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Ocelot Coordinate System

The coordinate system in Ocelot follows these conventions:

(x,x=pxp0),(y,y=pyp0),(τ=cΔt,p=ΔEp0c)\left (x, \quad x' = \frac{p_x}{p_0} \right), \qquad \left (y, \quad y' = \frac{p_y}{p_0} \right), \qquad \left (\tau = c\Delta t, \quad p = \frac{\Delta E}{p_0 c} \right)

Definitions

  • τ=ctsβ0\tau = c t - \frac{s}{\beta_0}: Longitudinal coordinate of the particle.
  • β0=v0c\beta_0=\frac{v_0}{c}: normalized velocity.
  • ss: Independent variable representing the distance along the beamline (i.e., the path length of the reference particle).
  • v0v_0 and p0p_0: Velocity and momentum of the reference particle, respectively.
  • tt: Time at which a particle reaches position ss along the beamline.

For the reference particle:

  • τ=0\tau = 0 for all ss.

For other particles:

  • τ<0\tau < 0: The particle arrives earlier than the reference particle.
  • τ>0\tau > 0: The particle arrives later than the reference particle.

Energy relation:

  • ΔE=EE0\Delta E = E - E_0, where E=γm0c2E = \gamma m_0 c^2 is the total energy of the particle.
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The Ocelot coordinate system is not canonical. For a canonical system, the sign of the τ\tau coordinate must be reversed. In that case, the system becomes identical to the MAD coordinate system.