Time Dilation is a fascinating concept in the realm of physics, particularly in the theory of relativity proposed by Albert Einstein. It describes how time can appear to pass at different rates for observers depending on their relative velocities or gravitational fields. In special relativity, time dilation occurs due to relative motion between observers, with time slowing down as one approaches the speed of light.
In general relativity, it arises from the influence of gravity, where stronger gravitational fields cause time to pass more slowly. This phenomenon has been confirmed through various experiments and has profound implications for our understanding of time and space.
In this article, we will learn what time dilation is, we also see its derivation and solve some important questions.
What is Time Dilation?
Time dilation is the phenomenon in which two bodies moving relative to each other (or even just a different intensity of gravitational field from each other) experience different rates of time flow.
It refers to a unique situation in which time can pass at different rates in different reference frames. It also depends on the relative velocity of one reference frame to another.
In layman's terms, time dilation is the measurement of elapsed time using two clocks. In addition, the appropriate time (one-position time) and observer time are two reference frames (two-position time). Furthermore, they are intertwined, and we can determine the time dilation of one by knowing the velocity and speed of the others.
The time dilation formula is given by,
T =T0 /√1−(v2/c2)
where,
T is the time observed
T0 is the time observed at rest v is the velocity of the object
c is the velocity of light in a vacuum (3 × 108 m/s2)
Derivation of Time Dilation
To compare the time measurements in the two inertial frames quantitatively, we can link the distances into each other, then quantify each distance in terms of the pulse's time of travel in the associated reference frame. The resulting equation can then be solved for T in terms of T0
The lengths D and L are the hypotenuse s of a right triangle. The Pythagorean theorem states that
s2 = D2 + L2
The distances travelled by the light pulse and the spacecraft in time in the earthbound observer's frame are 2s and 2L, respectively. In the astronaut's frame, the length D is the distance travelled by the light pulse in time T0. This gives us three equations to work with:
2s = cT; 2L = vT; 2D = cT0
In both inertial frames, we exploited Einstein's second postulate by taking the speed of light to be c. We can now plug these results into the Pythagorean theorem's prior expression:
s2 = D2+ L2
(c × T/2)2 = (c × T0/2)2 + (v × T/2)2
Then we rearrange to obtain
(c × T)2 - (v × T)2 = (c × T0)2
Finally, solving for T in terms of T0 gives us
T =T0 /√1−(v/c)2
This is equivalent to
T = γT0,
where γ is the relativistic factor (often called the Lorentz factor) given by
γ =1/√1−(v2/c2)
and v and c are the speeds of the moving observer and light, respectively.
Problem 1: Determine the relativistic time, if T0 is 7 years and the velocity of the object is 0.55c.
Solution:
Given:
T0 = 7 years
v = 0.55c
The Formula for time dilation is given by,
T =T0 /√1−(v2/c2)
T = 7/√1-(0.55)2(32 x 1016)/32 x 1016
T = 7/√1- (0.55)2
T=7/0.8351
T = 8.38 years
Problem 2: What is γ? If v=0.650c.
Solution:
γ = 1/√1−v2/c2
=1/√1−(0.650c)/c2
= 1.32
Problem 3: A particle travels at 1.90×108m/s and lives 2.1×108s when at rest relative to an observer. How long does the particle live as viewed in the laboratory?
Solution:
Δt = Δτ/√1−v2/c2
= 2.10×10−8s/√1−(1.90×108m/s)2/(3×108m/s)2
= 2.71×10−8s
Problem 4: How does time change over 10 years travelling at a speed of 50% of that of light?
Solution:
T0 =T x√1−(v2/c2)
= 10 years x √1 - 502/1002
=10 years x √1 - 2500/10000
= 10years x √1 - 0.25
= 10years x √0.75
= 10years x 0.866
T0= 8.66 years
Problem 5: Given v = 0.95c, T0 = 10 years. Find T which is the time that the earth bound brother measures?
Solution:
T = 10/√(1- (0.95c)2/c2)
T= 10/√(1- 0.952)
T = 10/ 0.312
T = 32 years
Worksheet: Time dilation
Problem 1: An astronaut travels from Earth to a distant star at a speed of 0.8c (where ccc is the speed of light). The distance to the star is 4 light-years (ly). Calculate the time experienced by the astronaut and the time experienced by an observer on Earth. Calculate the time experienced by an observer on Earth:
Problem 2: An astronaut travels at 0.5c. How much time passes for the astronaut if 10 years pass on Earth?
Problem 3: A spaceship travels to a star 10 light-years away at 0.9c. Calculate the travel time as observed from Earth and by the astronauts on the spaceship.
Problem 4: A particle travels at 0.99c for 2 seconds as measured by an observer on Earth. How much time does the particle experience?
Problem 5: Muons with a half-life of 2.2 microseconds travel at 0.98c. What is their observed half-life on Earth?
Problem 6: Twin A stays on Earth while Twin B travels at 0.8c to a star 4 light-years away and back. Calculate the age difference when Twin B returns.
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