
Since the track is frictionless, we can use the principle of conservation of mechanical energy. At point A, the particle has potential energy and no kinetic energy, while at point B, it will have both kinetic and potential energy.
Calculate Potential Energy Difference Between Points A and B:
\( U_A + KE_A = U_B + KE_B \)
At point A, \( KE_A = 0 \) and \( U_A = mgh = mg \times 1 \). At point B, \( KE_B = \frac{1}{2}mv^2 \) and \( U_B = mg \times 0.5 \).
Setting up the equation:
\( mg \times 1 = \frac{1}{2}mv^2 + mg \times 0.5 \)
Simplify and solve for v:
\[ mg = \frac{1}{2}mv^2 + \frac{mg}{2} \]
\[ \frac{mg}{2} = \frac{1}{2}mv^2 \]
\[ v = \sqrt{g} = \sqrt{10} \, \text{m/s} \]
The problem asks for the speed of a particle at point B after it starts from rest at point A and moves along a frictionless track. We are given the initial and final heights of the particle and the acceleration due to gravity.
Since the track is frictionless and the only force doing work is gravity (which is a conservative force), the total mechanical energy of the particle is conserved. The principle of conservation of mechanical energy states that the sum of the kinetic energy (KE) and potential energy (PE) of the particle remains constant throughout its motion.
The formula for conservation of energy is:
\[ KE_{initial} + PE_{initial} = KE_{final} + PE_{final} \]where Kinetic Energy \(KE = \frac{1}{2}mv^2\) and Gravitational Potential Energy \(PE = mgh\).
Step 1: Identify the initial and final states and list the given values.
Let's set the reference level for potential energy at the bottom of the track (h=0).
Step 2: Apply the principle of conservation of mechanical energy.
The total mechanical energy at point A must be equal to the total mechanical energy at point B.
\[ \frac{1}{2}mv_A^2 + mgh_A = \frac{1}{2}mv_B^2 + mgh_B \]Step 3: Substitute the known values into the conservation of energy equation.
\[ \frac{1}{2}m(0)^2 + m(10)(1) = \frac{1}{2}mv_B^2 + m(10)(0.5) \]Step 4: Simplify the equation.
The mass \(m\) is a common factor in all terms and can be canceled out.
\[ 0 + 10(1) = \frac{1}{2}v_B^2 + 10(0.5) \] \[ 10 = \frac{1}{2}v_B^2 + 5 \]Step 5: Solve the equation for the final speed \(v_B\).
Rearrange the equation to isolate the term with \(v_B^2\):
\[ \frac{1}{2}v_B^2 = 10 - 5 \] \[ \frac{1}{2}v_B^2 = 5 \] \[ v_B^2 = 10 \] \[ v_B = \sqrt{10} \, \text{m/s} \]The speed of the particle when it reaches point B is \(\sqrt{10} \, \text{m/s}\). This corresponds to option (B).
A black body is at a temperature of 2880 K. The energy of radiation emitted by this body with wavelength between 499 nm and 500 nm is U1, between 999 nm and 1000 nm is U2 and between 1499 nm and 1500 nm is U3. The Wien's constant, b = 2.88×106 nm-K. Then,

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A force \( (3x^2 + 2x - 5) \, \text{N} \) displaces a body from \( x = 2 \, \text{m} \) to \( x = 4 \, \text{m} \). The work done by this force is _________ J.
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The reaction : \(A_2 \rightleftharpoons 2A\)