2000
DOI: 10.1134/1.626826
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Study of parameters of the angular distribution of photoelectrons in the relativistic quadrupole approximation

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Cited by 7 publications
(2 citation statements)
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“…Here σ i is the total photoionization cross section for the ith atomic shell, β is the asymmetry parameter of the photoelectron angular distribution, which depends on the photon energy and on quantum numbers of the ith atomic shell, P 2 (cos θ) is the second-order Legendre polynomial and θ is the angle between the vectors of propagation of photon k and photoelectron p. However in a number of papers [4][5][6][7][8][9][10][11][12][13][14][15][16][17][18] the angular distribution has been demonstrated to differ essentially from that calculated within the dipole approximation even for low photoelectron kinetic energies just above the photoionization threshold. In [4][5][6][7][8][9] the influence of quadrupole terms on the angular distribution has been studied using the nonrelativistic treatment.…”
Section: Introductionmentioning
confidence: 99%
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“…Here σ i is the total photoionization cross section for the ith atomic shell, β is the asymmetry parameter of the photoelectron angular distribution, which depends on the photon energy and on quantum numbers of the ith atomic shell, P 2 (cos θ) is the second-order Legendre polynomial and θ is the angle between the vectors of propagation of photon k and photoelectron p. However in a number of papers [4][5][6][7][8][9][10][11][12][13][14][15][16][17][18] the angular distribution has been demonstrated to differ essentially from that calculated within the dipole approximation even for low photoelectron kinetic energies just above the photoionization threshold. In [4][5][6][7][8][9] the influence of quadrupole terms on the angular distribution has been studied using the nonrelativistic treatment.…”
Section: Introductionmentioning
confidence: 99%
“…In [4][5][6][7][8][9] the influence of quadrupole terms on the angular distribution has been studied using the nonrelativistic treatment. The quadrupole approximation has also been used in relativistic computations [15][16][17]. Advantage has been taken of the next octopole approximation in [18].…”
Section: Introductionmentioning
confidence: 99%