the high intensity frontier franco cervelli infn-pisa 7 nov, 2005

48
he High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005

Upload: silvia-golden

Post on 18-Jan-2016

217 views

Category:

Documents


4 download

TRANSCRIPT

Page 1: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005

The High Intensity Frontier

Franco Cervelli INFN-Pisa

7 Nov, 2005

Page 2: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005
Page 3: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005
Page 4: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005

Historically, many fundamental discoveries and Historically, many fundamental discoveries and measurements have come from accelerators measurements have come from accelerators which were not the highest which were not the highest energy machineenergy machine available at the time:available at the time:

• weak neutral currents at the CERN PS

• J/ at the AGS (Brookhaven)

• limits on the lepton-number conservation

• most of the parameters of CP violation

• etc.

Page 5: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005

Cu

rre

nt

(A

)

BEAM ENERGY, BEAM CURENT, AND BEAM BEAM ENERGY, BEAM CURENT, AND BEAM POWER OF WORLD’S PROTON MACHINESPOWER OF WORLD’S PROTON MACHINES

JHFJHF

JHFJHF

HIPSHIPS

Page 6: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005

BEAM FLUXES: ORDERS OF MAGNITUDEBEAM FLUXES: ORDERS OF MAGNITUDE

PHYTHIA: E = 30 GeV, I = 80 A

Page 7: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005
Page 8: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005
Page 9: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005
Page 10: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005
Page 11: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005
Page 12: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005

Required Fluxes

Page 13: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005

SUSY connection between Dμ , μ → e (LFV)

Page 14: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005

∼∼∼∼ ∼∼∼∼

χχ∼∼

In Supersymmetry (similar examples in other BSMs): In Supersymmetry (similar examples in other BSMs):

∝ f(Δmq2, λa ), a≥1∝ f(Δm

q2, λa ), a≥1∼∼

Sensitive to whether GIM suppression operates in the scalar quark sector: tests of scalar quark mixings and mass differences

Sensitive to whether GIM suppression operates in the scalar quark sector: tests of scalar quark mixings and mass differences

∝ C mt2 λ5 , C=complex, λ=sinθ

c∝ C m

t2 λ5 , C=complex, λ=sinθ

c

GIM suppression of light-quark contributions, dominated by high mass scales

GIM suppression of light-quark contributions, dominated by high mass scales

In the SM: In the SM:

Why study Rare Kaon Decays

Page 15: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005

is a crucial element in the exploration of the new physics discovered at the LHC.

Accuracies at the level of 10% would already provide precious quantitative information

K+ → π+ ν νK+ → π+ ν ν K0

L → π0 ν νK0L → π0 ν ν

K0L → π0 e+ e−K0L → π0 e+ e− K0

L → π0 μ+ μ−K0L → π0 μ+ μ−

A measurement of the 4 decay modes

Page 16: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005

HIF for QCD Physics

Page 17: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005

Objects of Interest

Mesons/Baryons

Molecules/Multiquarks

Hybrids

Glueballs

+ Effects due to the complicated QCD vacuum

Quark AntiQuark

Page 18: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005

How many isotopes are produced per second?

Page 19: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005

Proton Driver Rings

Page 20: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005

Design Goals

4-5 MW beam power on target

Very short pulse duration (~1 ns rms)

Very low beam loss (~10-4)

Note: most proton drivers under study are based on

synchrotrons (US, JKJ, UK)

Page 21: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005

European Scenarios

SPL + accumulator and compressor rings

5 GeV, 50 Hz synchrotron-based system

15 GeV, 25 Hz synchrotron-based system

30 GeV, 8 Hz slow cycling synchrotron

8 GeV, 16.67 Hz rapid cycling synchrotron for

ISIS/Fermilab, plus upgrades

Page 22: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005

Synchrotron-based Proton Drivers

Low energy linac (~150 MeV)

Booster synchrotrons to accumulate proton beam and perform some acceleration

Main synchrotrons to complete acceleration and compress the bunches.

Page 23: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005

Proton Driver Figure of Merit For a given power (4MW), target peak proton power

density ~ 1/(Kinetic energy T x frequency f). F=Tf is a useful figure of merit.

MACHINE T (GeV) f (Hz) FIGURE OF MERIT

CERN SPL+rings 2.2 50 110

RAL RCS Driver I 5.0 50 250

RAL RCS Driver II 15.0 25 375

CERN RCS 30.0 8 240

ISIS II 8.0 50 400

Page 24: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005

Proposed rotating tantalum target ring

Targetry

Many difficulties: enormous power density lifetime problemspion capture

Replace target between bunches:Liquid mercury jet or rotating

solid target

Stationary target:

Densham Sievers

Page 25: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005

HIF : Regional Activities

Page 26: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005
Page 27: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005

180 MeV H- Linac

Two 1.2 GeV, 50 Hz Rapid Cycling Synchrotrons

2 bunches of 2.5 1013 protons

4 bunches of 2.5 1013 protons

Two 5 GeV, 25 Hz Rapid Cycling Synchrotrons

Collimation

Injection

Momentum Ramping

RAL 5 GeV Proton Driver

Page 28: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005
Page 29: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005
Page 30: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005

Primary Beams

• 1012/s; 1.5-2 GeV/u; 238U28+

• Factor 100-1000 over present intensity• 2(4)x1013/s 30 GeV protons• 1010/s 238U92+ up to 35 GeV/u • up to 90 GeV protons

Secondary Beams

• Broad range of radioactive beams up to 1.5 - 2 GeV/u• Antiprotons 0 - 30 GeV

• Cooled beams• Rapidly cycling superconducting magnets

Key Technical Features

Storage and Cooler Rings

• Radioactive beams

• e-– A (or Antiproton-A) collider

• 1011 stored and cooled 0.8 - 14.5 GeV antiprotons

• Polarized antiprotons(?)

UNILACSIS

FRS

ESR

SIS 100/300

HESRSuperFRS

NESR

CR

RESR FLAIR

International FAIR Project: Characteristics

Page 31: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005
Page 32: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005
Page 33: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005
Page 34: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005

HIF : International Facilities

Page 35: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005
Page 36: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005
Page 37: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005

What at CERN?

Page 38: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005
Page 39: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005
Page 40: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005

HIF : in Italy

Page 41: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005
Page 42: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005
Page 43: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005

A Super-B Factory

Page 44: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005

Conclusions

Page 45: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005
Page 46: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005
Page 47: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005
Page 48: The High Intensity Frontier Franco Cervelli INFN-Pisa 7 Nov, 2005