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Atomic Energy Level Transitions

k m Photons in Astrophysics English 14 cards

Cards in this deck (14)

  1. 1Atomic Energy Level Transitionsenergy released per transition
    x
    number of atoms
    x
    likelihood of transition
  2. 2Energy Level Populationsn(l) g(l)
    --------- = -------- exp(Eu-El)/kT
    n(u) g(u)
    where g(u) is statistical weight
  3. 3Collisional Excitationcollisions between particles are important in energy level transitions - not just emission/absorption
  4. 4Einstein CoefficientsThe likelihood that an electron will transition between an upper and lower energy state is governed by the Einstein Coefficients
  5. 5- Jweighed mean intensity
    = integral (J*Phi df)
    =integral (incident field spectrum * normalised absorption profile)
  6. 6AulSpontaneous Emission Coefficient
    transition probability/time when
    electron transitions from Eu to El
  7. 7BluAbsorption Coefficient
    transition probability/time for electron transitioning from El to Eu
  8. 8Bul * Jbartransition probability/time for stimulated emission of a photon by an electron transitioning from Eu to El in the presence of an external radiation field
  9. 9Relationship Between the Coefficientsnl*Blu*Jbar = nu*Aul + nu*Bul*Jbar
  10. 10Coefficient Relationsgl*Blu = gu*Bul
    and
    Bul = c^2*Aul
    -------------
    2hf^3
  11. 11Total Flux in an Emission LineFlux is proportional to
    h*f0*nu*Aul
  12. 12Emission Line RatiosF(u1,l1) (Eu1-El1)*nu1*Au1,l1
    ------------- = ---------------------------------
    F(u2,l2) (Eu2-El2)*nu2*Au2,l2
  13. 13Origin of TransitionsE1 is the electric dipole term, the first term and dominant term . The higher order terms are M1 (magnetic dipole term), E2 (electric quadrupole term) etc.
  14. 14Forbidden TransitionsTransitions that proceed via higher order terms of the transition operator

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Photons in Astrophysics Flashcards on Atomic Energy Level Transitions, created by k m on 04/01/2019.
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