To find the radiation pressure on the object due to the electromagnetic wave, we start by understanding the concept of radiation pressure in physics. Radiation pressure is exerted upon any surface due to the exchange of momentum between the object and the incident electromagnetic wave. The formula to calculate radiation pressure \(P\) when the wave is completely absorbed is given by:
\(P = \frac{I}{c}\)
where:
Since the medium's refractive index is given as \(3\), the speed of light in the medium \(c_m\) is:
\(c_m = \frac{c}{n} = \frac{3 \times 10^8 \, \text{m/s}}{3} = 1 \times 10^8 \, \text{m/s}\)
Now, substitute the values into the radiation pressure formula:
\(P = \frac{6 \times 10^8 \, \text{W/m}^2}{1 \times 10^8 \, \text{m/s}} = 6 \, \text{Nm}^{-2}\)
Thus, the radiation pressure exerted on the object is \(6 \, \text{Nm}^{-2}\).
The radiation pressure \( P \) is given by:
\(P = \frac{I \cdot \mu}{c},\)
where:
- \( I \) is the intensity of the radiation,
- \( \mu \) is the absorption coefficient (fraction of radiation absorbed, here \( \mu = 1 \) for total absorption),
- \( c \) is the speed of light in a vacuum.
Substitute the given values:
- \( I = 6 \times 10^8 \, \text{W/m}^2 \),
- \( \mu = 3 \),
- \( c = 3 \times 10^8 \, \text{m/s} \).
Calculate \( P \):
\(P = \frac{I \cdot \mu}{c} = \frac{6 \times 10^8 \cdot 3}{3 \times 10^8}.\)
Simplify:
\(P = 6 \, \text{N/m}^2.\)
The Correct answer is: \(6 \, \text{Nm}^{-2}\)
Given below are two statements: one is labelled as Assertion (A) and the other is labelled as Reason (R).
Assertion (A): Electromagnetic waves carry energy but not momentum.
Reason (R): Mass of a photon is zero. In the light of the above statements.
choose the most appropriate answer from the options given below:
The dimension of $ \sqrt{\frac{\mu_0}{\epsilon_0}} $ is equal to that of: (Where $ \mu_0 $ is the vacuum permeability and $ \epsilon_0 $ is the vacuum permittivity)
Let one focus of the hyperbola \( H : \dfrac{x^2}{a^2} - \dfrac{y^2}{b^2} = 1 \) be at \( (\sqrt{10}, 0) \) and the corresponding directrix be \( x = \dfrac{9}{\sqrt{10}} \). If \( e \) and \( l \) respectively are the eccentricity and the length of the latus rectum of \( H \), then \( 9 \left(e^2 + l \right) \) is equal to:
