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The Center strives for synergy of theory, experimentation, and simulation, building upon service to the present-day needs of AFRD and other accelerator programs while looking toward subsequent generations of accelerators. Contact Center Head John Corlett or visit the Center for Beam Physics website. |
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Beam instrumentation and radiofrequency beam manipulations are longtime strengths of the Center, and are applied to both near- and long-term needs of high-energy physics. A major 2006 accomplishment was completion of the R&D phase of the prototype bunch-by-bunch luminosity monitor for the Large Hadron Collider. It has to give 1% resolution of the luminosity of bunches only 25 nanoseconds apart and survive intense radiation. Engineering of the final version is underway. |
Looking ahead to long-term HEP objectives, the Center continues its leadership role in R&D for a muon collider/neutrino factory. This work evaluates feasibility of technical approaches to an advanced muon storage ring to support research in neutrino science. A high-intensity muon storage ring is generally viewed as the ideal source of such neutrinos. LBNL is the lead laboratory in the Neutrino Factory and Muon Collider Collaboration, and also has key technical involvement in the Muon Ionization Cooling Experiment (MICE).
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A 201-MHz RF cavity for the Muon Ionization-Cooling Experiment is another recent achievement. Cooling the beam (making it more orderly prior to further acceleration) is both important to the success of a muon collider/neutrino factory and very challenging. Free muons are short-lived (about two microseconds in the laboratory frame of reference). By contrast, electron and ion colliders can store their beams for hours, in which time it makes millions of turns around the collider ring. A muon beam must be cooled sufficiently within a small fraction of that few microsecondsone of many technical challenges of such a collider. If a muon-based accelerator were built in the US, LBNL would desire and expect to play a major role, with responsibility for a major subsystem, such as the front end or perhaps the storage ring. |
In another effort, parlaying experience with front end systems for the the Spallation Neutron Source into benefits to high-energy physics, we and colleagues in the Ion Beam Technology Program are beginning to study certain aspects of a proton driver for neutrino studies. These aspects include low-level radiofrequency control sysems, rebuncher cavities, and the electron cloud effect. The future scope of these studies could include end-to-end physics modelinga capability that illustrates the ever-increasing integration of modeling and advanced computing into accelerator design.
Center for Beam Physics staff also have a tradition of making strong technical and scientific-leadership contributions outside the realm of high-energy physics, such as synchrotron light sources. In earlier years, the Center played pivotal roles in the design, construction and commissioning of the Advanced Light Source (ALS). This knowledge benefitted high-energy physics by way of PEP-II, the B-meson factory at the Stanford Linear Accelerator Center.
When that collaboratively built project became complete and operational, the Center's scientists and engineers brought the expertise back to LBNL, contributing beam dynamics, rf, and feedback systems to the ongoing enhancement and operational improvement of the Advanced Light Source, for example. While continuing to support the ALS, they are now working on accelerator physics and technologies necessary for next- generation synchrotron radiation sources. High repetition rate is a major focus of this work, as are free-electron lasers with output in the vacuum ultraviolet (VUV) and soft X ray regions of the spectrum.
The production of ultrafast beam pulses and the synchronization of lasers with them is another area of great interest for both our researchers and potential user communities as we evaluate the possibilities for a next-generation LBNL light source with characteristics beyond even the ALS. We are also collaborating with other institutions on such projects as FERMI@Elettra and the current-enhanced free-electron laser concept (E-SASE) for the Linac Coherent Light Source at the Stanford Linear Accelerator Center; a common theme of this and several other investigations is optical modification and control of electron beams.
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A still-evolving example of the synergy between groups within the Center, and of the spinoff benefits for various fields, is the study of the electron-cloud effect. The ECE is a consequence of the complicated interplay between the beam and the vacuum chamber. Clouds of electrons are generated from the chamber walls, whereupon they interfere with beams and systems in several ways. | |
With the aid of colleagues at LBNL (especially the National Energy Research Supercomputing Center and the Computational Research Department) and elsewhere, AMAC advances these capabilities and applies them to a wide variety of problems in present-day and next-generation accelerators. Theirs is a key element in the mutually supporting combination of experiment, theory, and simulation that helps the Center advance in its own endeavors and assist the work of others.
This ability to better predict, understand, and control makes accelerators both more effective and more cost-effective, with benefits to both high-energy physics and to other accelerator-based sciences such as inertial fusion energy. Besides the information available on their own website, AMAC is especially featured in CBP's chapter of the Research Highlights this year.
The Center's website has links to its groups and related endeavors.
The research on laser-plasma accelerators, born as the Centers LOASIS Group (Laser and Optical Accelerator Systems Integrated Studies), has been an AFRD program in its own right since May 2005.
Joe Chew
is responsible for this WWW document. Christine Celata is the cognizant supervisor. To
report technical problems, e-mail the www-afrd webmaster.
Draft corrected by CBP program head John Corlett 9/22/06.
Administrative and legal information on the AFRD homepage is applicable to this page.