high-energy circular colliders, + novel accelerating ... · future accelerators and technologies:...
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Future accelerators and technologies:
high-energy circular colliders,
+ novel accelerating technologies
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Philip Burrows
John Adams Institute, Oxford University
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c. 100 GeV
per beam
LEP
Synchrotron radiation
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Discovered Elder et al
1947 (General Electric)
Synchrotron radiation
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Power lost due to synchrotron radiation
P ~ E ** 4 / r**2
E = beam energy
r = radius of trajectory
Synchrotron radiation
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Power lost due to synchrotron radiation
P ~ E ** 4 / r**2
E = beam energy
r = radius of trajectory
For LEP each electron lost ~ 3 GeV per turn (3%!)
P = 10**-6 Watts/electron 18 MW total
Must be compensated by accelerating cavities
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Super Large Electron Positron collider?
500 GeV
beams?
(5 x LEP)
Synchrotron radiation
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Suppose we increase LEP beam energy (100 GeV) by factor 5: E 500 GeV, in the same tunnel
P ~ E ** 4 / r**2
Synchrotron radiation
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Suppose we increase LEP beam energy (100 GeV) by factor 5: E 500 GeV, in the same tunnel
P ~ E ** 4 / r**2
E increases by factor 5, so P increases by 5**4
this would give P = 5 **4 * 18 MW = 11 GW!
Synchrotron radiation
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Suppose we increase LEP beam energy (100 GeV) by factor 5: E 500 GeV, in the same tunnel
P ~ E ** 4 / r**2
E increases by factor 5, so P increases by 5**4
this would give P = 5 **4 * 18 MW = 11 GW!
Compensate by increasing radius r?
Need 10 x r to reduce P by 100 270km tunnel!
270km tunnel for e+e- ???
Synchrotron radiation: LHC?
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Is this a problem for LHC?
Synchrotron radiation: LHC?
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Is this a problem for LHC?
PSR ~ ( E / m0 ) 4
mproton ~ 2000 * melectron
Pproton ~ 2000-4 * Pelectron for same E
Even for LHC, E = 70 * LEP, each proton loses only
5 keV per turn (0.000 000 1% ~ negligible!)
Large Hadron Collider (LHC)
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High luminosity is critical
Event rate = luminosity x cross-section
R = L σ
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High luminosity is critical
Event rate = luminosity x cross-section
R = L σ
σ is ‘probability of something being produced’:
fixed by nature
to maximise R need to maximise L
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High luminosity is critical
Event rate = luminosity x cross-section
R = L σ
σ is ‘probability of something being produced’:
fixed by nature
to maximise R need to maximise L
For a collider, L = N1 N2 frep / ( 4π σx σy )
N1 particles/bunch of type 1 collide with N2 /bunch of type 2
frep is the bunch collision frequency
σx (σy) is the bunch size in x (y) at the interaction point
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LHC luminosity
L = N1 N2 frep / ( 4π σx σy )
N1 = N2 ≈ 1011 protons per bunch
frep = 2808 x 11,000
σx,y ≈ 16 μm (best)
L = 1011 1011 2800 11,000 / ( 4π 1.62 10-3 10-3 )
≈ 1034 / cm2 / s
Ignored crossing angle (300 240 urad) …
This needs to be taken account of for precisely evaluating L
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18CERN roadmap: High Energy frontiers
CLIC Workshop 2015
26-30 September 2015 - CERN
The HL-LHC Project
• New IR-quads Nb3Sn (inner triplets)
• New 11 T Nb3Sn (short) dipoles
• Collimation upgrade
• Cryogenics upgrade
• Crab Cavities
• Cold powering
• Machine protection
• …
Major intervention on more than 1.2 km of the LHC
Project leader: Lucio Rossi; Deputy: Oliver Brüning
F. Bordry
High Energy LHC (HE-LHC)?
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Challenge:
High-field
magnets
16T
Future circular collider (FCC)?
~ 100km tunnel
16T dipoles
40-50 TeV p beams
e- beams up to
~ 175 GeV
(limited by SR)
Future circular collider (FCC)?
Future circular collider (FCC)?
Future circular collider (FCC)?
Future circular collider (FCC)?
Future circular collider (FCC)?
Future circular collider (FCC)?
Future circular collider (FCC)?
Future circular collider (FCC)?
Future circular collider (FCCee)?
Future circular collider (FCCee)?
Future circular collider (FCCee)?
Future circular collider (FCCee)?
Future circular collider (FCCee)?
Future circular collider (FCCee)?
Very HE-LHC in future 100km tunnel??
Possible CEPC sites
CEPC SPPC ?
Luminosity vs. energy, circular vs. linear
Attempt to summarise: e+e-
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ILC: 250 GeV 500 GeV? 1000 GeV??
CLIC: 380 GeV 1500 GeV? 3000 GeV??
CEPC/ 250 GeV 350 GeV? 91,180 GeV
FCCee:
Guaranteed precision meas of Higgs (and top)
ILC + CLIC possibility of direct access to HH and ttH
CLIC (+ ILC) possibility of direct access to TeV scale
Attempt to summarise: pp
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HL-LHC: 7 TeV beams
HE-LHC: 13? TeV beams
FCC/SPPC: 40-50? TeV beams
As of today, we do not know if this extra energy reach is required or enough, let alone optimal!
Development of accelerators
Acceleration in a cylindrical cavity
z
zE0
E(z)
)(tE
g
R. Schmidt
TM 010 mode
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Typical accelerating cavities
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State of the art accelerating cavities
ILC goal: 35 MV / m
CLIC goal: 100 MV / m
SCRF Linac Technology
Approximately 20 years of R&D
Worldwide Mature technology
* site dependent
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1.3 GHz Nb 9-cell Cavities 16,024
Cryomodules 1,855
SC quadrupole package 673
10 MW MB Klystrons &
modulators436 / 471*
• solid niobium
• standing wave
• 9 cells
• operated at 2K (Lqd. He)
• 35 MV/m
• Q0 ≥ 1010
European XFEL @ DESY
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Largest
deployment of
SCRF
technology
- 100
cryomodules
- 800 cavities
- 17.5 GeV
The ultimate ‘integrated
systems test’ for ILC.
Commissioning with beam
started 2017
Industrial production - XFEL
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(Thanks to Nick Walker)
One vendor following ILC baseline recipe
quench limit
Field emission
Limit (XFEL spec.)
require
retreatment
status:01.06.2016
TDR
acceptance
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Maximum
Usable
0 10 20 30 40 500%
20%
40%
60%
80%
100%
0
5
10
15
20
25
30
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Gradient (MV/m)
yie
ld
co
unt
CLIC gradient status
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• Achieved 100 MV/m gradient in main-beam RF cavities
Electron accelerator development
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E167
Electron accelerator development
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E167
wakefield accelerators
Laser wakefield accelerators
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Can create
electric fields
10-100 GV / m
Beam-driven plasma wakefield accelerators
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Some e- had their
energy doubled
to c. 80 GeV
in 1m of plasma
40 GeV
Wim Leemans and Eric Esarey, Physics Today, March 2009
Concept of TeV e+e- collider based on laser-plasma
acceleration
Concept for beam-driven Plasma Wake Field TeV
Linear Collider
Drive beam accelerator
DR e- DR e+ main beam e-
injector main beam e+
injector
Beam Delivery and IR
PWFA cells
RF gun
RF separator
bunch compressor Drive beam distribution
PWFA cells
We have a long way to go …
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100 MeV gamma ray
bursts detected from
crab nebula
1015 eV electrons!
Not to mention 1020 eV (50J) cosmic rays!