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HAL Id: jpa-00246478

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An estimate of the uncertainty due to counting statistics in a novel type of neutron EDM experiment

D. Thompson

To cite this version:

D. Thompson. An estimate of the uncertainty due to counting statistics in a novel type of neutron EDM experiment. Journal de Physique I, EDP Sciences, 1992, 2 (3), pp.241-245. �10.1051/jp1:1992139�.

�jpa-00246478�

(2)

Classification Physics Abstracts

B.40F 14.20 29.25

An estimate of the uncertainty due to counting statistics in

a

novel type of neutron EDM experiment

D.

Thompson (*)

Ruthe~ord

Appleton Laboratory,

Didcot, OX11 OQX, G-B- (Recejved 5 July 1991, accepted in final form 8 November 199I)

Abstract. A novel type of EDM

experiment using

ultracold neutrons

produced

in a

supertherrnal

source,

coupled

with the dressed neutron

technique

has been

proposed.

Here an estimate is made of the

uncertainty

in the electric

dipole

moment of neutron that would arise from

neutron

counting

statistics in such an

experiment.

Golub

[I]

has

proposed

a novel method of

searching

for the electric

dipole

moment

(EDM)

of the neutron. Instead of

using Ramsey's separated

fields method

[2-5], polarized

ultra cold

neutrons

(UCN)

are to be

produced

in a

superthermal

UCN source

[6, 7] containing

a small

quantity

of

polarized

3He.

Absorption

of neutrons

by

3He takes

place

almost

entirely through

the channel in which the neutron and 3He

spins

are

anti-parallel [8].

The presence of an electric field the EDM of the neutron will alter the neutron

precession frequency changing

the

angle

between the neutron

spins

and the 3He

spins,

and hence

changing

the

absorption

rate.

A refinement to this idea

[9]

uses the dressed neutron

technique [10]

to

give

the 3He atoms

and the neutrons the same effective

magnetic

moment,

and, therefore,

the same

precession

frequency

in a

magnetic

field. In this paper, we calculate the

uncertainty

in the

EDM,

due to neutron

counting statistics,

for a

particularly simple

form of this

experiment.

Let there be an electric

Eo

and a

magnetic Bo

field

along

the z

axis,

and the initial conditions be 100fb neutron

polarization

and 100fb 3He

polarization,

both

along

+z.

Apply

a

w/2

tipping pulse

to rotate both the neutron

spins

and the 3He

spins

into the x-y

plane.

In the presence of the

dressing field,

and

ignoring

any EDM both the neutrons and the 3He will precess around z with the same

frequency.

Now

interrupt

the

dressing

field for

just long enough

to allow an

angle

of w/2 to build up between the neutrons and the 3He. In a reference

frame

rotating

at the common

precession frequency

the neutrons will now be

aligned along

the

y'

axis and the 3He

along

the x' axis.

Including

the effects of the EDM of the neutron, the

absorption probability

for the neutrons will be

P~(t)

=

( 1«~ (l

+ sin

wt)

+ «_

(I

sin

wt)i, (1)

(*)

Present address :

Department

of

Physics, University

of Zambia, PO Box 32379, Lusaka, Zambia.

(3)

242 JOURNAL DE PHYSIQUE I N° 3

where :

n~ is the 3He

density,

assumed constant

v is the relative

velocity

between the 3He and the neutrons

cr~ is the

absorption

cross section for

parallel spins

cr_ is the

absorption

cross section for

anti-parallel spins

and w =

2 d*

Eo/h

is the

precession frequency

due to the EDM.

We write d* for the EDM because the

dressing

field also reduces the effective EDM. For the

dressing

field needed to set the

magnetic

moments

equal

d*

=

0.7 d~

[9].

We also define :

T+ =

(n3

"+

v)~

the

lifetime,

due to

absorption by

the

3He,

that the neutrons would have if the neutron and 3He

spins

were

parallel

;

T- =

(n3

"-

v)~

the lifetime the neutrons would have if the

spins

were

anti-parallel

;

r~ the lifetime of the neutrons in the storage volume in the absence of

3He.

The evolution of the neutron

density n(t)

is then

dn n n I I n I I

I

To 2 r~ ~ r_ 2 r~ r_

~~~ °'~

=

nri nrj

~/2

(nrj ~/2)

sin wt

(2)

where

r/

=

rj

+ rj and

ri

=

rj

~j For small wt the

absorption

of the neutrons

by

the 3He includes a term linear in d*.

The solution to

equation (2),

with an initial

density

no, is

n(t)

= no

exp[- (rp

+

r/ ~/2)

t +

rj ~(cos

wt

1)/(2

w

)]. (3)

The

absorption

of the neutrons is to be monitored

by detecting

the scintillations

produced by

the reaction

products [I]

n +

~He

- ~H + p + 746 kev

(4)

The detection rate

dN~/dt

is the rate at which the neutrons in a volume V are absorbed

by

the

3He

)

=

Vn

(t) P~(t)

=

Vno

exp

[- (ri

+

rj ~/2)

t +

ri ~(cos

wt

1)/(2

w

)]

x

[r/

~/2 +

(ri ~/2)

sin

wt] (5)

For small wt we can

expand

the

trigonometrical

functions and we find that the number of

absorptions

detected in a storage time T is

Vno

jT

~

N ~ = exp

[- (rj

+ rj

/2) t] [rj

+ w ri (t rj t

/4)

dt 2

~

where x

=

(rp

+

r/ ~/2)

T.

When the direction of the electric field is reversed w

changes sign

and so there is a

change

in

(4)

counts between the situation with

E~

and Bo

parallel

and that with

Eo

and

Bo antiparallel.

If this

change

in counts is

AN,

then the effective EDM is

~

~ j

(rp

+

r/

~/2)~ j

~ ~

2

Eo Vno ri (rj ~[l (I

+

x) e~~]

+

r/ ~x~e~~/4)

~~~

Because the

change

in counts due to an EDM is

small,

the counts, for both

E~

and

Bo

parallel

and

Eo

and

Bo antiparallel,

will be

approximately equal

and

given by

~ ~

'~~

(rj r/ ~)/2

~ ~~ ~~~

and the

uncertainty

in

N~

will be

=

fi

and that in AN

=

fi. Bearing

in mind that

two measurement

cycles

are

required

to deduce

d*,

the

uncertainty

in d* per measurement

cycle

cr~~ is

5

~

( rp

+

r)

~/2 ~

(

l e~ ~

)

~

~~~

fi ri ~/Vno (rp ~[l (I

+

x) e~~]

+

r/ ~x~e~~/4)

~~~

When

comparing

different

experimental

methods it is more useful to look at the

uncertainty

per

day.

If we assume that

filling

the

storage

volume takes a

negligible

time

compared

to

T,

and we let s

= 86 400 the number of seconds in one

day,

the

uncertainty

per

day

is

«~~

~~~

fi

~ i

~(rp

+

r/

~/2)~

ix (I

e~ ~

)]

$ Eo ~/Vno' ri (rp ~[l (I

+

x) e~~]

+ rj

~x~e~~/4)

~~~~

It is the

uncertainty

per

day crj~

that must be minimized in order to

optimize

the

experiment. Setting

the

derivative,

with respect to x, of

equation (10) equal

to zero we have

r) 4[(1 e~~)~ (l

+

x~) x~]

=

(11)

rj~ x~e~~[x(2 e~~) 3(1 e~~)]

USIIIg Ti~

=

r/I

~r~

~ / ~ ~

~~ ~~~~~

~ ~ ~~~ ~~~~~~~~~ °~

~~~~~1°II (lo)

with

respect

to

rj

~/rj

=

3

[2(e~

I

x)/x~- Ii

±

(9[2(e~

I

x)/x~- 1]~

+

8(e~

I

x)/x~)

~

(12)

Equations (11)

and

(12)

were solved

simultaneously, using

a Hewlett Packard 48SX

calculator,

to

give

rj ~/rp

= l.007 and x

=

2.247

From this we deduce that the

optimal ~He density

is that which

gives

rj

= n~

v(cr~

+ cr_ =

rp

~, but we note that for the

experiment

described the lifetime of

the neutrons due to

absorption by

the

~He

is 2 r~. At the same time the

optimal

storage time T

is

= 1.5 To.

(5)

244 JOURNAL DE

PHYSIQUE

I N° 3

In the more

general

case where the neutron

polarization

is not 100

fb,

but

P~, equation (2)

should be

replaced by

~ o 2~~)Pnsinwt

~ ~

(j~~

so that the

uncertainty

per measurement

cycle

and per

day

are increased

by

a factor of

[P~[~ Similarly

for an

arbitrary ~He polarization P~

the

uncertainty

is increased

by '~3'

Using

the

optimal

values r~ = To and x

= 2.247 the dressed neutron

technique gives

an

uncertainty

in the effective

EDM,

per measurement

cycle,

of

h I

("+

+

"-~,

2.33

('~)

~~~

Eo' /~

~o "+ "-

(~n ~3'

and an

uncertainty

per

day

of

~~~ /~''0 fi lo' ))) )- l' ~n~~31

'~'~~ ~~~~

By

way of

comparison Ramsey's separated

fields

method,

with the

storage

time T

= To

optimized

for the minimum

uncertainty

per

day

has an

uncertainty

per measurement

cycle

of

"~

2~o' fi o ~

~~~~

o

where a

m

P(

and is

reported

to be 0.64

by

Smith et al.

[4].

The

uncertainty

per

day

is

~~ ,~ o fi' ~ro'

~ ~~~ ~~~~

A detailed

comparison

of the two methods is difficult without a concrete

experimental design

for the dressed neutron

method,

since

Golub,

Richardson and Lamoreaux

[9]

anticipate

substantial

improvements

in both neutron

density

and electric field

strength.

If we

simply

take the same values of

Eo,

no, V and To for the two cases, use the ideal

figures

of

P~

=

P~

= a

=

I and «~ = 0 and include a factor of 0.7 for the

lowering

of the effective EDM in the dressed neutron case, then the

uncertainty

in the EDM per

day

is

approximately

4.8 times

higher

for the dressed neutron method than for

Ramsey

method. The

anticipated

neutron

density

and electric field

strength [9]

should more than compensate for this.

References

[Ii GOLUB R., J.

Phys.

France 44 (1983) L321.

[2] RAMSEY N. F., Molecular Beams (Oxford

University

Press, 1956).

[3] ALTAREV I. S. et al., JETP Lett. 44 (1986) 460.

[4] SMITH K. F. et al., Phys. Lett. 8234 (1990) 191.

[5] SMITH K. F. et al., to be

published.

[6] GOLUB R. and PENDLEBURY J. M., Phys. Lett. 62A (1977) 337.

(6)

[7] GOLUB R. et al., Z.

Phys.

851(1983) 187.

[8] PASSELL L. and SCHERMER R. I.,

Phys.

Rev. 150 (1966) 146.

[9] GOLUB R., RICHARDSON D. J. and LAMOREAUX S. K., Ultra Cold Neutrons (Adam

Hilger,

Bristol, 1991).

[10] MUSKAT E., DUBBERS D. and SCHARPF O.,

Phys.

Rev. Lett. 58 (1987) 2047.

Proofs

not corrected

by

the author

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