1.2 Population inversion Absorption and Emission of radiation
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1 1.2 Population inversion Absorption and Emission of radiation Consider an atom or molecule with two energy levels, Ei and EkA direct, radiative transition between these states would be associated with a photon of frequency ν: hν = ΔE = Ek – EiEiEkMolecule in energy level EiConsider:What are the possible radiative transitions?What is the probability of a transition taking place?How does the number of photons change with the transition?
2 Three possible transitions: “Induced absorption”: Absorption and Emission of radiationThree possible transitions:“Induced absorption”:Molecule in Ei absorbs a photon and is excited to EkEiEkhνOne less photon of energy hνProbability of transition is: dPik/dt = Bik ρ(ν)dPik /dt is the probability per second of a molecule absorbing a photonBik is the Einstein coefficient of induced absorptionρ(ν) is the spectral energy density (the number of photons of frequency ν per unit volume)
3 (b) “Spontaneous emission”: Absorption and Emission of radiation(b) “Spontaneous emission”:Molecule in Ek decays spontaneously to Ei by emitting a photon in an arbitrary directionEiEkhνOne more photon of energy hν (arbitrary phase & direction)Probability of transition is dPki/dt = AkidPki /dt is the probability per second of the excited molecule emitting a photonAki is the Einstein coefficient of spontaneous emission (or the spontaneous transition probability)Spontaneous emission is not influenced by the presence of other photons in the medium
4 (c) “Induced emission” (or “stimulated emission”): Absorption and Emission of radiation(c) “Induced emission” (or “stimulated emission”):A photon of appropriate frequency induces the transition from Ekto EiEiEkhνhνOne more photon of energy hν. The new photon has the same frequency, phase, and direction at the original photonProbability of transition is dPki/dt = Bki ρ(ν)dPki /dt is the probability per second of the excited molecule emitting a photonBki is the Einstein coefficient of induced emission
5 How can we make practical use of induced emission? Absorption and Emission of radiationRelation between Bik and Bki:The Einstein coefficients of induced absorption and emission are directly related through the degeneracy, gx, of each level x:Bik = (gk/gi) BkiIn the case where each level has the same degeneracy (gi = gk), the Einstein coefficients of induced absorption and emission are identical– in other words, the probability of induced emission is the same as that of induced absorptionHow can we make practical use of induced emission?
6 Population inversionPopulation inversionA system with a population inversion is not in thermal equilibrium; populations of energy levels are not governed by the Boltzmann distributionIF we can alter the population distribution so that more molecules are in higher energy levels rather than lower energy levels, this is called population inversion.With a population inversion, photons passing through the gain medium will be amplified (by induced emission) rather than attenuated (by induced absorption).
7 Population inversionA resonator or cavity (produced by the two mirrors) is used to achieve selective feedback of some of the cavity modes in the cavity – that is, photons that travel on the axis between the mirrors are preferentially amplified over photons going in different directions:
8 I = I0 e–α z α = [Ni – (gk/gi) Nk] σ Threshold condition The probability of stimulated absorption and emission depends on the populations of the upper and lower states. With Ni molecules in level Ei and Nk molecules in level Ek , the intensity after distance z is:I = I0 e–α zwhere I0 is the initial intensity and the absorption coefficient, α, is:Here σ is the absorption cross-section and is related to Bikα = [Ni – (gk/gi) Nk] σWhen a population inversion exists (Nk > Ni) the intensity after distance z is greater than the initial intensity (I > I0).However, we also need to considerother photon losses in the cavity
9 ΔN = [(gk/gi)Nk – Ni] > (γ / 2σL) Threshold conditionPhotons may be lost in the cavity owing to transmission through the mirrors, scattering from surfaces and particles, diffraction losses, and absorption by other materials in the cavity. If all of these losses contribute to a loss coefficient, γ, then the intensity owing to cavity losses after a round trip in the cavity isI = I0 e– γFrom above, if the cavity has length L, the round trip gain (considering only the population inversion) is then:I = I0 e–2αLTo compensate for cavity losses, the threshold condition for amplification in the cavity is then:ΔN = [(gk/gi)Nk – Ni] > (γ / 2σL)
10 Can we sustain a population inversion in a given laser? Generating a population inversion“Pumping”: delivery of energy to produce a population inversionE3E4rapid relaxationE2rapid relaxationE3pumpE2pumppumplasinglasingE2lasingE1rapid relaxationE1E1Two-level systemThree-level systemFour-level systemNotes:A true two-level system cannot produce a population inversionOnly E1 is populated at thermal equilibrium (E2 >> E1)A three-level system must be pumped harder than a four-level system – that is, more molecules must be pumped into the excited level to produce lasingCan we sustain a population inversion in a given laser?
11 It is difficult to maintain a population inversion: Generating a population inversionIt is difficult to maintain a population inversion:Lasers that maintain a population inversion indefinitely produce continuous output – termed CW (for continuous wave) lasersLasers that have a short-lived population inversion produce pulsed output – these are pulsed lasersPulsed lasers may be of three types: “normal” pulsed lasers, Q-switched lasers, and mode-locked lasersPumping can be achieved either:1) optically – e.g., flashlamps (pulsed) or Hg arc lamps (CW operation)2) electrically – e.g., electric discharge in a gas and in semiconductor lasers
12 Rate equations for a four-level laser Box 3.1 (Telle)
13 Spectral characteristics of laser emission The photon emitted between two levels is not perfectly monochromatic. The linewidth is affected inter alia by:Natural lifetime (usually gives narrow linewidth)Molecular motion (Doppler broadening)Collisions (Pressure broadening, solvent effects)This linewidth results in a gain profile for the laser:Only that part of the gain profile that is above the threshold can lase.The gain profile must be considered together with the cavity modes to determine the laser spectrum