for any two points and is called the FIRST DIVIDED DIFFERENCE of relative to and It is denoted by
Let us assume that the function is linear. Then is constant for any two tabular points and i.e., it is independent of and Hence,
Thus, for a linear function if we take the points and then, i.e.,
Thus,
So, if is approximated with a linear polynomial, then the value of the function at any point can be calculated by using where is the first divided difference of relative to and
is defined as SECOND DIVIDED DIFFERENCE of relative to and
If is a second degree polynomial then is a linear function of Hence,
In view of the above, for a polynomial function of degree 2, we have Thus,
This gives,
From this we obtain,
So, whenever is approximated with a second degree polynomial, the value of at any point can be computed using the above polynomial, which uses the values at three points and
0 | 1 | 2 | |
0.1 | 0.16 | 0.2 | |
1.12 | 1.24 | 1.40 |
Therefore
322.8 | 324.2 | 325 | |
2.50893 | 2.51081 | 2.5118 |
So, That is, the second divided difference remains unchanged regardless of how its arguments are interchanged.
Now, we define the divided difference.
It can be shown by mathematical induction that for equidistant points,
In general,
where and is the length of the interval for
Solution:By definition, we have
so, Now since,
we get the desired result.
where,
Further show that for
Here, is called the remainder term.
It may be observed here that the expression is a polynomial of degree and for
Further, if is a polynomial of degree then in view of the Remark 12.2.6, the remainder term, as it is a multiple of the divided difference, which is 0 .