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Volumn 91, Issue 26, 2003, Pages

Fluctuations do matter: Large noise-enhanced halos in charged-particle beams

Author keywords

[No Author keywords available]

Indexed keywords

COMPUTER SIMULATION; CORRELATION METHODS; GALAXIES; MACHINE DESIGN; MATHEMATICAL MODELS; OSCILLATIONS; RESONANCE; RUNGE KUTTA METHODS; SPURIOUS SIGNAL NOISE;

EID: 1042277413     PISSN: 00319007     EISSN: 10797114     Source Type: Journal    
DOI: 10.1103/PhysRevLett.91.264801     Document Type: Article
Times cited : (20)

References (19)
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  • 4
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    • Kurennoy, S.1    Ryne, R.2
  • 8
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  • 10
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  • 12
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    • Allen, C.K.1
  • 13
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    • C.L. Bohn and I.V. Sideris, Phys. Rev. ST Accel. Beams 6, 034203 (2003); (Formula presented) is the spherically symmetric “case 5” potential of this reference. Given how Eq.� 2 is normalized, a representative size of the matched beam is (Formula presented); thus, we rescaled (Formula presented) for Model�II by 0.1 to facilitate comparing results with those of Model I.10.1103/PhysRevSTAB.6.034203
    • (2003) Phys. Rev. ST Accel. Beams , vol.6 , pp. 34203
  • 15
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    • W.H. Press et al, Numerical Recipes (Cambridge University Press, Cambridge, 1992); even with identical parameters, no two orbits are identical because the equation of motion includes randomness from the noise.
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    • Press, W.H.1


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