(a) Consider the ionization of atomic hydrogen, governed by the equation
H⇌p++e−,(22.104)
where p+ is a proton (equivalently a positively ionized hydrogen) and e− is an electron. Explain why
μH=μp+μe.(22.105)
Using the partition function for hydrogen atoms from eqn 21.50, and using eqn 22.103, show that
−kBTlnNpZ1p−kBTlnNeZ1e=−kBTlnNHZ1HeβR,(22.106)
where Z1x and Nx are the single-particle partition function and number of particles for species x respectively, and where R=13.6eV. Hence show that
nHnenp=h3(2πmekBT)3/2e−βR,(22.107)
where nx=Nx/V is the number density of species x, stating any approximations you make. Equation 22.107 is known as the Saha equation.
(b) Explain why charge neutrality implies that ne=np and conservation of nucleons implies nH+np=n, where n is the total number density of hydrogen (neutral and ionized). Writing y=np/n as the degree of ionization, show that
1−yy2=nλth3e−βR,(22.108)
where λth is the thermal wavelength for the electrons. Find the degree of ionization of a cloud of atomic hydrogen at 1000K and density 1020m−3.
(c) Equation 22.108 shows that the degree of ionization goes up when the density n goes down. Why is that?