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Aaron Axford Technical Student CERN, Geneva Nottingham Trent University Pyheadtail Comparison and Development Thanks to: Giovanni Iadarola, Giovanni Rumolo, Kevin Li Michael Schenk

Aaron Axford Technical Student CERN, Geneva Nottingham Trent University Pyheadtail Comparison and Development Thanks to: Giovanni Iadarola, Giovanni Rumolo,

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Page 1: Aaron Axford Technical Student CERN, Geneva Nottingham Trent University Pyheadtail Comparison and Development Thanks to: Giovanni Iadarola, Giovanni Rumolo,

Aaron Axford

Technical StudentCERN, Geneva

Nottingham Trent University

Pyheadtail Comparison and Development

Thanks to:Giovanni Iadarola,Giovanni Rumolo,Kevin LiMichael Schenk

Page 2: Aaron Axford Technical Student CERN, Geneva Nottingham Trent University Pyheadtail Comparison and Development Thanks to: Giovanni Iadarola, Giovanni Rumolo,

●Pyheadtail Overview

●Simulation Parameters

●Current Pyheadtail results compared with Headtail

●Comparison of Varying number of kicks

●Comparison of Varying Dt_ref

●Comparison of changing magnetic field

●Analysis of repeat simulations

Contents

Page 3: Aaron Axford Technical Student CERN, Geneva Nottingham Trent University Pyheadtail Comparison and Development Thanks to: Giovanni Iadarola, Giovanni Rumolo,

Differences for Pyheadtail from Headtail

● Presence of the chamber (Shape of the initial ecloud and an electromagnetic boundary)– Losses need to be implemented in order to

avoid unphysical motion of large amplitude electrons

● Magnetic field– For PyHDTL, B = 0.1T– For HDTL, H motion is frozen

Page 4: Aaron Axford Technical Student CERN, Geneva Nottingham Trent University Pyheadtail Comparison and Development Thanks to: Giovanni Iadarola, Giovanni Rumolo,

Current Pyheadtail results compared to Headtail

Aims● Show that the Pyheadtail model results are

comparable to Headtail

Page 5: Aaron Axford Technical Student CERN, Geneva Nottingham Trent University Pyheadtail Comparison and Development Thanks to: Giovanni Iadarola, Giovanni Rumolo,

Simulation ParametersQ26 Optics

Parameter Value

Intensity 1.5e11 ppb

Chamber Dimensions (MBB)

Chamber Dimensions (Drift)

X_aper = 6.5e-2mY_aper = 2.4e-2mX_aper = 2.8e-2mY_aper = 2.8e-2m

B_multip 1.2133e-1 Tesla

Ring Circumference 6911m

Synchrotron tune 0.059

Betatron tune (Horizontal) 26.13

Betatron tune (Vertical) 26.18

Rf voltage 2e6 V

Dh_sc 0.2e-3

Page 6: Aaron Axford Technical Student CERN, Geneva Nottingham Trent University Pyheadtail Comparison and Development Thanks to: Giovanni Iadarola, Giovanni Rumolo,

Simulation ParametersQ20 Optics

Parameter Value

Intensity 1.5e11 ppb

Chamber Dimensions (MBB)

Chamber Dimensions (Drift)

X_aper = 6.5e-2mY_aper = 2.4e-2mX_aper = 2.8e-2mY_aper = 2.8e-2m

B_multip 1.2133e-1 Tesla

Ring Circumference 6911m

Synchrotron tune 0.017

Betatron tune (Horizontal) 20.13

Betatron tune (Vertical) 20.18

Rf voltage 5.75e6 V

Dh_sc 0.2e-3

Page 7: Aaron Axford Technical Student CERN, Geneva Nottingham Trent University Pyheadtail Comparison and Development Thanks to: Giovanni Iadarola, Giovanni Rumolo,

Pyheadtail (Top) vs Headtail (Bottom)

Instability thresholdPyHDTL ≈ 4.2e11HDTL ≈ 3.6e11

Page 8: Aaron Axford Technical Student CERN, Geneva Nottingham Trent University Pyheadtail Comparison and Development Thanks to: Giovanni Iadarola, Giovanni Rumolo,

Pyheadtail (Top) vs Headtail (Bottom)

Page 9: Aaron Axford Technical Student CERN, Geneva Nottingham Trent University Pyheadtail Comparison and Development Thanks to: Giovanni Iadarola, Giovanni Rumolo,

Pyheadtail (Top) vs Headtail (Bottom)

Instability thresholdPyHDTL ≈ 3.1e11HDTL ≈ 3.2e11

Page 10: Aaron Axford Technical Student CERN, Geneva Nottingham Trent University Pyheadtail Comparison and Development Thanks to: Giovanni Iadarola, Giovanni Rumolo,

Pyheadtail (Top) vs Headtail (Bottom)

Page 11: Aaron Axford Technical Student CERN, Geneva Nottingham Trent University Pyheadtail Comparison and Development Thanks to: Giovanni Iadarola, Giovanni Rumolo,

Comparison of varying Number of kicks

Aims● Look for the effect of the number of kicks

simulated on the vertical motion and emittance– Check for any benefit using prime numbers

Page 12: Aaron Axford Technical Student CERN, Geneva Nottingham Trent University Pyheadtail Comparison and Development Thanks to: Giovanni Iadarola, Giovanni Rumolo,

Comparison of varying Number of kicks

Page 13: Aaron Axford Technical Student CERN, Geneva Nottingham Trent University Pyheadtail Comparison and Development Thanks to: Giovanni Iadarola, Giovanni Rumolo,

Comparison of varying Number of kicks

Page 14: Aaron Axford Technical Student CERN, Geneva Nottingham Trent University Pyheadtail Comparison and Development Thanks to: Giovanni Iadarola, Giovanni Rumolo,

Comparison of varying Dt_ref

Page 15: Aaron Axford Technical Student CERN, Geneva Nottingham Trent University Pyheadtail Comparison and Development Thanks to: Giovanni Iadarola, Giovanni Rumolo,

Comparison of varying Dt_ref

Page 16: Aaron Axford Technical Student CERN, Geneva Nottingham Trent University Pyheadtail Comparison and Development Thanks to: Giovanni Iadarola, Giovanni Rumolo,

Comparison of varying Dt_ref

Page 17: Aaron Axford Technical Student CERN, Geneva Nottingham Trent University Pyheadtail Comparison and Development Thanks to: Giovanni Iadarola, Giovanni Rumolo,

Comparison of varying Dt_ref

Page 18: Aaron Axford Technical Student CERN, Geneva Nottingham Trent University Pyheadtail Comparison and Development Thanks to: Giovanni Iadarola, Giovanni Rumolo,

Comparison of varying Dt_ref

Page 19: Aaron Axford Technical Student CERN, Geneva Nottingham Trent University Pyheadtail Comparison and Development Thanks to: Giovanni Iadarola, Giovanni Rumolo,

Number of kicks against Computation Time

Page 20: Aaron Axford Technical Student CERN, Geneva Nottingham Trent University Pyheadtail Comparison and Development Thanks to: Giovanni Iadarola, Giovanni Rumolo,

Comparison of varying Bo

Aims● Observe the outcome when using a Magnetic

field varying from 0.1Tesla to 1.9 Tesla

Page 21: Aaron Axford Technical Student CERN, Geneva Nottingham Trent University Pyheadtail Comparison and Development Thanks to: Giovanni Iadarola, Giovanni Rumolo,

Comparison of varying magnetic field

Page 22: Aaron Axford Technical Student CERN, Geneva Nottingham Trent University Pyheadtail Comparison and Development Thanks to: Giovanni Iadarola, Giovanni Rumolo,

Comparison of Repeated reading

Aims● Observe the difference with identical

simulations repeated

Page 23: Aaron Axford Technical Student CERN, Geneva Nottingham Trent University Pyheadtail Comparison and Development Thanks to: Giovanni Iadarola, Giovanni Rumolo,

Comparison of Repeated reading

Page 24: Aaron Axford Technical Student CERN, Geneva Nottingham Trent University Pyheadtail Comparison and Development Thanks to: Giovanni Iadarola, Giovanni Rumolo,

Comparison of Repeated reading

Strongly affected by the random number generator

Page 25: Aaron Axford Technical Student CERN, Geneva Nottingham Trent University Pyheadtail Comparison and Development Thanks to: Giovanni Iadarola, Giovanni Rumolo,

Summary

● PyHDTL shows a strong reliability with comparison to HDTL results for all tested optics and setups

● More investigation needed for varying of repeated simulations