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10-13 May 2009. New Opportunities in the Physics Landscape at CERN. Antiproton Decelerator (AD) Summary and Prospects. Klaus Jungmann, KVI, University of Groningen, NL. Physics Motivation Unique Possibilities Tests of Fundamental Theories Precision Measurements

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slide2
10-13 May 2009

New Opportunities in the Physics Landscape at CERN

Antiproton Decelerator (AD)

Summary and Prospects

Klaus Jungmann, KVI, University of Groningen, NL

  • PhysicsMotivation
  • Unique Possibilities
  • Tests of Fundamental Theories
  • Precision Measurements
  • Novel Techniques and Instrumentation
  • Applications
  • High Visibility

?

P

P

how do we work in physics
Sir Isaac Newton

(1642 - 1727)

Basic Principles on

which Scientists

work in Physics

First Theory

on Gravity

How do we work in Physics ?
slide5
FANTOM Study Week Gent 2007
  • A Theory is only as good as it is experimentally verified.
  • A Theory without experimental verification has no standing.
slide6
The Standard Model(s)

Dark Matter – Dark Energy …

  • Excellent Description of
  • ALL Observations
  • However, many Open Questions
  • Why 3 generations ?
  • Why some 30 parameters?
  • Why one electric charge ?
  • What about CP violation ?
  • Why matter-antimatter asymmetry?
  • …..
  • Gravitynot included
  • NoCombindTheoryofGravityand
  • Quantum Mechanics.
  • Contents of the Cosmos
  • What’s the other 96% beyond matter ?
slide7
?

Physics within the Standard Model:

complex systems, spectra, lifetimes…

+

-

u u

d

d u

d

N S

zX

e-

m-

b+

ne

Standard Model in Particle Physics

Gravitation

Grand

Unification

Electro-

Electro - Weak

Magnetism

Magnetism

Standard Model

Electricity

?

Weak

Strong

Strong

  • Speculative Models:
  • Supersymmetry, Cold dark matter, Tachyons, Radiativemuon generation,
  • Technicolor, Leptoquarks, Extra gauge bosons, Extra dimensions,
  • LeftRight Symmetry, Compositeness, Lepton flavour violation, ….
  • No Status in Physics , yet: “Not Even Wrong”

not yet known?

Physics outside the Standard Model:

new phenomena, new particles…

slide8
Experiments at the Frontiers of Standard Theory

Direct Search Frontier

Precision Frontier

complementary

approaches

slide9
Test of Fundamental Symmetries

PrecisonMeasurements

slide10
Since then CERN has a HIGHLY PUBLICLY VISIBLEprogram

on Low Energy Precision Testsof most fundamental theories

slide11
Precision requires Time

pbar-p q/m 45 years

electron g-2 60 years

muon g-2 45 years

muonium 1s-2s 15 years

Highly precise CPT & Gravity Tests

Proton and Antiproton

q/m compare to 0.1 ppb

Clock Comparisons

Proton and Antiproton

gravitational accceleration

equal to 1 ppm

p and pbar charge to mass ratio (circles)

p and pbar inertial mass ratio (squares)

slide12
Verifications of CPTSymmetry
  • Tests of particle/antiparticle symmetry (PDG)
    • Inconsistent definition of figure of merit: comparison difficult
    • Pattern of CPT violation unknown (P: weak interaction, CP: mesons)
      • → Arbitrary number joggling to get
        • “accuracy” better than experiments !!!
slide13
CPT– Violation & Lorentz Invariance Violation
  • Kosteleckyet al.:
  • Interaction with a finite strength
  • Figure of merit energy based
  • → Completely different systems appear much more interesting !
slide14
Mass [eV]

Verifications of CPT symmetry

Using the Kosteleckyet al. Standard Model Extension scheme

  • Tests of particle/antiparticle symmetry (PDG)
slide16
ATHENA

Scientists Create 'Star Trek' Antihydrogen in QuantityBy Alex DominguezAssociated Pressposted: 02:59 pm ET18 September 2002

ATRAP

Physical Review Letters 89, 213401 online (2002)

slide17
(Anti-)Hydrogen CPT Tests

DnHFS= cons. *a2 R+eQED+enucl +eweak + eCPT

Laser spectroscopy 1s-2s -------- Microwave spectroscopy

1s Hyperfine Structure

Dn1s2s= ¾ *R+eQED+enucl +eweak + eCPT

“Long distance” Interaction

“Contact” interaction

R= mec2 *a2/2 h

slide18
Line center accuracy in absence of systematic errors:
  • n = Dnexp. / (Sign./Noise) Dnexp. /  Nparticles

(Anti-)Hydrogen Spectroscopy*

Hydrogen 1s-2s Saturation Intensity Is = 0.9 W/cm2

Excitation Rate Re = 4p*84*(I/W/s*cm2)2/Dn/Hz

Photo Ionization Rate Rp = 9*I/W/s*cm2

Zeeman shift dnZ = 9.3*B Hz/T

ac Stark shift dnac = 1.7*I Hz /W*cm2

Velocity at 1mK V1K = 4 m/s

Time-of-flight broadening DnTOF= 3 kHz (1 mK, 600 mm beam diam.)

Lyman a detection efficiency 10-6 =  * effMCP (= 10-4 * 10-2)

1011 H-atoms (MIT Bose condensation)dn/n1s2s = 10-13(1s integration time)

Just one Problem: Lyman-a detection via field quenching => atoms can be used once only

(all 1s, mF states get equally populated)

Antihydrogenexperiments benefit from

more particles

* numbers verified

with L. Willmann

ph ground state hyperfine structure
pH Ground-state Hyperfine Structure

SIMULATION

Need less particles ( 2 pH / s ) because of narrow natural linewidth

from B. Juhasz

phe atom a naturally occurring trap for antiprotons
pHe+ Atom – a naturally occurring trap for antiprotons
  • • Serendipitously discovered by Tokyo group at KEK
  • • 3-body system, Metastable
  • • ~ 3% of stopped antiprotons survive with average lifetime of ~ 3 ms
  • • Precision laser spectroscopy by ASACUSA:
  • - best test of 3-body QED theories
  • - proton-antiproton mass & charge comparison(PDG)
  • Enters CODATA constant adjustment significantly

Hayano, Yamazaki et al.

slide22
CPT Tests @CERN AD
  • At the CERN AD a number of unique, important CPT tests
  • were already conducted and improved ones are on their way :
    • ASACUSApHe , pHe+ , pH , p
    • ATRAP p , pH
    • ALPHA pH
  • One can expect significant steering of Model Building and
  • High Visibility next to a robust discovery potential.
slide23
(Anti-)Hydrogen Gravity Tests

F= - m*g ?

The Remaining eagerly awaited GravityTest

Hydrogen

F=m*g ?

F=m*g

  • Lyman –a laser required
  • Lyman –a laser developed

Unique Possibility

slide24
Gravity Tests @CERN AD
  • At the CERN AD is the place to answer the most urgent
  • question on antimatter gravity :
    • AEGIS pH
    • ATRAP pH
    • Free Fall pH
  • One can expect an answer to a most fundamental question
  • to question, which only can be answered by experiment!
  • High Visibility next to a robust discovery potential.
antiprotonic radioactive atoms
ASACUSA

using RFQD &MUSAHI

Antiprotonic Radioactive Atoms
  • VOLUME 87, NUMBER 8 P H Y S I C A L R E V I E W L E T T E R S 20 AUGUST 2001
      • Neutron Density Distributions Deduced from Antiprotonic Atoms
        • A. Trzcin´ska, J. Jastrze ¸bski, and P. Lubin´ski
        • Heavy Ion Laboratory, Warsaw University, PL-02-093 Warsaw, Poland
          • F. J. Hartmann, R. Schmidt, and T. von Egidy
        • Physik-Department, TechnischeUniversitätMünchen, D-85747 Garching, Germany
          • B. Klos
          • Physics Department, Silesian University, PL-40-007 Katowice, Poland
          • (Received 28 March 2001; published 2 August 2001)

Highest Uncertainty Arising from Theory

slide27
Antiproton Radio-Therapy

A significant win (factor ~4)

in a sensitive window for

tumor treatment

and healthy tissue sparing

Carbon

Antiprotons

slide28
Physics within Standard Model and Applied Research

@CERN AD

  • At the CERN AD also SM physics and Applied Research is
  • conducted:
    • ASACUSAp-nucleus annihilation, atomic collisions
    • Double-Strangeness p-nucleus dedicated experiment
    • Production
    • PAX p polarization, p – p interactions
    • ACE p radiation-therapy
    • ……
  • One can expect deeper insights and the development of
  • novel techniques to the benefit of physics and society.
slide30
Antiproton Decelerator (AD) @ CERN
  • Started operation July 6, 2000
  • Antiproton capture, deceleration, cooling
  • Pulsed extraction
  • Many Experiments
    • ASACUSA
    • ATRAP
    • ALPHA
    • AEGIS
    • Free Fall
    • PAX
    • ACE
    • …..
  • Request for more and
  • better antiproton beams
    • To speed up progress
    • To boost accuracy
  •  ELENA
slide31
Consequent Future Development

[email protected]

ELENAprovides 10-100 times more particles

?Possible [email protected](Heidelberg)  ELENA ??

slide32
FLAIR @ /FAIR

Factor 100 more pbar trapped or

stopped in gas targets than now

FLAIR

NESR

slide33
New Facilities @CERN AD or GSI/FAIR
  • New Facilities can provide up to 100 times more particles:
    • MUSASHI ASACUSA ‘s device to recycle p’s
    • ELENA Generic low cost CERN solution,
    • Start possible now
    • FLAIR GSI/FAIR solution not before 2015
  • One can expect faster progress and better results from more p’s
  • → CERN and GSI should synchronize
slide34
Summary and Conclusions
  • Highly Motivated Urgent Antiproton Experiments
    • with robust Discovery Potential and High Visibility
    • CPT, Gravity, Determination of Fundamental Constants,
    • SM Physics, Applications (Therapy)
  • Unique Facility worldwide until beyond 2015
  • Creative and Innovative Increasing Community
    • Young people
    • Novel Techniques and Novel Technology
  • Physics Program good on Time Path
  • Physics Program needs more particles
    • →ELENAwell motivated
  • Productive and Prosperous Future Ahead

Low Energy Antiproton contributions to Physics just started

Precision takes Time Care and Particles

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