Synchrotron Radiation in MAD-X
Andrea Latina
- A. Latina (CERN) - Mar 3, 2017
Synchrotron Radiation in MAD-X Andrea Latina A. Latina (CERN) - - - PowerPoint PPT Presentation
Synchrotron Radiation in MAD-X Andrea Latina A. Latina (CERN) - Mar 3, 2017 Physics recap The average energy loss by a radiating particle is: E = P t , with 3 r e c 3 4 E P = 2 , Instantaneous radiated power 2 ( Ze ) 2 r e =
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ρ:
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x + θ2 y:
x + θ2 y
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x + θ2 y
x + h2 y
pt = orbit(6)
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◮ tmbend:
x + h2 y
2
2
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◮ tmcorr:
x + θ2 y
◮ tmquad: from the definition of quadrupole kick
x + θ2 y = (k1L)2 x2 + (−k1L)2 y2 = (k1L)2
x + θ2 y
1L
◮ tmsext: from the definition of sextupole kick:
x + θ2 y =
2
2
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◮ tmmult, tmoct, tmrfmult, tmcrab follow the scheme:
x + θ2 y
◮ tmdpdg and tmbb do not implement radiation.
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x + θ2 y
◮ ttmult:
◮ for each particle, at entrance and at exit ◮ defines const = 1
3 aradγ3, uses elrad
◮ defines
curv = sqrt((dipr + dxt(jtrk))**2 + (dipi + dyt(jtrk))**2) / elrad
◮ then
if (!quantum)
else trphot(el,curv,rfac,deltas);
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◮ ttcorr:
curv = sqrt(dpx**2 + dpy**2) / el
rfac = arad * gammas**3 * (dpx**2 + dpy**2) / (three * el)
◮ A significant limitation of this implementation (an error?) is that the synchrotron
◮ ttrfmult, tttquad, tttdipole:
◮ trphot:
◮ This concentrates the effect of all photons in one location, not considering the
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◮ Issues in Track
1 4πǫ0 e2 c , and then slices the element in
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◮ Abandon the assumption β ≈ 1 ◮ Enrich MAD-X dictionary with pre-defined values for arad (better: improve
◮ Suggest a split of the radiating elements in more than two parts, and apply
◮ Implement radiation damping effects of RF-Multipoles in Emit.
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