D. Barton
Brookhaven National Laboratory
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Proceedings of the 2005 Particle Accelerator Conference | 2005
I. Ben-Zvi; Vladimir N. Litvinenko; D. Barton; D. Beavis; M. Blaskiewicz; Joseph Brennan; A. Burrill; R. Calaga; P. Cameron; Xiangyun Chang; R. Connolly; Y. Eidelman; A. Fedotov; W. Fischer; D. Gassner; H. Hahn; M. Harrison; A. Hershcovitch; H.-C. Hseuh; A. Jain; P. Johnson; D. Kayran; J. Kewisch; R. Lambiase; W. W. MacKay; G. Mahler; N. Malitsky; G. McIntyre; W. Meng; K.A.M. Mirabella
We report progress on the R&D program for electron-cooling of the Relativistic Heavy Ion Collider (RHIC). This electron cooler is designed to cool 100 GeV/nucleon at storage energy using 54 MeV electrons. The electron source will be a superconducting RF photocathode gun. The accelerator will be a superconducting energy recovery linac. The frequency of the accelerator is set at 703.75 MHz. The maximum electron bunch frequency is 9.38 MHz, with bunch charge of 20 nC. The R&D program has the following components: The photoinjector and its photocathode, the superconducting linac cavity, start-to-end beam dynamics with magnetized electrons, electron cooling calculations including benchmarking experiments and development of a large superconducting solenoid. The photoinjector and linac cavity are being incorporated into an energy recovery linac aimed at demonstrating ampere class current at about 20 MeV.
Proceedings of the 2005 Particle Accelerator Conference | 2005
I. Ben-Zvi; D. Barton; D. Beavis; M. Blaskiewicz; J.M. Brennan; A. Burrill; R. Calaga; P. Cameron; Xiangyun Chang; R. Connolly; D. Gassner; J. Grimes; H. Hahn; A. Hershcovitch; H.C. Hseuh; P. Johnson; D. Kayran; J. Kewisch; R. Lambiase; Vladimir N. Litvinenko; G. McIntyre; W. Meng; T. Nehring; A. Nicoletti; D. Pate; B. Oerter; J. Rank; T. Rao; T. Roser; T. Russo
Next generation light-sources, electron coolers, high-power FELs, Compton X-ray sources and many other accelerators were made possible by the emerging technology of high-power, high-brightness electron beams. In order to get the anticipated performance level of ampere-class currents, many technological barriers are yet to be broken. BNL’s Collider-Accelerator Department is pursuing some of these technologies for its electron cooling of RHIC application, as well as a possible future electron-hadron collider. We will describe work on CW, high-current and high-brightness electron beams. This will include a description of a superconducting, laser-photocathode RF gun and an accelerator cavity capable of producing low emittance (about 1 micron rms normalized) one nano-Coulomb bunches at currents of the order of one ampere average.
ieee particle accelerator conference | 2007
I. Ben-Zvi; J. Alduino; D. Barton; D. Beavis; M. Blaskiewicz; J.M. Brennan; A. Burrill; R. Calaga; P. Cameron; Xiangyun Chang; A. Drees; A. Fedotov; W. Fischer; G. Ganetis; D. Gassner; J. Grimes; H. Hahn; Lee Hammons; A. Hershcovitch; H.C. Hseuh; D. Kayran; J. Kewisch; R. Lambiase; D. Lederle; Vladimir N. Litvinenko; C. Longo; W. W. MacKay; G. Mahler; G. Mclntyre; W. Meng
The physics interest in a luminosity upgrade of RHIC requires the development of a cooling-frontier facility. Detailed calculations were made of electron cooling of the stored RHIC beams. This has been followed by beam dynamics simulations to establish the feasibility of creating the necessary electron beam. The electron beam accelerator will be a superconducting Energy Recovery Linac (ERL). An intensive experimental R&D program engages the various elements of the accelerator, as described by 24 contributions to the 2007 PAC.
Proceedings of the 2005 Particle Accelerator Conference | 2005
F. Pilat; L. Ahrens; M. Bai; D. Barton; J. Beebe-Wang; M. Blaskiewicz; J.M. Brennan; D. Bruno; P. Cameron; R. Connolly; J. DeLong; T. D'Ottavio; A. Drees; W. Fischer; G. Ganetis; C. Gardner; J. W. Glenn; P. Harvey; Thomas Hayes; H.C. Hseuh; H. Huang; P. Ingrassia; U. Iriso; R. Lee; Vladimir N. Litvinenko; Yun Luo; W. W. MacKay; G. Marr; A. Marusic; R. Michnoff
The 5thyear of RHIC operations, started in November 2004 and expected to last till June 2005, consists of a physics run with Cu-Cu collisions at 100 GeV/u followed by one with polarized protons (pp) at 100 GeV [1]. We will address here the overall performance of the RHIC complex used for the first time as a Cu-Cu collider, and compare it with previous operational experience with Au, PP and asymmetric d-Au collisions. We will also discuss operational improvements, such as a squeeze to 85cm in the high luminosity interaction regions from the design value of 1m, system improvements, machine performance and limitations, and address reliability and uptime issues.
ieee particle accelerator conference | 2007
A. Drees; L. Ahrens; J. Alessi; M. Bai; D. Barton; J. Beebe-Wang; M. Blaskiewicz; K.A. Brown; M. Brennan; D. Bruno; J. Butler; R. Calaga; P. Cameron; R. Connolly; T. D'Ottavio; W. Fischer; W. Fu; G. Ganetis; J. W. Glenn; M. Harvey; T. Hayes; H.C. Hsueh; H. Huang; J. Kewisch; R.C. Lee; Vladimir N. Litvinenko; Y. Luo; W. W. MacKay; G. Marr; A. Marusic
After the last successful RHIC Au-Au run in 2004 (Run-4), RHIC experiments now require significantly enhanced luminosity to study very rare events in heavy ion collisions. RHIC has demonstrated its capability to operate routinely above its design average luminosity per store of 2times1026 cm-2 s-1. In Run-4 we already achieved 2.5 times the design luminosity in RHIC. This luminosity was achieved with only 40% of the total possible number of bunches filled, and with beta* = 1 m. However, the goal is to reach 4 times the design luminosity, an average of 8times1026 cm-2 s-1, by reducing the beta* value and increasing the number of bunches to the accelerator maximum of 111. In addition, the average time at store was expected to be increased by a factor of 1.1 to about 60% of calendar time. We present an overview of the changes that increased the instantaneous luminosity, luminosity lifetime and integrated luminosity of RHIC Au-Au operations during Run-7 even though the goal of 60% time at store could not be reached.
10th European Particle Accelerator Conference, EPAC 2006 | 2006
V. Ptitsyn; L. Ahrens; M. Bai; D. Barton; J. Beebe-Wang; M. Blaskiewicz; S. Bravar; K.A. Brown; J.M. Brennan; D. Bruno; G. Bunce; R. Calaga; P. Cameron; R. Connolly; J. DeLong; T. D'Ottavio; A. Drees; A. Fedotov; W. Fischer; G. Ganetis; H. Hahn; T. Hayes; H.C. Hseuh; H. Huang; P. Ingrassia; D. Kayran; J. Kewisch; R. Lee; Vladimir N. Litvinenko; A. U. Luccio
EPAC 2008 - 11TH BIENNIAL EUROPEAN PARTICLE ACCELERATOR CONFERENCE; GENOA, ITALY; 20080623 through 20080627 | 2008
C. Montag; N. Abreu; L. Ahrens; M. Bai; D. Barton; A. Bazilevsky; J. Beebe-Wang; M. Blaskiewicz; J.M. Brennan; K.A. Brown; D. Bruno; G. Bunce; R. Calaga; P. Cameron; R. Connolly; T. D'Ottavio; A. Drees; A. Fedotov; W. Fischer; G. Ganetis; C. Gardner; J. W. Glenn; T. Hayes; H. Huang; P. Ingrassia; D. Kayran; J. Kewisch; R. Lee; Vladimir N. Litvinenko; A. Luccio
SPIN PHYSICS: 18th International Spin Physics Symposium | 2009
C. Montag; M. Bai; W. W. MacKay; T. Roser; N. Abreu; L. Ahrens; D. Barton; J. Beebe-Wang; M. Blaskiewicz; J.M. Brennan; K.A. Brown; D. Bruno; G. Bunce; R. Calaga; P. Cameron; R. Connolly; T. D Ottavio; A. Drees; A. Fedotov; W. Fischer; G. Ganetis; C. Gardner; J. W. Glenn; T. Hayes; H. Huang; P. Ingrassia; D. Kayran; J. Kewisch; R. Lee; F. Lin
Presented at | 2008
C. Gardner; R. Lee; K.A. Brown; P. Ingrassia; T. Hayes; R. Than; M. Harvey; J. Morris; E. Pozdeyev; P. Thieberger; F. Severino; V. Ptitsyn; S. Tepikian; M. Bai; G. Marr; C. Montag; T. Satogata; J. Beebe-Wang; J. Sandberg; R. Connolly; F. Pilat; G. Robert-Demolaize; A. Marusic; P. Sampson; K. Smith; S.Y. Zhang; A. Della Penna; J. Butler; D. Barton; C. Carlson
20th Russian Conference on Charged Particle Accelerators, RuPAC 2006 | 2006
D. Kayran; I. Ben-Zvi; D. Barton; D. Beavis; M. Blaskiewicz; J.M. Brennan; A. Burrill; R. Calaga; P. Cameron; Xiangyun Chang; R. Connolly; D. Gassner; H. Hahn; A. Hershcovitch; H.C. Hseuh; P. D. Johnson; J. Kewisch; R. Lambiase; Vladimir N. Litvinenko; W. Meng; G. McIntyre; T. Nehring; A. Nicoletti; D. Pate; J. Rank; T. Roser; T. Russo; J. Scaduto; K. Smith; T. Srinivasan-Rao