Status on 25 Mg(n,  ) and neutron flux in 2012 Bologna, 27 November 2013 C. Massimi.

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Presentation transcript:

Status on 25 Mg(n,  ) and neutron flux in 2012 Bologna, 27 November 2013 C. Massimi

Outline 2012 Flux –Detectors & data –Flux and its uncertainty Mg(n,  ) –RSA, examples –MACS, preliminary Conclusions

2012 Flux – Available data ExperimentRUNS Total protons Usable protons DST available ? 238 U(n,  ) × ×10 18 ✔ 92,93 Zr(n,  ) × ×10 18 ✔ 87 Sr(n,  ) × ✗ 235 U Fiss.Tag × ×10 18 ✔ 59 Ni(n,  ) × ×10 18 ✔ TOTAL1.34× ×10 18 Capture collimator (1.8 cm) Experiment Total protons Used protons Fission angular distribution 2.0× ×10 18 Fission collimator (8 cm) Fission collimator (8 cm)

2012 Flux – Available data ExperimentSiMon MicroMegas 10 B MicroMegas 235 U PTB 238 U(n,  ) ✔✗✗✗ 92,93 Zr(n,  ) ✔✗ 87 Sr(n,  ) ✔✗✗ 235 U Fiss.Tag. ✔✗✔✗ 59 Ni(n,  ) ✔✗✗✗ Capture collimator (1.8 cm) Fission collimator (8 cm) Fission collimator (8 cm) ExperimentPPAC 235 U Fission angular distribution ✔

2012 Flux – SiMon data DST version 11, an improved routine exists but not used yet Amplitude Spectrum Silicon 1 TOF > 10 4 ns  No  -flash TOF > 10 4 ns  No  -flash n+ 6 Li  α + 3 H

2012 Flux – SiMon data DST version 11, an improved routine exists but not used yet Amplitude Spectrum Silicon 2 TOF > 10 4 ns  No  -flash TOF > 10 4 ns  No  -flash n+ 6 Li  α + 3 H

2012 Flux – SiMon data DST version 11, an improved routine exists but not used yet Amplitude Spectrum Silicon 3 TOF > 10 4 ns  No  -flash TOF > 10 4 ns  No  -flash n+ 6 Li  α + 3 H

2012 Flux – SiMon data DST version 11, an improved routine exists but not used yet Amplitude Spectrum Silicon 4 TOF > 10 4 ns  No  -flash TOF > 10 4 ns  No  -flash n+ 6 Li  α + 3 H

2012 Flux – SiMon data TOF spectrum, gate on 3 H peak Silicon keV 87 kev 35 kev ~ 0.5 eV

2012 Flux – SiMon data TOF spectrum, gate on 3 H peak Silicon eV

2012 Flux – SiMon data TOF spectrum, gate on 3 H peak Silicon 3 ~ 0.5 eV

2012 Flux – SiMon data TOF spectrum, gate on 3 H peak Silicon 4 ~ 0.5 eV

2012 Flux – SiMon data Rejection of radiofrequency(?)  signals in coincidence --- No conditions signal --- No coincidences (30 ns)

2012 Flux – SiMon data Rejection of radiofrequency(?)  Energy deposition Solution Electronic noise not present in parasitic bunches Solution Electronic noise not present in parasitic bunches

2012 Flux – SiMon data Beam stability  Ratio of beam monitors

2012 Flux – SiMon data Beam stability  Ratio of beam monitors “protons” / “pkup” R.M.S. ~ 4,3 % R.M.S. ~ 5,4 % --- Dedicated beam --- Parasitic beam

2012 Flux – SiMon data Detector stability  Ratios of Sili counts Vs … Ratio Average Before rej. R.M.S. Before rej. SILI 1 / PROT1.82× % SILI 2 / PROT1.43× % SILI 3 / PROT1.32× % SILI 4 / PROT1.68× % Average After rej. R.M.S. After rej. 1.85× % 1.47× % 1.33× % 1.69× % Conditions: 1.Amplitude  3 H peak 2.TOF  thermal region Conditions: 1.Amplitude  3 H peak 2.TOF  thermal region

2012 Flux – SiMon data Detector stability  Ratios of Sili counts Vs … Ratio Average Before rej. R.M.S. Before rej. SILI 1 / SILI % SILI 1 / SILI % SILI 1 / SILI % SILI 2 / SILI % SILI 2 / SILI % SILI 3 / SILI % Average After rej. R.M.S. After rej % % % % % % Conditions: 1.Amplitude  3 H peak 2.TOF  thermal region Conditions: 1.Amplitude  3 H peak 2.TOF  thermal region

2012 Flux – SiMon data SiMon Counts normalized to protons

2012 Flux – SiMon data SiMon Counts normalized to pkup

2012 Flux – SiMon data SiMon Counts normalized to protons

2012 Flux – SiMon data Uncertainty due to counting statistic 87 kev 35 kev 6 kev E n < 0.5 eV

2012 Flux – SiMon data L FLUX = m L CAPT = m L FLUX = m L CAPT = m From flux to capture

2012 Flux – SiMon data Comparison with previous years Difference at thermal > 10% Average difference 10%

2012 Flux – SiMon data Comparison with previous years 12 – 45  s 1 MeV – 90 keV Difference at high energy ? 260 keV

SiMon data not enough E n > few keV SiMon efficiency not well known simulation or experimental ratio (2011 data)? E n > few keV SiMon efficiency not well known simulation or experimental ratio (2011 data)?

SiMon Vs PPAC data 2012 PPAC data from Esther Leal Cidoncha 2012 PPAC data from Esther Leal Cidoncha

SiMon Vs PPAC data Matching region PPAC – SIMON 3 – 25 keV Matching region PPAC – SIMON 3 – 25 keV 3% systematic uncertainty depending on the matching region

SiMon Vs PPAC data

SiMon + PPAC data --- Evaluated This work 2012 SiMon PPAC Flux from 0.03 eV < E n < 1 MeV

SiMon + PPAC data --- Evaluated This work % systematic uncertainty depending on the matching region Same shape

Flux 2011 – Evaluated This work 2012 ATTENTION to normalization ATTENTION to normalization 197 Au 56 Fe Real situation

Flux 2011 – 2012 Real situation

New 25 Mg(n,  ) measurement … why ? Because of the limitations in 2003 measurement … why ? Because of the limitations in 2003 measurement 1.Sample –MgO, powder sample –Transmission experiment on nat Mg sample 2.n_TOF facility Phase-I: –Water as neutron moderator 3.Measurement –Few data collected Physical Review C 85 (2012)

New 25 Mg(n,  ) measurement … why ? Because of the limitations in 2003 measurement … did we improve? … why ? Because of the limitations in 2003 measurement … did we improve? 1.Sample –MgO, powder sample –Transmission experiment on nat Mg sample 2.n_TOF facility Phase-I: –Water as neutron moderator 3.Measurement –Few data collected  Yes a lot –Metal sample –Transmission experiment on enriched 25 Mg sample  Yes –Borated water  NO –Again few data collected

25 Mg(n,  ) first resonance Recall: 2003 capture data normalized to this resonance

25 Mg(n,  ) first resonance Recall: 2003 capture data normalized to this resonance Γ  =1.73±0.03 eV

25 Mg(n,  ) first resonance Recall: 2003 capture data normalized to this resonance Γ  =1.73±0.03 eV Γ  =1.5±0.5 eV

25 Mg(n,  ) first resonance Recall: 2003 capture data normalized to this resonance Γ  =1.73±0.03 eV Γ  =1.5±0.5 eV Γ  =1.28±0.03 eV

25 Mg(n,  ) up to 100 keV Clean up resonances list Clean up resonances list

25 Mg(n,  ) up to 100 keV Check with transmission data from GELINA

25 Mg(n,  ) up to 300 keV … RSA ongoing

25 Mg(n,  ) up to 100 keV Check with transmission data from GELINA

25 Mg(n,  ) - MACS Maxwellian-averaged capture cross section ~ % lower than previously reported Maxwellian-averaged capture cross section ~ % lower than previously reported

25 Mg(n,  ) - MACS Maxwellian-averaged capture cross section ~ % lower than previously reported Maxwellian-averaged capture cross section ~ % lower than previously reported

Conclusions 2012 flux, obtained from the combination of SiMon and PPAC data, available: –uncertainty due to counting statistic < 4% –systematic uncertainty ~ 3% for E n > 30 keV 25 Mg(n,  ) measurement at n_TOF –RSA, check with transmission data –MACS 20% lower than previously reported  important astrophysical implication –Uncertainty reduced

Cristian Massimi Dipartimento di Fisica e Astronomia

Neutron Sensitivity Preliminary study: ε N,BICRON ~ 10 -4

Silicon 2 - stability Ni campaign

Silicon 2 - stability

Flux 2010 – 2011 – 2012

Flux 2011 – 2012

Mg sample OLD sample (powder) PropertyValue Mass MgO3.19 g Diameter22 mm Thickness2.3 mm Areal density1.234x10 -2 at/b New sample (metallic) PropertyValue Mass Mg3.94 g Diameter20 mm Thickness7 mm Areal density3.00x at/b Enrichment 95.75% 24 Mg ~ 3%, 26 Mg ~ 1.2% Enrichment % 24 Mg ~ 1.83 % 26 Mg ~ 0.31 % INFN paid ~ $13 500