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Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM Experimental Techniques EDMs in Storage Rings Prospects of the Field EDMs in Storage Rings: Powerful Probes of Physics Beyond the SM and of CP- Violation

Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

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Page 1: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Yannis K. Semertzidis

Brookhaven National Laboratory

Seminar IUCF, 21 May 2004

•EDMs: Why are they important?•Our Universe: The Symmetry that isn’t•EDM Experimental Techniques•EDMs in Storage Rings•Prospects of the Field

EDMs in Storage Rings: Powerful Probes of Physics Beyond the SM

and of CP-Violation

Page 2: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Questions Physicists Ask:

Page 3: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

A Permanent EDM Violates both T & P Symmetries:

Page 4: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Spin is the only vector…

0d

Phenom.: only thecomponent alongthe spin survives...

+

-

+

-

dd

Page 5: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

A Permanent EDM Violates both T & P Symmetries:

+

-

+

-

+

-T

P

Page 6: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

A Permanent EDM Violates both T & P Symmetries:

EdEdH

ˆˆ

PEdH

EdEdH

ˆˆ

EdH

T

Page 7: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Reality Check: Induced EDMs…

EEdH

TOK

PEEdH

OK

Edd

EdH

1st order Stark effect. Forbidden!

EEdH

2nd order Stark effect. Allowed!

Page 8: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Reality Check: MDMs are Allowed…

BdH

BdBdH

ˆˆT

PBdH

BdBdH

ˆˆ

Page 9: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

T-Violation CP-ViolationCPT

Andrei Sakharov 1967:

CP-Violation is one of three conditions to enable a universe containing initially equal amounts of matter and antimatter to evolve into a matter-dominated universe, which we see today….

Page 10: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Before 1929:

• Universe is Static-Eternal

• Cosmological Constant is Invented to Stabilize it!

• Dirac Equation 1928:1. g=2 for Point-like, Spin ½ Particles

2. Negative Energy States

Flashback

Page 11: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Hubble 1929:

• Universe is Expanding

• …If the Universe Expands… a Beginning and a BIG BANG!

• Km/MPa/s or 10-18s-1 75/ aaH

• Discovery of Positron by Anderson: 1933

Page 12: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

At Accelerators:

• 1955: Antiproton Discovery at Berkeley

• 1956: Antineutron Discovery

• 1957: Parity Violation, Lee-Yang

• 1964: CP-Violation at Brookhaven

• Universe: Matter Dominated; Initial Condition Maintained by B, L Number Conservation.

Page 13: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Andrei Sakharov 1967:

• Three conditions to enable a universe containing initially equal amounts of matter and antimatter to evolve into a matter-dominated universe, which we see today:

• Proton Decay (Baryon Number Violation)

• CP-Violation

• Universe Undergoes A Phase of Extremely Rapid Expansion

Page 14: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Extension of the SM Needed?

• SM: CP-Violation not Enough by Several Orders of Magnitude for Baryogenesis

Page 15: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

SM Versus SUSY:

One CP-Violating Phase (CKM).SM:

42 CP-Violating Phases!SUSY:

Page 16: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

ála Fortson

d

Page 17: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

EdBdt

sd

Usual Experimental Method

Small Signal

Compare the Zeeman FrequenciesWhen E-field is Flipped:

dE421 +

-

TNEd

11

Page 18: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Schiff Theorem:A Charged Particle at Equilibrium Feels no Force……An Electron in a Neutral Atom Feels no Force Either:

0int EEE extTot

…Otherwise it Would be Accelerated…

Page 19: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Neutron EDM Limits

0.1

1

10

100

1000

10000

100000

1000000

50 60 70 80 90

Year

10^

-25

e-cm

Neutron EDM Vs Year

Page 20: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Neutron EDM at LANSCEAiming for a Factor of 50

Page 21: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

3

Page 22: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM
Page 23: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Q=CV

Page 24: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

S. Lamoreaux at “Lepton Moments”, June 2003

E=5MV/m,T=108s

R&D

Page 25: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Cost of the n-EDM Experiment at LANSCE

• $10M for the experimental apparatus

• $9M for the Beamline

• R&D?

• Total $19M plus R&D

Page 26: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Schiff Theorem:A Charged Particle at Equilibrium Feels no Force……An Electron in a Neutral Atom Feels no Force Either. However:

0intint BEEF extTot

…the net E-field is not zero!

Page 27: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

1960 1970 19901980 20102000

10-30

10-28

10-26

10-24

10-22

10-20E

xper

imen

tal L

imit

on

de (

e . c

m)

Electron EDM

Cs

CsXe* Hg

Cs

Tl

Tl??

Tl

Page 28: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Current Atomic EDM Limits

• Paramagnetic Atoms, 205Tl: electron |de| < 1.610-27e·cm (90%CL)

PRL 88, 071805 (2002)

• Diamagnetic Atoms, 199Hg Nucleus: |d(199Hg)| < 2.110-28e·cm (95%CL)

PRL 86, 2505 (2001)

Page 29: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM
Page 30: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM
Page 31: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Electric Dipole Moments in Storage Rings

e.g. 1T corresponds to 300 MV/m!

Buddt

sd

Page 32: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Spin Precession in g-2 Ring(Top View)

Bm

eaa

Momentumvector

Spin vector

Page 33: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Spin Precession in g-2 Ring(Top View)

Bm

eaa

Momentumvector

Spin vector

Page 34: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

• The Muon Storage Ring: B ≈ 1.45T, Pμ≈3.09 GeV/c

Page 35: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

4 Billion e+ with E>2GeV

aa

t

tAeNdtdN

cos1/ 0

Page 36: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

B

a edm

Ron McNabb’s Thesis 2003: C.L. 95% cme107.2 19

x

y

z

edm

m

e Ba

B

2

Indirect Muon EDM limit from the g-2 Experiment

a

edm

tan

Page 37: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Canceling g-2 with a Radial E-field

x

y

z

B

edm

edm

m

e

)1

1(

2 c

EaBa

B

c

E

2

B

c

E

m

e

2Eω

Page 38: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Radial E-field to Cancel/Control the g-2 Precession

• Radial E-Field: 2aBcER

The method works well for particles with small anomalous magnetic moment a, e.g. Muons (a = 0.0011), Deuterons (a = -0.143), etc.

c

EaBa

m

ea

1

12

Page 39: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Spin Precession in g-2 Ring(Top View)

Bm

eaa

Momentumvector

Spin vector

Page 40: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Spin Precession in EDM Ring(Top View)

0a

Momentumvector

Spin vector

Page 41: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

The muon spin precesses vertically (Side View)

BVdEddt

sd

B

Page 42: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

The muon spin precesses vertically (Side View)

BVdEddt

sd

B

Page 43: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Two Major Ideas:

• Radial E-field to Cancel the g-2 Precession

• Injecting CW and CCW

• Sensitivity: 10-24 e·cm statistical (1 yr, 0.75MW)

• Sensitivity: 10-27 e·cm systematic error

• Muon EDM LOI: (http://www.bnl.gov/edm) to J-PARC.

Page 44: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Muon EDM Letter of Intent to J-PARC/Japan, 2003

• †Spokesperson

• # Resident Spokesperson

#

Page 45: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Expected Muon EDM Value from a

)tan( 10 27

cme 10 210

SUSY22

CP

ad

CPiSUSYSUSY

DM

eDD

Dd

Dm

ea

FDDL

,

,2

and ,2

1 where

,2

1

2

1

2

1 5*5

Page 46: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Predictions in Specific Models

The predicted value for the electron is 10 times lessthan the current experimental limit.

50 effect at 10-24 ecm Exp. Sensitivity!

Page 47: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Predictions in Specific Models

Experimental Goal

T. Feng, et al., hep-ph/0305290“Lepton Dipole Moments and Rare Decays in the CP-Violating MSSM with Non-Universal Soft-Supersymmetry Breaking”

Page 48: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

g-2 Values

• Electron 0.0016 done

• Muon 0.0016 doing

• Proton 1.8 ------

• Deuteron -0.15 OK!

Page 49: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Deuteron Coherence Time

• E, B field stability

• Multipoles of E, B fields

• Vertical (Pitch) and Horizontal Oscillations

• Finite Momentum Acceptance ΔP/P

At this time we believe we can do p~10s

Page 50: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Deuteron EDM Signal:

• Radial E-Field:

Rd

RR

Ea

ad

a

aEdBcEd

dt

sd

2

2

1

1

2aBcER

e.g. for ER = 3.5MV/m, d = 10-27e·cm; ωd = 0.3µrad/s

Page 51: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Enhancement of EDM Signalby Canceling the g-2 Precession

• Edm Signal Rate: 0.3rad/s

• With Cancellation: a 0.1 rad/s; Max vertical spin amplitude within 10s: 1rad

• Without Cancellation: a 106 rad/s; Max vertical spin amplitude within 10s: 0.1prad

Page 52: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Nuclear Scattering as Deuteron EDM polarimeter

IDEA:- make thick target defining aperture- scatter into it with thin target

D

L

U

R

R

“extraction”target - ribbon

“defining aperture”primary target

detectorsystem

Target could beAr gas (higher Z).

Target “extracts” byCoulomb scattering deuterons onto thickmain target. There’snot enough goodevents here towarrant detectors.

Hole is largecompared tobeam. Every-thing that goesthrough holestays in thering.

Detector is far enoughaway that doughnutillumination is not anacceptance issue:Δ < R.

Ed Stephenson’s

Page 53: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Deuteron Statistical Error (200MeV):

TotcRp

dfTNAPaE

a

18

2

p : 10s. Polarization Lifetime (Coherence Time)A : 0.5 The left/right asymmetry observed by the polarimeterP : 0.55. The beam polarizationNc : 41011d/cycle. The total number of stored particles per cycleTTot: 107s. Total running time per yearf : 0.01 Useful event rate fractionER : 3.5MV/m. Radial electric field

cme102 28 d per year

Page 54: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Sources of Deuteron Systematic Errors:

• Out of Plane Electric Field (Ev)

• Geometrical Phases (2nd Order Effects)

• Tensor Polarization (E.S.: Different Dependence on a …)

• Polarimeter Detector Related Effects

Page 55: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Effect of Vertical Component of E

0)( vv ruBEeF

c

E

u

EBr

vv

c

EB

c

EBB

c

EBcBEE

Bm

eg

zr

zrr

zrrzz

r

**

*

*

0

2

Ec

E

m

eg

c

E

m

eg

22

v

22

• Deuterons β=0.2, γ=1.02, ω=13105 θE rad/s

Page 56: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

CW vs CCW

B

B

E EE-Field doesNOT flip sign!

Page 57: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Effect of Vertical Component of E• Clock Wise and Counter-Clock Wise Injection:

Background: Same Sign Signal: Opposite Sign

• Protons β=0.15, γ=1.01, ω100105 θE rad/s• Deuterons β=0.2, γ=1.02, ω 10105 θE rad/s• Muons β=0.98, γ=5, ω 2105 θE rad/s

• Other Diagnostics Include Injecting Forward vs Backward Polarized Beams as well as Radially Pol.

Page 58: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Ev Issues:

• Temporal Changes (CW and CCW every 10s)

• Changes Correlated with B-Field Reversals (Fabry-Perot Resonator)

• E-Field Multipoles Couple to Beam Moments (Pickup Electrodes; Beam Moment Manipulation)

Page 59: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Tilt-meter Measurements at the g-2 Ring with 1nrad Resolution

Page 60: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Systematic Error Symmetries(+) Same as EDM; (-) is opposite

SpinRelated

PolarimeterRelated

Page 61: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Deuteron EDM Ring Lattice

Page 62: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Deuteron EDM Signal is Strong:

• Radial E-field Controls g-2 Precession Rate

• Intense Polarized Deuteron Beams

• Long Spin Coherence Time 10s

• Polarimeters: Large Left/Right Asymmetry

Page 63: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Deuteron EDM Systematics:

• EV: CW vs CCW Injection

• Geometrical Phases: Local Cancellation of g-2 and CW vs CCW Injection

• Preliminary Flattening of Ring to 10-9rad: Beam Dynamics Resonance and Beam Position Monitors. The Spin Itself is Sensitive…

• Detector Related Effects: CW vs CCW Injection, Spin Flip at Injection

• Leakage Current is a Second Order Effect!

Page 64: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Deuteron EDM to 10-27 ecm Sensitivity Level is 100 times better than 199Hg

• T-odd Nuclear Forces: dd =210-22 ξ e·cm with the best limit for ξ<0.5 10-3 coming from the 199Hg EDM limit (Fortson, et al., PRL 2001), i.e. dd < 10-25 e·cm.

(Sushkov, Flambaum, Khriplovich Sov. Phys. JETP, 60, p. 873 (1984) and Khriplovich and Korkin, Nucl. Phys. A665, p. 365 (2000)).

Page 65: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

dd = dp + dn (I. Khriplovich)

It Improves the Current Proton EDM Limit by a Factor of ~10,000 and a Factor 60-100 on Neutron.

Page 66: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Deuteron (D) EDM at 310-

27ecm

Relative strength of various EDM limits as a function of left handed down squark mass (O. Lebedev, K. Olive, M. Pospelov and A. Ritz, hep-ph/0402023)

( ) NND n p Dd d d d

Page 67: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Possible Locations for a Deuteron EDM Experiment:

• Brookhaven National Laboratory

• Indiana University Cyclotron Facility

• KVI/The Netherlands

Proposal This Year…

$20-30M

Page 68: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

We are Studying

• Target and Polarimetry (Deuteron case)

• E-field Directional/Amplitude Stability

• Beam and Spin Dynamics

Page 69: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

EDMs

Questions Physicists Ask:

Page 70: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Electric Dipole Moment Searches:

• Exciting Physics, Forefront of SUSY/Beyond SM Search.

• Revolutionary New Way of Probing EDMs, Muon and Deuteron Cases-Very Exciting.

• EDM Experiments could Solve the Long Standing Mystery of Matter Asymmetry in our Universe

Summary

Page 71: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Extension of the SM Needed?

• SM: CP-Violation not Enough by Several Orders of Magnitude for Baryogenesis

• Leptogenesis: CP-Violation in Neutrino Mixing?

• Heavy, Weakly Interacting, Right-Handed Neutrinos Produced in Early Universe

• Their Decays Produces Lepton Number Asymmetry.

• Further Interactions Conserving B-L Convert it to Baryon Number Asymmetry

Page 72: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Parameter Values of Muon EDM Experiment

• Radial E-Field:• E=2MV/m

• Dipole B-field: B~0.25T

• Muon Momentum:

• Need NP2=1016 for 10-24e.cm. Muon EDM LOI: (http://www.bnl.gov/edm) to J-PARC, <one year of running.

2aBcE

5 MeV/c,500 P

Page 73: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

d(muon) < 710-19

Left-Right

10-20

10-22

10-24

d e.cm

MultiHiggs SUSY

Electro-magnetic

neutron:

electron:

1960 1970 1980 1990 2000 2010 2020 2030

10-28

10-29

Current status of EDMs

d(electron) < 1.6 10-

27

d(neutron) < 6 10-

26

d(proton) < 6 10-23

la Sauer

d(199Hg) < 2.1 10-28

Page 74: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

E-field Stability: Major Breakthrough Idea by Neil Shafer-Ray

E-field Stability of Order 10-8 to 10-9

Page 75: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Parameter Values of Muon EDM Experiment

• Radial E-Field:• E=2MV/m• Dipole B-field: B ~ 0.25T , R ~ 10m

• Muon Momentum:

• Need NP2=1016 for 10-24e.cm. Muon EDM LOI: (http://www.bnl.gov/edm) to J-PARC, <one year of running.

• F. Farley et al., hep-ex/0307006

2aBcE

5 MeV/c,500 P

Page 76: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Parameter Values of a Deuteron EDM Experiment

• Radial E-Field:

ER=3.5MV/m

• Dipole B-field: B~0.1-0.5T; Ring Radius: R~15-30m

• Deuteron Momentum:

• YkS et al., hep/ex-0308063

2aBcER

5.0 GeV/c, 1 dP

Page 77: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Deuteron EDM to 10-27 ecm Sensitivity Level is 100 times better than 199Hg

• T-odd Nuclear Forces: dd =210-22 ξ e·cm with the best limit for ξ<0.5 10-3 coming from the 199Hg EDM limit (Fortson, et al., PRL 2001), i.e. dd < 10-25 e·cm.

(Sushkov, Flambaum, Khriplovich Sov. Phys. JETP, 60, p. 873 (1984) and Khriplovich and Korkin, Nucl. Phys. A665, p. 365 (2000)).

Page 78: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

dd = dp + dn (I. Khriplovich)

It Improves the Current Proton EDM Limit by a Factor of ~10,000 and a Factor 60-100 on Neutron.

Page 79: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Possible Improvements:

• Higher ER Fields: 14MV/m with gas to slow down free electrons.

• Longer Storage Time than 10s while Maintaining Polarization (Coherence Time).

Page 80: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Deuteron Statistical Error:

TotcRp

dfTNAPaE

a2

2

15.6

p : Polarization Lifetime (Coherence Time)A : The left/right asymmetry observed by the polarimeterP : The beam polarizationNc : The total number of stored particles per cycleTTot: Total running timef : Useful event rate fractionER : Radial electric field

Page 81: Yannis K. Semertzidis Brookhaven National Laboratory Seminar IUCF, 21 May 2004 EDMs: Why are they important? Our Universe: The Symmetry that isn’t EDM

Signal and Background:

Ea

ad

dt

ds2

1

Ecdt

ds E2