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Nuclear matrix elements. measured quantity. quantity of interest. 1 / T 1/2 = PS * NME 2 * (m / m e ) 2. The big unknown. Started worldwide effort for a coherent program to reduce NME uncertainty down to 30%, summary report available nucl-ex/0511009. - PowerPoint PPT Presentation
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Nuclear matrix elements
1 / T1/2 = PS * NME2 * (m / me)2
measured quantity quantity of interest
The big unknownStarted worldwide effort for a coherentprogram to reduce NME uncertainty down to 30%, summary report availablenucl-ex/0511009
Needs international coherent efforthttp://www.ippp.dur.ac.uk/0NU2B/2005.html
Nuclear matrix elements1 / T1/2 = PS * ME2 * (m / me)2
0+
1+
(A,Z)
(A,Z+1)
(A,Z+2)0+
charge exchange(p,n), (3He,t)
muon capturebeta- decays
antineutrino-capture
nu N scattering
Theory: Shopping list what to measure to improve calculationsExperiment: Where can it be measured, who?
„Ultimate dream“: coherent effort, strategy paper to get things done
Q - values
charge exchange(n,p), (d,2He)
EC/beta+ decays
Phase space decay rate scales with Q5
2 decay rate scales with Q11
Q-value (keV)
Isotope Nat. abund. (%)
(PS 0v)–1 (yrs eV2)
(PS 2v) –1 (yrs)
Ca 48 4271 0.187 4.10E24 2.52E16Ge 76 2039 7.8 4.09E25 7.66E18Se 82 2995 9.2 9.27E24 2.30E17Zr 96 3350 2.8 4.46E24 5.19E16Mo 100 3034 9.6 5.70E24 1.06E17Pd 110 2013 11.8 1.86E25 2.51E18Cd 116 2802 7.5 5.28E24 1.25E17Sn 124 2288 5.64 9.48E24 5.93E17Te 130 2529 34.5 5.89E24 2.08E17Xe 136 2479 8.9 5.52E24 2.07E17Nd 150 3367 5.6 1.25E24 8.41E15
Matrix elements2 matrix elements determined by intermediate 1+ states
0 matrix elements different
Outcome: Working packages
• Working package 1: Charge exchange reactions
• Working package 2: Q-value measurements
• Working package 3: Muon capture
• Working package 4: Double elecron capture
• Working package 5: Neutrino nucleus scattering
• Working package 6: Nucleon exchange reaction
Urgency: Some facilities might vanish in the near future!!!
WP1: Charge exchangeCurrently: (d,2He) and (3He,t)
Further:ft-values of EC fixing g_ppEM transitions to IASnuclear deformations.r.c.
WP2: Q-valuesOnly 76Ge known very accurate
Atomic traps
Reasons:
- Good energy resolution detectors- Presence of nearby background lines
- Enhancement in EC/EC modes if levels are degenerate
WP3: Ordinary Muon capture
NNR05-Workshop Neutrino nuclear responses in particle and astro nuclear physics• -- Double beta decays and low-energy astro neutrinos-----• Dec. 1-4, CASTHarima, Osaka Japan • Neutrinos involved in and astro nuclear physics are mostly low-
energy(0.01-0.1 GeV) neutrinos, and accordingly the responses are spin isospin responses with low multi-polarities of L= 0~3.
• In fact the spin isospin responses for the lowest multi-pole of L=0• have extensively been studied at RCNP, MSU, KVI, TUDA and
others. High E-resolution systems there are very powerful.
http://www.spring8.or.jp/e/conference/appeal/nnr05/