Chapter 2: Problem 192
A body is moving in \(\mathrm{x}\) direction with constant acceleration \(\alpha\). Find the difference of the displacement covered by it in nth second and \((\mathrm{n}-1)\) th second. (A) \(\alpha\) (B) \((\alpha / 2)\) (C) \(3 \alpha\) (D) \((3 / 2) \alpha\)
Short Answer
Expert verified
The difference of the displacement covered by the body in the nth second and (n-1)th second is \((\frac{3}{2})\alpha\).
Step by step solution
01
Understand the equations of motion
To solve this problem, we will use the equations of motion, which describe the relationship between the position, velocity, acceleration, and time for a body in motion.
One of the equations we will use is derived from the initial velocity(u) and acceleration(a): \(v = u + at\)Where v is the final velocity and t is the time taken.
Another equation of motion we'll use relates position(x), initial velocity(u), acceleration(a), and time(t): \(x = ut + \frac{1}{2}at^2\)
We will use these equations to calculate the position at time t and then find the difference of the displacement covered by the body in the nth second and (n-1)th second.
02
Calculate the displacement at nth second and (n-1)th second
To calculate the displacement at nth second, we can use the equation for position: \(x_n = ut_n + \frac{1}{2}\alpha t_n^2\)
Similarly, the displacement at (n-1)th second can be found using the equation for position: \(x_{n-1} = ut_{n-1} + \frac{1}{2}\alpha t_{n-1}^2\)
It's important to notice that the displacement values found in these steps represent the total displacement from the start until the end of the nth second and (n-1)th second, respectively.
03
Finding the displacement covered in nth second and (n-1)th second
To find the displacement covered during the nth and (n-1)th seconds, we need to subtract the displacement that occurred during the previous seconds.
Displacement covered during nth second: \(Δx_n = x_n - x_{n-1}\)
Displacement covered during (n-1)th second: \(Δx_{n-1} = x_{n-1} - x_{n-2}\)
04
Calculate the difference of the displacement
Now, we can find the difference of the displacements covered during the nth second and (n-1)th second:
\(Δx = Δx_n - Δx_{n-1}\)
Substituting the values from Step 3:
\(Δx = (x_n - x_{n-1}) - (x_{n-1} - x_{n-2})\)
Using the position equations from Step 2:
\(Δx = {(ut_n + \frac{1}{2}\alpha t_n^2) - (ut_{n-1} + \frac{1}{2}\alpha t_{n-1}^2)} - {(ut_{n-1} + \frac{1}{2}\alpha t_{n-1}^2) - (ut_{n-2} + \frac{1}{2}\alpha t_{n-2}^2)}\)
Simplify the equation:
\(Δx = {u(t_n - t_{n-1}) + \frac{1}{2}\alpha (t_n^2 - t_{n-1}^2)} - {u(t_{n-1} - t_{n-2}) + \frac{1}{2}\alpha (t_{n-1}^2 - t_{n-2}^2)}\)
Since the time intervals are 1 second each:
\(Δx = {u(1) + \frac{1}{2}\alpha (n^2 - (n-1)^2)} - {u(1) + \frac{1}{2}\alpha ((n-1)^2 - (n-2)^2)}\)
Simplifying further:
\(Δx = {\frac{1}{2}\alpha (n^2 - (n-1)^2 - (n-1)^2 + (n-2)^2)}\)
Expanding and simplifying the terms:
\(Δx = {\frac{1}{2}\alpha (2 - 3n + n^2 + n^2 - 4n + 4)}\)
05
Determine the answer from the equation
After simplification, we have:
\(Δx = {(\frac{3}{2})\alpha}\)
This corresponds to option (D). Therefore, the difference of the displacement covered by the body in the nth second and (n-1)th second is \((\frac{3}{2})\alpha\).
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Key Concepts
These are the key concepts you need to understand to accurately answer the question.
Constant Acceleration
In the world of physics, constant acceleration plays a significant role when analyzing motion. Constant acceleration means that the rate of change of velocity stays the same over time. Whether an object is speeding up or slowing down, the magnitude of its acceleration does not vary.
This concept is crucial as it simplifies how we can predict the motion of objects. When acceleration is constant, it allows us to use a set of equations known as the equations of motion to calculate different properties of motion.
Here's why constant acceleration is important:
This concept is crucial as it simplifies how we can predict the motion of objects. When acceleration is constant, it allows us to use a set of equations known as the equations of motion to calculate different properties of motion.
Here's why constant acceleration is important:
- It allows for the prediction of future motion.
- It makes calculations straightforward since the acceleration value doesn’t change.
- It applies to a wide range of practical scenarios, from vehicles on a straight road to objects in free fall.
Displacement Calculation
Displacement is a key concept in kinematics. It refers to the change in position of an object and is a vector quantity, meaning it has both magnitude and direction. In our problem, we're looking to calculate the difference in displacement for a moving body. This process involves leveraging the equation of motion that relates initial velocity, acceleration, and time.
When calculating displacement, especially with constant acceleration, you'll use the equation:
When calculating displacement, especially with constant acceleration, you'll use the equation:
- For displacement at a specific second, you have: \(x = ut + \frac{1}{2}at^2\)
- Here, \(u\) represents initial velocity, \(a\) is acceleration, and \(t\) is time elapsed.
Kinematics
Kinematics is a branch of physics that focuses on the geometry of motion without taking into consideration the forces causing it. It describes how objects move using equations that relate time, displacement, velocity, and acceleration.
The foundational principles of kinematics involve several key equations known as the equations of motion:
The foundational principles of kinematics involve several key equations known as the equations of motion:
- Velocity-time equation: \(v = u + at\)
- Displacement-time equation: \(x = ut + \frac{1}{2}at^2\)
- Velocity-displacement equation: \(v^2 = u^2 + 2ax\)
Physics Problem Solving
Physics problem solving often requires a methodical approach. When faced with a problem like the one provided, involving motion and time, it's critical to identify which physics concepts and models apply.
Here’s a simple approach to solving such problems:
Here’s a simple approach to solving such problems:
- Break down the problem into smaller parts.
- Identify known and unknown variables.
- Choose the right equations that link these variables.
- Solve step by step, checking units and results at each stage.