢ finedivisions. ThenIS(RA)-S(OAI SISA) -RIFIR-SON|< 545 =e.Conversely, suppose the condition of the proposition holds. Let €, — 0+ as n — o andlet dg, denote the gauge which goes with €,. Without loss of generality, assume that d¢,