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B. Lee Roberts, PANIC05, Santa Fe, 27 October, 2005 - p. 1 /35 Muon (g-2) Status and Plans for the Future B. Lee Roberts Department of Physics Boston University [email protected] http://physics.bu.edu/roberts.html

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Muon (g-2). Status and Plans for the Future. B. Lee Roberts Department of Physics Boston University. [email protected] http://physics.bu.edu/roberts.html. Magnetic moments, g-factors. Lepton Flavor Violation Muon MDM (g-2) chiral changing Muon EDM. The Muon Trio:. Dirac,. - PowerPoint PPT Presentation

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Page 1: Muon (g-2)

B. Lee Roberts, PANIC05, Santa Fe, 27 October, 2005 - p. 1/35

Muon (g-2)

Status and Plans for the Future

B. Lee RobertsDepartment of Physics

Boston University

[email protected] http://physics.bu.edu/roberts.html

Page 2: Muon (g-2)

B. Lee Roberts, PANIC05, Santa Fe, 27 October, 2005 - p. 2/35

Magnetic moments, g-factors

Page 3: Muon (g-2)

B. Lee Roberts, PANIC05, Santa Fe, 27 October, 2005 - p. 3/35

The Muon Trio:• Lepton Flavor Violation

• Muon MDM (g-2) chiral changing

• Muon EDMDirac, Pauli moment

Page 4: Muon (g-2)

B. Lee Roberts, PANIC05, Santa Fe, 27 October, 2005 - p. 4/35

Electric and Magnetic Dipole Moments

Transformation properties:

An EDM implies both P and T are violated. An EDM at a measureable level would imply non-standard model CP. The baryon/antibaryon asymmetry in the universe, needs new sources of CP.

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Present EDM Limits

Particle Present EDM limit(e-cm)

SM value(e-cm)

n

future exp 10-24 to 10-25 *

final limit will be better, * projected.

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Unlike the EDM, there is a large SM value for the MDM

The Electron: to the level of the experimental error (4ppb),

Contribution of μ, (or anything heavier than the electron) is ≤4 ppb.

For the muon, the relative contribution of heavier particles

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Standard Model Value for (g-2)

Page 8: Muon (g-2)

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SM value dominated by hadronic issues:

• Lowest order hadronic contribution ( ~ 60 ppm)

• Hadronic light-by-light contribution ( ~ 1 ppm)

The error on these two contributions will ultimately limit the interpretation of a more precise muon (g-2) measurement.

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Lowest Order Hadronic contribution from e+e-

annihilation

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a(had) from hadronic decay?

• Assume: CVC, no 2nd-class currents, isospin breaking corrections.

• n.b. decay has no isoscalar piece, while e+e- does• Many inconsistencies in comparison of e+e- and decay:

- Using CVC to predict branching ratios gives 0.7 to 3.6 discrepancies with reality.

- F from decay has different shape from e+e-.

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New Physics; SUSY (with large tanβ )

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SUSY connection between a , dμ , μ → e

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Muon (g-2) : E821

• Superconducting “superferric” storage ring– superconducting inflector– fast muon kicker– magic , – direct muon injection with a fast non-

ferric kicker

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Use an E field for vertical focusing

spin difference frequency = s - c

0

Page 15: Muon (g-2)

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Spin Precession Frequencies: in B field with both an MDM and EDM

The motional E - field, β X B, is much stronger (~GV/m) than laboratory electric fields.

Page 16: Muon (g-2)

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Spin Precession Frequencies: in B field with both an MDM and EDM

The EDM causes the spin to precess out of plane and increases ||

The motional E - field, β X B, is much stronger (~GV/m) than laboratory electric fields.

Page 17: Muon (g-2)

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Spin Precession Frequencies: in B field with both an MDM and EDM

The if the EDM were 2.8 x 10-18 e cm, a would increase by 2.9 ppm.

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Muon (g-2): Store ± in a storage ring

magnetic field averaged over azumuth in the storage ring

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Muon (g-2) Present precision: ± 0.5 ppm

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Can we improve the sensitivity of this confrontation between experiment and

theory?• Yes

– E969 at BNL has scientific approval to go from 0.5 ppm → 0.2ppm

– At a more intense muon facility we could do better.

Will Theory Improve beyond 0.6 ppm?• Yes

– better R measurements from: KLOE, BaBar, Belle, SND and CMD2 at Novosibirsk

– More work on the strong interaction

• Theory could eventually improve to ~0.2 ppm

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Exclusion/Limitations on New Physics

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B. Lee Roberts, PANIC05, Santa Fe, 27 October, 2005 - p. 22/35

SUSY, dark matter, (g-2)

CMSSM (constrained minimal supersymmetric model)

scal

ar m

ass

gaugino mass

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Future Comparison: E969 = now

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Future Comparison: E969

Historically (g-2) has played an important role in restricting models of new physics.

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E969 at BNL

• Scientific approval in September 2004– at present: no funds for construction or running

• Goal: total error = 0.2 ppm– lower systematic errors– more beam

Page 26: Muon (g-2)

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Strategy of the improved experiment

• More muons – E821 was statistics limited stat = 0.46 ppm, syst = 0.3 ppm– Backward-decay, higher-transmission beamline– Double the quadrupoles in the decay line

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Strategy of the improved experiment

• New, open-end inflector • Upgrade detectors, electronics, DAQ

x 2 in flux

Page 28: Muon (g-2)

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E969: Systematic Error Goal

Systematic uncertainty (ppm)

1998 1999 2000 2001 E969Goal

Magnetic field – p 0.5 0.4 0.24 0.17 0.1

Anomalous precession – a 0.8 0.3 0.3 0.21 0.1

Page 29: Muon (g-2)

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aμ implications for the muon EDM

This paper, published before our February 2001 announcement predicts a large muon EDM, and a corresponding SUSY contribution to aμ comparable to what we might be observing, with the e- EDM predicted to be 0.1 of the present limit.

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aμ implications for the muon EDM

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Dedicated EDM measurement:• operate with ≈ 5 << 29.3• use a radial E-field to turn off (g-2)

precession

• Place detectors above and below the vacuum chamber and look for an up/down asymmetry which builds up with time

Page 32: Muon (g-2)

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Beam Needs: NP2

• the figure of merit is Nμ times the polarization. We need

to reach the 10-24 e-cm level.• Since SUSY calculations range from 10-22 to

10-32 e cm, more muons is better.

= 5*10-7

(Up+

Dow

n)

time (s)

(Up-

Dow

n)

Page 33: Muon (g-2)

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Where E821 came from:

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Today:

All E821 results were obtained with a “blind” analysis.

world average

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Summary

• (g-2) provides a precise check of the standard model, and accesses new physics in a way complementary to other probes.

• (g-2) provides serious constraints on physics beyond the standard model.

• The hadronic contribution will eventually set the limit on useful precision, but substantial improvement can and will be made, both in theory and experiment beyond the present situation.

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Recent News from Novosibirsk

• SND has just released their results (hep-ex/0506076) for the cross section e+e- → + - over the . – Error on dispersion integral 50% higher

than CMD2– Good agreement with CMD2– Completely independent from CMD2

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Improved transmission into the ring

InflectorInflector aperture

Storage ring aperture

E821 Closed End P969 Proposed Open End

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Beyond E969?

• It’s not clear how far we can push the present technique.

• To get to 0.06 ppm presents many challenges.

• Perhaps a new storage ring design, and a smaller aperture. – detectors for another factor of 4 will be

very challenging.• At a proton driver/neutrino factory

we certainly we can get more muons

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E969: Systematic Error Goal

• Field improvements will involve better trolley calibrations, better tracking of the field with time, temperature stability of room, improvements in the hardware

• Precession improvements will involve new scraping scheme, lower thresholds, more complete digitization periods, better energy calibration

Systematic uncertainty (ppm)

1998 1999

2000 2001

E969

Goal

Magnetic field – p 0.5 0.4 0.24 0.17 0.1

Anomalous precession – a

0.8 0.3 0.3 0.21 0.1

Page 41: Muon (g-2)

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Better agreement between exclusive and inclusive (2) data than in 1997-1998 analyses

Agreement between Data (BES) and pQCD (within correlated systematic errors)

use QCD

use data

use QCD

Evaluating the Dispersion Integral

from A. Höcker ICHEP04

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Tests of CVC (A. Höcker – ICHEP04)

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Shape of F from e+e- and hadronic decay

zoom

Comparison between t data and e+e- data from CDM2 (Novosibirsk)

New precision data from KLOE confirms

CMD2