List-I | List-II | ||
(P) | 2000 K | (1) | The radiation at peek wavelength can lead to the emission of photo e\(^-\) from a metal of work function 4 eV |
(Q) | 3000 K | (2) | The radiation at peek wavelength is visible to the human eye |
(R) | 5000K | (3) | The radiation at peek emission wavelength will result in the widest central maximum of a single slit diffraction |
(S) | 10000K | (4) | The power emitted per unit area is \(\frac{1}{16}\) of that emitted by a black body at a temperature of 6000K. |
(5) | The radiation at peak emission wavelength can be used to image human bone. |
The correct answer is : P\(\rightarrow\)3; Q\(\rightarrow\)4; R\(\rightarrow\)2; S\(\rightarrow\)1
\(\lambda\times T=b\)
\(\lambda=\frac{b}{T}\)
\(E=\frac{hc}{\lambda}=\frac{hcT}{b}\)
\(E=(\frac{hc}{eb})\times T\,eb\)
\(E=\frac{1.24\times10^{-6}}{2.9\times10^{-3}}\times T\,ev\)
\(E=(0.428\times 10^{-3}\times T)\,\,eV\)
(P) T = 2000K \(\Rightarrow\) E = 0.856eV
(Q) T = 3000K \(\Rightarrow\) E = 1.284eV
(R) T = 5000K \(\Rightarrow\) E=2.14eV
(S) T = 10000K \(\Rightarrow\) E=4.28eV
\[ \lambda_m T = b \]
For option (P) the temperature is minimum, hence \(\lambda_m\) will be maximum.
\[ \lambda_m = \frac{b}{T} = \frac{2.9 \times 10^{-3}}{2000} = 1.45 \times 10^{-6} \, \text{m} = 1450 \, \text{nm} \]
\[ \sin \theta = \frac{\lambda}{d} \]
\[ 2\theta = \text{width of central maximum} \]
\[\Rightarrow \text{width} \propto \lambda \]
\(\Rightarrow\) maximum width for (P)
\[ P \rightarrow 3 \]
For option (Q), \(T = 3000\)
\[ \lambda_m = \frac{b}{T} = \frac{2.9 \times 10^{-3}}{3000} \]
\[ \lambda_m = 0.96 \times 10^{-6} = 966.6 \, \text{nm} \]
\[ P_{3000} = 6A(3000)^4 \]
\[ P_{6000} = 6A(6000)^4 \]
\[ \frac{P_{3000}}{P_{6000}} = \left( \frac{1}{2} \right)^4 = \frac{1}{16} \]
\[ P_{3000} = \frac{1}{16} P_{6000} \]
\[ Q \rightarrow 4 \]
For (R), \(T = 5000 \, \text{K}\)
\[ \lambda_m = \frac{2.9 \times 10^{-3}}{5 \times 10^{3}} = 0.58 \times 10^{-6} = 580 \, \text{nm} \]
\(\Rightarrow\) Visible to human eyes
\[ R \rightarrow 2 \]
For (S), \(T = 10,000 \, \text{K}\)
\[ \lambda_m T = b \Rightarrow \lambda_m = \frac{2.9 \times 10^{-3}}{10,000} = 290 \, \text{nm} \]
\[ \phi = 4 \, \text{eV} \]
\[ \lambda_m = \frac{1240}{4} = 310 \, \text{nm} \]
To emit photoelectron
\[ \lambda_0 < \lambda_T \]
\(\Rightarrow S \rightarrow 1\)
The correct Answer is : P\(\rightarrow\)3; Q\(\rightarrow\)4; R\(\rightarrow\)2; S\(\rightarrow\)1
Thermodynamics in physics is a branch that deals with heat, work and temperature, and their relation to energy, radiation and physical properties of matter.
A thermodynamic system is a specific portion of matter with a definite boundary on which our attention is focused. The system boundary may be real or imaginary, fixed or deformable.
There are three types of systems:
A system undergoes a thermodynamic process when there is some energetic change within the system that is associated with changes in pressure, volume and internal energy.
There are four types of thermodynamic process that have their unique properties, and they are:
The Zeroth law of thermodynamics states that if two bodies are individually in equilibrium with a separate third body, then the first two bodies are also in thermal equilibrium with each other.
The First law of thermodynamics is a version of the law of conservation of energy, adapted for thermodynamic processes, distinguishing three kinds of transfer of energy, as heat, as thermodynamic work, and as energy associated with matter transfer, and relating them to a function of a body's state, called internal energy.
The Second law of thermodynamics is a physical law of thermodynamics about heat and loss in its conversion.
Third law of thermodynamics states, regarding the properties of closed systems in thermodynamic equilibrium: The entropy of a system approaches a constant value when its temperature approaches absolute zero.