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Echidna Jim Went For A Swim

RRP $14.99

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Its a fun day at the beach for all the animals! They splash and surf and paddle and bob with their blow-up beach toys. But what will happen when prickly Echidna Jim joins in?

About the Author

Phil Cummings is a South Australian children's fiction author. Born in Port Broughton, his first book, Goodness Gracious , was published in 1989. Since then he has published over 40 children's novels.

Two of Cummings' works have been turned into theatrical productions. Windmill Performing Arts produced a production of Boom Bah! in 2008, and John Schumann composed a musical version of Danny Allen was here for the 2012 Festival of Music.


High Energy Polarized Proton Beams

RRP $629.99

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This book deals with the acceleration and storage of polarized proton beams in cyclic accelerators. Polarized proton beams with hundreds of GeV are, for example, essential for resolving the spin crisis, i.e., for understanding the angular momentum distribution inside nucleons. Experience with the Relativistic Heavy Ion Collider at the Brookhaven NationalLaboratory(RHICatBNL)hasshownthatpolarizationat205GeV can be obtained, and tests at the pre-accelerating Alternating Gradient S- chrotron(AGS)haveshownthatatleastupto24GeV, thebeampolarization canbequiteundisturbedwhentheacceleratoriswelladjusted, exceptats- cial energies where resonances occur. In particular, it has not been necessary to study closely the variation of the protons spin directions across the phase space of the beam. However, at very high energies such as in RHIC, TEVA- TRON, HERA-p, LHC, or a future VLHC, new phenomena can occur that can lead to a signi?cantly diminished beam polarization. For these high energies, it is necessary to look in more detail at the spin motion at each point in phase space, and for this the invariant spin ?eld provestobeausefultool.This?eldgivesrisetoanadiabaticinvariantofsp- orbit motion, and it de?nes the maximum time-average polarization that is usable in a particle physics experiment. Furthermore, the invariant spin ?eld allows the amplitude dependent spin tune to be de?ned and computed and thereby opens the way to a clear evaluation of the e?ects of higher-order spin orbit resonances. In particular, the strengths and the depolarizing e?ects of these resonances can only be determined once the amplitude-dependent spin tune has been computed."



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