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Inductive Definition and Structural Induction Class Notes To explain what are inductive definitions and structural induction, we start with, in section 1, a simple abstractionthe natural numbers. And then in section 2, we show how to deploy


  1. Inductive Definition and Structural Induction Class Notes To explain what are inductive definitions and structural induction, we start with, in section 1, a simple abstraction—the natural numbers. And then in section 2, we show how to deploy these techniques into data structure design and algorithm analysis, via one concrete example: linked list. 1 Natural Numbers Given the informal definitions of a natural number: a natural number is either: 1. zero; or 2. a natural number following another natural number. we can write it in an inductive definition form: n → Zero → Succ n Given this inductive definition, we write a mapping function f from a given natural number n to an integer: � 0 , if n = Zero; f ( n ) = 1 + f ( m ) , if n = Succ m. note that function f is also inductively defined. Just like ordinary integers, we can also define operations on natural num- bers. Here is the definition of addition: � if n 1 = Zero; n 2 , n 1 ⊕ n 2 = Succ ( m ⊕ n 2 ) , if n 1 = Succ m. Given the inductive definitions for natural numbers and the addition op- erations, we can now prove the 1

  2. Thm 1: f ( n 1 ⊕ n 2 ) = f ( n 1 ) + f ( n 2 ) . Proof. Induction on n 1 . Case Zero left = f (Zero ⊕ n 2 ) = f ( n 2 ) . right = f (Zero) + f ( n 2 ) = 0 + f ( n 2 ) = f ( n 2 ) . Case Succ m left = f (Succ m ⊕ n 2 ) = f (Succ ( m ⊕ n 2 )) = 1 + f ( m ⊕ n 2 ) = 1 + f ( m ) + f ( n 2 ) . right = f (Succ m ) + f ( n 2 ) = 1 + f ( m ) + f ( n 2) . QED. By making use of addition, we can define multiplication on two natural numbers n 1 and n 2 : � Zero , if n 1 = Zero; n 1 ⊗ n 2 = n 2 ⊕ ( m ⊗ n 2 ) , if n 1 = Succ m. It is left an exercise to prove that Thm 2: f ( n 1 ⊗ n 2) = f ( n 1) × f ( n 2) . As a final example, we define an equality testing function � on two natural numbers n 1 and n 2 :  Succ Zero , if n 1 = Zero ∧ n 2 = Zero;    Zero , if n 1 = Zero ∧ n 2 = Succ m ;  n 1 � n 2 = Zero , if n 1 = Succ m ∧ n 2 = Zero;    if n 1 = Succ s ∧ n 2 = Succ t.  s � t, It is also left as an exercise to prove Thm 3: f ( n 1 � n 2) = ( f ( n 1) = f ( n 2)) . 2

  3. 2 Linked List The real power of inductive definitions and structural induction is in that it can be used to define a rather large set of useful data structures, say, linked list, binary trees, red-black trees, and so on. In this section, we illustrate the main idea by studying an inductively defined linked list. Informal description: a linked list is either 1. an empty list without any data; or 2. a linked list with a head node, followed by another linked list. And write into inductive definition form: list → Empty → Cons ( T, list ) We can define a function f on list l : � 0 , if l = Empty; f ( l ) = 1 + f ( m ) , if l = Cons ( x, m ) . intuitively, f counts the length of the list l . To concatenate two lists l 1 and l 2 , we write another inductively defined function g : � if l 1 = Empty; l 2 , g ( l 1 , l 2 ) = Cons ( x, g ( m, l 2 )) , if l 1 = Cons ( x, m ) . Intuitively, list concatenation does not change the list length, this fact is represented by Thm 4: f ( g ( l 1 , l 2 )) = f ( l 1 ) + f ( l 2 ) . Proof. By induction on l 1 . Case Empty left = f ( g (Empty , l 2 )) = f ( l 2 ) . right = f (Empty) + f ( l 2 ) = f ( l 2 ) . 3

  4. Case Cons ( x, m ) left = f ( g (Cons ( x, m ) , l 2 )) = f (Cons ( x, g ( m, l 2 ))) = 1 + f ( g ( m, l 2 )) = 1 + f ( m ) + f ( l 2 ) right = f (Cons ( x, m )) + f ( l 2 ) = 1 + f ( m ) + f ( l 2 ) . QED. As a final example, if we reverse a linked list by function f : � Empty , if l = Empty; h ( l ) = g ( h ( m ) , Cons ( x, Empty)) , if l = Cons ( x, m ) . then we can prove Thm 5: f ( h ( l )) = f ( l ) . Proof left to you. 4

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