World population growth. From the dawn of humanity to 1830 , world population grew to one billion people. In 100 more years (by 1930 ) it grew to two billion, and 3 billion more were added in only 60 years (by 1990 ). In 2016 , the estimated world population was 7.4 billion with a relative growth rate of 1.13 % . (A) Write an equation that models the world population growth, letting 2016 be year 0 . (B) Based on the model, what is the expected world population (to the nearest hundred million) in 2025 ? In 2033 ?
World population growth. From the dawn of humanity to 1830 , world population grew to one billion people. In 100 more years (by 1930 ) it grew to two billion, and 3 billion more were added in only 60 years (by 1990 ). In 2016 , the estimated world population was 7.4 billion with a relative growth rate of 1.13 % . (A) Write an equation that models the world population growth, letting 2016 be year 0 . (B) Based on the model, what is the expected world population (to the nearest hundred million) in 2025 ? In 2033 ?
World population growth. From the dawn of humanity to
1830
, world population grew to one billion people. In
100
more years (by
1930
) it grew to two billion, and
3
billion more were added in only
60
years (by
1990
). In
2016
, the estimated world population was
7.4
billion with a relative growth rate of
1.13
%
.
(A) Write an equation that models the world population growth, letting
2016
be year
0
.
(B) Based on the model, what is the expected world population (to the nearest hundred million) in
2025
? In
2033
?
Use the definition of continuity and the properties of limits to show that the function is continuous at the given number a.
f(x) = (x + 4x4) 5,
a = -1
lim f(x)
X--1
=
lim
x+4x
X--1
lim
X-1
4
x+4x
5
))"
5
))
by the power law
by the sum law
lim (x) + lim
X--1
4
4x
X-1
-(0,00+(
Find f(-1).
f(-1)=243
lim (x) +
-1 +4
35
4 ([
)
lim (x4)
5
x-1
Thus, by the definition of continuity, f is continuous at a = -1.
by the multiple constant law
by the direct substitution property
4 Use Cramer's rule to solve for x and t in the Lorentz-Einstein equations of special relativity:x^(')=\gamma (x-vt)t^(')=\gamma (t-v(x)/(c^(2)))where \gamma ^(2)(1-(v^(2))/(c^(2)))=1.
Pls help on both
Chapter 2 Solutions
Finite Mathematics for Business, Economics, Life Sciences, and Social Sciences (14th Edition)
University Calculus: Early Transcendentals (4th Edition)
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