Nuclear Physics AS08 (1990) 2G%-214~ North-Holland
209~
RECENT RESULTS ON NN PHYSICS
D.V. BUGG Queen Mary College, London El 4NS, UK
New np elastic data of Abegg et al. stabilise I= 0 phase shifts from 200 to 500 MeV. New data of Hutcheon et al. on KSS for pp + dn+ at 515 MeV agree well with the amplitude analysis of Bugg, Hasan and Shypit and correct a sign error in some published data of Cantale et al. A new analysis is reported of all current data of NN -LNNa from 420 to 800 MeV. A strong threshold cusp is observed in the NA S wave; it is not yet clear whether or not a bound state pole (quasi-deuteron)is required. In other partial waves, phases of amplitudes are negative or weakly positive and rule out dibaryon resonances.
1. NN ELASTIC PNASE SHIFTS There have recently been two precise measurements of np elastic scattering at 1 TRIDMF. Firstly, Abegg et al. have measured the ratio DT/RT at 160° at four 7 energies from 223 to 492 MeV with errors tO.01. Secondly, the same group- has measured
at 220, 325 and 425 MeV from 52 to 145' with errors of ANN* ANO and AoN %O.Ol to 0.02. These data stabilise significantly3 the I= 0 phase shifts from 200 to 500 MeV, although there are no large systematrc changes. In partrcular, 4 cl is much improved and smoother, and agrees well with the latest predrction of the Bonn potential.
f
2, PP +D?r
At TRIDMF, Kutcheon et al.5 have recently measured the spin transfer parameter KSS in pp + dn+ at 515 MeV.
0.15
Results, shown in Fig. 1, agree 0.10
reasonably well with the Latest amplitude analysis of Bugg, Hasan and Shypit6. Theydisagree in sign with results of Cantale J et al. The Geneva group now
Unceriojnties due to errorbarson iTl1and T21
0.05 a : 000 w -3 -0.05
agree that their &LS(x) and ezs(x) results at 447 and 515 MeV should be reversed in sign and their sLS(z) and ~~~(2) data should be reversed in sign at all energies, The amplitude
1
-0.15
0
I
30
I
I
t
,
60 90 120 150 oeuteronc-m.angle
1 181)
Fig. 1. KsS data of Hutcheon et al. and the prediction of Bugg,Hasanand Shyprt,
0375-9474 I90 / $3.500 Else&rScience Pubfishers B.V. (North-Holland)
21oc
D.V. Bugg I Recent results on NN physics
of Bugg, Hasan and Shypit used ratios
analysis
of data and is unaffected
by
these sign changes.
3. AMPLITUDE
ANALYSIS
An outstanding
OF NN -+ NNa: DATA AND INGREDIENTS
issue is whether
or not there exist broad dibaryon
(or bound states) in the range 5008 al. first proposed their existance AaT data. analysis ever,
in the Argand
Hidaka
et
on the basis of peaks and dips in AaL and
diagrams
that the opening
A resonance
to be coupled
strongly
to NA, and it 1s
of the NN + NA channel will produce
channel bearing
(via analyticity)
a strong resemblancetothe
at s= so should produce
NN -+ NN and NN -f NA, hence wave amplitude
are observed In NN elastic phase shift 13 for D2, F3 and 3~2 (and possibly 3F4). How-
are well known
cusps in the elastic loops.
resonances
Well defined half-loops
these states
certain
800 MeV of proton beam energy.
an amplitude
a rapid anti-clockwise
= (6
0
observed half-1 In both
- 6)
phase variation
in the partial
for NN + NA.
An amplitude
analysis
is in progress
using
the complete
set of world
data on
NN -+ NNn. of Wicklund et The main data sets are: (i) doldS1, ANo, AS0 and A 9 LPO at 800 MeV, al. at 569 and 806 MeV, (ii) do/da and AN0 of Hancock et al. plus AN0 and recoil proton NN' D9f' DLQ 12 and Riley et al. at 650, 733 and 800 polarisation AooNo of Hollas et al. 13 at 492, 576, MeV, (iv) ALL, ASL, ANL, ANo, ASo, AI0 and AOL of Shypit et al. 14 at 650 and 800 MeV of Bhatia et al. 643, 729 and 796 MeV, (v) ANN and ALL at (iii) Wolfenstein
parameters
D
650 and 800 MeV, and (vi) ANN, ASS, PtL, ASL, AN0 and AON at 510, 465 and 420 15 et al. ++ In this analysis, partial wave amplitudes are parametrrsed for pp + nA as
MeV of Waltham
fL,J where
= AI, J(s)
BL J(s) eioLtJcs)
BL J is the Born partial
exchange'and
(1)
,
wave amplitude
A and 4 are real parameters
Born amplitudes
++ for pp + nA
via single
fitted to the data at each energy.
The
take the form MA
BL,J a MA - M
(2)
- ir A (Mpn+) gL,J(B'e")' Pr+
is the mass of the pn+ pair and MA, rA are a Layson P+ The function parametrising the nN P33 phase shift accurately.
where M
standard
angular momentum
decompostion
form gL,J gives the
in terms of 8, the production
angle of
and Treiman-Yang angles of the A decay. the A++ and (El,+) the Gottfried-Jackson + The amplitudes for pp + pA are added coherently with isospin Clebsch-Gordan coefficient dependence
l/3 and with
identical
parameters
to
(1) and (2) but kinematrc
on M,,+ and 8', 8', $I', the angles describing
the nr+ pair.
211c
D.V. Bugg I Recent results on NN physics
The small nN partial in Born approximation S wave)
waves
in 3Pl + 3Sl, which
the elastic
NN phase
Sll, S31, Pl3, P31 and Pll are presently
(+= O), except
is a large amplitude; Later,
shift.
to 6NN, but this requires
has been investigated,
< 1890 MeV; below
events
this mass,
included
for the xN
here A is fitted and $ = 6NN,
it is the intention
that all $Iwill be set
a full partial wave decomposition,
The NN final state interaction role for M(np)
for NN + NS (where S stands
not yet Implemented.
but appears
are discarded
to play no In order to
avoid this complication. One might determined
think that the 16 helicity
amplitudes
using 31 spin configurations.
a spin change AS = 2 or 3 and are accurately (AL dominantly the alignment
Also, density matrix
0 or 1).
of the A via the dependence
for NN -+ NA could only be
However,
8 of the amplitudes
predicted
by OPE at low momenta
elements
for A decay determine
of observables
is that all partial waves are well determined 5 3 PO + 3Po and '02 + 3D2). very small ('So + Do, Results
are presented
in Table
but merely
phase
a parametrisation
The
which
are
1, setting 4(s) = 6 (s) + $(s). Note that 16 NN have pointed out) and Lee" (as Hoshizaki
shift
of the effect
Fig. 2 shows that 6F becomes
on 6, 9 and 9.
except for those
upshot
~5~ is not the NA elastic
involve
of the final state interaction.
the NA elastic
phase shift in the limit of weak
scattering. Ryskin whether
absolute
or whether
18
and Strakovsky phases
dibaryon
A __----
N have questioned
are well determined,
resonances
&F
&NN
might be
present
in -all (dominant) partial waves. The answer is that the OPE contributions to 'GL and 3H5 amplitudes
0
N
N
from 650 to 800
MeV are large and act as a powerful interferometer, with an accuracy
defining
absolute
of 6- 9O.
phases
Furthermore,
Fig. 2.
The motivation
behind
form chosen for equn.
at low energies, between
theinEerference 3 NN -f NA and the Pl + 3Sl NN + NS amplitude
the
(1).
is large.
There
is a
strong NN repulsion in the initial state of the latter partial wave and a mild 0 (~10 1 repulsion in the IIN final S state. It therefore appears an unlikely candidate
for a partial
reference
phase.
wave which will resonate,
Allowing
and can be used to fix a
for the initial and ITN phases,
the fits are consistent
with 6 = O", with an error of again 6 - 9“. This gives a second NS determination of absolute phases, consistent with the first.
independent
4. INTERPRETATION For NA P and D waves,
6, takes small positive
values
or is negative,
D.V. Bugg I Recent results on NN physics
212c
Table
1. Current Errors
scaling
factors A and phases
are statistical.
Angles
6F for NN + NA amplitudes.
are in degrees.
-----_ Energy 576
643
729
(1)
(1)
(1)
1.35kO.6 (1) ------~-
-5.25 2.2
-2.8~ 1.0
-4.5+ 0.6
-2.8* 0.4
1.3-+ 0.3
0.3+ 0.2
0.7* 0.1
0.682 0.06
3Pl 2; 5P2 :a2 "2 ! 5D I 5 2l P3 i
-1.85t 0.2
1.09+0.15
0.33+ 0.03
1.3+ 0.5
1.32 0.2
0.92 0.2
-4.5f 0.8
-4.5t 0.4
2.9+ 0.4
3.4+ 0.4
1.7 * 0.2
1.2+0.14
1.06 ? 0.12
1.18kO.08
1.05i: 0.16 0.78 f 0.16
0.70+0.08
-2.8
(1)
(1) (1)
(0.851)
(0.771)
(0.761)
(0.741)
(1)
(1)
(1)
(1)
(1)
(1)
3.1+ 0.3
0.14
1.05& 0.10
(0)
(0)
(0)
(16)
(0)
(0)
1.12kO.08
+0.3
(1)
I3.95+
5D 3O pO
796
-4.8f 1.4 3.1tO.6
SF
-1.54fO.14 1.62eO.08
0.78kO.02 (1)
2.2 * 0.2
0.92+0.06
1.4
0.82 f 0.04
(0)
(0)
232 9
(0)
43f8
46? 7
(0)
12i: 6
-4? 7
(0)
-9? 16
C-20)
-35+ 10
-73+5
(0)
C-10)
C-15)
-27f 5
-37c3
11* 11
-2f 6
6+5
56t9
43+ 7
36? 4
(0)
(0)
C-7) 18? 7
(0) (0) 92 14
ruling
out dibaryon
resonances.
phases
are positive;
however,
partial
+0.12
0.84+ 0.02
7f7
-4*4
24+4
11+2
/
(0)
(0)
;
-7* 7
-30"8
-6026
I
16+ 5
13f4
18+ 2
~
determined,
1
(MeV)
492
and is sensitive
waves are modified,
The one possible this partial
eg by leaving
not make too much of this partial For the NA S wave,
wave
(major systematic
is in
falling
I
3 PO, where
is very weak and poorly shifts when the small ?rN
out the small P waves).
wave until
BF takes values
exception
~-
its determination
One should
is more certain.
from 56' at 492 MeV to 11' at
796 MeV, as shown in Fig. 3. A similar result has been deduced by Ferreira, 19 The large values and Dosch from data on rrd elastic scattering.
de Andrade
of 6 near threshold call for some quantitative explanation. F It seems likely It is clear that the NA threshold plays a dominant role. that the open channel NA -+ NN will
lead to a dependence
l/vNA for the NA total
213~
D.V. Bugg I Recent results on NN physics
smeared
optical
theorem,
6F
(deg)
a step in Im fL J(NA -+ NA) at
this implies threshold.
the
Using
cross section.
Of course,
out by the width
of the A.
this step requires
analyticity,
50
this siep wrll be
i
By
1
1
25
a cusp
x
in Re f
+ NA) at threshold. L,.J(NA What needs to be done, but has not yet
been done,
is to see whether
channel K matrix
or whether nearby
state or virtual
between analysis
Fig. 3.
his formalism needs
800 (MeV)
The NA
S wave phase.
for a
state.
claims that a bound
Hoshizaki"
a few MeV of the NA threshold,
large coupling
600
Lab energy
length
there is a requirement
appears within introduces
scattering
(with complex k for the A)
bound
400
the coupled
for NN, rd and NA can be
fitted with a simple prescription
f
0 !-_
to NNn channels
and the assumptions
i.e. a quasi-deuteron;
state pole however,
he
other than NA, and the consistency built
into the current
amplitude
clarification.
REFERENCES 1) R. Abegg
et al. Phys. Rev. C38 (1988) 2173.
2) R. Abegg
et al. submitted
3) D.V. Bugg submitted 4) R. Machleidt, York,
to Phys. Rev. C
to Phys. Rev. C.
Adv. Nucl. Phys.
19 (eds. J.W. Negele
and E. Vogt, Plenum,
New
1988) p. 189.
5) D.A. Hutcheon
et al. TRILJMF preprint
1989.
6) D.V. Bugg, A. Hasan and R.L. Shypit, Nucl. Phys. A477 7) G. Cantale 8) H. Hidaka
et al. Helv.
Phys. Acta 60 (1987) 398.
et al. Phys. Lett.
70B (1977) 479.
9) A.B. Wicklund
et al. Phys. Rev. D35 (1987) 2670.
10) A.D. Hancock
et al. Phys. Rev. C27 (1983) 2742.
11) C. Hollas
(1988) 546.
et al. Phys. Rev. Lett.
55 (1985) 29 and prrvate
communication.
12) P.J. Riley et al. Phys. Lett. B197 (1987) 23, 13) R.L. Shypit et al. Phys. Rev. Lett. 60 (1988) 901. 14) T.S. Bhattia
et al. Phys. Rev. C28 (1983) 2071.
15) C.E. Waltham
et al. Nucl. Phys. A433
16) N. Hoshrzaki, 17) T.-S.H.
LJnrv. of Kyoto
Lee, ANL preprint
18) M.G. Ryskin 19) E. Ferreira,
preprrnt
(1988).
(1989)
and 1.1. Strakovsky, S.C.B.
(1985) 649.
de Andrade
Phys. Rev. Lett. and H.G. Dosch,
61 (1988) 2384.
Phys. Rev. C36 (1987)
1916.