001     53868
005     20230217124346.0
017 _ _ |a This version is available at the following Publisher URL: http://pre.aps.org
024 7 _ |a 10.1103/PhysRevE.74.027401
|2 DOI
024 7 _ |a WOS:000240238200076
|2 WOS
024 7 _ |a 2128/2237
|2 Handle
037 _ _ |a PreJuSER-53868
041 _ _ |a eng
082 _ _ |a 530
084 _ _ |2 WoS
|a Physics, Fluids & Plasmas
084 _ _ |2 WoS
|a Physics, Mathematical
100 1 _ |a Khattak, F.Y.
|b 0
|0 P:(DE-HGF)0
245 _ _ |a Comparison of experimental and simulated K-alpha yield for 400nm ultra-short laser irradiation
260 _ _ |a College Park, Md.
|b APS
|c 2006
264 _ 1 |3 online
|2 Crossref
|b American Physical Society (APS)
|c 2006-08-29
264 _ 1 |3 print
|2 Crossref
|b American Physical Society (APS)
|c 2006-08-01
300 _ _ |a 027401
336 7 _ |a Journal Article
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336 7 _ |a article
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440 _ 0 |a Physical Review E
|x 1539-3755
|0 4924
|v 74
500 _ _ |a Record converted from VDB: 12.11.2012
520 _ _ |a Ti K alpha emission yields from foils irradiated with similar to 45 fs, p-polarized pulses of a frequency-doubled Ti:sapphire laser are presented. A simple model invoking vacuum heating to predict absorption and hot electron temperature was coupled with the cross section for K-shell ionization of Ti and the Bethe-Bloch stopping power equation for electrons. The peak predicted K alpha emission was in generally good agreement with experiment. This contrasts strongly with previous work at the fundamental frequency. Similar predictions using particle-in-cell (PIC) code simulation to estimate the number and temperature of hot electrons also gave good agreement for yield.
536 _ _ |a Scientific Computing
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542 _ _ |i 2006-08-29
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|u http://link.aps.org/licenses/aps-default-license
588 _ _ |a Dataset connected to Web of Science
650 _ 7 |a J
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700 1 _ |a Percie du Sert, O.A.M.B.
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700 1 _ |a Riley, D.
|b 2
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700 1 _ |a Foster, P. S.
|b 3
|0 P:(DE-HGF)0
700 1 _ |a Divall, E. J.
|b 4
|0 P:(DE-HGF)0
700 1 _ |a Hooker, C.J.
|b 5
|0 P:(DE-HGF)0
700 1 _ |a Langley, A. J.
|b 6
|0 P:(DE-HGF)0
700 1 _ |a Smith, J.
|b 7
|0 P:(DE-HGF)0
700 1 _ |a Gibbon, P.
|b 8
|u FZJ
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773 1 8 |a 10.1103/physreve.74.027401
|b American Physical Society (APS)
|d 2006-08-29
|n 2
|p 027401
|3 journal-article
|2 Crossref
|t Physical Review E
|v 74
|y 2006
|x 1539-3755
773 _ _ |a 10.1103/PhysRevE.74.027401
|g Vol. 74, p. 027401
|p 027401
|n 2
|q 74<027401
|0 PERI:(DE-600)2844562-4
|t Physical review / E
|v 74
|y 2006
|x 1539-3755
856 7 _ |u http://dx.doi.org/10.1103/PhysRevE.74.027401
|u http://hdl.handle.net/2128/2237
856 4 _ |u https://juser.fz-juelich.de/record/53868/files/84540.pdf
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913 1 _ |k P41
|v Scientific Computing
|l Supercomputing
|b Schlüsseltechnologien
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914 1 _ |y 2006
915 _ _ |0 StatID:(DE-HGF)0010
|a JCR/ISI refereed
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920 1 _ |k ZAM
|l Zentralinstitut für Angewandte Mathematik
|d 31.12.2007
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999 C 5 |a 10.1103/PhysRevLett.59.52
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999 C 5 |a 10.1103/PhysRevA.13.1278
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|2 Crossref
999 C 5 |1 W. E. Burcham
|y 1979
|2 Crossref
|t Elements of Nuclear Physics
|o W. E. Burcham Elements of Nuclear Physics 1979
999 C 5 |a 10.1063/1.867001
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999 C 5 |a 10.1103/PhysRevE.62.R5927
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999 C 5 |a 10.1103/PhysRevLett.95.085002
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999 C 5 |a 10.1103/PhysRevE.71.016406
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