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High Energy Polarized Proton Beams: A Modern View (Springer Tracts in Modern Physics)
 
 
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High Energy Polarized Proton Beams: A Modern View (Springer Tracts in Modern Physics) [Hardcover]

Georg Heinz Hoffstaetter (Author)

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Book Description

September 21, 2006 0387346791 978-0387346793 1

This book examines the acceleration and storage of polarized proton beams in cyclic accelerators. Basic equations of spin motion are reviewed, the invariant spin field is introduced, and an adiabatic invariant of spin motion is derived. The text presents numerical methods for computing the invariant spin field, and displays the results in numerous illustrations. This book offers a more lucid view of spin dynamics at high energy than has hitherto been available.


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This monograph begins with a review of the basic equations of spin motion in particle accelerators. It then reviews how polarized protons can be accelerated to several tens of GeV using as examples the preaccelerators of HERA, a 6.3 km long cyclic accelerator at DESY / Hamburg. Such techniques have already been used at the AGS of BNL / New York, to accelerate polarized protons to 25 GeV. But for acceleration to energies of several hundred GeV as in RHIC, TEVATRON, HERA, LHC, or a VLHC, new problems can occur which can lead to a significantly diminished beam polarization. For these high energies, it is necessary to look in more detail at the spin motion, and for that the invariant spin field has proved to be a useful tool. This is already widely used for the description of high-energy electron beams that become polarized by the emission of spin-flip synchrotron radiation. It is shown that this field gives rise to an adiabatic invariant of spin-orbit motion and that it defines the maximum time average polarization available to a particle physics experiment. These concepts make it possible to optimize a high-energy accelerator for storing highly polarized beams. The utility of the invariant spin field is illustrated by simulations of spin motion in HERA and in other high-energy accelerators. Various methods for computing the invariant spin field, the adiabatic spin invariant, and the amplitude dependent spin tune are presented. Moreover, several high-energy spin-orbit dynamical effects will be discussed which go beyond conventional models of spin dynamics and were observed in simulations with these novel methods. The book is suitable for researchers of the field and for introducing students to this field of research.

About the Author

The author teaches Physics at Cornell University and has specialized in the Physics of Beams and Accelerator Technology. He has worked in three internationally important facilities, the laboratory of elementary particle physics (LEPP) that operates the CESR e+/e- collider at Cornell University (New York State), the high energy physics laboratory DESY / Hamburg (Germany) that operates the HERA e/p collider and the nuclear physics facility NSCL / Michigan (USA). Together with colleagues from an international collaboration he has been analyzing the possibility of storing polarized protons at 920 GeV in HERA, a 6.3 km long high-energy accelerator in Hamburg, and in other large particle accelerators.


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Inside This Book (learn more)
Key Phrases - Statistically Improbable Phrases (SIPs): (learn more)
invariant spin field, stroboscopic averaging, flattening snakes, orbital tunes, transport quaternion, snake matching, snake scheme, stroboscopic average, normalized vertical amplitude, spill tune, polarized proton acceleration, snake angles, phase space amplitudes, spill motion, orbit tunes, betatron phase advance, imperfection resonances, single resonance model, spin perturbations, spin rotation angle, radiative polarization, accelerator chain, polarized proton beams, vertical optics, partial snake
Key Phrases - Capitalized Phrases (CAPs): (learn more)
Siberian Snakes, World Scientific, University of Michigan, Particle Accelerators, Polarization Team, Central Design Group, Proceedings of Polarized Protons, American Institute of Physics, Particle Accelerator School, Spin Time
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