2020
DOI: 10.1103/physrevlett.125.155703
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Atomic and Electronic Structure of Solid-Density Liquid Carbon

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Cited by 11 publications
(4 citation statements)
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“…35,36 Aside from photon spectroscopy and imaging experiments, the AQUA beamline will also allow for resonant inelastic X-ray scattering, electron spectroscopies, and photofragmentation measurements. 37,38 In order to reach the water window, a GeV electron beam (either from PWFA or from the X-band RF linac at full power) is sent to ten Apple-X undulators with a period of 18 mm. Those undulators will produce SASE FEL light, with typical parameters (simulated with Genesis 39 ) reported in tab.…”
Section: Aqua Beamlinementioning
confidence: 99%
“…35,36 Aside from photon spectroscopy and imaging experiments, the AQUA beamline will also allow for resonant inelastic X-ray scattering, electron spectroscopies, and photofragmentation measurements. 37,38 In order to reach the water window, a GeV electron beam (either from PWFA or from the X-band RF linac at full power) is sent to ten Apple-X undulators with a period of 18 mm. Those undulators will produce SASE FEL light, with typical parameters (simulated with Genesis 39 ) reported in tab.…”
Section: Aqua Beamlinementioning
confidence: 99%
“…Based on these almost unique features, several spectroscopical methods, employed daily at synchrotron light-sources, such as X-ray absorption (XAS), linear and circular magnetic dichroism (XMLD/XMCD) and resonant inelastic scattering (RIXS), were extended into the time-domain. Moreover, the advent of fully coherent radiation sources, such as FERMI, has allowed pushing non-linear optical spectroscopies, normally exploited exclusively at table-top light-sources in the infrared (IR) or optical regimes, into the EUV/SXR wavelengths [9][10][11][12]. Nonetheless, the next step to push the current standards in ultrafast X-ray science is strongly constrained by the possibility of designing and performing time-resolved experiments exclusively engaging EUV, SXR and HXR pulses.…”
Section: Introductionmentioning
confidence: 99%
“…Use of the Beer–Lambert law assumes negligible reflectivity at normal incidence, which holds for carbon at 300 eV (refractive index n ≈ 1). 19 The FEL photon energy is varied to probe π* (285.7 eV) and σ* (309.2 eV) regions from the 1s core state. Knowledge of the pulse envelope is essential for correctly determining the pulse intensity; the seeded FERMI FEL is known to deliver pulses with a Gaussian envelope, similar to the sin 2 envelopes commonly used in theoretical calculations.…”
mentioning
confidence: 99%
“…The observed transmission is subsequently compared to the linear Beer–Lambert law. Use of the Beer–Lambert law assumes negligible reflectivity at normal incidence, which holds for carbon at 300 eV (refractive index n ≈ 1) . The FEL photon energy is varied to probe π* (285.7 eV) and σ* (309.2 eV) regions from the 1s core state.…”
mentioning
confidence: 99%