May 2004 @ CERN Physics with a Multi-MWProton Source 1 Klaus Jungmann, Physics with a Megawatt Proto...

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Physics at a Megawatt Proton Source, CERN, May 25-27, 2004 What is Fundamental What is Fundamental Forces and Symmetries Forces and Symmetries Fundamental Fermions Fundamental Fermions Discrete Symmetries Discrete Symmetries Properties of Known Basic Interactions Properties of Known Basic Interactions ~ 1GeV versus ~ 30 GeV proton driver ~ 1GeV versus ~ 30 GeV proton driver Klaus Jungmann, Kernfysisch Versneller Instituut,Groningen Aspects of Aspects of only scratching some examples only scratching some examples

Transcript of May 2004 @ CERN Physics with a Multi-MWProton Source 1 Klaus Jungmann, Physics with a Megawatt Proto...

Page 1: May 2004 @ CERN Physics with a Multi-MWProton Source 1 Klaus Jungmann, Physics with a Megawatt Proto Source, CERN 25 May 2004 Fundamental Symmetries and.

Physics at a Megawatt Proton Source, CERN, May 25-27, 2004

• What is FundamentalWhat is Fundamental • Forces and SymmetriesForces and Symmetries• Fundamental FermionsFundamental Fermions• Discrete SymmetriesDiscrete Symmetries• Properties of Known Basic InteractionsProperties of Known Basic Interactions• ~ 1GeV versus ~ 30 GeV proton driver~ 1GeV versus ~ 30 GeV proton driver

Klaus Jungmann, Kernfysisch Versneller Instituut,Groningen

Aspects ofAspects of

only scratching some examplesonly scratching some examples

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Physics at a Megawatt Proton Source, CERN, May 25-27, 2004

Klaus Jungmann, Kernfysisch Versneller Instituut,Groningen

Drawing on : Work of NuPECC Long Range Plan Working group on Fundamental

Interactions, 2003 :

H. Abele (D), L. Corradi (I), P. Herczeg (USA), I.B. Khriplovich (RU),

O. Nviliat (F), N. Severijns (B), L. Simons (CH), C. Weinheimer (D),

H.W. Wilschut (NL), K. Jungmann (NL)

H. Leeb (A), C. Bargholtz (S)

Assisted by: W. Heil, P. Indelicato, F. Maas, K. Pachucki, R.G Timmermans,

C. Volpe, K. Zuber

NSAC Long Range Plan 2002

EURISOL Physics Case 2004

Aspects ofAspects of

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The Nature of Neutrinos Oscillations / Masses / 02-decay

T and CP Violation edm’s, D (R) coeff. in -decays, D0

Rare and Forbidden Decays 02-decay, n-nbar, M-Mbar, e 3e, N e

Correlations in -decay non V-A in-decay

Unitarity of CKM-Matrix n-,-, (superallowed -decays

Parity Nonconservation in Atoms Cs, Fr, Ra, Ba+, Ra+

CPT Conservation n, e, p,

Precision Studies within The Standard Model

Constants, QCD,QED, Nuclear Structure

Theoretical Support Positions at Universities

Experimentalists and Theorists

High Power Proton Driver Several MW Target Research

Cold and Ultracold Neutrons

Low Energy Radioactive Beams

Improved Trapping Facilities

Underground Facilities

Physics TopicsPhysics Topics Adequate EnvironmentAdequate EnvironmentHuman resources

Facilities

of NuPECC working group 2003

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The Nature of Neutrinos Oscillations / Masses / 02-decay

T and CP Violation edm’s, D (R) coeff. in -decays, D0

Rare and Forbidden Decays 02-decay, n-nbar, M-Mbar, e 3e, N e

Correlations in -decay non V-A in-decay

Unitarity of CKM-Matrix n-,-, (superallowed -decays

Parity Nonconservation in Atoms Cs, Fr, Ra, Ba+, Ra+

CPT Conservation n, e, p,

Precision Studies within The Standard Model

Constants, QCD,QED, Nuclear Structure

Theoretical Support Positions at Universities

Experimentalists and Theorists

High Power Proton Driver Several MW Target Research

Cold and Ultracold Neutrons

Low Energy Radioactive Beams

Improved Trapping Facilities

Underground Facilities

Physics TopicsPhysics Topics Adequate EnvironmentAdequate EnvironmentHuman resources

Facilities

Relating to a MW Proton Machine

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Physics TopicsPhysics Topics

Offer unique possibilities to gain

inside into fundamental processes

and into yet unexplained observed

facts in nature

Offer possibilities to measure

needed fundamental constants

with unprecedented accuracy

Relating to a MW Proton Machine

High Power Proton DriverHigh Power Proton Driver

To obtain sufficient particles

- Statistics Limitations

- Understanding Systematics

To enable Novel Techniques

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fundamental := “ forming a foundation or basis a principle, law etc. serving as a basis”

Forces and SymmetriesForces and Symmetries

Global Symmetries Conservation Laws• energy• momentum• electric charge• lepton number• charged lepton family number• baryon number• …..

Local Symmetries Forces• fundamental interactions

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fundamental := “ forming a foundation or basis a principle, law etc. serving as a basis”

Standard ModelStandard Model • 3 Fundamental Forces

• ElectromagneticElectromagnetic Weak Weak StrongStrong• 12 Fundamental Fermions

• Quarks, Leptons• 13 Gauge Bosons

• ,W+, W-, Z0, H, 8 Gluons

However However • many open questions

• Why 3 generations ? • Why some 30 Parameters?• Why CP violation ?• Why us?• …..

• GravityGravity not included

• No Combind Theory of GravityGravity and Quantum MechanicsQuantum Mechanics

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Fundamental Interactions – Standard Model

StrongStrong

GravitationGravitation

??

MagnetismMagnetism

ElectricityElectricityMaxwell

Glashow,Salam, t'Hooft,

Veltman,WeinbergWeakWeak

ElectroElectro --MagnetismMagnetism

ElectroElectro --WeakWeakStandard ModelStandard Model

GrantGrandUnificationUnification

not yet known?not yet known? Physics outside Standard ModelPhysics outside Standard ModelSearches for New PhysicsSearches for New Physics

Physics within the Standard ModelPhysics within the Standard Model

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Neutrinos Neutrino Oscillations Neutrino Masses

Quarks Unitarity of CKM Matrix

Rare decays Baryon Number Lepton Number/Lepton Flavour

New Interactions in Nuclear and Muon -Decay

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E

LmP ij

4sin)2(sin)(

222

Neutrino-ExperimentsNeutrino-ExperimentsRecent observations could be explained by oscillations of massive neutrinos.

Many Remaining Problems• really oscillations ?• sensitive to m2

• Masses of Neutrino • Nature of Neutrino

• Dirac• Majorana

Neutrinoless Double -Decay

• Direct Mass Measurements are indicated Spectrometer• Long Baseline Experiments -beams new neutrino detectors ?

SuperkamiokandeSNO

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Neutrino-ExperimentsNeutrino-ExperimentsAre there new detection schemes ?Are there new detection schemes ?

• Water CherenkovWater Cherenkov• ScintillatorsScintillators• ........

• Directional sensitivity for low energies ?

• Air shower ?Air shower ?• Salt Domes ?Salt Domes ?

Only for Non- Accelerator Neutrinos ?

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Neutrinos Neutrino Oscillations Neutrino Masses

Quarks Unitarity of CKM Matrix

Rare decays Baryon Number Lepton Number/Lepton Flavour

New Interactions in Nuclear and Muon -Decay

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Unitarity of Cabbibo-Kobayashi-Maskawa MatrixUnitarity of Cabbibo-Kobayashi-Maskawa Matrix

0*** tbtdcbcdubud VVVVVV

1|||||| 222 ubusud VVV

Unitarity:

Nuclear-decays

= 0.0032 (14)Neutron decay= 0.0083(28)= 0.0043(27)

Often found:

If you pick yourfavourite Vus !

)2(9992.0)4(0041.0)4(008.0

)3(041.0)8(9740.0)4(223.0

)12(0036.0)4(223.0)13(9754.0

tbtstd

cbcscd

ubusud

VVV

VVV

VVV

CKM Matrix couples weak and mass quark eigenstaes:

0.9739(5) 0.221(6)

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Unitarity of Cabbibo-Kobayashi-Maskawa MatrixUnitarity of Cabbibo-Kobayashi-Maskawa Matrix

Nuclear-decays

= 0.0032 (14)Neutron decay= 0.0083(28)= 0.0043(27)

Experimental Possibilities

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CKM UnitarityCKM Unitarity

• May relate to New PhysicsHeavy Quark Mixing, Z‘,Extra Dimensions, Charged Higgs, SUSY, exotic muon decays, ... , more generations !

• Unfortunatetly: Situation is a mess !

VVud ud :: superallowed -decays 0.9740(3)(4)

neutron decay 0.9729(4)(11)(4) pion- decay 0.9737(39)(2)

VVus us :: Hyperons

e

eProblem !

• What can be done? Improve reliability of experiments independently pion- decay (theory clean!) , maybe: neutron- decay

Analyse existing K data, Ke3 experiments

Search for exotic muon decays Improve Theory

Numbers Compiled byW. Marciano,March ‘04

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Neutrinos Neutrino Oscillations Neutrino Masses

Quarks Unitarity of CKM Matrix

Rare decays Baryon Number Lepton Number/Lepton Flavour

New Interactions in Nuclear and Muon -Decay

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Muon Experiments Possible at a CERN Neutrino Factory -Expected Improvements

Muon Physics Possibilities at Muon Physics Possibilities at Any High Power Proton DriverAny High Power Proton Driver i.e. i.e. 4 MW 4 MW

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Old Muonium for Muonium-Antimuonium Conversion ?Old Muonium for Muonium-Antimuonium Conversion ?

• P(M) sin2 [const * (GMM/GF)*t]*exp[-*t]

• Background exp(- n *t) ; n-fold coincidence detection

• For GMM << GF M gains over Background• P(M) / Background t2 * exp[+(n-1)* *t]

Pulsed ACCELERATORPulsed ACCELERATOR

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Neutrinos Neutrino Oscillations Neutrino Masses

Quarks Unitarity of CKM Matrix

Rare decays Baryon Number Lepton Number/Lepton Flavour

New Interactions in Nuclear and Muon -Decay

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Vector [Tensor]

+

e

Scalar [Axial vector]

+

e

New Interactions in Nuclear and Muon New Interactions in Nuclear and Muon -Decay-Decay

In Standard Model:Weak Interaction is

V-A

In general -decaycould be also

S , P, T

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Parity Parity Nonconservation in Atoms Nuclear Anapole Moments Parity Violation in Electron-Scattering

Time Reversal and CP-Violation Electric Dipole Moments R and D Coefficients in -Decay

CPT Invariance

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Beautiful confirmation of Standard Model

in the past !

Only little chances to contribute to forefront

(except leptoquark scenarios)

Usefull for measureing neutron distributions

Usefull to explore e.g. anapole moments

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Parity Parity Nonconservation in Atoms Nuclear Anapole Moments Parity Violation in Electron-Scattering

Time Reversal and CP-Violation Electric Dipole Moments R and D Coefficients in -Decay

CPT Invariance

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1.610-27

Start TRIP

•199Hg

Radium potential

de (SM) < 10-37

Some Some EDMEDM Experiments compared Experiments compared

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EDMs – Where do they come from ?(are they just “painted“ to particles? Why different experiments? )

electron intrinsic ? quark intrinsic ? muon second generation different ? neutron/ proton from quark EDM ? property of strong

interactions ? new interactions ? deuteron basic nuclear forces CP violating?

pion exchange ? 6Li many body nuclear mechanism ? heavy nuclei (e.g. Ra, Fr) enhancement by CP-odd nuclear

forces,

nuclear “shape“ atoms can have large enhancement,

sensitive to electron or nucleus EDMs molecules large enhancement factors , sensitive

to electron EDM

.....

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How does a ring edm experiment work ?How does a ring edm experiment work ?

• Exploit hugemotional electric fields for relativistic particles in highmagnetic fields • stop g-2 precession• observe spin rotation

For muons exploitdecay asymmetry

•Concept works•also for (certain)•Nuclei: d, 6Li, 213Fr, . .

N+ N+ N+

• One could use -decay• In general:any sensitive polarimeterworks

One needs for a successful experiment:• polarized, fast beam• magnetic storage ring• polarimeter

N+

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Some Candidate NucleiSome Candidate Nuclei

30y0.0119+2.84137/213755Cs

22 min<0.02+1.173/222387Fr

82.8 m+0.195+0.5101/27532Ge

-0.1426+0.8574121H

3.6 m0.083+0.4761/215769Tm

-0.1779+0.8220163Li

-0.12152.5507/212351Sb

-0.0305+2.7897/213957La

T 1/2

Reduced Anomaly

a

/NSpin JNucleus

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• R and D test both TTime RReversal VViolation

• DD most potential

• RR scalar and tensor (EDM, a)• technique D measurements yield a, A, b, B

TTime RReversal VViolation in -decay: Correlation measurements

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Parity Parity Nonconservation in Atoms Nuclear Anapole Moments Parity Violation in Electron-Scattering

Time Reversal and CP-Violation Electric Dipole Moments R and D Coefficients in -Decay

CPT Invariance

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?

1810m

mmr

0

00

K

KK||

K

12102avga

|e

ae

a|3101.2

avgg

|e

ge

g|

er

CPTbreakb,a μμ Invariance LorentzbreakH,d,c,b,a μνμνμνμμ

?

CPT and Lorentz Non-Invariant Models

CPT tests

Are they comparable - Which one is appropriate

Use common ground, e.g. energies

Leptons in External Magnetic Field

Bluhm , Kostelecky, Russell, Phys. Rev. D 57 ,3932 (1998)

For g-2 Experiments :

Dehmelt, Mittleman,Van Dyck, Schwinberg, hep- ph/9906262

μμ qAiiD

0Dμγ5γμνidνDμγμνicμνσμνH21μγ5γμbμγμamμDμ(iγ

equation DIRAC violating Lorentz and CPT generic

ψ)

2clm

aΔω

lupspinE

|ldownspinEl

upspinE|

lr

l34bl

aωlaωaΔω

avg

ll2

l

cl

a|aa|

cm

ωr

24103.5μr21101.2er :: muonelectron

CPTCPT – ViolationLorentz Invariance Violation

What is best CPT test ?

New Ansatz (Kostelecky)

• K0 10-18 GeV/c2

• n 10-30 GeV/c2

• p 10-24 GeV/c2

• e 10-27 GeV/c2

• 10-23 GeV/c2• Future:

Anti hydrogen 10-18 GeV/c2

often quoted:

• K0- K0 mass difference (10-18)

• e- - e+ g- factors (2* 10-12)

• We need an interaction with a finite strength !

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Electromagnetism and Fundamental Constants QED, Lamb Shift Muonium and Muon g-2 Muonic Hydrogen and Proton Radius Exotic Atoms Does QED vary with time?

QCD Strong Interaction Shift Scattering Lengths

Gravity Hints of strings/Membranes?

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Properties of known Basic InteractionsProperties of known Basic Interactions

Search for New PhysicsWhat are the hardronic corrections?

• e++e- hadrons• e++e- + hadrons

New activities Planned• statistics limited experiment• J-PARC, BNL • Fundamental constants needed• Muonium

“Proton Radius”

Muonic Hydrogen Lamb Shift

Pionic Hydrogen

Strong Interaction Shift

Muon g-2

Newest Theory Offer: 2.4 from Experiment

0, + mass differenceoverlooked ?

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Electromagnetism and Fundamental Constants

QED, Lamb Shift Muonium and Muon g-2 Muonic Hydrogen and Proton Radius Exotic Atoms Does QED vary with time?

QCD Strong Interaction Shift Scattering Lengths

Gravity Hints of strings/Membranes?

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Standing Waves of Ultra Cold NeutronsStanding Waves of Ultra Cold Neutronsin a gravitational fieldin a gravitational field

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Non Newtonian Gravity

Best Test 1 to 5 m

Grenoble GatchinaHeidelberg Cern

Standing Waves of Ultra Cold NeutronsStanding Waves of Ultra Cold Neutrons

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High power Proton DriverHigh power Proton Driver ~ 1GeV ~ 30 GeV~ 1GeV ~ 30 GeV

- -- -

The Nature of Neutrinos Oscillations / Masses / 02-decay

T and CP Violation edm’s, D (R) coeff. in -decays, D0

Rare and Forbidden Decays 02-decay, n-nbar, M-Mbar, e 3e, N e

Correlations in -decay non V-A in-decay

Unitarity of CKM-Matrix n-,-, (superallowed -decays

Parity Nonconservation in Atoms Cs, Fr, Ra, Ba+, Ra+

CPT Conservation n, e, p,

Precision Studies within The Standard Model

Constants, QCD,QED, Nuclear Structure

Physics TopicsPhysics Topics

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ConclusionConclusionParticle Physics –Nuclear Physics ?Particle Physics –Nuclear Physics ?

• Gregory Breit,

when asked at Yale whether a new colleague should be an atomic theorist, a nuclear theorist, an astro-physcist or work in the then new field of particle physics:

> There are only Good Theorists and bad ones <> There are only Good Theorists and bad ones <• Accordingly:

It‘s time to build jointly a powerful machine to serve Good It‘s time to build jointly a powerful machine to serve Good

Physics. A Multi-Megawatt Proton Driver has a very Large Physics. A Multi-Megawatt Proton Driver has a very Large

Potential to serve Good Physics, particularly in the merging Potential to serve Good Physics, particularly in the merging

fields of nuclear, particle and astro-physics.fields of nuclear, particle and astro-physics.

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Thank YOU !

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SPARES