High energy density nuclear physics at UC Berkeley, LLNL, and...
Transcript of High energy density nuclear physics at UC Berkeley, LLNL, and...
High energy density nuclear physics at UC Berkeley, LLNL, and LBNL
Karl van Bibber & Lee Bernstein
NIF
HFNG
88” A Bay Area collaboration has formed to study Nuclear Plasma Interactions and related phenomena Primary tools are NIF and other Laser HED platforms Supporting measurements and instrument development at the LBNL 88” cyclotron, and the UC Berkeley HFNG We acknowledge funding by the UC Office of the President A major proposal for a UC HED S&T Center involving four campuses & three labs has just been submitted
Team HFNG UC Berkeley Ka-‐Ngo Leung Cory Waltz Leo Kirsch Jay James Karl van Bibber Keeton Ross Joe Labrum BGC Paul Renne Tim Becker
LLNL Lee Bernstein
LBNL Rick Firestone
MSU/UMass Lowell Andy Rogers
The HFNG primarily designed for 39Ar/40Ar daLng technique for geochronology and paleochronology – requires 39K(n,p)39Ar Our design enables both 2.45 MeV and thermal neutrons, either internal to the target or in an external beamline
Background of the High Flux Neutron Generator (HFNG)
HFNG designed by Ka-‐Ngo Leung for the Berkeley Geochronology Center Supported by NSF ARRA funding Expected Neutron Flux (over 4π) ≈ 5 × 1011 neutrons/sec
D-‐D Fusion ReacLon:
Deuteron Deuteron
3He Neutron
D + D → 3He + n
Q = 2.45 MeV
Cooling ConnecLons
Target
RF Ion Source
Matching networks for RF
Turbopump Major components: 120 kV, 200 A Power supply 30 A RF Generators Impedance Matching Networks for RF Turbopump Cooling System Poly Shielding
The Generator
Shielding
Opera=on
RF Ion Source
RF Ion Source
Target
Deuterium Injected
RF ON
RF ON
High Voltage ON
Deuterium imbeds into target
Enough deuterium imbedded in target for collisions to occur
D-‐D Fusion!
First neutrons were produced on July 25, 2014 115In (n,n’) 115mIn ( 4.49 h, 336 keV γ )
• 100 kV anode voltage • 1 mA ion current • (0.2-‐2) × 108 n/sec
The Indium disk used to measure the neutron flux from HFNG was the idenKcal foil which measured the first neutrons from NIF in 2010
Next steps: suppression of back-streaming electrons to enable current to reach goal of ~ 1 A & thus ~ 1011 n/sec Strategy for suppression involves both permanent magnets in the anode, and a ‘shroud’ to capture electrons Movie (right): Plasma without magnets & graphite shield Movie (left): Plasma with magnets & graphite shield We can now run with ~ 4 mA A full shield is being designed with the assistance of Comsol modeling
Our collaboration is pursuing a multi-component program to measure nuclear-plasma interactions in HED plasmas
Mau Chen, Andrea Kritcher, Bob Heeter, Darren Bleuel, Dawn Shaughnessy, Carol Velsko, Bill Cassata, Laura Hopkins, K. Moody, N. Gharibyan, D.H.G. Schneider
LLNL
Bethany Goldblum, Brian Daub, Karl Van Bibber, Jasmina Vujic, Joshua Brown, Nick Brickner, O. Clamens, O. Nunez
University of California - Berkeley
Vincent Meot, Gilbert Gosselin, Pascal Morel, Phillipe Franck, Charles Reverdin CEA-DAM
A. Yasunobu, M. Nakai, H. Azechi
ILE-Osaka
Lawrence Livermore National Laboratory 9 This work was performed under the auspices of the U.S. DOE by Lawrence Livermore National Laboratory
under contract DE-AC52-07NA27344. Lawrence Livermore National Security, LLC
Classes of Nuclear Plasma Interactions (NPI)
10
Nucleus HEDP
Photons
Photo-absorption Time Reverse: γ-ray decay
Photons
N N*
efree ebound
Atomic-nuclear (electron) interactions NEEC, NEET, IES*
Time Reverse: IC-decay
Atom electrons photons
N N*
Lawrence Livermore National Laboratory 10 This work was performed under the auspices of the U.S. DOE by Lawrence Livermore National Laboratory
under contract DE-AC52-07NA27344. Lawrence Livermore National Security, LLC
NPI-induced population of low-lying excited states changes the spin of the compound nucleus leading to alterations in neutron capture rates in stellar plasmas
*Bao & Kappeler At. Dat. Nucl. Dat. Tables 76, 70–154 (2000)
SEF kT( ) = σ HEDP
σGS
=2Ji +1( )σ Ex = Ei( )
i=0
∞
∑ e−Ei /kT
σGS 2Ji +1( )i=0
∞
∑ e−Ei /kT
AZ A+1Z
Sn
NEEC/T
These rates remain entirely unmeasured
0 2 4 6 8 10
Excitation energy E* (MeV)
10!4
10!3
10!2
10!1
100
101
102
103
104
LIfe
time
of s
ingl
e CN
sta
te (p
s)
J/pi= 0.0+ J/pi= 1.0+ J/pi= 2.0+ J/pi= 3.0+ J/pi= 4.0+ J/pi= 5.0+ J/pi= 6.0+ J/pi= 7.0+ J/pi= 8.0+ J/pi= 9.0+ J/pi= 10.0+ J/pi= 11.0+ J/pi= 12.0+ J/pi= 13.0+ J/pi= 14.0+ J/pi= 15.0+ J/pi= 16.0+ J/pi= 17.0+ J/pi= 18.0+ J/pi= 19.0+
Energy (MeV) 0 2 4 6 8 10
Excitation energy E* (MeV)
10!4
10!3
10!2
10!1
100
101
102
103
104
LIfe
time
of s
ingl
e CN
sta
te (p
s)
J/pi= 0.0+ J/pi= 1.0+ J/pi= 2.0+ J/pi= 3.0+ J/pi= 4.0+ J/pi= 5.0+ J/pi= 6.0+ J/pi= 7.0+ J/pi= 8.0+ J/pi= 9.0+ J/pi= 10.0+ J/pi= 11.0+ J/pi= 12.0+ J/pi= 13.0+ J/pi= 14.0+ J/pi= 15.0+ J/pi= 16.0+ J/pi= 17.0+ J/pi= 18.0+ J/pi= 19.0+
Higher spin states are less Likely emit neutrons
Life
time
(ps)
0 2 4 6 8 10
Excitation energy E* (MeV)
10!4
10!3
10!2
10!1
100
101
102
103
104
LIfe
time
of s
ingl
e CN
sta
te (p
s)
J/pi= 0.0+ J/pi= 1.0+ J/pi= 2.0+ J/pi= 3.0+ J/pi= 4.0+ J/pi= 5.0+ J/pi= 6.0+ J/pi= 7.0+ J/pi= 8.0+ J/pi= 9.0+ J/pi= 10.0+ J/pi= 11.0+ J/pi= 12.0+ J/pi= 13.0+ J/pi= 14.0+ J/pi= 15.0+ J/pi= 16.0+ J/pi= 17.0+ J/pi= 18.0+ J/pi= 19.0+
Lawrence Livermore National Laboratory 11 This work was performed under the auspices of the U.S. DOE by Lawrence Livermore National Laboratory
under contract DE-AC52-07NA27344. Lawrence Livermore National Security, LLC
We have attempted to observe NPI-induced population of low-lying nuclear states through the observation of prompt γ-rays in a HEDP formed using a high energy laser
60 beams 30 kJ at 3ω Variable pulse shape P ≥ 60TW
The Omega laser at LLE
Lawrence Livermore National Laboratory 12 This work was performed under the auspices of the U.S. DOE by Lawrence Livermore National Laboratory
under contract DE-AC52-07NA27344. Lawrence Livermore National Security, LLC
The experiments at Omega were designed to directly detect NEEC decay in hohlraum targets
169Tm hohlraum (10 μm thick)"
38 drive beams"
1 ns laser pulses were used to heat the interior of the Tm hohlraum to > 5 keV.
-Tm atoms undergo NEEC to 8.41 keV excited state closely matches L-shell e- energies
-gamma decay is measured 2-4 ns later using Omega x-ray diagnostics 169Tm
3/2+
1/2+ 0
8.4 keV 4.1 ns
Lawrence Livermore National Laboratory 13 This work was performed under the auspices of the U.S. DOE by Lawrence Livermore National Laboratory
under contract DE-AC52-07NA27344. Lawrence Livermore National Security, LLC
8-9 keV γ-rays can be detected with standard crystal x-ray spectrometers at Omega
High collection efficiency Bragg crystal allows γ’s to be seen above x-ray background
F=12.5 cm!
XRFC & FILM!
Source!
θBragg=12o!
Highly Oriented Pyrolytic Graphite (HOPG) crystal
Spectral Range: 6.8-12 keV Reflectivity ~3 mrad Solid angle Ωdet~5×10-5
Lawrence Livermore National Laboratory 14 This work was performed under the auspices of the U.S. DOE by Lawrence Livermore National Laboratory
under contract DE-AC52-07NA27344. Lawrence Livermore National Security, LLC
Our first LLE experiments in 2012 produced confusing results: Did we observe NEEC or atomic metastable states in 169Tm?
M. Chen simulaKons
NEEC rate in blowoff plasma
Detected late time spectrum
Met
asta
ble
st
ate N
EE
C?
?
Au HED plasmas: M.B. Schneider et al, Phys. Plasmas 13, 112701 (2006)
Lawrence Livermore National Laboratory 15 This work was performed under the auspices of the U.S. DOE by Lawrence Livermore National Laboratory
under contract DE-AC52-07NA27344. Lawrence Livermore National Security, LLC
On May 7 we revisited this approach at Omega using 187Os (test case), 192Os (control) and 169Tm half-raums
The control allows us to separate nuclear from atomic physics effects:
Half-raum with washer reduces blow-off plasma location ambiguity.
187Os
3/2-‐
1/2-‐ 0 keV
9.76 keV
192Os
2+
0+ 0 keV
206 keV
NEEC
γ (2.4ns)
Th/Os plum
e
Ti
Control
t = 3 ns
t = 4 ns
t = 5 ns
t = 6 ns
169Tm
The 2012 “phantom” is gone
10-5
0.0001
7000 7500 8000 8500 9000 9500 1 104 1.05 104
Osmium 187 @ 3nsOsmium 192 @ 3ns
Arbitra
ry Un
its
E (eV)
10-6
10-5
0.0001
7000 7500 8000 8500 9000 9500 1 104 1.05 104
Osmium 187 @ 4nsOsmium 192 @ 4ns
Arbitra
ry Un
its
E (eV)
10-6
10-5
0.0001
7000 7500 8000 8500 9000 9500 1 104 1.05 104
Osmium 187 @ 5nsOsmium 192 @ 5ns
Arbitra
ry Un
its
E (eV)
Os
Lawrence Livermore National Laboratory 16 This work was performed under the auspices of the U.S. DOE by Lawrence Livermore National Laboratory
under contract DE-AC52-07NA27344. Lawrence Livermore National Security, LLC
The candidate peak is still there
AZ A-1Z
Sn
g m
Isomer de-excitation can be used to observe NPIs on excited states in HED plasmas as well*
*G. Gosselin & P. Morel Phys. Rev. C 70 064603 (2004)
X keV t1/2 > 20 ps
AZ
X+ΔE keV
i
f
Ideal case
Γf→i ≈ Γf→g
g
e- γ
Ground State
Isomer
Ground State
Isomer
Via discrete states Via the quasi-continuum
Lawrence Livermore National Laboratory 17 This work was performed under the auspices of the U.S. DOE by Lawrence Livermore National Laboratory
under contract DE-AC52-07NA27344. Lawrence Livermore National Security, LLC
The National Ignition Facility (NIF) at LLNL provides an HEDP with 20x longer confinement times than LLE
192 beams 1.8 MJ at 3ω Variable pulse shape (20ns) P ~ 500TW
Up to 1016 neutrons which can be used to make
isomers
Lawrence Livermore National Laboratory 18 This work was performed under the auspices of the U.S. DOE by Lawrence Livermore National Laboratory
under contract DE-AC52-07NA27344. Lawrence Livermore National Security, LLC
Our programs also includes a component focused on NPI-induced reactions taking place on highly-excited states altering the population of isomers
AZ
A+1Z
Sn
Bf
The situation could be even more complicated if fission is an open channel (e.g., the r-process)
NEE*/NRF
Current Assum
pLon
Sn+En
0 2 4 6 8 10
Excitation energy E* (MeV)
10!4
10!3
10!2
10!1
100
101
102
103
104
LIfe
time
of s
ingl
e CN
sta
te (p
s)
J/pi= 0.0+ J/pi= 1.0+ J/pi= 2.0+ J/pi= 3.0+ J/pi= 4.0+ J/pi= 5.0+ J/pi= 6.0+ J/pi= 7.0+ J/pi= 8.0+ J/pi= 9.0+ J/pi= 10.0+ J/pi= 11.0+ J/pi= 12.0+ J/pi= 13.0+ J/pi= 14.0+ J/pi= 15.0+ J/pi= 16.0+ J/pi= 17.0+ J/pi= 18.0+ J/pi= 19.0+
Energy (MeV) 0 2 4 6 8 10
Excitation energy E* (MeV)
10!4
10!3
10!2
10!1
100
101
102
103
104
LIfe
time
of s
ingl
e CN
sta
te (p
s)
J/pi= 0.0+ J/pi= 1.0+ J/pi= 2.0+ J/pi= 3.0+ J/pi= 4.0+ J/pi= 5.0+ J/pi= 6.0+ J/pi= 7.0+ J/pi= 8.0+ J/pi= 9.0+ J/pi= 10.0+ J/pi= 11.0+ J/pi= 12.0+ J/pi= 13.0+ J/pi= 14.0+ J/pi= 15.0+ J/pi= 16.0+ J/pi= 17.0+ J/pi= 18.0+ J/pi= 19.0+
Whether this happens depends on τ(J), σNPI, and Φe,γ
Life
time
(ps)
0 2 4 6 8 10
Excitation energy E* (MeV)
10!4
10!3
10!2
10!1
100
101
102
103
104
LIfe
time
of s
ingl
e CN
sta
te (p
s)
J/pi= 0.0+ J/pi= 1.0+ J/pi= 2.0+ J/pi= 3.0+ J/pi= 4.0+ J/pi= 5.0+ J/pi= 6.0+ J/pi= 7.0+ J/pi= 8.0+ J/pi= 9.0+ J/pi= 10.0+ J/pi= 11.0+ J/pi= 12.0+ J/pi= 13.0+ J/pi= 14.0+ J/pi= 15.0+ J/pi= 16.0+ J/pi= 17.0+ J/pi= 18.0+ J/pi= 19.0+
?
Lawrence Livermore National Laboratory 19 This work was performed under the auspices of the U.S. DOE by Lawrence Livermore National Laboratory
under contract DE-AC52-07NA27344. Lawrence Livermore National Security, LLC
A NIF experiment using this approach is planned using a 134Xe-doped exploding pusher to make 133mXe and 133gXe in and out of a HEDP
We maximize both neutron flux and plasma density by placing a 134Xe dopant nuclei in a direct-drive target
…plus a “control” sample outside the plasma in a sample positioner 50cm from the target
Glass/CH pusher (10 µm)
Fusion neutrons interact with Xe on way out of target
DT gas 0.03% 134Xe
5.243 d 11/2-
3/2+
133Xe 2.19 d
All of the Xe gets hots
50 cm
None of the Xe gets hots
RDIGS ≡
NRAGS133mXe
NRAGS133g Xe
NDIM133mXe
NDIM133g Xe
≠1→ NPI
Lawrence Livermore National Laboratory 20 This work was performed under the auspices of the U.S. DOE by Lawrence Livermore National Laboratory
under contract DE-AC52-07NA27344. Lawrence Livermore National Security, LLC
The radiochemical team at NIF has shown that it can collect radioactive Xenon from exploding pushers with high efficiency
From NIF chamber turbo pumps
> 50% of gaseous material in NIF chamber can be retrieved
Exploding pusher
0.03% Xenon
2 mm
Lawrence Livermore National Laboratory 21 This work was performed under the auspices of the U.S. DOE by Lawrence Livermore National Laboratory
under contract DE-AC52-07NA27344. Lawrence Livermore National Security, LLC
≥100 µm metal foil
197Au beam
≈1 µm 13C target
196,198Au
Excited 198/196Au* residuals made via binary transfer from 13C recoils into a Bismuth foil “plasma target”
In the “close” target NEEC can occur on quasi-continuum states.
In the “far” target, Au has decayed to ground state or isomer, and NEEC will occur on these states.
A “beam-foil” experiment is scheduled for 10/14 at LBNL to try and observe NPIs on highly excited state in 196Au via isomer de-excitation
+
196,198Au***
Lawrence Livermore National Laboratory 22 This work was performed under the auspices of the U.S. DOE by Lawrence Livermore National Laboratory
under contract DE-AC52-07NA27344. Lawrence Livermore National Security, LLC
130 MeV 13C
Gold Target Layers (1 micron)
Aluminum Degrader Foils (25 microns)
Gold Monitor Foil
Aluminum Stopping Foils
Maximum m/g ratio occurs at 8.5 MeV/nucleon.
In preparation for this experiment we performed an excitation function measurement that has produced a publication worthy result in its own right
Lawrence Livermore National Laboratory 23 This work was performed under the auspices of the U.S. DOE by Lawrence Livermore National Laboratory
under contract DE-AC52-07NA27344. Lawrence Livermore National Security, LLC
Step 1 • Make radioacLve gold using the RCNP AVF cyclotron via natPt(p,xn). • Proton Beam: 20 MeV, 1μA (min), 1.5cm diameter
Step 2 • Count acLvity of radioacLve targets • Isotope: 194Au; Peak Energy:328.464keV; Peak Intensity: 60.4%
Step 3 • Collect debris with our models in GEKKO XII Target Chamber • Various models, with different sizes and materials
Step 4 • Perform chemistry to prepare a sample for counLng using HPGe detector
Step 5 • Count again and compare with the results in Step 3 to obtain the collecLon efficiency
We are now planning to develop enhanced debris collection techniques at ILE-Osaka using radioactive Au nuclei produced at the RCNP cyclotron
GEKKO chamber
Debris Collector
RCNP collimator
Many thanks to the team at ILE, including Dr. Arikawa Yasunobu!
Lawrence Livermore National Laboratory 24 This work was performed under the auspices of the U.S. DOE by Lawrence Livermore National Laboratory
under contract DE-AC52-07NA27344. Lawrence Livermore National Security, LLC
Summary
1 A multi-institutional collaboration has been assembled at and around UCB 1 To pursue neutron-induced nuclear science measurements 2 To study the elusive topic of nuclear-plasma interactions
2 We are pursuing a multi-component approach to try and observe the elusive phenomena of NPIs:
1 On nuclear ground states using Laser-driven HEDPs at Omega in 169Tm and 187Os 2 On excited nuclear states via isomer de-excitation in 133Xe at NIF 3 On excited states via isomer de-excitation in 196,198Au using the LBNL 88-Inch cyclotron.
3 We are also working to develop enhanced debris collection at ILE-Osaka 1 This is the 1st step toward using a combination of long- and short-pulse lasers to observe NPIs
Thanks for your attention!
Lawrence Livermore National Laboratory 25 This work was performed under the auspices of the U.S. DOE by Lawrence Livermore National Laboratory
under contract DE-AC52-07NA27344. Lawrence Livermore National Security, LLC