Assume a dilute nondegenerate ideal mixture in thermal and chemical equilibrium, electrical neutrality Ne=Np, and ground-state hydrogen only. Choose the zero of internal energy as a separated proton and electron, so the atom has energy −R. Its single-particle partition function contains eR/(kBT):Their ratio has one remaining power of V. Neglecting binding mass in mH≃mp makes the translational mass factor (memp/mH)3/2≃me3/2. For unresolved ground-state spin states, gegp/gH=1: including proton spin gives 2×2/4, or omitting it consistently gives 2×1/2. The given law of mass action therefore yieldsThis is the Saha equation with the degeneracy convention used by the source. Equivalently ne2/nH=(2πmekBT/h2)3/2e−R/(kBT).
Zsp,e=geV(h22πmekBT)3/2,Zsp,p=gpV(h22πmpkBT)3/2,
Zsp,H=gHV(h22πmHkBT)3/2eR/(kBT).
NHNe2=V(h22πmekBT)3/2e−R/(kBT).
Define fractional ionization as x=np/(nH+np) and use electrical neutrality. For x=0.01 and ne=109m−3, nH=(1−x)ne/x=99ne. Thus the density form of the Saha equation requiresSolving this monotone equation, conveniently after taking its logarithm, givesThe thermal energy is only about 2.2% of the 13.6 eV ionization energy. Ionization is not decided by setting kBT=R: the high-energy tail and the large translational state-count factor in chemical equilibrium allow a residual ionized fraction at a much lower temperature. This is the equilibrium estimate for the stipulated density and fraction, without inferring an expansion age from it.
(h22πmekBT)3/2e−13.6eV/(kBT)=99ne≃1.01×107m−3.
T≃3.48×103K,kBT≃0.300eV.
Low excited states lie many thermal energies above the ground state at the inferred temperature, so their contributions to the atomic internal partition function are exponentially suppressed. For hydrogen, E2−E1=10.2 eV and the level degeneracy ratio is g2/g1=4. HenceThe ground-state approximation is therefore excellent for this level under the assumed thermal-equilibrium conditions. A formal sum over infinitely many isolated-atom Rydberg states needs a physical high-level cutoff in a plasma; it should not be used to overturn the finite-level Boltzmann estimate. Radiation-driven nonequilibrium populations would require a different model.
Nn=1Nn=2=4e−10.2eV/(kBT)≃6.8×10−15.
Ancestors (10)
- S16
- 2012
- Past exam of the short options paper shared by Prelims and Parts A and B of the physics course of the University of Oxford
- Short options paper shared by Prelims and Parts A and B of the physics course of the University of Oxford
- Physics course of the University of Oxford
- Undergraduate course of the University of Oxford
- Course of the University of Oxford
- University of Oxford
- List of universities
- Home
Discussion (0)
New discussionThere are no discussions about this article yet.
Articles by others on the same topic (0)
There are currently no matching articles.