Difference between revisions of "Thermodynamics of Black-Body Radiation"
Line 19: | Line 19: | ||
<div id="bbrazm2"></div> | <div id="bbrazm2"></div> | ||
<div style="border: 1px solid #AAA; padding:5px;"> | <div style="border: 1px solid #AAA; padding:5px;"> | ||
− | === Problem | + | === Problem 2 === |
Find number of photons in black-body radiation of temperature $T$ in volume $V$, which have frequencies in the interval $\left[ \omega ,\omega +d\omega \right]$. | Find number of photons in black-body radiation of temperature $T$ in volume $V$, which have frequencies in the interval $\left[ \omega ,\omega +d\omega \right]$. | ||
<div class="NavFrame collapsed"> | <div class="NavFrame collapsed"> | ||
Line 32: | Line 32: | ||
<div id="bbrazm3"></div> | <div id="bbrazm3"></div> | ||
<div style="border: 1px solid #AAA; padding:5px;"> | <div style="border: 1px solid #AAA; padding:5px;"> | ||
− | === Problem | + | === Problem 3 === |
Find total photon number of black body radiation in volume $V$ at temperature $T$. | Find total photon number of black body radiation in volume $V$ at temperature $T$. | ||
<div class="NavFrame collapsed"> | <div class="NavFrame collapsed"> | ||
Line 45: | Line 45: | ||
<div id="cmb_td_1"></div> | <div id="cmb_td_1"></div> | ||
<div style="border: 1px solid #AAA; padding:5px;"> | <div style="border: 1px solid #AAA; padding:5px;"> | ||
− | === Problem | + | === Problem 4 === |
Estimate number of photons in a gas oven at room temperature and at maximum heat. | Estimate number of photons in a gas oven at room temperature and at maximum heat. | ||
<div class="NavFrame collapsed"> | <div class="NavFrame collapsed"> | ||
Line 58: | Line 58: | ||
<div id="bbrazm4"></div> | <div id="bbrazm4"></div> | ||
<div style="border: 1px solid #AAA; padding:5px;"> | <div style="border: 1px solid #AAA; padding:5px;"> | ||
− | === Problem | + | === Problem 5 === |
Find energy of photons in black-body radiation of temperature $T$ in volume $V$, which have frequencies in the interval $\left[ \omega ,\omega +d\omega \right]$. | Find energy of photons in black-body radiation of temperature $T$ in volume $V$, which have frequencies in the interval $\left[ \omega ,\omega +d\omega \right]$. | ||
<div class="NavFrame collapsed"> | <div class="NavFrame collapsed"> | ||
Line 71: | Line 71: | ||
<div id="bbrazm5"></div> | <div id="bbrazm5"></div> | ||
<div style="border: 1px solid #AAA; padding:5px;"> | <div style="border: 1px solid #AAA; padding:5px;"> | ||
− | === Problem | + | === Problem 6 === |
Calculate free energy, entropy and total energy of black-body radiation. | Calculate free energy, entropy and total energy of black-body radiation. | ||
<div class="NavFrame collapsed"> | <div class="NavFrame collapsed"> | ||
Line 84: | Line 84: | ||
<div id="bbrazm6"></div> | <div id="bbrazm6"></div> | ||
<div style="border: 1px solid #AAA; padding:5px;"> | <div style="border: 1px solid #AAA; padding:5px;"> | ||
− | === Problem | + | === Problem 7 === |
Calculate thermal capacity of black-body radiation. | Calculate thermal capacity of black-body radiation. | ||
<div class="NavFrame collapsed"> | <div class="NavFrame collapsed"> | ||
Line 97: | Line 97: | ||
<div id="bbrazm7"></div> | <div id="bbrazm7"></div> | ||
<div style="border: 1px solid #AAA; padding:5px;"> | <div style="border: 1px solid #AAA; padding:5px;"> | ||
− | === Problem | + | === Problem 8 === |
Find pressure of black-body radiation and construct its state equation. | Find pressure of black-body radiation and construct its state equation. | ||
<div class="NavFrame collapsed"> | <div class="NavFrame collapsed"> | ||
Line 110: | Line 110: | ||
<div id="bbrazm8"></div> | <div id="bbrazm8"></div> | ||
<div style="border: 1px solid #AAA; padding:5px;"> | <div style="border: 1px solid #AAA; padding:5px;"> | ||
− | === Problem | + | === Problem 9 === |
Find adiabate equation for the photon gas of black-body radiation. | Find adiabate equation for the photon gas of black-body radiation. | ||
<div class="NavFrame collapsed"> | <div class="NavFrame collapsed"> | ||
Line 123: | Line 123: | ||
<div id="cmb3"></div> | <div id="cmb3"></div> | ||
<div style="border: 1px solid #AAA; padding:5px;"> | <div style="border: 1px solid #AAA; padding:5px;"> | ||
− | === Problem | + | === Problem 10 === |
Why CMB cannot be used to warm up food like in the microwave oven? | Why CMB cannot be used to warm up food like in the microwave oven? | ||
<div class="NavFrame collapsed"> | <div class="NavFrame collapsed"> | ||
Line 137: | Line 137: | ||
<div id="cmb6"></div> | <div id="cmb6"></div> | ||
<div style="border: 1px solid #AAA; padding:5px;"> | <div style="border: 1px solid #AAA; padding:5px;"> | ||
− | === Problem | + | === Problem 11 === |
The binding energy of electron in the hydrogen atom equals to $13.6\ | The binding energy of electron in the hydrogen atom equals to $13.6\ | ||
eV$. What is the temperature of Planck distribution, with this | eV$. What is the temperature of Planck distribution, with this |
Revision as of 19:50, 1 October 2012
Problem 1
Show that the photon gas in thermal equilibrium has zero chemical potential.
Problem 2
Find number of photons in black-body radiation of temperature $T$ in volume $V$, which have frequencies in the interval $\left[ \omega ,\omega +d\omega \right]$.
Problem 3
Find total photon number of black body radiation in volume $V$ at temperature $T$.
Problem 4
Estimate number of photons in a gas oven at room temperature and at maximum heat.
Problem 5
Find energy of photons in black-body radiation of temperature $T$ in volume $V$, which have frequencies in the interval $\left[ \omega ,\omega +d\omega \right]$.
Problem 6
Calculate free energy, entropy and total energy of black-body radiation.
Problem 7
Calculate thermal capacity of black-body radiation.
Problem 8
Find pressure of black-body radiation and construct its state equation.
Problem 9
Find adiabate equation for the photon gas of black-body radiation.
Problem 10
Why CMB cannot be used to warm up food like in the microwave oven?
The relic radiation, or CMB, corresponds to the black-body radiation with temperature $T_{CMB}=2.725\:K.$ According to the main principle of thermodynamics, heat cannot transfer from a less heated body to more heated one, and thus the body (food in our case), which initially had temperature $T_0>T_{CMB},$ will emit more energy in the environment then absorb back, until the equilibrium installs with the CMB radiation at temperature $T_{CMB}.$
Problem 11
The binding energy of electron in the hydrogen atom equals to $13.6\ eV$. What is the temperature of Planck distribution, with this average photon energy?
The Planck distribution has maximum at frequency $\omega_m = 2.822 kT/\hbar.$ Then one obtains $ kT = 13.6/2.822 = 4.82\mbox{eV}$ and $T\approx 5.6 \cdot {10^4}\mbox{K}$.