Consideration of the threshold of secondary electrons in photoelectron yield spectroscopy (PYS)
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作者:
Yagyu S.
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Advanced Electronic Materials Center, National Institute for Materials Science, Tsukuba, Ibaraki 305-0003, 3-13, SakuraAdvanced Electronic Materials Center, National Institute for Materials Science, Tsukuba, Ibaraki 305-0003, 3-13, Sakura
Yagyu S.
[1
]
Yoshitake M.
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Advanced Electronic Materials Center, National Institute for Materials Science, Tsukuba, Ibaraki 305-0003, 3-13, SakuraAdvanced Electronic Materials Center, National Institute for Materials Science, Tsukuba, Ibaraki 305-0003, 3-13, Sakura
Yoshitake M.
[1
]
Kim T.
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Advanced Electronic Materials Center, National Institute for Materials Science, Tsukuba, Ibaraki 305-0003, 3-13, SakuraAdvanced Electronic Materials Center, National Institute for Materials Science, Tsukuba, Ibaraki 305-0003, 3-13, Sakura
Kim T.
[1
]
Chikyow T.
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Advanced Electronic Materials Center, National Institute for Materials Science, Tsukuba, Ibaraki 305-0003, 3-13, SakuraAdvanced Electronic Materials Center, National Institute for Materials Science, Tsukuba, Ibaraki 305-0003, 3-13, Sakura
Chikyow T.
[1
]
机构:
[1] Advanced Electronic Materials Center, National Institute for Materials Science, Tsukuba, Ibaraki 305-0003, 3-13, Sakura
Atmospheric temperature - Secondary emission - Photoelectrons - Photons;
D O I:
10.3131/jvsj2.53.187
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摘要:
The threshold of secondary electrons in photoelectron yield spectroscopy (PYS) was examined using numerical calculations based on Fowler's formula, and was measured on a Cu(111) surface as a function of the surface temperature. In the numerical calculations, the yields are affected by surface temperature at around the threshold. The yield to the power of 1/2 shows a linear relationship of over 0.04 eV per 100 K from the threshold as a function of energy. The estimated threshold shifts to a lower energy with increasing surface temperature, by 0.003 eV per 100 K. The estimated thresholds also decrease with increasing value of the multiplier of n in Fowler's formula. In experiments, the threshold of Cu(111) at room temperature is estimated to be 4.8 eV ± 0.05 eV. The amount of change in the threshold caused by variation in surface temperature is interpreted in terms of the effects of the intrinsic Fowler's formula and lattice expansion.
机构:
Univ Gustave Eiffel, COSYS, LISIS, 5 Bd Descartes, Champs Sur Marne, France
Univ Tunis El Manar, Lab Spect Atom Mol & Applicat LSAMA, Tunis, TunisiaUniv Gustave Eiffel, COSYS, LISIS, 5 Bd Descartes, Champs Sur Marne, France
Laamiri, K.
Garcia, G. A.
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Synchrotron SOLEIL, Lorme Merisiers, St Aubin BP 48, F-91192 Gif Sur Yvette, FranceUniv Gustave Eiffel, COSYS, LISIS, 5 Bd Descartes, Champs Sur Marne, France
Garcia, G. A.
Nahon, L.
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Synchrotron SOLEIL, Lorme Merisiers, St Aubin BP 48, F-91192 Gif Sur Yvette, FranceUniv Gustave Eiffel, COSYS, LISIS, 5 Bd Descartes, Champs Sur Marne, France
Nahon, L.
Ben Houria, A.
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Univ Tunis El Manar, Lab Spect Atom Mol & Applicat LSAMA, Tunis, TunisiaUniv Gustave Eiffel, COSYS, LISIS, 5 Bd Descartes, Champs Sur Marne, France
Ben Houria, A.
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Feifel, R.
Hochlaf, M.
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Univ Gustave Eiffel, COSYS, LISIS, 5 Bd Descartes, Champs Sur Marne, FranceUniv Gustave Eiffel, COSYS, LISIS, 5 Bd Descartes, Champs Sur Marne, France