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NUMEN Determining the Nuclear Matrix Elements of Neutrinoless Double Beta Decays by Heavy-Ion Double Charge Exchange Reactions   Proponenti: F. CAPPUZZELLO1,2,

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Presentation on theme: "NUMEN Determining the Nuclear Matrix Elements of Neutrinoless Double Beta Decays by Heavy-Ion Double Charge Exchange Reactions   Proponenti: F. CAPPUZZELLO1,2,"— Presentation transcript:

1 NUMEN Determining the Nuclear Matrix Elements of Neutrinoless Double Beta Decays by Heavy-Ion Double Charge Exchange Reactions Proponenti: F. CAPPUZZELLO1,2, C. AGODI1, D.L. BONANNO3, D.G. BONGIOVANNI3, V. BRANCHINA1,3, L. CALABRETTA1, A. CALANNA1, D. CARBONE1, M. CAVALLARO1, M. COLONNA1, A. CUNSOLO1, G. CUTTONE1, A. FOTI1,3, P. FINOCCHIARO1, V. GRECO1,2, G. LANZALONE1,4, F. LONGHITANO3, D. LO PRESTI2,3, A. MUOIO1,5, L. PANDOLA1, D. RIFUGGIATO1, S. TUDISCO1 1 INFN – LABORATORI NAZIONALI DEL SUD, CATANIA, ITALY 2 DIPARTIMENTO DI FISICA E ASTRONOMIA, UNIV. DI CATANIA, CATANIA, ITALY 3 INFN – SEZIONE DI CATANIA, CATANIA, ITALY 4 UNIV. DEGLI STUDI DI ENNA "KORE", ENNA, ITALY 5 UNIV. DEGLI STUDI DI MESSINA, MESSINA, ITALY Collaborazioni attivate INFN LNF INSTITUTO DE FISICA DA UNIVERSIDADE DE SAO PAULO, BRAZIL INST. DE FISICA DA UNIV. FEDERAL FLUMINENSE, NITEROI, BRAZIL CICANUM, UNIVERSIDAD DE COSTA RICA, SAN JOSE, COSTA RICA DEP. OF PHYSICS AND HINP, THE UNIV. OF IOANNINA, IOANNINA, GREECE INSTITUT FÜR THEORETISCHE PHYSIK, GIESSEN UNIVERSITY, GERMANY DÉPARTEMENT DE PHYSIQUE, UNIVERSITÉ HASSAN II – CASABLANCA, MOROCCO CERN BROKHAVEN NATIONAL LABORATORY INSTITUTE OF MODERN PHYSICS, CHINESE ACADEMY OF SCIENCES, LANZHOU, CHINA RCNP, OSAKA UNIVERSITY, OSAKA, JAPAN Spokespersons: F. Cappuzzello and C. Agodi LNS CSNIII, 31 Marzo 2015

2 Great new physics inside
Double β-decay Within standard model Beyond standard model Great new physics inside but one should know Nuclear Matrix Element

3 Search for 0 decay. A worldwide race
Experiment Isotope Lab Status GERDA 76Ge LNGS Phase I completed Migration to Phase II CUORE0 /CUORE 130Te Data taking / Construction Majorana Demonstrator SURF Construction SNO+ SNOLAB R&D / Construction SuperNEMO demonstrator 82Se (or others) LSM Candles 48Ca Kamioka COBRA 116Cd R&D Lucifer 82Se DCBA many [Japan] AMoRe 100Mo [Korea] MOON

4 but requires Nuclear Matrix Element (NME)!
New physics for the next decades but requires Nuclear Matrix Element (NME)! Calculations (still sizeable uncertainties): QRPA, Large scale shell model, IBM ….. Measurements (still not conclusive for 0): (+, -) single charge exchange (3He,t), (d,2He) electron capture transfer reactions … A new experimental tool: heavy-ion Double Charge-Exchange (DCE) E. Caurier, et al., PRL 100 (2008) N. L. Vaquero, et al., PRL 111 (2013) J. Barea, PRC 87 (2013) T. R. Rodriguez, PLB 719 (2013) 174 F.Simkovic, PRC 77 (2008) N. Auerbach, Ann. Of Phys. 192 (1989) 77 S.J. Freeman and J.P. Schiffer JPG 39 (2012) D.Frekers, Prog. Part. Nucl. Phys. 64 (2010) 281 J.P. Schiffer, et al., PRL 100 (2008)

5 More about NME For L = 0 decays Gamow-Teller like Fermi like
Warning: Normally the coupling constants gA and gV are kept out form the matrix element and we talk of reduced matrix elements

6 State of the art NME calculations
Courtesy of Prof. F.Iachello

7 A new esperimental tool: DCE

8 Double charge exchange reactions
(+,-), (20Ne,20O), ββ decay (20Ne,20F) (20Ne,18O) (20Ne,22Ne) 76Se 78Se 76Ge 74Ge 76As 77Se 75As 77As 75Ge (18O,18Ne) (18O,18F) (18O,20Ne) (18O,16O)

9 Double charge exchange reactions Abandoned for  physics
Pion DCE (π+, π-) or (π-, π+) Zero spin Very different mechanism for Gamow-Teller (GT) K.K. Seth et al., Phys.Rev.Lett. 41 (1978) 1589 Direct mechanism: isospin-flip processes Heavy Ion DCE Very low cross sections Sequential mechanism: two-proton plus two-neutron transfer or vice-versa D.R.Bes, O. Dragun, E.E. Maqueda, Nucl. Phys. A 405 (1983) 313.

10 Heavy-ion DCE Sequential nucleon transfer mechanism 4th order:
Brink’s Kinematical matching conditions 1 D.M.Brink, et al., Phys. Lett. B 40 (1972) 37 Meson exchange mechanism 2nd order: 2

11 0 vs HI-DCE Initial and final states: Parent/daughter states of the 0ββ are the same as those of the target/residual nuclei in the DCE; Spin-Isospin mathematical structure of the transition operator: Fermi, Gamow-Teller and rank-2 tensor together with higher L components are present in both cases; Large momentum transfer: A linear momentum transfer as high as 100 MeV/c or so is characteristic of both processes; Non-locality: both processes are characterized by two vertices localized in two valence nucleons. In the ground to ground state transitions in particular a pair of protons/neutrons is converted in a pair of neutrons/protons so the non-locality is affected by basic pairing correlation length; In-medium processes: both processes happen in the same nuclear medium, thus quenching phenomena are expected to be similar; Relevant off-shell propagation in the intermediate channel: both processes proceed via the same intermediate nuclei off-energy-shell even up to 100 MeV.

12 About the reaction mechanism

13 Connection between -decay and Single Charge Exchange
Y. Fujita Prog. Part. Nuc. Phys. 66 (2011) F. Osterfeld Rev. Mod. Phys. 64 (1992) 491 H. Ejiri Phys. Rep. 338 (2000) T.N. Taddeucci Nucl. Phys. A 469 (1997) 125 (3He,t): In general for B(GT)>0.05 𝐵(𝐺𝑇) [(3He,t);𝑞=0] 𝐵(𝐺𝑇) [β−decay] =1±0.05 Similar results for the (d,2He) g.s. Tz=1/2 Tz=-1/2 (3He,t) b decay 1.01 2.21 2.74 2.98 0.98 2.17 2.65 2.88 5+ 3+ 7+ 2Jπ 2713Al14 2714Si13 Strong interaction Weak interaction

14 For heavier projectiles
(7Li,7Be) 𝐵(𝐺𝑇) [(7Li,7Be);𝑞=0] 𝐵(𝐺𝑇) [β−decay] =1±0.2 S. Nakayama PRC 60 (1999) Confirmed by us on different nuclei: 11Be, 12B, 15C, 19O Microscopic and unified theory of reaction and structure is mandatory for quantitative analyses Best results for transitions among isospin multiplets in the projectiles as (7Ligs(3/2-),7Begs(3/2-)) (18Ogs(0+),18Fgs(1+)) should be better than (7Li,7Be) even if not really explored to now See also F.Cappuzzello et al. Phys.Lett B 516 (2001) 21-26 F.Cappuzzello et al. EuroPhys.Lett 65 (2004) S.E.A.Orrigo, et al. Phys.Lett. B 633 (2006) C.Nociforo et al. Eur.Phys.J. A 27 (2006) M.Cavallaro Nuovo Cimento C 34 (2011) 1

15 Single CEX 116Sn(18O,18F)116In at 25 MeV/u
Single CEX 40Ca(18O,18F)40K at 15 MeV/u 3.5° < θlab < 4.5° Preliminary analysis! x-section (2MeV < Ex < 3MeV) ≈ 0.5 mb/sr x-section (within 1 MeV) ≈ 0.17 mb/sr Extracted upper limit for B(GT) < 0.8 B(GT) from (d,2He) = 0.4 S.Rakers, et al., PRC 71 (2005) Extracted B(GT) = 0.087 B(GT) from (3He,t) = 0.083 Y. Fujita

16 NME 2 - decay NME 0 - decay q-transfer like ordinary β-decay
(q ~ 0.01 fm-1 ~ 2 MeV/c) only allowed decays possible (L=0) neutrino enters as virtual particle, q~0.5fm-1 (~ 100 MeV/c) degree of forbiddeness weakened L=0,1,2…… Single state dominance Closure approximation

17 Methodology for NME 2 - decay
Assumption: all the signs are positive in the coherent sum of the amplitudes! (3He,t) (β– type) (d, 2He) (β+ type)

18 Methodology for NME 0 - decay
DCE Suhonen

19 Factorization of the charge exchange cross-section
. . . -decay transition strengths (reduced matrix elements) for single CEX: 𝑑𝜎 𝑑Ω 𝑞,𝜔 = 𝜎 𝛼 𝐸 𝑝 ,𝐴 𝐹 𝛼 𝑞,𝜔 𝐵 𝑇 (𝛼) 𝐵 𝑃 (𝛼) For small q 𝜎 𝐸 𝑝 ,𝐴 =𝐾( 𝐸 𝑝 ,0) 𝐽 𝑆𝑇 2 𝑁 𝑆𝑇 𝐷 unit cross-section 𝐹 𝑞,𝜔 = 𝐾( 𝐸 𝑝 ,𝜔) 𝐾( 𝐸 𝑝 ,0) 𝑒 − 1 3 𝑞 2 𝑟 2 𝑒 𝑝 𝜔 − 𝑎 0 generalization to DCE: 𝑑𝜎 𝑑Ω 𝐷𝐶𝐸 𝑞,𝜔 = 𝜎 𝛼 𝐷𝐶𝐸 𝐸 𝑝 ,𝐴 𝐹 𝛼 𝐷𝐶𝐸 𝑞,𝜔 𝐵 𝑇 𝐷𝐶𝐸 𝛼 𝐵 𝑃 𝐷𝐶𝐸 𝛼 For small q 𝜎 𝛼 𝐷𝐶𝐸 𝐸 𝑝 ,𝐴 =𝐾( 𝐸 𝑝 ,0) 𝐽 ′ 𝑆𝑇 2 𝑁 𝑆𝑇 𝐷 𝐹 𝛼 𝐷𝐶𝐸 𝑞,𝜔 = 𝐾( 𝐸 𝑝 ,𝜔) 𝐾( 𝐸 𝑝 ,0) 𝑒 − 𝑞 𝑟 𝑒 − ( 𝑞 − 𝑞 1 ) 2 𝑟 𝑒 𝑝 𝜔 − 𝑎 0

20 The unit cross section Single charge-exchange Double charge-exchange
𝜎 𝐸 𝑝 ,𝐴 =𝐾( 𝐸 𝑝 ,0) 𝐽 𝑆𝑇 2 𝑁 𝑆𝑇 𝐷 𝜎 𝛼 𝐷𝐶𝐸 𝐸 𝑝 ,𝐴 =𝐾( 𝐸 𝑝 ,0) 𝐽 ′ 𝑆𝑇 2 𝑁 𝑆𝑇 𝐷 J’ST Volume integral of the VSTGVST potential, where 𝐺= 𝑛 |𝑛 𝑛| 𝐸 𝑛 −( 𝐸 𝑖+ 𝐸 𝑓 )/2 is the intermediate channel propagator (including off-shell) JST Volume integral of the VST potential 𝜎 𝛼 𝐷𝐶𝐸 𝐸 𝑝 ,𝐴 is the Holy Graal If known it would allow to determine the NME from DCE cross section measurement, whatever is the strenght fragmentation

21 The volume integrals Volume integrals are larger at smaller energies
They enter to the fourth power in the unit cross section! GT-F competion at low energy

22 INFN-LNS

23 The Superconducting Cyclotron (CS) at LNS

24 MAGNEX Achieved resolution Energy E/E  1/1000 Angle Δθ  0.2°
F. Cappuzzello et al., MAGNEX: an innovative large acceptance spectrometer for nuclear reaction studies, in Magnets: Types, Uses and Safety (Nova Publisher Inc., NY, 2011) pp. 1–63. F.Cappuzzello et al., Nature Comm (2015) Achieved resolution Energy E/E  1/1000 Angle Δθ  0.2° Mass Δm/m  1/160 Optical characteristics Measured values Maximum magnetic rigidity 1.8 T m Solid angle 50 msr Momentum acceptance -14.3%, +10.3% Momentum dispersion for k= (cm/%) 3.68 Quadrupole Dipole Focal Plane Detector Scattering Chamber

25 (18O,18Ne) DCE reactions at LNS
270 MeV 0° < θlab < 10° Q = -5.9 MeV 18O and 18Ne belong to the same multiplet in S and T Very low polarizability of core 16O Sequential transfer processes very mismatched Qopt  50 MeV Target T = only T = 2 states of the residual

26 Experimental Set-up 18O7+ beam from Cyclotron at 270 MeV (10 pnA, 3300 C in 10 days) 40Ca solid target 300 μg/cm2 Ejectiles detected by the MAGNEX spectrometer Unique angular setting: -2° < lab< 10° corresponding to a momentum transfer range from 0.17 fm-1 to about 2.2 fm-1 Measured 18O + 40Ca 18F + 40K 18Ne + 40Ar 20Ne + 38Ar 16O + 42Ca Not measured

27 Particle Identification
Z identification A identification 22Ne 21Ne 20Ne Na 19Ne 18Ne Ne F Xfoc(m) Eresid (ch) A. Cunsolo, et al., NIMA484 (2002) 56 A. Cunsolo, et al., NIMA481 (2002) 48 F. Cappuzzello et al., NIMA621 (2010) 419 F. Cappuzzello, et al. NIMA638 (2011) 74 Eresid (ch)

28 The role of the transfer reactions
270 MeV Suppression of the 40Ca(18O,16O)42C channel 0°< θlab<10° Very weak 40Ca 42Ca counts 38Ar 40Ar d/d(L=0; =0)  10 b/sr Lmax = 8 Lmax = 6 g.s.* L = 2 Suppression of L = 0 in the pair transfer Lmax = 4 g.s. L = 0 Suppression of L > 0 in the double pair transfer E* (MeV)

29 Single charge exchange
Many overlapping states 2- is the strongest low lying transition 0+, 1+, 4- also present 1+ and 0+ cross section compatible with known values of B(GT) and B(F) 40Ca 40K 40Ar

30 270 MeV 40Ca 42Ca 38Ar 40Ar The 40Ar 0+ ground state is well separated from the first excited state 2+ at 1.46 MeV FWHM ~ 0.5 MeV

31 preliminary 40Cag.s.(0+)(18O,18Ne)40Arg.s. (0+) @ 270 MeV
𝑑𝜎 𝑑Ω 𝐷𝐶𝐸 𝑞,𝜔 = 𝜎 𝛼 𝐷𝐶𝐸 𝐸 𝑝 ,𝐴 𝐹 𝛼 𝐷𝐶𝐸 𝑞,𝜔 𝐵 𝑇 𝐷𝐶𝐸 𝛼 𝐵 𝑃 𝐷𝐶𝐸 𝛼 𝑑𝜎 𝑑Ω 𝐷𝐶𝐸 𝑞,𝜔 = 𝜎 𝛼 𝐷𝐶𝐸 𝐸 𝑝 ,𝐴 𝐹 𝛼 𝐷𝐶𝐸 𝑞,𝜔 𝐵 𝑇 𝐷𝐶𝐸 𝐺𝑇 𝐵 𝑃 𝐷𝐶𝐸 𝐺𝑇  0.20 to be compared with 0.11 preliminary

32 Preliminary matrix elements
Pure GT Pure F A measurement at another energy is important to consolidate this NME Pauli blocking about 0.14 Pauli blocking corrected result 1.9 to speculate on 48Ca

33 The NUMEN goals

34 The unit cross section (an ambitious task)
Studying if the 𝜎 𝛼 𝐷𝐶𝐸 𝐸 𝑝 ,𝐴 is a smooth (and thus controllable) function of Ep and A is the most ambitious goal of our project This requires that a systematic set of appropriate data is built, facing the relative experimental challenges connected with the low cross sections and resolution requests Goal N.1 for NUMEN

35 Measured DCE cross section and theory
The degree of complexity of DCE cross sections and 0 is comparable The measured DCE cross sections provide a powerful tool for theory in order to give very stringent constraints in the NME estimation The DCE processes can be artificially generated in the lab! (Few labs. as the LNS) A new generation of DCE constrained 0 NME theoretical calculations can emerge Promoting this kind of evolution is a main purpose of our project Goal N.2 for NUMEN

36 DCE cross sections and sensitivity of 0 experiments
Providing relative NME information on hot cases of 0 is strongly required by the community in order to compare the sensitivity of different half-life experiments This could impact in future development of the field Goal N.3 for NUMEN

37 Conclusions and Outlooks
Exciting new fundamental physics is emerging beyond the standard model Basic role of nuclear physics in the game Many facilities for 0 half life, but not for the NME Pioneering experiments at RCNP (Osaka) and LNS (Catania) are showing that the (18O,18Ne) cross section can be suitably measured First results for the (18O,18Ne) are encouraging, showing that quantitative information on 0 NME are at our reach

38 LNS can realistically compete
The role of LNS What we put on the table We have MAGNEX, perhaps the most suitable instrument for these studies We have a long tradition in heavy-ion physics, experimental and theoretical We have a solid experience in accelerator physics What we need to upgrade We need to carefully explore other targets and reactions as (20Ne,20O) or (12C,12Be) We need to have a factor more beam current from the accelerator LNS can realistically compete

39 40Ca(18O,18Ne)40Ar Projectile Target B(GT) = 3.27 B(GT) = 1.09 18O 18F
Super-allowed transition GT strength not fragmented Y. Fujita, private communication 40Ar 40Ca 40K 4- 1+ 2.73 g.s. 0+ B(GT)=0.069(6) B(GT)=0.023 B(GT)total < 0.15 Target GT strength not much fragmented

40 About 40Ca ground state Pauli blocked
1f5/2 1f7/2 1d3/2 2s1/2 1d5/2 1p1/2 1p3/2 1s1/2 n p n p n p |40Cag.s.>=0.88|[1d3/21d3/2]0+> |[1f7/21f7/2]0+>+0.06 |[1f5/21f5/2]0+> Pauli blocked

41 Double Charge Exchange on 40Ca ground state
1f5/2 1f5/2 1f7/2 1f7/2 1d3/2 1d3/2 2s1/2 2s1/2 1d5/2 1d5/2 1p1/2 1p1/2 1p3/2 1p3/2 1s1/2 1s1/2 n p n p n p 40Cag.s. 40Kg.s. 40Arg.s.

42 40Ca response to charge exchange
BGT=0.069(6) About half of the total GT strenght goes to the 2.73 MeV state of 40K Courtesy of Prof. Y. Fujita

43 Survey of heavy-ion DCE

44 Collaborazioni internazionali
INFN - Laboratori Nazionali del Sud, Catania, Italy; INFN – Sezione di Catania, Catania, Italy; Dipartimento di Fisica e Astronomia, Università di Catania, Catania, Italy; INFN – Laboratori Nazionali di Frascati What next? ……………………… Instituto de Fisica Nuclear, Universidade de Sao Paulo, Brasil Instituto de Fisica, Universidade Federal Fluminense, Niteroi, Rio de Janeiro, Brazil Department of Physics and HINP, The University of Ioannina, Ioannina, Greece Institute of Modern Physics, Chinese Academy of Sciences, 509 Nanchang Road, Lanzhou, China LRSA, Department of Physics, Faculty of Science Ben M'Sik, University Hassan II Mohammedia-Casablanca, Morocco What next? ………………………….

45 Past experimental attempts
124 MeV 51 MeV 10° < θlab < 30° Q = -4.8 MeV θlab = 8° Q = MeV J. Cerny, et al., Proc. 3° Int. Conf. on Nuclei Far from Stability, Cargese, 1976 D.M.Drake, et al., Phys. Rev. Lett. 45 (1980) 1765 C.H.Dasso, et al., Phys. Rev. C 34 (1986) 743

46 Past experimental attempts
24Mg(18O,18Ne)24Ne at 1.37GeV J.Blomgren, et al., Phys. Lett. B 362 (1995) 34

47 Double charge exchange reactions at RCNP (Japan)
80 AMeV Grand Raiden spectrometer Beam energy 80AMev Beam intensity 25 pnA Limitation: Energy resolution 1.2 MeV Interest for 48Ca (CANDLES) T. Uesaka et al., Prog. of Theor. Phys. 196 (2012) 150 H.Matsubara et al. Few Body Syst DOI /s

48 Preliminary FPD cost estimation
Gas tracker Detector cost estimate: GEM foils (~ 5 kCHF), Readout PCB (~ 15 kCHF), Mechanics (~ 30 – 40 k€ -??) Gas system (MKS like): ~ 20 k€ HV system (CAEN): ~ 10 k€ Readout system, possible solution (tbc) with APV25 + SRS (from RD51): ~ 150 k€ Global cost (order of magnitude): ~ 250 k€ Silicon detector wall Silicon detectors (for 108 ions/cm2): ~ 130 k€ Silicon mechanics: ~ 35 k€ Silicon electronics: ~ 60 k€ Power supply: ~ 80 k€ Global cost (order of magnitude): ~ 300 k€

49 - - + Induction Pads GASSIPLEX Proportional Wires (750 V)
SINGOLA PAD Induction Pads Proportional Wires Frisch Grid Silicon detectors STRIP - + Induction Pads GASSIPLEX PC cathode Proportional Wires (750 V) DC1 DC2 DC3 DC4 Frisch grid (0 V) - Drift electrons

50 The reconstruction problem
The image at the focus is meaningful if it can give us information about the object in its position! To see means to reconstruct Inversion of the transport matrix Geometrical Parameters measured at the FPD Physical Parameters at the target The optical aberrations make this reconstruction difficult F. Cappuzzello, et al., NIM A 638, (2011) 74

51 MAGNEX: a ray-reconstruction spectrometer
Possible definition: spectrometer reconstructing a net image by an optically aberrated one Practically One needs High order inversion algorithms (10th order for MAGNEX) Specialized Focal Plane Detectors (FPD) to measure positions and angles at the focus Detailed knowledge of the magnetic field maps inversion Long learning step

52 The 40Ca(18O,18Ne)40Ar case: To be compared to:
Assuming pure GT The 40Ca(18O,18Ne)40Ar case: 𝑑𝜎 𝑑Ω 𝐷𝐶𝐸 𝑞,𝜔 = 𝜎 𝛼 𝐷𝐶𝐸 𝐸 𝑝 ,𝐴 𝐹 𝛼 𝐷𝐶𝐸 𝑞,𝜔 𝐵 𝑇 𝐷𝐶𝐸 𝛼 𝐵 𝑃 𝐷𝐶𝐸 𝛼 87 μb/sr 0.72 0.17 To be compared to: B2[GT;18Ogs(0+) 18Fgs(1+)] * B2[GT;40Cags(0+) 40K0-6MeV(1+)] = = 3.56 Y. Fujita private communication 0.098 D.J.Mercer et al. Phys. Rev. C 49 (1994) 3104

53 The 40Ca(18O,18Ne)40Ar case: To be compared to:
Assuming pure F The 40Ca(18O,18Ne)40Ar case: 𝑑𝜎 𝑑Ω 𝐷𝐶𝐸 𝑞,𝜔 = 𝜎 𝛼 𝐷𝐶𝐸 𝐸 𝑝 ,𝐴 𝐹 𝛼 𝐷𝐶𝐸 𝑞,𝜔 𝐵 𝑇 𝐷𝐶𝐸 𝛼 𝐵 𝑃 𝐷𝐶𝐸 𝛼 39 μb/sr 0.77 0.36 To be compared to: B2[F;18Ogs(0+) 18Fgs(1+)] * B2[F;40Cags(0+) 40K0-6MeV(1+)] = 0.138 = 4.00 0.55 Y. Fujita private communication D.J.Mercer et al. Phys. Rev. C 49 (1994) 3104

54 A quick historical background
1986: first discovery of 2 decay predicted by Maria Goeppert Mayer in 1935 (today found in 12 nuclei) 1998: discovery of neutrino oscillations and the non-zero mass of neutrinos, predicted by Pontecorvo in 1957 2013: discovery of Higgs boson and start of the era of research beyond the standard model The Higgs mechanism cannot explain the mass of neutrinos

55 Double β-decay 𝑍 𝐴 𝑋 𝑁 → 𝑍−2 𝐴 𝑌 𝑁+2 + 2𝑒 − + 2 𝜈 Process mediated by the weak interaction occurring in even-even nuclei where the single -decay is energetically forbidden The role of the pairing force

56 ββ-decay 2 double β-decay
Does not distinguish between Dirac and Majorana Experimentally observed in several nuclei since 1987  and anti- can be distinguished  and anti- are the same 2) 0 double β-decay Neutrino has mass Neutrino is Majorana particle Violates the leptonic number conservation Experimentally not observed Beyond the standard model

57 Normal vs inverted hierarchy
Neutrino oscillation experiments sensitive to m

58 Matter vs Antimatter Leptonic number = 0 at Big Bang All the physics we know does conserve the leptonic number Why the matter dominates over antimatter? Majorana neutrinos can explain that since they do not conserve leptonic number!

59 From Jouni Suhonen, JYFL (Finland)

60 From Jouni Suhonen, JYFL (Finland)

61 Beyond the standard model
Seesaw mechanism Dirac mass will be the same order as the others. (0.1~10 GeV) Right handed Majorana mass will be at GUT scale 1015 GeV

62 Moving towards hot-cases
Caveat The (18O,18Ne) reaction is particularly advantageous, but it is of β+β+ kind; None of the reactions of β-β- kind looks like as favourable as the (18O,18Ne). (18Ne,18O) requires a radioactive beam (20Ne,20O) or (12C,12Be) have smaller B(GT) In some cases gas target will be necessary, e.g. 136Xe or 130Xe In some cases the energy resolution is not enough to separate the g.s. from the excited states in the final nucleus  Coincident detection of -rays A strong fragmentation of the double GT strength is known in the nuclei of interest compared to the 40Ca.

63 Major upgrade of LNS facilities
The CS accelerator current upgrade (from 100 W to 5-10 kW); The MAGNEX focal plane detector will be upgraded from 1 khz to 100 khz The MAGNEX maximum magnetic rigidity will be increased An array of detectors for -rays measurement in coincidence with MAGNEX will be built The beam transport line transmission efficiency will be upgraded from about 70% to nearly 100% The target technology for intense heavy-ion beams will be developed

64 MAGNEX Focal Plane Detector
Entrance window Ion trajectory Silicon detectors Cathode (-950V) Frisch grid (0V) Induction pads DC wires (750V) φfoc - + 57 Silicon Detectors → Eres 5 Proportional Wires → ΔE 4 Induction Strip → X1,X2,X3,X4 → Xfoc,θfoc 4 Drift Chamber (DC) → Y1,Y2,Y3,Y4 → Yfoc,φfoc Ion identification Ray-reconstruction C.Boiano et al., IEEE 55 (2008) 3563 M.Cavallaro et al. EPJ A 48: 59 (2012) D.Carbone et al. EPJ A 48: 60 (2012) Section view

65 It works fine but it is limited to 1 kHz
We need to go to 100 kHz A major upgrading is required but preserving the good tracking and particle identification

66 The proposed idea (gas tracker)
From To GEM (THGEM, WALL, Micromega) gas tracker Multiwire gas tracker Ion trajectories Long occupancy (0.5 ms) Very high rate capability (few MHz/mm2)

67 Gas tracker with GEM readout
Preliminary study Courtesy of G. Bencivenni INFN-LNF Gas tracker with GEM readout operated at low pressure (10 mbar*) and low gain (G~100) drift length ~ 200 mm; TPC thickness ~ 50 mm; TPC length ~ 1000 mm Gas mixture (tbd): Ar/CO2  Vdrift ~ 50 µm/ns GEM foils 50x1000 mm2 (n. 3 amplification stages) Readout PCB (resistive - tbd) segmented in 40 rows of pads (1x1 mm2, tbd)  40 kchs XY space resolution (with analog readout – charge centroid - tbd)  σXY ~ 200 – 300 µm Z space resolution (by drift time measurement : σT ~ ns)  σZ = Vdriftx σT ~ 500µm Possible issues (to be studied carefully): gas mixture, resistive PCB segmentation, ion feedback, electronics sensitivity * See for example arXiv: (Property of LCP-GEM in Pure Dimethyl Ether at Low Pressure): in 20 Torr DME, G~50-300

68 The proposed idea (PID wall)
From To Wall of 60 stopping 7 X 5 cm2 silicon pad detectors Wall of ~ X 1 cm2 telescopes of SiC – CsI detectors PID function decoupled from gas tracker Double-hit probability at 100 kHz < 1% Acceptable uncertainties in the absolute cross section measurement Much smaller maintenance cost First irradiation tests successfully performed in collaboration with CNR Double-hit probability at 100 kHz > 30% Large uncertainties in the absolute cross section measurement High-cost for breaking with localized exposure

69 The proposed idea - -ray calorimeter
MAGNEX to measure high resolution energy spectra for well identified reaction products An array of scintillators (NaI, CsI, LaBr3…) to improve the energy resolution in the energy spectra, with good efficiency

70 The Phases of NUMEN project
LNS Phase1: The experimental feasibility Phase2: “hot” cases optimizing the experimental conditions and getting first results Phase3: The facility Upgrade (Cyclotron, MAGNEX, beam line, …..): Phase4 : The systematic experimental campaign Preliminary time table year 2013 2014 2015 2016 2017 2018 2019 2020 Phase1 Phase2 Phase3 Phase4

71 An intense experimental activity in phase 2

72 An intense R&D activity in phase 2

73 Attività NUMEN prevista 2015
Esperimento al CS (LNS) MAGNEX, richiesta tempo macchina per le prime reazioni: primo fascio febbraio 116Sn (18O,18Ne) 116Cd 116Cd (20Ne,20O) 116Sn Sviluppo prototipi del tracciatore a gas su tecnologie GEM, THGEM, WELL, Micromega Sviluppo prototipi del telescopio di identificazione su tecnologia SiC+CsI Test di scintillatori Sviluppo prototipi schede di elettronica di front-end e digitalizzazione Technical Design Report per nuovi rivelatori Sviluppo modelli teorici

74 A fundamental property
The complicated many-body heavy-ion scattering problem is largely simplified for direct quasi-elastic reactions V (r ,) = U (r) + W(r ,) Optical potential Residual interaction For charge exchange reactions the W(r ,) is ‘small’ and can be treated perturbatively In addition the reactions are strongly localized at the surface of the colliding systems and consequently large overlap of nuclear densities are avoided Accurate description in fully quantum approach, eg. Distorted Wave techniques Microscopic derived double folding potentials are good choices for U (r) Microscopic form factors work for charge exchange reactions


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