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Collimator irradiation studies in the Argonne Advanced Photon Source at energy densities expected in next-generation storage ring light sources

J. Dooling, M. Borland, W. Berg, J. Calvey, G. Decker, L. Emery, K. Harkay, R. Lindberg, G. Navrotksi, V. Sajaev, S. Shoaf, Y. P. Sun, K. P. Wootton, A. Xiao, A. Grannan, and A. H. Lumpkin
Phys. Rev. Accel. Beams 25, 043001 – Published 8 April 2022

Abstract

The Advanced Photon Source (APS) team is building a fourth-generation storage ring (4GSR), replacing the present double-bend achromat lattice with a multibend achromat system thereby allowing the production of ultrabright x-ray beams. The new lattice enables a 2-order-of-magnitude reduction in horizontal beam emittance and a factor of two increase in beam current. The result is an electron beam of very high energy and power densities. Initial predictions suggest many common ultrahigh-vacuum-compatible materials struck by the full-intensity electron beam will be damaged. Two experimental beam abort studies have been conducted on collimator test pieces in the present APS SR to inform the design of a fully-functional machine protection system for APS 4GSR operations at 200 mA. A comprehensive suite of diagnostics was utilized during the studies. The diagnostics used in these experiments are not new, but employed in different ways to obtain unique data sets. With these sets now in hand, we are developing new numerical tools to guide collimator design using pelegant [M. Borland, elegant: A flexible SDDS-compliant code for accelerator simulation, Technical Report No. LS-287, Advanced Photon Source, 2000; Y. Wang and M. Borland, Implementation and performance of parallelized elegant, in Proceedings of the 2007 Particle Accelerator Conference, http://cern.ch/AccelConf/p07/PAPERS/THPAN095.PDF, pp. 3444–3446], mars [N. V. Mokhov and S. I. Striganov, Fermilab-conf-07/008-ad, AIP Conf. Proc. 896, 50 (2007)], and flash [B. Fryxell et al., flash: An adaptive mesh hydrodynamics code for modeling astrophysical thermonuclear flashes, Astrophys. J. Suppl. Ser. 131, 273 (2000); P. Tzeferacos et al., Laboratory evidence of dynamo amplification of magnetic fields in a turbulent plasma, Nat. Commun. 9, 591 (2018)].

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  • Received 7 May 2021
  • Accepted 28 February 2022

DOI:https://doi.org/10.1103/PhysRevAccelBeams.25.043001

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Accelerators & Beams

Authors & Affiliations

J. Dooling*, M. Borland, W. Berg, J. Calvey, G. Decker, L. Emery, K. Harkay, R. Lindberg, G. Navrotksi, V. Sajaev, S. Shoaf, Y. P. Sun, K. P. Wootton, and A. Xiao

  • Advanced Photon Source, Argonne National Laboratory, 9700 South Cass Avenue, Argonne, Illinois 60439, USA

A. Grannan

  • Nuclear Science and Engineering, Argonne National Laboratory, 9700 South Cass Avenue, Argonne, Illinois 60439, USA

A. H. Lumpkin

  • Argonne Associate, Argonne National Laboratory, 9700 South Cass Avenue, Lemont, Illinois 60439, USA

  • *dooling@anl.gov

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Vol. 25, Iss. 4 — April 2022

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