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BiBTeX citation export for THPOPT067: Propagation of Gaussian Wigner Function Through a Matrix-Aperture Beamline

@inproceedings{nash:ipac2022-thpopt067,
  author       = {B. Nash and D.T. Abell and N.B. Goldring and P. Moeller and I.V. Pogorelov},
  title        = {{Propagation of Gaussian Wigner Function Through a Matrix-Aperture Beamline}},
  booktitle    = {Proc. IPAC'22},
% booktitle    = {Proc. 13th International Particle Accelerator Conference (IPAC'22)},
  pages        = {2755--2758},
  eid          = {THPOPT067},
  language     = {english},
  keywords     = {radiation, synchrotron, emittance, synchrotron-radiation, ECR},
  venue        = {Bangkok, Thailand},
  series       = {International Particle Accelerator Conference},
  number       = {13},
  publisher    = {JACoW Publishing, Geneva, Switzerland},
  month        = {07},
  year         = {2022},
  issn         = {2673-5490},
  isbn         = {978-3-95450-227-1},
  doi          = {10.18429/JACoW-IPAC2022-THPOPT067},
  url          = {https://jacow.org/ipac2022/papers/thpopt067.pdf},
  abstract     = {{We develop a simplified beam propagation model for x-ray beamlines that includes partial coherence as well as the impact of apertures on the beam. In particular, we consider a general asymmetric Gaussian Schell model, which also corresponds to a Gaussian Wigner function. The radiation is thus represented by a 4x4 symmetric second moment matrix. We approximate rectangular apertures by Gaussian apertures, taking care that the loss in flux is the same for the two models. The beam will thus stay Gaussian through both linear transport and passage through the apertures, allowing a self-consistent picture. We derive expressions for decrease in flux and changes in second moments upon passage through the aperture. We also derive expressions for the coherence lengths and analyze how these propagate through linear transport and Gaussian apertures. We apply our formalism to cases of low emittance light source beamlines and develop a better understanding about trade-offs between coherence length increase and flux reduction while passing through physical apertures. Our formulae are implemented in RadiaSoft’s Sirepo Shadow application allowing easy use for realistic beamline models.}},
}