Mathematics Times – July 2019

(Ben Green) #1

SECTION-
5.Sol:


meets the parabola y x^2 at twopoints

B 1,1 and also at F  1,1.

The region, say R 1 bounded by the three curves
is a part of the given set. It is easier obtain its
area, say by horizontal than by vertical
slicing. On R 1 , y varies from 1 to 4. For each

y 0  1, 4 , the intersection of R 1 with the

liney y 0 is the segment from  y 0 ,1to

0

8
, 0
y

 
 
 

. It is shown by DE in the figure


above. Its length is^0
0

8
y
y

. Hence

4
0

(^10)
8
y dy
y
 
    
 



3 4
2
1

2
(8 log )
3

y
e
y

y y



 

16 2
8log 4
e 3 3
  

14
16 log 2
e 3
 

So A is correct.

SECTION-
5.Sol: Given an ellipse
2 2
: 2 2 1


x y
E
a b

  (1)

let us first identify the rectangle, say R,of
maximum area inscribed in E and sides parallel
to the axes of E. If a bcos , sin  is its
vertex in the first quadrant, the other vertices
are obtained by taking reflections into the axes.
So the sides of this rectangle are 2 cosa 
and 2 sinb . Hence its area is
4 absin cos  2 ab 2  which is maximum

when
4


.

So, the rectangle R of maximum area has its

vertices at ,
2 2

 a b 
  
 

.

Next, we have to find an ellipse E'with sides
parallel to those of R and having the largest
area. Clearly, the marjor and minor axes
ofE'must be the lengthand the width of R,
i.e. 2 a and 2 brespectively. So,
2 2
' : 2 2 1

2 2

x y
E
a b

 
(2)

This construction of interlacing ellipses and
rectangles then goes on. The figure above
shows the construction ofR 1 from E 1 and
E 2 fromR 1.
The crucial observation is that the lengths of
the semi-major and semi-minor axes each form
a geometric progression with common

ratio

1
2

. We have a b 1  3, 1 2. Hence for


the n th ellipse En,we have

 

1

3
2

an n (3)

and  ^1

2
2

bn n (4)

Note that the ratio of the major to the minor

axis of each ellipse is the same, as follows

3
2

.

Since the eccentricity depends only on this
ratio, (A) is immediately ruled out. Further this
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