Charged particles detectors Arrays (2)
Low Energy Heavy Ions Reactions (~ 5-10 MeV/A)
Ancillary Detectors (EUROBALL)
§ Internal conversion electrons: MiniOrange ICEMOS
§ Heavy fragments detection:
- recoiling ions: RFD
- fission fragments: SAPHIR
- binary reactions products: BRS
Internal conversion electrons
Internal conversion
is an electromagnetic processcompeting
withg -decay:
if g-decay is inhibited the energy
can be given directly to an electron of the atom
b
ex
E
E
E
e-= -
Eex = energy of nuclear state Eb = electron binding energy
decay of isomeric state
of 113In
conversion electrons are the only
monenergetic electrons
in the ~ 100 keV – MeV range Þ very important for calibrationsN.B. Following decay by internal electron conversion the atom is left with a vacancy, filled by electrons from higher shells Þ emission of X-rays
e
t
l l
l =
g+
total decay probability of nuclear state
g-decay internal conversion
Example:
b
-decay of
203Hg
continuous
b- spectrum internal conversion K and L lines (from 279.2 keV)
electron energies:
electron binding energies
5 3 . 2
3
1
E n Z
e
e
µ ´
= l
ga l
internal conversion coefficient
a depends on
- atomic number Z - transition energy Ee; - multipolarity M or E
Ee [MeV]
a
Þ conversion electrons give information on:
§ g-multipolarity
§ E0 transitions
(forbidden for EM transitions)
0+ ® 0+
can only go by conversion electrons detailed calculations
ICEMOS
(Internal Conversion Electron MiniOrange Spectrometer)
conversion electrons are selected
from the high atomic background of d-electrons using a magnetic lens
focusing only electrons of a given energy
source detectorSi(Li) thickness = 6 mm T = 77 K
ring of 6 permanent
magnets
SmCo5 magnets lenght 4.1 cm width 4.3 cm
Radial field B = (85±19)mT
Very compact geometry: position inside EUROBALL scattering chamber
transmission peak e ~ 5%
Important requirement :
high g-ray efficiency (EUROBALL) & similar electron conversion efficiency (ICEMOS) to performe
electron – g coincidences
g spectrum
e- spectrum electron-g coincidences
Example: Study of decay-out of SD band in
135Nd
(Example of transition from NORMAL to SUPERFLUIDquantum mechanical system)
SD band
ND band
B. Aengenvoort et al., Eur. Phys. J. A1 (1998)359 establishment of multipolarity
of linking transitions
SUPER Deformed
(rigid rotor, normal system)
E
*e
NORMAL minimum
SUPER deformed minimum FEEDING
of SD bands
DECAY-OUT of SD bands:
Coupling between ordered and chaotic states
NORMAL Deformed
(reduced moment of inertia, superfluid system)
Recoil Filter Detector
(18 detectors ~ 1p)
e ~ 65%
beam
important in the study of fusion reactions characterize by:
1. Many evaporation residua 2. Large fraction of fission
3. Large amount of particle emission
residues identification & v/c determination via TOF
18 elements in 3 rings:
- 6 + 6 + 12 detectors
- angular range 1.4°-6.7°
- e ~ 65%
individual element:
- thin mylar foil (0.5 -2 mm) - thin fast, plastic scintillator
è N.B. scattered beam does not hit directly the scintillators
- recoiling ions hitting the mylar foil knock out electrons;
- electrons are accelerated by 20 kV and focused on the plastic scintillators
D t ~ 0.1 ns
co un ts
E
g[keV]
mean velocity correction
<b> ~ 2.8%
true velocity correction mylar foil
electrodes
electron trajectories
# electrons
µ
energy released by the ionsummed signal = # electrons x 20 kV ~ 100 x 20 kV = 2 MeV
Þ TOF: residue identification
Þ tracking of reaction products
Þ v/c determination
(better Doppler correction)
20 kV
A = 45
4 keV
157Gd(36Ar,4n)189Pb, Ebeam = 173 MeV
189
Pb angular distribution
189
Pb energy distribution
particle evaporation after target
detected ions Angular & energy distributions
of recoiling ions are strongly modified passing through the target:
much broader distributions
Þ average
v/c correction can be rather poorfor v/c ³ 3 %
K. Sphor et al., Acta. Phys. B26 (1995)297
PHYSICS CASE for RFD
Robustness of Shell Correction at T>0 in SHE Nuclei
Super Heavy Nuclei
most striking manifestation of shell structure in nuclei:
- Z > 100 nuclei are at the limit of Coulomb instability
- large shell correction energy provides additional binding (up to 8 MeV)
Z > 100 Search for
limiting spin and excitation energy SHE nucleus can substain
Z=102:
254No
2n
is the only open/detectable channel253
No +
251No < 1%
48 Ca + 208 Pb à 256 No*
2n 1n 3n
E
beam= 215-219 MeV Q
value~ -150 MeV
s(
254No) ~ 3 µb
2n
254No
• chemistry
o SHIP
H.W. Gaggeler et al., NPA502(1989)561c
Recoil Filter Detector
@ AGATA-Demonstrator
(INFN-Legnaro)
Additional detectors around AGATA:
HELENA Array
Large LaBr
3Array
(also if AD not complete)TOF TOF
Pu ls e H ei gh t (En er gy )
beam CN beam CN
26
Mg (@128 MeV) +
120Sn à
146Sm*
(GASP + RFD, DeAngelis et al., March 2009)
RFD has been succesfully used
to identify the heavy nucleus 220
Th
nuclei220
Th
fission
RFD- measurements with a continuous beam
scattered beam
recoils
Eloss vs Egamma
RFD signal Ampl.
g-projectile g-recoil
Fission Fragments
From spontaneus fission or induces fission (ex. n-rich Nuclei)
Study of g-decay in coincidence with fission fragments:
Þ
EUROBALL + Fission Fragment detector detection of g-g-g coincidencesout of a cascade of 10 g-rays
132Sn
78Ni
r-process
Neutron (N)
Proton (Z)
Saphir
(Saclay-Acquitane-Photovoltaic cell for Isomer Research)
Solar cell Array
important in the study of
spontaneus fission or induced fission (ex. n-rich Nuclei)
Information on:
1. fragment mass 2. released energy
3. momentum for Doppler correction 4. angle of fragments
Alternative to:
-
Si surface barrier
(expensive, severe radiation damage) -
Gas detector (PPAC)
(difficult to handle, care for thin window) 2.
4 cm 4 cm
monocrystalline polycrystalline
preamp Si p-type wafer
Ag Ag
(for charge collection) titanium-oxide
§ low resistivity: r < 3W/cm2
Þ NO need of bias voltage
§ large capacitance: C~20-30 nF/cm2
Þ small signal from preamp: V=Q/C
(difficulty in extrating light particle from noise)
best performances: A>50, E>30 MeV
fragment energy versus pulse height
x E
) ' (
) '
( a a M x b b M
E = + + +
a, a’, b, b’ = calibation coefficients
Pulse-height-defect :
the pulse height observed for heavy ions is substantially less than observed for light ions
at the same energy, as a result of:
- larger dE/dx in entrance window & dead layers - loss of energy by nuclear collisions
producing recoiling ions with low energy
(reduced efficieny for electron-hole pair production) - high rate of electron-hole pair recombination
along ion track (dense plasma)
reponse function of solar cell
252Cf spontaneus fission source
§ DM = 7-8 amu
§ DEcell ~ DESurface Barrier
§ e ~ 100%
§ Dt ~ 20 ns
§ g-ray transmission ~ 100%
§ count rate: up to 5 kHz
Pulse height spectra
Solar cell Surface barrier
H = heavy fragments (low energy) L = low fragments (high energy)
H H
L L
massspectrum
252Cf source M=145
M=86
barrel geometry: e ~ 45%
Other use of solar cells:
Fission cross section measurements (French Nuclear Waste project)
barrel geometry: e ~ 45%
Structure of neutron-rich isotopes produced by 12C+238U nduced fission:
observation of 18 new isomeric states t~ few ns ® few µs
fragments stopped in Saphir:
isomeric decay at rest without Doppler 119In
g-spectra detected in Dt = 50 ns- 1 µs after detection of 2 fragments in Saphir
isomer t = 240 ns
decay time spectrum for 152 keV transition depopulating 25/2+ isomer
t = 240 ns
gate on 1020 keV
x
x
BRS (Binary Spectrometer) Multi-Nucleon Transfer a -cluster nuclei, …
24
Mg
24Mg
12
C
14C
22Mg
Frontiers of Nuclear Physics
EXOTIC NUCLEI
48Ca
66Ni
64Ni
46Ca
Multi-nucleon transfer A~50
48Ca + 64Ni @ 6MeV/A