Newest Viewed Downloaded

The Cryogenic Neutron Electric Dipole Moment ExperimentJim Grozier University of Sussex, UK

The Cryogenic Neutron Electric Dipole Moment Experiment

Jim Grozier University of Sussex, UK

Overview

Why EDM? - Theoretical Background The Method of Ramsey Resonance Previous Experiments Ultra-Cold Neutrons The Cryogenic Experiment

EDMs and Time Reversal Symmetry

Picture a spherical particle spinning in a particular direction It just looks like the same particle turned upside down Imagine it running backwards in time Now, imagine it is “pear-shaped” Imagine it running backwards in time It no longer looks like the original particle turned upside down!

CPT Conservation

If T is violated, so is CP ....... Basic assumption: CPT IS INVARIANT

CP violation: 1964

     KS KL Long-lived neutral kaon KL  3 (CP = -1) Short-lived neutral kaon KS  2 (CP = +1) ...but sometimes KL  2, so CP is violated. Conclusion: Nature distinguishes matter from antimatter. e.g. KL - e+ e preferred over KL + e- e. This is the only mechanism we know of for explaining the baryon asymmetry of the universe.

Measurement principle

B E mB Measure Larmor spin precession freq in parallel & antiparallel B and E fields: ... or slower. dn makes precession faster...

Ramsey Method of Separated Oscillating Fields

4. 3. 2. 1. Free precession... Apply /2 spin flip pulse... “Spin up” neutron... Second /2 spin flip pulse.

Ramsey resonance

Phase gives freq offset from resonance

The Room-Temperature Experiment

N S Four-layer mu-metal shield High voltage lead Quartz insulating cylinder Coil for 10 mG magnetic field Upper electrode Main storage cell Hg u.v. lamp PMT to detect Hg u.v. light Vacuum wall Mercury prepolarising cell Hg u.v. lamp RF coil to flip spins Magnet UCN polarising foil UCN guide changeover Ultracold neutrons (UCN) UCN detector

EDM Limits & Theoretical Predictions

Factor ~10 per 8 years Experimental Limit on d (e m) 1960 1970 1980 1990 f ~ 1 Left-Right 10-34 10-22 10-24 10-26 10-32 Multi Higgs SUSY f ~ a/p Standard Model Electro- magnetic neutron: electron: 10-36 10-38 10-40 2000 10-22 10-32 Barr: Int. J. Mod Phys. A8 208 (1993)

Statistical limits

h / 2  E T N d = Factor Current Increase Total increase = x 80 (x200 with new beamline) Polarisation+detection  = 0.75 x 1.5 Electric field: E = 106 V/m x 2.0 Precession period: T = 130 s x 1.8 Neutrons counted: N = 6 x 106 /day x 14.9 (with new beamline) x 2.6

The Neutron Mirror

n n n s s B vc depends on orientation of neutron spin, so can polarise by transmission. >> interatomic spacing; neutrons see Fermi potential VF Critical velocity for reflection: ½mvc2 = VF Ultracold neutrons (UCN): v  6 m/s: total internal reflection possible.

UCN production in Liquid 4He

11 K: l = h/p = 8.9 Å Landau-Feynman dispersion curve for 4He excitations Free neutron dispersion curve: kT = h2/2ml2 (= 2p/l) /1010m-1 Neutrons at 11 K downscatter by emission of phonon Upscattering suppressed: Boltzmann factor e-E/kT means not many 11 K phonons present

Neutron Detection Rate

time (sec) Beam off Excess neutrons at low T due to UCN production & storage Neutron count vs. time

Institut Laue-Langevin, Grenoble

Tower 1 ... ... & Tower 2

Main Vessel, Tower 2 & DAQ Equipment

The Equipment: Cross-Section

0.

The Ramsey Cell

UCN Detection in Liquid Helium

Solid-state detectors developed for use in LHe Thin surface film of 6LiF: n + 6Li  a + 3H

Showing 1 - 20 of 23 items Details

Name: 
edmtalk(jim)
Author: 
P.Harris
Company: 
CPES
Description: 
The Cryogenic Neutron Electric Dipole Moment ExperimentJim Grozier University of Sussex, UK
Tags: 
neutron | ucn | spin | detect | edm | time | detector | ramsey
Created: 
6/1/2000 8:36:13 PM
Slides: 
23
Views: 
5
Downloads: 
0
Rating: 
0


> Comment



Share this presentation
|

Comments

Share this presentation:

|
Sitemap