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Question: Sea of electrons, which are free electrons in conductor lattice, can be called as Fermi gas. At temp...

Sea of electrons, which are free electrons in conductor lattice, can be called as Fermi gas. At temperature TT, the de Broglie wavelength of electrons is λ\lambda. If temperature of conductor is increased by ΔT(ΔTT)\Delta T (\Delta T \ll T), then new de Broglie wavelength of electron is best given by

A

λ(1+ΔTT)\lambda \left(1+\frac{\Delta T}{T}\right)

B

λ(1ΔTT)\lambda \left(1-\frac{\Delta T}{T}\right)

C

λ(1ΔT2T)\lambda \left(1-\frac{\Delta T}{2T}\right)

D

λ(1+ΔT2T)\lambda \left(1+\frac{\Delta T}{2T}\right)

Answer

λ(1ΔT2T)\lambda \left(1-\frac{\Delta T}{2T}\right)

Explanation

Solution

The de Broglie wavelength (λ\lambda) of a particle is given by λ=hp\lambda = \frac{h}{p}, where hh is Planck's constant and pp is the momentum. The momentum is related to the kinetic energy (EkE_k) by p=2mEkp = \sqrt{2mE_k}, where mm is the mass of the particle. Thus, the de Broglie wavelength is inversely proportional to the square root of the kinetic energy: λ1Ek\lambda \propto \frac{1}{\sqrt{E_k}} For a classical gas, the average kinetic energy per particle is directly proportional to the absolute temperature: EkTE_k \propto T. Although the question mentions "Fermi gas," the options provided suggest a simplified model where the temperature dependence of the relevant electron energy follows the classical gas behavior. Therefore, we can assume: EkTE_k \propto T Combining these relationships, we get: λ1T\lambda \propto \frac{1}{\sqrt{T}} Let λ1\lambda_1 be the de Broglie wavelength at temperature T1=TT_1 = T, and λ2\lambda_2 be the new wavelength at temperature T2=T+ΔTT_2 = T + \Delta T. We can write: λ1=CT1/2\lambda_1 = C \cdot T^{-1/2} λ2=C(T+ΔT)1/2\lambda_2 = C \cdot (T + \Delta T)^{-1/2} where CC is a constant of proportionality. Now, we can express λ2\lambda_2 in terms of λ1\lambda_1: λ2=CT1/2(1+ΔTT)1/2\lambda_2 = C \cdot T^{-1/2} \left(1 + \frac{\Delta T}{T}\right)^{-1/2} λ2=λ1(1+ΔTT)1/2\lambda_2 = \lambda_1 \left(1 + \frac{\Delta T}{T}\right)^{-1/2} Given that ΔTT\Delta T \ll T, we can use the binomial approximation (1+x)n1+nx(1+x)^n \approx 1+nx for small xx. Here, x=ΔTTx = \frac{\Delta T}{T} and n=12n = -\frac{1}{2}. (1+ΔTT)1/21+(12)(ΔTT)=1ΔT2T\left(1 + \frac{\Delta T}{T}\right)^{-1/2} \approx 1 + \left(-\frac{1}{2}\right) \left(\frac{\Delta T}{T}\right) = 1 - \frac{\Delta T}{2T} Substituting this approximation back into the expression for λ2\lambda_2: λ2λ1(1ΔT2T)\lambda_2 \approx \lambda_1 \left(1 - \frac{\Delta T}{2T}\right) Thus, the new de Broglie wavelength is approximately λ(1ΔT2T)\lambda \left(1 - \frac{\Delta T}{2T}\right).