A microwave-plasma source generates a transient diatomic radical AB

PHYSICS · Multi-part · Fermi University Physics · Atomic, Molecular & Optical Physics · Molecular structure and spectra · Molecular structure and spectra

Deriving the Spectrum, Ch Electronic spectra of diatomic molecules

Problem

A microwave-plasma source generates a transient diatomic radical AB, and a diagnostics team records its electronic, photoelectron and Raman spectra in the same run. Treat every electronic band origin as a pure vibronic term νv′v′′=Te+G′(v′)−G′′(v′′)\nu_{v'v''}=T_e+G'(v')-G''(v'') with G(v)=ωe(v+12)−ωexe(v+12)2G(v)=\omega_e(v+\tfrac12)-\omega_ex_e(v+\tfrac12)^2, ignore rotational structure throughout, and use c=2.998×1010 cm s−1c=2.998\times10^{10}\,\mathrm{cm\,s^{-1}}, kB=8.617×10−5 eV K−1k_{\rm B}=8.617\times10^{-5}\,\mathrm{eV\,K^{-1}} and 1 cm−1=1.23984×10−4 eV1\,\mathrm{cm^{-1}}=1.23984\times10^{-4}\,\mathrm{eV}. ((a)) Nine band origins of a BB-XX system of AB, in cm−1\mathrm{cm^{-1}}, are tabulated below by upper level v′v' (rows) and lower level v′′v'' (columns): Data (band origins in cm−1\mathrm{cm^{-1}} for lower level v′′=0v''=0, 11, 22): for v′=0v'=0: 29874.2529874.25, 29034.2529034.25, 28204.2528204.25; for v′=1v'=1: 30458.2530458.25, 29618.2529618.25, 28788.2528788.25; for v′=2v'=2: 31026.2531026.25, 30186.2530186.25, 29356.2529356.25. Use row and column differences in this Deslandres table to obtain ωe′\omega_e', ωe′xe′\omega_e'x_e' (upper state) and ωe′′\omega_e'', ωe′′xe′′\omega_e''x_e'' (lower state). ((b)) Bands with v′≤5v'\le5 are Doppler-limited, of width 0.05 cm−10.05\,\mathrm{cm^{-1}}, with full fluorescence. From v′=6v'=6 upward every band suddenly broadens to 2.10 cm−12.10\,\mathrm{cm^{-1}} and its fluorescence quantum yield falls to 1.0%1.0\%, although v′=6v'=6 lies far below the dissociation limit of the BB state. Name the mechanism responsible for this onset, and find the radiative rate constant kradk_{\rm rad} and the extra non-radiative rate constant that switches on above v′=6v'=6. ((c)) A He I photoelectron spectrum of AB (hν=21.2 eVh\nu=21.2\,\mathrm{eV}) shows two bands. The first has its v′=0v'=0 line at an ionisation energy of 10.5 eV10.5\,\mathrm{eV} and only two further lines beyond it. The second has its v′=0v'=0 line at 13.0 eV13.0\,\mathrm{eV} and a long progression of at least eight further lines. Find the kinetic energy of the photoelectrons in the v′=0v'=0 line of each band, and state which of the two orbitals removed is the more strongly bonding, with your reasoning. ((d)) The same plasma is probed by Raman scattering with a 532.0 nm532.0\,\mathrm{nm} laser. At the AB vibrational shift of 840 cm−1840\,\mathrm{cm^{-1}} (the same as ΔG1/2′′\Delta G''_{1/2} found in part (a)), the Stokes line is 7.87.8 times more intense than the anti-Stokes line. Find the gas temperature.

Browse the problem library