Virtual Neutron Method applied to the study of 17 O(n,  ) 14 C reaction Marisa Gulino LNS - INFN, Catania & Università di Enna “Kore”

Slides:



Advertisements
Similar presentations
Meeting – Prague, June 2011 Jaromir Mrazek, NPI ASCR Rez Nuclear Astrophysics in NPI ASCR Rez, Czech Republic Outline: Hardware Indirect methods Experiments.
Advertisements

Nuclear Astrophysics Experiments in ATOMKI Gy. Gyürky Institute of Nuclear Research (ATOMKI) Debrecen, Hungary.
Alpha Stucture of 12 B Studied by Elastic Scattering of 8 Li Excyt Beam on 4 He Thick Target M.G. Pellegriti Laboratori Nazionali del Sud – INFN Dipartimento.
Reaction dynamics of light nuclei around the Coulomb barrier Alessia Di Pietro INFN-Laboratori Nazionali del Sud ARIS 2014Alessia Di Pietro,INFN-LNS.
(p,g) reaction via transfer reaction of mirror nuclei and direct measurement of 11C(p,g)12N at DRAGON Bing Guo For nuclear astrophysics group China Institute.
The Role of 12 C( 12 C,n) in the Astrophysical S-Process Brian Bucher University of Notre Dame.
Astrophysical Reaction Rate for the Neutron-Generator Reaction 13 C(α,n) in Asymptotic Giant Branch Stars Eric Johnson Department of Physics Florida State.
Astrophysical S(E)-factor of the 15 N(p,α) 12 C reaction at sub-Coulomb energies via the Trojan-horse method Daniel Schmidt, Liberty University Cyclotron.
15 N Zone 8 Zone 1 Zone 28 p Zone 1 Zone O Zone 1 Zone 4 Zone 8 Zone N 16 O p Reaction rates are used to determine relative abundance of elements.
Astrophysical Factor for the CNO Cycle Reaction 15 N(p,  ) 16 O Adele Plunkett, Middlebury College REU 2007, Cyclotron Institute, Texas A&M University.

1 Role of the nuclear shell structure and orientation angles of deformed reactants in complete fusion Joint Institute for Nuclear Research Flerov Laboratory.
Astrophysical S(E)-factor of the 15N(p,α)12C reaction at sub-Coulomb energies via the Trojan-horse method Daniel Schmidt, Liberty University Cyclotron.
25 9. Direct reactions - for example direct capture: Direct transition from initial state |a+A> to final state B +  geometrical.
Measurements of cross-sections of neutron threshold reactions and their usage in high energy neutron measurements Ondřej Svoboda Nuclear Physics Institute,
New methods to measure the cross sections of 12 C+ 12 C fusion reaction Xiao Fang Department of Physics University of Notre Dame.
Recent Results for proton capture S-factors from measurements of Asymptotic Normalization Coefficients R. Tribble Texas A&M University OMEG03 November,
Studies of neutron cross-sections by activation method in Nuclear Physics Institute Řež and in The Svedberg Laboratory Uppsala and experimental determination.
Searching for the Low-Energy Resonances in the 12 C( 12 C,n) 23 Mg Reaction Cross Section Relevant for S-Process Nucleosynthesis Brian Bucher University.
Nuclear Astrophysics at LNS Claudio Spitaleri Claudio Spitaleri Catania University-Italy Laboratori Nazionali del Sud- Catania-Italy Meeting LEA COLLIGA.
Breakup effects of weakly bound nuclei on the fusion reactions C.J. Lin, H.Q. Zhang, F. Yang, Z.H. Liu, X.K. Wu, P. Zhou, C.L. Zhang, G.L. Zhang, G.P.
Cross-sections of Neutron Threshold Reactions Studied by Activation Method Nuclear Physics Institute, Academy of Sciences of Czech Republic Department.
Nucleus-Nucleus 2012San Antonio (TX) 18 F+p  15 O + CRIB 1.
ANC Techniques and r-matrix analysis Santa Fe, April 2008 ANC Techniques and r-matrix analysis Grigory Rogachev.
Study of unbound 19 Ne states via the proton transfer reaction 2 H( 18 F,  + 15 O)n HRIBF Workshop – Nuclear Measurements for Astrophysics C.R. Brune,
ALNA- Accelerator Laboratory for Nuclear Astrophysics Underground Heide Costantini University of Notre Dame, IN, USA INFN, Genova, Italy.
Nucleus Nucleus 2015 – Catania June 2015 Catania, June 25 th 2015 Univ. degli Studi di Napoli Federico II & INFN - Napoli Study of cluster structures.
Nucleosynthesis in AGB Stars: the Role of the 18 O(p,  ) 15 N Reaction Marco La Cognata.
Institute for Structure and Nuclear Astrophysics Nuclear Science Laboratory E381: Search of potential resonances in the 12 C+ 12 C fusion reaction using.
This project is funded by the NSF through grant PHY , and the Universities of JINA. The Joint Institute for Nuclear Astrophysics Henderson DUSEL.
Beijing, Sept 2nd 2004 Rachele Di Salvo Beam asymmetry in meson photoproduction on deuteron targets at GRAAL MENU2004 Meson-Nucleon Physics and the Structure.
FLUORINE DESTRUCTION IN STARS: FIRST EXPERIMENTAL STUDY OF THE 19 F(p,α 0 ) 16 O REACTION AT ASTROPHYSICAL ENERGIES Marco La Cognata INFN-LNS Catania.
Reaction studies with low-energy weakly-bound beams Alessia Di Pietro INFN-Laboratori Nazionali del Sud NN 2015Alessia Di Pietro,INFN-LNS.
Institute for Structure and Nuclear Astrophysics Nuclear Science Laboratory The 12 C+ 12 C fusion reaction at stellar energies Xiaodong Tang (Aggie since.
Effects Of Distortion On Trojan Horse Applications Rosario Gianluca Pizzone INFN – Laboratori Nazionali del Sud Catania.
Indirect Techniques ( I) : Asymptotic Normalization Coefficients and the Trojan Horse Method NIC IX R.E. Tribble, Texas A&M University June, 2006.
The experimental evidence of t+t configuration for 6 He School of Physics, Peking University G.L.Zhang Y.L.Ye.
Laboratori Nazionali del Sud Start EXCYT status and perspectives L. CELONA on behalf the EXCYT collaboration Istituto Nazionale di Fisica Nucleare-Laboratori.
Status and future of ASFIN (AstroFIsica Nucleare) Stefano Romano Univ. Catania & INFN – LNS LNS 28 giugno 2010 Giants Padova - 28 – 30 aprile 2014.
Indirect measurements of the -3 keV resonance in the 13 C(α, n) 16 O reaction: the THM approach Marco La Cognata.
Exploring the alpha cluster structure of nuclei using the thick target inverse kinematics technique for multiple alpha decays. Marina Barbui June, 23 rd,
Shuya Ota: Japan Atomic Energy Agency, Rutgers University H. Makii, T. Ishii, K. Nishio, S. Mitsuoka, I. Nishinaka : Japan Atomic Energy Agency M. Matos,
Investigation of the freeze-out configuration in the 197 Au Au reaction at 23 AMeV A.Sochocka Department of Physics, Astronomy and Applied Computer.
Exploring the alpha cluster structure of nuclei using the thick target inverse kinematics technique for multiple alpha decays. The 24 Mg case Marina Barbui.
1 Cross sections of neutron reactions in S-Cl-Ar region in the s-process of nucleosynthesis C. Oprea 1, P. J. Szalanski 2, A. Ioan 1, P. M. Potlog 3 1Frank.
Study of the properties of the superheavy nucleus Z = 117 produced in the 249Bk + 48Ca reaction А.А. Voinov for the collaboration of for the collaboration.
Beta decay spectroscopy studies of novae and x-ray bursts
The Trojan Horse Method As A Tool To Investigate Low-energy Resonances: The 18O(p,α)15N and 17O(p,α)14N Cases Marco La Cognata.
Modified r-matrix analysis of the 19F(p,a)16O HOES reaction
Study of the 17O(n,α)14C reaction: extension of the Trojan Horse Method to neutron induced reactions Hello, I’m Giovanni Luca Guardo and I’ll talk about.
Relativistic Kinematics for the Binding Energy of Nuclear Reactions
Bare nucleus astrophysical S(E) factors of the
György Gyürky Institute for Nuclear Research (Atomki)
Laboratori Nazionali del Sud of INFN
Direct measurements for nuclear
Cross-section Measurements of (n,xn) Threshold Reactions
Marilena AvrigeanuMarilena Avrigeanu
Rosario Gianluca Pizzone
THE DIRECT 18O(p, γ)19F CAPTURE AND THE ANC METHOD
György Gyürky Institute of Nuclear Research (Atomki) Debrecen, Hungary
A new investigation of the Hoyle state in 12C via the
Jiansong Wang for NIMROD Collaboration
EUROPEAN ORGANIZATION FOR NUCLEAR RESEARCH
Searching for states analogous to the 12C Hoyle state in heavier nuclei using the thick target inverse kinematics technique. Marina Barbui 5/17/2018, Galveston,
Sensitivity of reaction dynamics by analysis of kinetic energy spectra of emitted light particles and formation of evaporation residue nuclei.
Status of the A=56, 64, and 68 X-ray burst waiting points
Elastic alpha scattering experiments
Direct Measurement of the 8Li + d reactions of astrophysical interest
O. Svoboda, A. Krása, A. Kugler, M. Majerle, J. Vrzalová, V. Wagner
Catalin Borcea IFIN-HH INPC 2019, Glasgow, United Kingdom
Presentation transcript:

Virtual Neutron Method applied to the study of 17 O(n,  ) 14 C reaction Marisa Gulino LNS - INFN, Catania & Università di Enna “Kore”

 Why studying 17 O(n,  ) 14 C reaction  From Trojan Horse Method to Virtual Neutron Method  The experiments  data analysis and results  Why studying 17 O(n,  ) 14 C reaction  From Trojan Horse Method to Virtual Neutron Method  The experiments  data analysis and results INPC 2013 Firenze, Italy 2-7 JUNE 2013 SUMMARY

INPC 2013 Firenze, Italy 2-7 JUNE 2013 THE 17 O(n,  ) REACTION: status of art NUCLEAR REACTORS the neutron induced reaction on 14 N and 17 O are the dominant sources of the radioactive isotope 14 C (T 1/2 = 5730 yr). NUCLEAR ASTROPHYSICS In the inhomogeneous big-bang model the 14 C may act as a bottleneck in the production of elements heavier than A=17 anomalies in 18 O/ 16 O and 17 O/ 16 O ratios found in asymptotic giant branch stars and in circumstellar Al 2 O 3 meteorite grains neutron poison in the nucleosynthesis of the s-process elements O+n ± ± ± ± O The cross section of this reaction is characterized by the presence of several narrow resonant states in the 18 O compound nucleus.

INPC 2013 Firenze, Italy 2-7 JUNE 2013 THE 17 O(n,  ) REACTION: status of art Data from: P. E. Koehler and S. M. Graff, Phys. Rev. C 44, 2788 (1991). H. Schatz, F. Kaeppeler, P. E. Koehler, M. Wiescher, and H. P. Trautvetter, Astrophys. J. 413, 750 (1993). R. M. Sanders, Phys. Rev. 104, 1434 (1956) from J. WAGEMANS et al. PHYSICAL REVIEW C (2002) INFLUENCE OF SUBTRESHOLD RESONANCE “ The reaction rate at the astrophysical relevant temperatures was calculated and found to be a factor of 2–2.5 lower than previously adopted.“ DIFFERENCES IN EXPERIMENTAL DATA “The significant impact of the presence of the negative-energy p-wave resonance on the reaction rate was shown.”

INPC 2013 Firenze, Italy 2-7 JUNE 2013 INDIRECT METHODS: Trojan Horse Method reminder IDEA (C. Spitaleri, 1990): Extract the cross section  2Body for A + x  B + b from Quasi-free reaction channel data of a three body reaction T + A  B + b + s where T shows a strong clusterization in x+s A T s x B b E TA = T-A relative energy E C =T-A Coulomb barrier E Ax = E Bb – Q 2body (pcp)

INPC 2013 Firenze, Italy 2-7 JUNE 2013 From TROJAN HORSE to VIRTUAL NEUTRON METHOD A d p n B b spectator participant Detected particles If the Quasi-free mechanism is selected in PWIA the cross section of the reaction n+A  B+b can be deduced N

INPC 2013 Firenze, Italy 2-7 JUNE 2013 FIRST APPLICATION: THE 6 Li(n,  ) REACTION 6 Li d p n 3H3H  spectator participant Detected particles 6 Li(n,  ) 3 H d( 6 Li,  3 H)p J. of Phys. G, Nucl. Part.Phys. 37, (2010) 6 Li(n,  )t cross section ___direct data OTH data

INPC 2013 Firenze, Italy 2-7 JUNE 2013 THE 17 O(n,  ) REACTION: the 17 O+d experiments 14 N+  +n 17 O+d 14 C+  +p 17 O+p  14 N+  17 O+n  14 C+  Two experiments have been - Catania, – Notre Dame, IN, USA EXPERIMENTAL SET-UP MeV CD 2 IC PSD 5° 30°

INPC 2013 Firenze, Italy 2-7 JUNE 2013 THE 17 O(n,  ) REACTION: Identification of reaction channel ONCONC  Carbon selection by  E-E spectra  Coincidence between kinematical calculations and experimental data Q- value of the 17 O+d  14 C+  +p reaction  P

INPC 2013 Firenze, Italy 2-7 JUNE 2013 THE 17 O(n,  ) REACTION: Evidences of QF mechanism A more sensitive check of the predominance of the QF reaction mechanism is achieved by investigating the shape of the experimental momentum distribution of the n and p inside deuteron. DWBA

INPC 2013 Firenze, Italy 2-7 JUNE 2013 THE 17 O(n,  ) REACTION: cross section 11 LNS Experiment ND Experiment PHYSICAL REVIEW C 87, (R) (2013) I) subtreshold level II) resonance populated in l=3 missing in the direct data III) corresponding to the direct data IV) corresponding to the direct data I II III IV III IV

INPC 2013 Firenze, Italy 2-7 JUNE 2013 THE 17 O(n,  ) REACTION: angular distribution 12 PHYSICAL REVIEW C 87, (R) (2013) cos  cm l i =1 l i =0, l i =2 l i =3 l i =1 I II III IV I II l i =1l i =3 III IV l i =2l i =1 l i =0 angular distributions have been measured for the first time

INPC 2013 Firenze, Italy 2-7 JUNE 2013 THE 17 O(n,  ) REACTION: Comparison with direct data N N Data correction for the penetrability of the centrifugal barrier PHYSICAL REVIEW C 87, (R) (2013)

INPC 2013 Firenze, Italy 2-7 JUNE 2013 CONCLUSIONS

M Gulino 1,2, C. Spitaleri 1,3, X.D. Tang 4, G.L. Guardo 1,3, L. Lamia 3, S. Cherubini 1,3, B. Bucher 4, V. Burjan 5, M. Couder 4, P. Davies 4, R. deBoer 4, X. Fang 4, V.Z. Goldberg 6, Z. Hons 5, V. Kroha 5, L. Lamm 4,†, M. La Cognata 1, C. Li 7, C. Ma 4, J. Mrazek 5, A.M. Mukhamedzhanov 6, M. Notani 4, S. OBrien 4, R.G. Pizzone 1, G.G. Rapisarda 1,3, D. Roberson 4, M.L. Sergi 1, W. Tan 4, I.J. Thompson 8, M. Wiescher 4 1 INFN Laboratori Nazionali del Sud, Catania, Italy 2 Università degli Studi di Enna “KORE”, Enna, Italy 3 Dipartimento di Fisica ed Astronomia, Università degli Studi di Catania, Catania, Italy 4 Department of Physics and Joint Institute for Nuclear Astrophysics, University of Notre Dame, IN, USA 5 Nuclear Physics Institute of ASCR, Rez, Czech Republic 6 Cyclotron Institute,Texas A&M University,College Station, TX, USA 7 China Institute of Atomic Energy, Beijing, China 8 Lawrence Livermore National Laboratory, Livermore, CA, USA Contact M Gulino 1,2, C. Spitaleri 1,3, X.D. Tang 4, G.L. Guardo 1,3, L. Lamia 3, S. Cherubini 1,3, B. Bucher 4, V. Burjan 5, M. Couder 4, P. Davies 4, R. deBoer 4, X. Fang 4, V.Z. Goldberg 6, Z. Hons 5, V. Kroha 5, L. Lamm 4,†, M. La Cognata 1, C. Li 7, C. Ma 4, J. Mrazek 5, A.M. Mukhamedzhanov 6, M. Notani 4, S. OBrien 4, R.G. Pizzone 1, G.G. Rapisarda 1,3, D. Roberson 4, M.L. Sergi 1, W. Tan 4, I.J. Thompson 8, M. Wiescher 4 1 INFN Laboratori Nazionali del Sud, Catania, Italy 2 Università degli Studi di Enna “KORE”, Enna, Italy 3 Dipartimento di Fisica ed Astronomia, Università degli Studi di Catania, Catania, Italy 4 Department of Physics and Joint Institute for Nuclear Astrophysics, University of Notre Dame, IN, USA 5 Nuclear Physics Institute of ASCR, Rez, Czech Republic 6 Cyclotron Institute,Texas A&M University,College Station, TX, USA 7 China Institute of Atomic Energy, Beijing, China 8 Lawrence Livermore National Laboratory, Livermore, CA, USA Contact INPC 2013 Firenze, Italy 2-7 JUNE 2013 Thanks to the COLLABORATION