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000041319 0247_ $$2DOI$$a10.1103/PhysRevLett.93.224801
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000041319 041__ $$aeng
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000041319 084__ $$2WoS$$aPhysics, Multidisciplinary
000041319 084__ $$2PACS$$a29.27.Bd
000041319 084__ $$2PACS$$a29.27.Hj
000041319 084__ $$2PACS$$a41.75.Ak
000041319 1001_ $$0P:(DE-HGF)0$$aLeonova, M. A.$$b0
000041319 245__ $$aAchieving 99.9% proton spin-flip efficiency at higher energy with a small rf dipole
000041319 260__ $$aCollege Park, Md.$$bAPS$$c2004
000041319 300__ $$a224801
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000041319 440_0 $$04925$$aPhysical Review Letters$$v93$$x0031-9007
000041319 500__ $$aRecord converted from VDB: 12.11.2012
000041319 520__ $$aWe recently used a new ferrite rf dipole to study spin flipping of a 2.1 GeV/c vertically polarized proton beam stored in the COSY Cooler Synchrotron in Julich, Germany. We swept the rf dipole's frequency through an rf-induced spin resonance to flip the beam's polarization direction. After determining the resonance's frequency, we varied the frequency range, frequency ramp time, and number of flips. At the rf dipole's maximum strength and optimum frequency range and ramp time, we measured a spin-flip efficiency of 99.92+/-0.04%. This result, along with a similar 0.49 GeV/c IUCF result, indicates that, due to the Lorentz invariance of an rf dipole's transverse integralBdl and the weak energy dependence of its spin-resonance strength, an only 35% stronger rf dipole should allow efficient spin flipping in the 100 GeV BNL RHIC Collider or even the 7 TeV CERN Large Hadron Collider.
000041319 536__ $$0G:(DE-Juel1)FUEK244$$2G:(DE-HGF)$$aBetrieb und Weiterentwicklung des Kühler-Synchrotrons COSY$$cM04$$x0
000041319 588__ $$aDataset connected to Web of Science
000041319 650_7 $$2INSPIRE$$ap: storage ring
000041319 650_7 $$2INSPIRE$$ap: polarized beam
000041319 650_7 $$2INSPIRE$$aspin: rotator
000041319 650_7 $$2INSPIRE$$aRF system: bending magnet
000041319 650_7 $$2INSPIRE$$abending magnet: ferromagnet
000041319 650_7 $$2INSPIRE$$apolarization: transverse
000041319 650_7 $$2INSPIRE$$aJuelich COSY PS
000041319 7001_ $$0P:(DE-HGF)0$$aKrisch, A. D.$$b1
000041319 7001_ $$0P:(DE-HGF)0$$aMorozov, V. S.$$b2
000041319 7001_ $$0P:(DE-HGF)0$$aRaymond, R. S.$$b3
000041319 7001_ $$0P:(DE-HGF)0$$aWong, V. K.$$b4
000041319 7001_ $$0P:(DE-Juel1)VDB5067$$aGebel, R.$$b5$$uFZJ
000041319 7001_ $$0P:(DE-Juel1)131234$$aLehrach, A.$$b6$$uFZJ
000041319 7001_ $$0P:(DE-Juel1)VDB964$$aLorentz, B.$$b7$$uFZJ
000041319 7001_ $$0P:(DE-Juel1)131248$$aMaier, R.$$b8$$uFZJ
000041319 7001_ $$0P:(DE-Juel1)VDB1283$$aPrasuhn, D.$$b9$$uFZJ
000041319 7001_ $$0P:(DE-Juel1)VDB5074$$aSchnase, A.$$b10$$uFZJ
000041319 7001_ $$0P:(DE-Juel1)VDB5270$$aStockhorst, H.$$b11$$uFZJ
000041319 7001_ $$0P:(DE-HGF)0$$aEversheim, D. P.$$b12
000041319 7001_ $$0P:(DE-HGF)0$$aHinterberger, F.$$b13
000041319 7001_ $$0P:(DE-HGF)0$$aUlbrich, K.$$b14
000041319 773__ $$0PERI:(DE-600)1472655-5$$a10.1103/PhysRevLett.93.224801$$gVol. 93, p. 224801$$p224801$$q93<224801$$tPhysical review letters$$v93$$x0031-9007$$y2004
000041319 8567_ $$uhttp://hdl.handle.net/2128/1663$$uhttp://dx.doi.org/10.1103/PhysRevLett.93.224801
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