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We used commercially available (PHASIS, Switzerland) epitaxial gold films grown on (001)-oriented mica muscovite by rf magnetron sputtering.
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We used commercially available (PHASIS, Switzerland) epitaxial gold films grown on (001)-oriented mica muscovite by rf magnetron sputtering.
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13
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S: sound velocity, ρ : density, and Β: linear thermal expansion coefficient).
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S: sound velocity, ρ : density, and Β: linear thermal expansion coefficient).
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K ≈5× 107 W m-2 K-1 we estimate a characteristic cooling time of about 4-5 ns.
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K ≈5× 107W m-2 K-1 we estimate a characteristic cooling time of about 4-5 ns.
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The electronic contribution to the final pressure after electron-lattice equilibration is neglected due to the much smaller electronic specific heat.
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The electronic contribution to the final pressure after electron-lattice equilibration is neglected due to the much smaller electronic specific heat.
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Similar to the Bragg-peak shift (Fig.) the broadening of the rocking curves exhibits an oscillatory time dependence (large shift maximum broadening). Since each measured rocking curve represents an average over 900 pulses we attribute this mainly to the pulse-to-pulse energy fluctuations of the 400 nm pumpulse (≈20%) which result in corresponding pulse-to-pulse fluctuations of the actual Bragg-peak shift and lead to an apparent broadening of the averaged rocking curve.
-
Similar to the Bragg-peak shift (Fig.) the broadening of the rocking curves exhibits an oscillatory time dependence (large shift maximum broadening). Since each measured rocking curve represents an average over 900 pulses we attribute this mainly to the pulse-to-pulse energy fluctuations of the 400 nm pump pulse (≈20%) which result in corresponding pulse-to-pulse fluctuations of the actual Bragg-peak shift and lead to an apparent broadening of the averaged rocking curve.
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