Journey Along the Neutron Dripline &Production: transfer, fission, fragmentation &Predicted...
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Transcript of Journey Along the Neutron Dripline &Production: transfer, fission, fragmentation &Predicted...
Journey Along the Neutron Dripline
Production: transfer, fission, fragmentation Predicted vanishing of the shells has major influence… Proof of existence is easy, 2 or 3 is sufficient Proof of non-existence is much more difficult “Nuclei” beyond the dripline
Along the dripline from Z=0 to ….
Detection of Neutron Clusters
F. M. Marques et al., Phys. Rev. C65 (2002) 044006
14Be 10Be + 4n or 4n
F. M. Marques et al., Phys. Rev. C65 (2002) 044006
4n or not?
F. M. Marques et al., Phys. Rev. C65 (2002) 044006
Superheavy Hydrogen 5H
A. A. Korshennikov et al., Phys. Rev. Lett. 87 (2001) 092501
Observation of 10He
A. A. Korshennikov et al., Phys. Lett. B326 (1994) 31
N=7 and the Level Inversion in 11Be
Level Inversion of 11Be
Configurations of 10Li
s1/2 + p3/2
2- or 1-
p1/2+ p3/2
2+ or 1+
200
160
120
80
10 5 0
Indirect Measurements
ER(10Li) (MeV)
Cou
nts
H. G. Bohlen et al., Nucl. Phys. A616 (1997) 254c
16C(12C, 12N)10Li, ELab = 357 MeV
Invariant-Mass Spectroscopy
M. Zinser et al., Nucl. Phys. A619 (1997) 151
d/d
Td (
barn
/MeV
)Pb Target
C Target
Decay Energy (MeV)0 1 2 3
3
2
1
00.3
0.2
0.1
0.0
Relative Velocity Measurements
Experimental Setup
Detector
1 meter
O
Li
Neutron Detectors
BeTarget
O18
9
18
9 FragmentQuadrupole Doublet
Dipole
A = (N/Z=2) +1 Nuclei
n
3H
6He8He
7Be
8Li 9Li
8B
9C
11Li
11Be10Be 12Be 14Be
12B 13B 14B 15B
10C 11C 15C14C 16C 18C17C 19C
17B
10Li
19B
p 2H
4He3He
6Li 7Li
9Be
10B 11B
12C 13C 20C 22C
16B13Be
7He
4H
Calibration Reaction
7He 6He + n
ER = 440±30 keV
Г = 160 ±30 keV
R.A. Kryger et al., Phys. Rev. C47 (1993) R2439
s-wave Strength in 10Li
p 67%1/2
s 33%1/2
Dec
ay P
roba
bili
ty
Cou
nts
MT et al., Phys. Rev. C59 (1999) 111
Virtual States
0 0.1 0.2 0.3 0.4 0.5M o m en tu m k [f m -1 ]
0.1
1
10
100
1000
W(k
) [
fm3 ]
9Be(12Be,9Li+n)XE s ,p ,d ( in itia l)= -3 .1 7 ,-3 .8 5 ,-4 .9 5 M eVl= 0 a s= -5 ,-1 0 ,-2 0 ,-5 0 f ml= 1 E 1 = 0 .1 , 0 .5 , 1 M eVl= 2 E 2 = 2 .0 M e V
N o I
N o I
E ħ2/2ma2
Scattering Length Calculations
EDecay (MeV)
Yie
ld (
arb
. un
its)
0
10
20
30
40
50
-1.5 -1.0 -0.5 0.0 0.5 1.0 1.5
vn-vf (cm/ns)
0.1
1.0
0.0 0.2 0.4 0.6 0.8 1.0
Yie
ld (
arb
. un
its)
0
-2-1
-5
-10
-100
-30-20
-50
0-5
-10
-100
-30
-20
-50
Energy Relative velocity
9He
L. Chen et al., Phys. Lett. B505 (2001)
The N=7 Isotones
8 7 6 5 4 3 2Atom ic Num ber Z
-14
-12
-10
-8
-6
-4
-2
0
2
E*-
Sn
[M
eV]
14N 13C 12B 11Be 10Li 9He15O
0 10
r [fm ]
0 10 20 30 40
r [fm ]
0 10 20
r [fm ]
15O
11Be
10Li0.5 M eV
1/2+
1/2 -
Vanishing of the N = 8 Shell
9Be – 13C – 17O11Be – 15C
8Li – 12B – 16N
N=8
A. Ozawa et al., Phys. Rev. Lett. 84 (2000) 5493
Extension to Unbound Nuclei
10Li
9He and 13Be
A. Ozawa et al., Phys. Rev. Lett. 84 (2000) 5493
Halo Nucleus 11Li
“A nuclear helium atom…” held together by the attractive long-range-part of the NN force
The Earth
Apollo 17 Crew, NASA
http://antwrp.gsfc.nasa.gov/apod/ap010204.html
RMS-Radii of Lithium Isotopes
Rrm
s (fm
)
Neutron
9Li
Borromean Nucleus: 11Li
Heiko Scheit
Neutron
Unbound Subsystems
n
9Li
n
9Li
n n
10Li 10Li 10Li 10Li Di-neutron Di-neutron
Origin of the Borromean Rings
Il collegio fu costruito su un'area di case e terreni in parte già appartenenti alla famiglia Borromeo su progetto dell'architetto Pellegrino Pellegrini figlio di Tibaldo (1527-1596); la fama della costruzione di questo "palazzo per la Sapienza" inizia con il Vasari nella seconda edizione delle Vite del 1568.
VISITA VIRTUALE DEL COLLEGIO
http://borromeo.unipv.it/visita.htm
Piano nobile
Sala bianca
Sala minore superiore, essa deve il suo nome alle pareti non affrescate. Il motivo decorativo della finta tappezzeria è costituito dai tre anelli intrecciati indicanti il legame inscindibile tra le famiglie Borromeo, Visconti e Sforza. Già originariamente adibita a concerti vocali e strumentali secondo le indicazioni del 1592 date da Federico Borromeo, costituì sala di ricevimento del principe patrono, tuttora comunica tramite doppie porte con l'appartamento poi ristrutturato a camere per studenti negli anni sessanta. Di queste stanze riservate ai soggiorni pavesi rimane interamente affrescata con decorazione ottocentesca la camera da letto. In questo secolo e fino agli anni della ristrutturazione l'appartamento del Patrono ospitò la biblioteca, la sala bianca ne fu sala di consultazione, di questa antica funzione sono rimasti gli armadi bassi per conservare le annate delle riviste.
Translation:
The decorative motif of the fake drapery is constituted by the three connected rings, indicating the indestructible link between Borromeo, Visconti and Sforza families.
http://borromeo.unipv.it/visita.htm, V. Maddalena
DNA
Borromean Rings
Title frame by Scott KimFrom the video "Not Knot"Copyright 1990 by the Geometry Center,University of Minnesotahttp://www.geom.umn.edu
EMSL CollaboratoryWilliam R. Wiley Environmental Molecular Sciences LaboratoryPacific Northwest National Laboratory (PNNL), Richland, Washingtonhttp://www.emsl.pnl.gov:2080/docs/collab/
Prof. Nadrian C. Seeman, Department of Chemistry New York Universityhttp://seemanlab4.chem.nyu.edu/borro.html
Knot Theory
Symbol forCollaborations
More Borromean Rings
Paul BourkeBrain Dynamics Research LaboratoryMelbourne, Australiahttp://www.mhri.edu.au/~pdb/geometry/borromean/
John Robinson, The University of Wales, Bangohttp://www.bangor.ac.uk/SculMath/image/symbscul.htm
Mike Bailey,San Diego Supercomputer Centerhttp://www.sdsc.edu/GatherScatter/GSspring95/gsspring_a17.html
Art
Telemanufacturing
Geometry
Other Usage of the Rings
Recognizing the Importance of Undergraduate Science Education,Robert C. Hilborn, APS News February 1997
UndergraduateScience EducationPre-College
Science Education
Graduate Educationand Research
Brunnian Links
http://www.cs.ubc.ca/nest/imager/contributions/scharein/brunnian/brun6-rem3.mpg
Robert SchareinDepartment of Computer ScienceUniversity of British Columbiahttp://www.cs.ubc.ca/nest/imager/contributions/scharein/brunnian/brunnian.html
Determination of Dripline…
Evidence for Particle Instability of 13Be and 14Be
A.G.Artukh, V.V.Avdeichikov, J.Ero, G.F.Gridnev, V.L.Mikheev, V.V.Volkov, J.Wilczynski
Phys.Lett. 33B, 407 (1970)
Discovery of Two Isotopes, 14Be and 17B, at the Limits of Particle Stability
J.D.Bowman, A.M.Poskanzer, R.G.Korteling, G.W.Butler
Phys.Rev.Lett. 31, 614 (1973)
Ground State of 13Be
13Be Relative Velocity Spectrum
s-wave, as = -20fm
d-wave,EDecay = 2MeV
Background
v - v (cm /n s)n f
Cou
nts
0
1 0 0
2 0 0
3 0 0
4 0 0
5 0 0
-3 .0 -2 .0 -1 .0 0 .0 1 .0 2 .0 3 .0
Could 16Be be bound?
-202468
1012141618
6 8 10 12 14 16A
1n 2
n Se
para
tion
Ene
rgie
s (M
eV)
2n Separation Energy 1n Separation Energy
16Be: Constant Z (=4) Extrapolation
16Be ??
16Be : Constant N (=12) Extrapolation
-505
10152025303540
3 4 5 6 7 8 9 10 11 12 13
Z
1n 2
n S
epar
atio
n E
ner
gie
s (M
eV)
2n Separation Energy 1n Separation Energy
No 16Be
16Be: Constant A (=16) Extrapolation
-5
0
5
10
15
20
25
30
3 4 5 6 7 8 9 10
Z
1n 2
n S
epar
atio
n E
ner
gies
(M
eV)
2n Separation Energy 1n Separation Energy
16Be
Shell Model Calculation
16Be ?? 19B and 22C are boundB.A. Brown, private communications
Previous Measurements
H. Sakurai et al., Phys. Lett. 448B, 180 (1999) A.C. Muller and R. Anne, NIM B56, 557 (1991)
16Be ??
Coupled Cyclotron Facility at the NSCL
40Ar7+
12.3 MeV/A140 MeV/A
4.9A
1.0A470nA
280nA
6.0 Tm
40Ar7+
40Ar18+
No Evidence for 16Be
16Be is not bound 16Be is not bound
Neutron Radioactivity
First Observation of -delayed Two-Neutron Radioactivity
L.C. Carraze et al., Phys. Rev. Lett. 43 (1979) 1652
9Be+2n
10Be+n11Be
11Li-
n2n
T1/2=8.7ms
Search for Neutron Radioactivity
16B
1 2 s
/ 1
3 2
p /
11
2 s
/ 2
1 2 s
/ 1
1 2 p
/ 1
3 2 p
/ 1
5 2 /
d 1
Last neutron
V (
MeV
) Centrifugal (l=2)
Radius (fm)
-40
-20
0
20
2010 15
-60
60
40
5
Nuclear
Total
16B Potential
E = 10 keV T1/2 = 3.7·10-16sE = 1 keV T1/2 = 1.1·10-13s
16B Lifetime Measurements
13 14 15
16
17
H. G. Bohlen et al., Nucl. Phys. A583 (1995) 775
J. D. Bowman et al., Phys. Rev. C9 (1974) 836
M. Langevin et al., Phys. Lett. 150B (1985) 71
Lifetime of 16B
10-9
10-10
10-11
10-12
10-13
10-14
10-15
10-16
10-17
10-18
10-19
10-20
10-2110-7
10-8
Direct LifetimeMeasurements:Time of Flight
Indirect Measurement:width of state < 200 keV
with: = ħ 2·10-21s
Possible range for the 16B lifetime
Stopping of Fragments
16C + 12C 15B 17C + 12C 16B
Beams of 17C, 16C
Secondary Target:114 mg/cm2 12C
5cm
Si-E Si-E
Production of 16B
13 B 15B
0
20
30
40
10
0 20 40 60 80Mass (arb. units)
Cou
nts
16C + Target 15B + p16C + Target 15B + p 17C + Target 16B + p17C + Target 16B + p
13B 15B
16B
Mass (arb. units)
0
30
60
90
120
Cou
nts
0 20 40 60 80
Energy Spectra
16C + Target 15B + p16C + Target 15B + p
600 650 700 750Energy (MeV)
5
10
15
Cou
nts
17C + Target 16B + p17C + Target 16B + p
Cou
nts
Energy (MeV)
5
10
15
600 650 700 750 800
New Limits for 16B
10-9
10-10
10-11
10-12
10-13
10-14
10-15
10-16
10-17
10-18
10-19
10-20
10-2110-7
10-8
Possible range for the 16B lifetime
Reduction of almost 2 orders of magnitude
New results
New Shell Structure?
Z=8
N=8
N=16 ?
N=20
??
Evidence for N=16 Shell
A. Ozawa et al., Phys. Rev. Lett. 84 (2000) 5493
Search for 21B
Session SD - Nuclear Structure IV: Light Nuclei.
ORAL session, Saturday morning, October 20
Illima, Outrigger Wailea Resort
[SD.007] Search for 21BY. Yamaguchi, T. Suzuki, T. Izumikawa, T. Kato, Y. Kawamura (Niigata University, Japan), A. Ozawa, T. Yamaguchi, T. Zheng, R. Kanungo, T.Ohnishi, T. Suda, I. Tanihata, K. Yoshida (RIKEN, Japan), S. Momota (Kochi University of Technology, Japan), K. Kimura (Nagasaki Institute of Applied Science, Japan)
We performed search for 21B with a 95A MeV beam of 40Ar for the first time. Recently, we observed that a new magic number N=16 appears in very neutron-rich nuclei so that the very neutron-rich 21B may be bound. The production cross section of AB isotopes (A = 15,17,19,21) on Be and Ta targets have been measured through projectile fragmentation. Particles were identified by the time of flight (TOF), the energy loss (ΔE), and the magnetic rigidity (Bρ) using the fragment separator RIPS at RIKEN. We observed no event of 21B. The upper limit for the production cross section as well as the comparison with the empirical parametrization code (EPAX) will be presented.
First Joint Meeting of the Nuclear Physicists of the American and Japanese Physical Societies,
October 17 - 20, 2001, Maui, Hawaii
Search for 26O
Cou
nts
Z
4 98765 1 0 11
1 0 1
1 0 3
1 0 2
C2 0
N2 3
B1 7B e1 4
O2 6F2 9
N e3 2N a3 5
D. Guillemaud-Mueller, et al. Phys. Rev. C41 (1990) 937M. Fauerbach, et al. Phys. Rev. C53 (1996) 647
26O
Search for 28O / Existence of 31F
H. Sakurai et al., Phys. Lett. 448B, 180 (1999)
2n Separation Energy Systematics
shell closure subshell deformation
Fe
Cs
50 56
Two-Neutron Separation Energies
Double Magic 78Ni
Search for 78Ni
V.A. Rubchenya and J. Äystö, Nucl. Phys. A701 (2002) 127c
Experimental Limit
0.1 μb
Calculation
1 nb
Observation of 78Ni
M. Bernas et al., Phys. Lett. B415 (1997) 111
0.3 nb
Identification of New IsotopesIo
niza
tion
Cha
mbe
r
J. Benlliure et al. Nucl. Phys. A660 (1999) 87
238UFragmentation950 MeV/u
Time of Flight
Ion
start stop
E (Ionization chamber or Si)
Total Energy
Fission of Fission Fragments??
0.0 20.0 40.0 60.0 80.0 100.0 120.0 140.0N (A-Z)
0.0
10.0
20.0
30.0
40.0
50.0
60.0
70.0
80.0
Z
r-processpath
rp-processpath
RI yield in ions/s
>1012
1010
108
102
1.0110-4
10-6
106
104
R e g io n o fK n o w n N u c le i