The electric form factor of the proton
G can also be measured during this experiment with a minimum of overhead and
additional instrumentation. There are two ways of determining G with polarized
ammonia targets: measuring the inclusive cross section asymmetry for elastic e-p
scattering on the polarized hydrogen nuclei in NH , and measuring the asymmetry for
electrodisintegration of the deuteron, with detection of the polarized protons in
ND
. Both methods can be used in the present experiment. The former approach is of
interest for an accurate determination of G, the latter method provides an ideal
test of our understanding of the reaction mechanism of the
reaction used for the determination of G as the same
reaction with the same potential complications (FSI, MEC) is used to measure a
known quantity , G.
For a precise determination of G the easiest way is the measurement of the asymmetry
by detecting the electrons scattered elastically from the protons in ammonia. The experimental asymmetry
is related to
through the beam and target polarizations
and
, and the dilution factor f, which is just the ratio of the number of polarizable
hydrogen nuclei
times the e-p unpolarized cross section
to the sum of
the number of nuclei of each atomic species in the target material times their
respective e-A cross sections
, integrated over the experimental
width of the elastic peak:
In the region of energy loss of the elastically scattered electrons,
is dominated by the quasielastic scattering contribution. For an estimate of the rates,
the full magnitude of
can be calculated with the aid of the QFS code of
Lightbody and O'Connell. The experimental width of the elastic peak has been estimated
from the beam and final electron energy resolutions, spectrometer angular resolution
and contributions from energy losses and multiple scattering in the target and electron
path. The estimates range from
MeV at low Q
to 17 MeV at high
Q
.
For the input values of ,
, and using the HMS solid angle
acceptance of 10.4 msr we have computed the expected counting rates and required time to
measure
with a 2% statistical precision. The luminosity assumed is the
same as that of the
part of this proposal: 40
Hz cm
. The
results are shown in the table 3.
In this type of measurement, a correction has to be made for the asymmetry (entirely
quasielastic) induced by the polarization of the nitrogen. This small systematic effect
can be estimated with reasonable accuracy from the shape of the scattered electron
spectrum on both sides of the elastic peak. Its magnitude is small because the
contribution to this asymmetry comes from the unpaired proton in N only, the
paired nucleons in this nucleus cannot be polarized. In addition, this asymmetry can
actually be computed from the easily measured polarization of
N and its shell
structure, which places the unpaired seventh proton in a
state, with a net
1/3 probability of being aligned opposite to the
N spin. Measurements of the
N polarization in
NH
indicate that
% for
%, so the expected nitrogen contribution is
% of the proton asymmetry. The uncertainty in this
contribution is less than 10%.
The above estimates show that is a highly competitive method for a
precision determination of G. The corresponding data taking times are actually
considerably smaller than the ones discussed in the
proposal of Perdrisat et al (PR89-014).
Of more direct interest to the determination of G is the option to measure
G via the reaction. This reaction involves the same
complications as the
reaction used for the determination of
G and a measurement of the known G allows to check our understanding
of the reaction mechanism in an ideal way. FSI and MEC influence
and
in a nearly identical way.
Such a measurement of G via is obviously much easier than
the measurement of G: G is much larger than G, and the detection
efficiency for protons is close to one. The rate for G is 10 - 100 times higher.
The main difficulty involved with the detection of protons is that the strong target magnetic field produces a substantial deflection of the protons. For the integrated field times path length magnitude of 1.34 Tesla-meters table 4 shows the total vertical deflection of the protons at the plastic detector location.
The column labelled contains the deflections of the
scattered electrons that start in the horizontal plane;
are the
deflections of the corresponding protons that also leave the scattering point
horizontally;
on the other hand is the deflection angle of the
protons associated with electrons that enter the spectrometer at the horizontal plane
after being deflected downward, from an upward initial direction. The latter protons
would correspond to an electron phase space that is symmetric about the horizontal
plane and therefore are the preferred ones for detection. Their deflections are
tabulated in the last column. It should be pointed out that these values correspond to
protons along the central momentum transfer. For momentum transfers corresponding to the
upper or lower limits of the electron spectrometer's horizontal acceptance, the
deflections (in parentheses) are smaller or larger, respectively. The worst case is for
Q
=0.5 (GeV/c)
.
The contributions of the polarized protons in nitrogen are somewhat larger than in the
case of inclusive measurements, even if ND
is used, because the nitrogen
polarization is
of the deuteron, so the correction is -1/18 = -5.5%, a
correction that easily can be calculated to the accuracy desired for the check envisaged
here.
On the other hand this choice of
N as
target material has the very important additional advantage of entirely eliminating the
nitrogen polarization contributions to the neutron measurement since
will be
measured with electron-neutron coincidence spectra, which obviously contain no proton
contamination, except from second order processes, as discussed elsewhere in the
proposal.