Phys. Rev. ST Accel. Beams 8, 010701 (2005) [12 pages]

Proposed continuous wave energy recovery operation of an x-ray free electron laser

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J. Sekutowicz, S. A. Bogacz, D. Douglas, P. Kneisel, and G. P. Williams
Thomas Jefferson National Accelerator Facility (JLab), 12000 Jefferson Avenue, Newport News, Virginia 23606, USA

M. Ferrario
Istituto Nazionale di Fisica Nucleare, Via E. Fermi 40, 00044 Frascati, Italy

I. Ben-Zvi, J. Rose, J Smedley, and T. Srinivasan-Rao
Brookhaven National Laboratory, Upton, New York 11973, USA

L. Serafini
Istituto Nazionale di Fisica Nucleare, Via Celoria 16, 20133 Milan, Italy

W.-D. Möller, B. Petersen, D. Proch, and S. Simrock
Deutsches Elektronen-Synchrotron, Notkestrasse 85, 22603 Hamburg, Germany

P. Colestock
Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA

J. B. Rosenzweig
University of California Los Angeles, 405 Hilgard Avenue, Los Angeles, California 90095, USA

Received 16 December 2003; published 10 January 2005

Commissioning of two large coherent light facilities (XFELs) at SLAC and DESY should begin in 2008 and 2011, respectively. In this paper we look further into the future, hoping to answer, in a very preliminary way, two questions. First: What will the next generation of XFEL facilities look like? Believing that superconducting technology offers advantages such as high quality beams with highly populated bunches, the possibility of energy recovery and higher overall efficiency than warm technology, we focus this preliminary study on the superconducting option. From this belief the second question arises: What modifications in superconducting technology and in the machine design are needed, as compared to the present DESY XFEL, and what kind of research and development program should be proposed to arrive in the next few years at a technically feasible solution with even higher brilliance and increased overall conversion of ac power to photon beam power? In this paper we will very often refer to and profit from the DESY XFEL design, acknowledging its many technically innovative solutions.


©2005 The American Physical Society

URL: http://link.aps.org/doi/10.1103/PhysRevSTAB.8.010701
DOI: 10.1103/PhysRevSTAB.8.010701
PACS: 29.27.–a, 29.17.+w

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