apologies mass-driven physics mass programs now...
TRANSCRIPT
• apologies • mass-driven physics• mass programs now• comparisons• what should we do?
Physics opportunities with EURISOL (16-21 January 2006)
Motivationmetrology: 28Si atomic mass standard (kg)
and other fundamental constants(Rainville et al., Science 2004)
atomic physics: QED test - atomic binding energy)(Verdu et al., PRL 2004)
weak interaction: nuclear astrophysics: CVC and SM tests nucleosynthesis, cosmochronology
→ orientation of mass models
nuclear structure: shells, shapes, pairs, halos
Dave L.
Plenty of ApfelStrudel
“Hey guys, is there any
Apfelstrudel left ?”
nuclear structure from the mass surface
nuclear structure from the mass surface
180 185 190 195 200 205
-0.6
-0.4
-0.2
0.0
0.2
0.4 ISOLTRAP data
Δn ground state
N (80Hg)125115 120110105100
δ<r2> ground state
δ<r2> isomeric state (J. Bonn et al., 1972)
δ<r2 >
(fm2 )
A (80Hg)
0.6
0.8
1.0
1.2
1.4
Δn (M
eV)
S. Schwarz et al., Nuc. Phy. A (2000)
Pairing: nuclear fine structure from the mass surface
S2n : 30 MeV; shell gap: 3 MeV; pairing gap: 0.3 MeV ⇒ δm ≤ 10−7
m
Test of the CVC hypothesis and CKM unitarity
comparative half-life ofsuperallowed β emitters
5/ 2-
0+
22Mg
26mAl
62Ga
74Rb
62Zn
14O
38mK
f (Q5) statistical rate functiont (T1/2,b) partial half-lifeδC nucleus-dependent correction
)1(2)1)(1( 2 V
RVCR G
KftFtΔ+
=−+≡ δδ
9 decays measuredwith ±0.1% in Ft
other 0+ → 0+ emittersaccessible
require: δm/m ≤ 3 10-8
known masses
r-process pathβ − decay path
β decay
one / two-delayed
neutron decay
p-isotopes-isotoper-isotope
PbTl
Hg
HfLuYbTmEr
AuPtIrOsReWTa
PoBi
At
neutron number 126
sstable isotopes-process path
β
Stellar Nucleosynthesis(A ∼ 200)
D. Lunney et al., ENAM 1995 (Arles)
mass model comparisons
See: Lunney, Pearson & Thibault, Rev. Mod. Phys. 75 (2003)
35 40 45 50 55 60 65 70 752
3
4
5
6
7
Z
N =
82
shel
l gap
(MeV
) EXP FRDM Duflo-Zuker HFB-2
‘‘…might even be relevant for the study of mass redistribution following super nova explosions...’’
Techniques
Indirect (energy)
reactions:A(a,b)BQ = MA+ Ma- Mb- MB
decays:A → B + αQα = MΒ− MΑ
Direct (mass spectrometry)
time of flight:
TOF = (m/q) (L/Bρ )
cyclotron frequency:
fc = qB/mISOL(keV)
FIFS(MeV)
PRODUCTIONSCHEME
betterprecision
bett
erse
nsiti
vity
‘the best of both worlds’
gas cellRFQ
SHIPTRAP (GSI)ESR (GSI)
CPT (ANL)LEBIT (NSCL)
TITAN (TRIUMF)
SPEGCSS2 (GANIL)
ISOLTRAP (CERN)MISTRAL (CERN)
SMILETRAP (MSI)
RIKENRING
FSU-TRAP
JYFLTRAP
MAFFTRAP
UW-PTMS
mass measurement programs at GANIL
Resolving power: 104
extremely sensitive
SPEG
SPEGtime-of-flight
+ magnetic rigiditym = q Bρ T / L
CSS1
H. Savajols et al., ENAM 2004
4
9
14
19
24
29
34
16 18 20 22 24 26 28 30 32
N
Si
PS
Cl
Ar
Ca
S 2n[MeV
]
PRELIMINARY
mass measurement programs at GANIL
CSS1 CSS2
CSS2time-of-flight:
phase differencewith acceleration
(longer flight path)
see M. Chartier J. Phys. G (2005)NUSTAR Proceedings
mass measurement programs at GSI
Isochronous Modevery fast
but not so precise
Schottky Modevery precise
but cooling slow
Experimental Storage Ring:Δm/m = γt
2 Δf/f + (γt2 − γ2) Δv/v
IMS 2002M. Matos, Ph.D(2004)
SMS 2002E. Kaza, Ph.D(2004)
Yu. Litvinov, Ph.D. (2003):~ 600 species in the ring
466 masses measured(117 calibration masses)139 masses from links200 improved masses75 new mass values
IMSJ. Stadlmann et al., Phys. Lett. (2004)
For drip line physics discussion see: Novikov et al., Nucl Phys A (2002)
mass is input parameter for halo models
see Y. Litvvinov et al. Nucl. Phys. A (2005)
RF
B
referencebeam
ion counterISOLDE60 kV beam
RF
1 m
magnet
slit 0.4 mm
FAST: short T1/2
fc fc
frequency (kHz)
505000 505100 505200
trans
mitt
edio
n si
gnal
(cou
nts) f = (n + ½) fc
MISTRAL: Mass measurements at ISOLDE with a Transmission RAdiofrequency spectrometer on-Line
C. Bachelet et al.,Eur. Phys. J. A (2005)
11Li(T1/2 = 8.6 ms)
CERN Courier, May 2004
Superlarge nuclei at ISOLDE vie for attention with the superdeformed and the superheavy
ISOLDECERN, Geneva
proton beam1 GeV HRS
GPS
REX-ISOLDE
MISTRALISOL-TRAP10 m
1 m
The mass spectrometer ISOLTRAP
2 cm
hyperbolicPenning trap:precision massmeasurement
cylindricalPenning trap:
isobar separa-tion & cooling
20cm
Gas-filled RF-Paul trap: universal beamcollector
low energy bunchescontinuous60 keV ISOLDE beam
N = 40 Shell closure ?
-0.5
0
0.5
1
1.5
2
2.5
3
3.5
24 26 28 30 32 34 36 38 40
Proton number Z
ΔN
(MeV
)
N=39N=40N=41N=38
39
38
40
41
40 shell closure?in between 39 and 41
C. Guénaut, ‘Is N=40 magic?’(Ph.D., U. Paris-Sud, 2005
SHIPTRAP facility at GSI
ISOL facility for transuranium nuclides
92Mo (58Ni,xpyn) 147Ho→ new masses for 147Ho, 147,148Er (∼10−6)
(M. Block et al., ENAM04)
trapcoolercooler
ionguidemass
separator
JYFLTRAP at the IGISOL facility in Jyväskylä
ISOLDE elementsJYFLTRAP masses from IGISOL:
V. Kolhinen, NIMB (2004) & Ph.D.S. Rinta-Antila et al., PRC (2004)A. Jokinen, ENAM04 (2004)
U. Hager et al., PRL (2006)
Canadian Penning Trap (CPT) facility at ANL
22Mg: Savard et al., PRC (2004)68Se: Clark et al., PRL (2003)
252Cf fragmts : Wang et al., ENAM04beam
Low Energy Beam & Ion Trap (LEBIT) facility at NSCL/MSU
http://www.nscl.gov/lebit
G. Bollen et al.,ENAM 2004
∞ 106 103 100 10-310-9
10-8
10-7
10-6
10-5
10-4
JYFL COOL
CPT
ESR SMS
ISOLTRAP
ESRIMS
MISTRAL
CSS2
SPEG
rela
tive
unce
rtain
ty
half life (seconds)
Performance of the various methods
See: Lunney, Pearson & Thibault, Rev. Mod. Phys. 75 (2003) 1021
JYFLTRAPLEBIT
SHIPTRAP
reactions and decays(so-called ‘indirect’ techniques)
Decay studies: masses byproducts (Q-values)Z = 114/116: Oganessian et al., PRC (2004)
135Tb p decay: P.J. Woods et al., PRC (2004)130Eu p decay: C.N. Davids et al., PRC (2004)233Am α decay: M. Sakama et al., PRC (2004)265Bh α decay: Z.G. Gan et al., EPJA (2004)130Cd β decay: I. Dillmann et al., PRL (2003)
Reactions: masses of unbound nuclides15F: W. A. Peters et al., PRC (2003)11N: V. Guimarães et al., PRC (2003)25O: W. Mittig et al., (2004)
Mass values for the most exotic species
Also: 26Si (p,t) 28SiJ. Caggiano et al.(NUSTAR05)
Q25
Q26
Q31
Q33
Q35
MAYAradioactivebeam
D3P
D4P
26F (d,3He) 25O reaction
- - - - - - - - -
- - -
+ + + + + + + ++ + +
XYZ
SPEG
masses of unbound nuclides using MAYA at GANIL
See poster of C.-E. Demonchy
Z
Y X
MAYA
MAFF facility at FRM-II
Münich Accelerator for Fission Fragments
trap
n-rich nuclides
trap
funnel
Bavarium
D. Habs et al., ENAM 2004(MAFF workshop 04/2005)
ISAC beam
TRIUMF Ion Trap (TITAN) facility
Paul trapCooling and
Bunching (1-5ms)
EBITRapid charge
breeding (2-30 ms) Wien filterm/q selection
Penning trapPrecision mass measurement
(~ 10-100ms)
J. Dilling et al. ENAM04
Mass measurements
• T1/2 ≈10 ms
• δm/m < 1⋅10-8
•Operational 2006
fc = qB/m
Multiple-Reflection TOF-MS
Casares, Geissel, Plass, Scheidenberger, Wollnik et al.(Proc. 48th ASMS Conf. Mass Spectrom. Allied Topics, Long Beach, CA, 2000)
Ion SourceReflector 1 Reflector 2
MCP-Detector
mass measurement accuracy (~ ppm)short measurement durations (< 1 ms)
Beyond the horizonBeyond the horizon
GSI ’s futureFacility for Antiproton andIon Research(FAIR)
FAIRTRAP(MATS)
→ K. BlaumFAIR RINGS(ILIMA)
Preliminary Experimental Layout – Side View
2.0
4.5
4.8
test -ions
cooler-trapprecision-trap
RFQ - cooler/buncher
EBIT
Side View
Roof crane (2 T)
8.0
Detectors:- FT-ICR- TOF-ICR- Si(Li) electron
EBIT:charge breeding
q/m selection:charge breeding
Cooler trap:beam preparation
Precision trap:measurements
The Setup
LASPEC (GSI-FAIR Low-Energy Branch)W. Noertershaeuser (P. Campbell)
Gas-Catcher+ LIS
nuclides with known massesG.Audi et al., Nucl. Phys. A729 (2003) 3
stable nuclei
measured with FRS-ESR
observed nuclei
r-process
2028
50
82
8
8
20
28
50
82
126
nuclides with known masses
stable nuclei
to be measured with the FRS-ESRobserved nuclei
r-process
2028
50
82
8
8
20
28
50
82
126
nuclides with known masses
stable nuclei
to be measured with FAIR facilityobserved nuclei
r-process
2028
50
82
8
8
20
28
50
82
126
stellar nucleosynthesis
ConclusionsNo one experiment to unlock the secret of the nucleus
‘‘key’’ experiments key experimental programs‘‘pilot’’ experiments (systematic studies)
Ground-state properties (masses, radii, moments):fundamental axis of nuclear structureneeded due to absence of reliable model predictionsexamples of ISOL measurements par excellence
EURISOL ‘competitors’: FAIR/MAFF/RIA/SPIRAL2
78Ni; 100Sn; 110Zr; 60Ca; 48Ni; 42Si; 40Mg; 30Netrans-uraniums (à la SHIPTRAP)