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Hadron Collider Accelerator Basics Mike Syphers, Fermilab - PowerPoint PPT Presentation

Hadron Collider Accelerator Basics Mike Syphers, Fermilab Introduction; Magnets; RF Acceleration Transverse Motion; Accelerator Lattice Errors and Adjustments Challenges at High E/L Luminosity Optimization Introduction Will touch on


  1. Hadron Collider Accelerator Basics Mike Syphers, Fermilab Introduction; Magnets; RF Acceleration Transverse Motion; Accelerator Lattice Errors and Adjustments Challenges at High E/L Luminosity Optimization

  2. Introduction Will touch on technology, but mostly discuss the physics of particle accelerators, especially relevant to hadron colliding beams synchrotrons Will cover: - luminosity; how to meet the requirements? - basic principles; develop “the jargon” - a few major issues encountered at high energy, luminosity

  3. Fixed Target Energy vs. Collider Energy Beam/target particles: E 0 ≡ m p c 2 Fixed Target Collider E, � E, − � p p E , � p E 0 , 0 2 2 E ∗ , � p E ∗ , 0 E ∗ 2 = ( m ∗ c 2 ) 2 + ( pc ) 2 [ E 0 + E ] 2 = m ∗ c 2 = 2 E E 2 0 + 2 E 0 E + ( E 2 0 + ( pc ) 2 ) = = 2 E 0 γ coll 2 E 0 [1 + γ F T ] 1 / 2 √ m ∗ c 2 = 100,000 TeV FT synch. == 14 TeV LHC

  4. Fixed Target Energy vs. Collider Energy Nucleon-Nucleon Collisions Beam/target particles: E 0 ≡ m p c 2 2000 Fixed Target Collider Collider Threshold Energy (GeV) E, � E, − � p p 1500 E , � p E 0 , 0 CM Energy (GeV) 2 2 1000 E ∗ , � p E ∗ , 0 500 E ∗ 2 = ( m ∗ c 2 ) 2 + ( pc ) 2 [ E 0 + E ] 2 = m ∗ c 2 = 2 E E 2 0 + 2 E 0 E + ( E 2 0 + ( pc ) 2 ) = (46 GeV) Fixed Target = 2 E 0 γ coll 2 E 0 [1 + γ F T ] 1 / 2 √ m ∗ c 2 = 0 0 200 400 600 800 1000 Incident Beam Energy (GeV)

  5. Luminosity Experiments want “collisions/events” -- rate? � Σ � Fixed Target Experiment: · ρ · A · ℓ · N A · ˙ N beam R = A ℓ A ρ N A ℓ ˙ N beam · Σ = L · Σ ≡ Σ ex.: N beam = 10 24 / cm 3 · 100 cm · 10 13 / sec = 10 39 cm − 2 sec − 1 L = ρ N A ℓ ˙ � Σ � Bunched-Beam Collider: = · N · ( f · N ) R A N particles f N 2 = · Σ A f N 2 (10 34 cm − 2 sec − 1 for LHC) L ≡ Σ A 1, of N area, A

  6. Integrated Luminosity Bunched beam is natural in collider that “accelerates” (more later) L = f 0 BN 2 A f 0 = rev. frequency B = no. bunches In ideal case, particles are “lost” only due to “collisions”: B ˙ ( n = no. of detectors N = − L Σ n receiving luminosity L ) L 0 So, in this ideal case, L ( t ) = � 2 � � � n L 0 Σ 1 + t BN 0

  7. Ultimate Number of Collisions � Since then, #events = L ( t ) dt · Σ R = L · Σ So, our integrated luminosity is � T L 0 T L 0 T/I 0 I ( T ) ≡ L ( t ) dt = 1 + L 0 T ( n Σ /BN 0 ) = I 0 · 1 + L 0 T/I 0 0 asymptotic limit: 250 20 I 0 ≡ BN 0 L ( t ) I ( t ) Luminosity (/microbarn/sec) 200 Integrated Luminosity (/pb) n Σ 15 150 so, ... 10 100 L = f 0 BN 2 5 50 A 0 0 0 10 20 30 40 50 0 10 20 30 40 50 time(hr) time(hr) (will come back to luminosity at the end)

  8. How to Make Collisions? Simple Model of Synchrotron: - Accelerating device + magnetic field to bring particle back to accelerate again Field Strength -- determines size, ultimate energy of collider p ρ = e B ; R = ρ /f ( f ≈ 0 . 8 − 0 . 9) - ex: “packing fraction” B = 1 . 8 T , p = 450 GeV / c f = 0 . 85 → R ≈ 1 km

  9. Magnets iron-dominated magnetic fields N turns per pole of current I "#$%&#'()#%&*$+' B = 2 µ 0 N · I !"#$%&%$'( )#*++!(% ! d - iron will “saturate” at about 2 Tesla Superconducting magnets - field determined by distribution of currents B θ = µ 0 J “Cosine-theta” distribution r J = 0 2 d r B y = µ 0 J B x = 0 , d 2 + J − J current density, J

  10. Superconducting Designs Numerical µ 0 J Tevatron B = 2 d Example : 1000 A / mm 2 · (10 mm) · 10 3 mm 4 π T m / A = - 10 7 2 m 1 st SC accelerator = 6 T - 4.4 T; 4 o K LHC -- 8 T; 1.8 o K

  11. Acceleration Principal of phase stability - McMillan (U. California) and Veksler (Russia) Imagine: particle circulating in field, B ; along orbit, arrange particle to pass through a cavity with max. voltage V, oscillating at frequency h x f rev (where h is an integer); suppose particle arrives near time of zero-crossing - net acceleration/deceleration = eV sin ( �� t ) if arrives late, more voltage is applied; arrives early, gets less - thus, a restoring force --> energy oscillation “Synchrotron Oscillations” in general, lower momentum particles take longer, arrive late gain extra momentum next, slowly raise the strength of B; if raised adiabatically, oscillations continue about the “synchronous” momentum, defined by p/e = B . R for constant R This is the principle behind the synchrotron, used in all major HEP accelerators today

  12. Longitudinal Motion Say ideal particle arrives at phase � s : dE s = f 0 eV sin φ s ∼ dB dt dt Particles arriving nearby in phase, and nearby in energy will oscillate about these ideal conditions ... • Phase Space ∆ E plot: φ Regions of Stability Adiabatic increase of bend field generates stable phase space regions; particles oscillate, follow along “bunched” beam; h = f rf / f rev = # of possible bunches

  13. Bunched Beam Bunch by adiabatically raising voltage of RF cavities

  14. Buckets, Bunches, Batches, ... Stable phase space region is called a bucket. - Boundary is the separatrix; only an approximation - � s = 0, � -- particles outside bucket remain in accelerator “DC beam” - For other values of � s -- particles outside bucket are lost • DC beam from injection is lost upon acceleration Bunches of particles occupy buckets; but not all buckets need be occupied. Batches (or, bunch trains) are groupings of bunches formed in specific patterns, often from upstream accelerators

  15. Acceleration Stable regions shirnk as begin to accelerate If beam phase space area is too large (or if DC beam exists), can lose particles in the process

  16. Keeping Focused In addition to increasing the particle’s energy, must keep the beam focused transversely along its journey Early accelerators employed what is now called “weak focusing” y d R 0 x

  17. Room for improvement... With weak focusing, for a given transverse angular deflection, x max ∼ R 0 √ n θ Thus, aperture ~ radius ~ energy Cosmotron (1952) (3.3 GeV)

  18. Room for improvement... With weak focusing, for a given transverse angular deflection, x max ∼ R 0 √ n θ Thus, aperture ~ radius ~ energy Bevatron (1954) (3.3 GeV) (6 GeV) Could actually sit inside the vacuum chamber!! beam direction

  19. Strong Focusing Think of standard focusing scheme as alternating system of focusing and defocusing lenses (today, use quadrupole magnets) Quadrupole will focus in one transverse plane, but defocus in other; if alternate, can have net focusing in both - for equally spaced infinite set, net focusing requires F > L/2 F = focal length, L = spacing - FODO cells:

  20. Separated Function Until late 60’s, synchrotron magnets (wedge-shaped variety) both focused and steered the particles in a circle. (“combined function”) With Fermilab Main Ring and CERN SpS, use “dipole” magnets to steer, and use “quadrupole” magnets to focus Quadrupole magnets, with alternating field gradients, “focus” particles about the central trajectory -- act like lenses Thin lens focal length: x ( s ) s F Fermilab Logo Tevatron: and L = 30 m

  21. Example: FNAL Main Injector Bending Magnets Focusing Magnets

  22. Particle Trajectories 1 FODO “cell” � � ∂ B y K ( s ) = e Analytical Description: ∂ x ( s ) p - Equation of Motion: (Hill’s Equation) - Nearly simple harmonic; so, assume soln.:

  23. Particle Trajectories 1 FODO “cell” � � ∂ B y K ( s ) = e Analytical Description: ∂ x ( s ) p - Equation of Motion: (Hill’s Equation) - Nearly simple harmonic; so, assume soln.:

  24. Particle Trajectories 1 FODO “cell” � � ∂ B y K ( s ) = e Analytical Description: ∂ x ( s ) p - Equation of Motion: (Hill’s Equation) - Nearly simple harmonic; so, assume soln.:

  25. Particle Trajectories 1 FODO “cell” � � ∂ B y K ( s ) = e Analytical Description: ∂ x ( s ) p - Equation of Motion: (Hill’s Equation) - Nearly simple harmonic; so, assume soln.:

  26. Hill’s Equation and the “Beta Function” So, taking and assuming - then, differentiating our solution twice, and plugging back into Hill’s Equation, we find that for arbitrary A, � ... � ψ �� + β � � x �� + K ( s ) x � β ψ � = cos[ ψ ( s ) + δ ] A β ( β � ) 2 � � − 1 + 1 β �� β − ( ψ � ) 2 + K � + A sin[ ψ ( s ) + δ ] = 0 β 4 β 2 2 • Since must have � > 0, first term --> • With this, the remaining term implies differential equation for � which is, Upon simplifying... �

  27. Hill’s Equation and Beta (cont’d) Typically, dK/ds = 0 ; so, � β 4 In a “drift” region (no focusing), 2 - Thus, beta function is a parabola in drift regions x � mm � 0 • If pass through a waist at s = 0 , then, Through focusing region (quad, say), K = const � 2 � 4 0 L 2 L 3 L 4 L longitudinal position - Thus, beta function is a sin/cos or sinh/cosh function, with an offset • “driven harmonic oscillator,” with constant driving term So, optical properties of synchrotron ( � ) are now decoupled from particle properties ( A, � ) and accelerator can be designed in terms of optical functions; beam size will be proportional to � 1/2

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