E.C. Simpson C. Ugalde M. Heil P.J. LeBlank R.J. DeBoer H. Costantini E. Uberseder R.E. Azuma C.R. Brune J. Goerres M.M. Wiescher “ In addition, the authors.

Slides:



Advertisements
Similar presentations
Neutron-induced Reactions
Advertisements

Cross section measurements with the Karlsruhe 4 BaF 2 Detector using a 3.7 MV Van de Graaff accelerator M. Weigand, S. Walter, F. Käppeler, R. Plag and.
R-Matrix Analysis of 15 N(p,  0 ) 16 O using the program AZURE. P.J. LeBlanc April 23 rd, 2008 Sante Fe, NM.
Combined evaluation of PFNS for 235 U(n th,f), 239 Pu(n th,f), 233 U(n th,f) and 252 Cf(sf) (in progress) V.G. Pronyaev Institute of Physics.
Analysis report of SN1006 D.Nishida( Kyoto-Univ.) JPS meeting Autumn 2005 Osaka.
Nuclear Astrophysics Lecture 1 Tues. April 24, 2012 Prof. Shawn Bishop, Office 2013, Ex
JINA Frontiers 2005 Lifetimes of the astrophysically important states in 19 Ne Wanpeng Tan University of Notre Dame Collaborators: J. Görres, M. Wiescher,
Beta-decay directly to continuum K Riisager Dept. of Physics and Astronomy Aarhus University.
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.
N  p + e   e    e   e +  Ne *  Ne +  N  C + e   e Pu  U +  Fundamental particle decays Nuclear.
Status of TACTIC: A detector for nuclear astrophysics Alison Laird University of York.
Forschungszentrum Karlsruhe in der Helmholtz-Gemeinschaft Neutron capture cross sections on light nuclei M. Heil, F. Käppeler, E. Uberseder Torino workshop,

The R-matrix method and 12 C(  ) 16 O Pierre Descouvemont Université Libre de Bruxelles, Brussels, Belgium 1.Introduction 2.The R-matrix formulation:
“Super-radiance” and the width of exotic baryons N. Auerbach V. Zelevinsky A. Volya This work is supported by NSF grant PHY and in part by a grant.
25 9. Direct reactions - for example direct capture: Direct transition from initial state |a+A> to final state B +  geometrical.
Pierre Descouvemont Université Libre de Bruxelles, Brussels, Belgium The 12 C(  ) 16 O reaction: dreams and nightmares theoretical introduction.
Boris Pritychenko Nuclear Physics Data Compilation for Nucleosynthesis Modeling, Trento, May 29 – June 1, 2007 MACS and Astrophysical Reaction Rates from.
The Theory of Partial Fusion A theory of partial fusion is used to calculate the competition between escape (breakup) and absorption (compound-nucleus.
Structure of 8 B through 7 Be+p scattering 1 Jake Livesay, 2 DW Bardayan, 2 JC Blackmon, 3 KY Chae, 4 AE Champagne, 5 C Deibel, 4 RP Fitzgerald, 1 U Greife,
New methods to measure the cross sections of 12 C+ 12 C fusion reaction Xiao Fang Department of Physics University of Notre Dame.
Experimental investigation of stellar 12 C+ 12 C fusion toward extremely low energies by direct and indirect methods Xiao Fang University of Notre Dame.
Error bars for reaction rates in astrophysics: the R-matrix theory context. Claudio Ugalde University of North Carolina.
Spectral Analysis of Archival SMM Gamma-Ray Flare Data Gerald Share 1,2, Ronald Murphy 2, Benz Kozlovsky 3 1 UMD, 2 NRL, 3 Tel Aviv Univ. Supported under.
If the Coordinates system is. R r b (impact parameter.
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.
ANC Techniques and r-matrix analysis Santa Fe, April 2008 ANC Techniques and r-matrix analysis Grigory Rogachev.
Three-body radiative capture reactions in astrophysics L.V. Grigorenko K.-H. Langanke and M. Zhukov FLNR, JINR, Dubna and GSI, Darmstadt.
CCFE is the fusion research arm of the United Kingdom Atomic Energy Authority EAF-2010 – the best of a generation Jean-Christophe Sublet, Lee Packer Euratom/CCFE.
Institute for Structure and Nuclear Astrophysics Nuclear Science Laboratory E381: Search of potential resonances in the 12 C+ 12 C fusion reaction using.
L.D. Blokhintsev a, A.N. Safronov a, and A.A. Safronov b a Skobeltsyn Institute of Nuclear Physics, Moscow State University, Moscow, Russia b Moscow State.
ERNA: Measurement and R-Matrix analysis of 12 C(  ) 16 O Daniel Schürmann University of Notre Dame Workshop on R-Matrix and Nuclear Reactions in Stellar.
June 6, 2006 CALOR 2006 E. Hays University of Chicago / Argonne National Lab VERITAS Imaging Calorimetry at Very High Energies.
THEORETICAL PREDICTIONS OF THERMONUCLEAR RATES P. Descouvemont 1.Reactions in astrophysics 2.Overview of different models 3.The R-matrix method 4.Application.
Institute for Reference Materials and Measurements (IRMM) Geel, Belgium CRP Th - U, Vienna December 2004.
00 Cooler CSB Direct or Extra Photons in d+d  0 Andrew Bacher for the CSB Cooler Collaboration ECT Trento, June 2005.
13 december 2002H.L. / KVI PAC Meeting1 Pionic fusion: comparison of different spin/isospin channels Study coherence of pion production, role of clustering.
Santa Tecla, 2-9 October 2005Marita Mosconi,FZK1 Re/Os cosmochronometer: measurements of relevant Os cross sections Marita Mosconi 1, Alberto Mengoni 2,
Studying FSR at threshold for  events O. Shekhovtsova, G.V. lnf 3/1/05 Radiative meeting Disclaimer: everything is preliminary!!!
Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 1.
Data Needs in Nuclear Astrophysics, Basel, June 23-25, 2006 Nuclear Astrophysics Resources of the National Nuclear Data Center B. Pritychenko*, M.W. Herman,
Indirect measurements of the -3 keV resonance in the 13 C(α, n) 16 O reaction: the THM approach Marco La Cognata.
Global R-Matrix Analysis of the 12 C(α,γ) 16 O Reaction NN2012 Carl Brune Ohio University, Athens Ohio May 28, 2012.
Proposed Laboratory Simulation of Galactic Positron In-Flight Annihilation in Atomic Hydrogen Benjamin Brown, Marquette University, Milwaukee, WI, USA.
Jun Chen Department of Physics and Astronomy, McMaster University, Canada For the McMaster-NSCL and McMaster-CNS collaborations (5.945, 3+ : **) (5.914,
Report (2) on JPARC/MLF-12B025 Gd(n,  ) experiment TIT, Jan.13, 2014 For MLF-12B025 Collaboration (Okayama and JAEA): Outline 1.Motivation.
The 18 F(p,  ) 15 O reaction and RIB developments F. de Oliveira Santos.
Fabien Zehr Double π photoproduction Glasgow 28 March 2006 Double π photoproduction at threshold and in the second resonance region With Crystal Ball and.
R-Matrix Methods and an Application to 12C(α,γ)16O
Modified r-matrix analysis of the 19F(p,a)16O HOES reaction
David Mountford University of Edinburgh
Stanislav Pospíšil et al, Brightness Vidyo meeting
Neven Soić, Ruđer Bošković Institute, Zagreb, Croatia
Resonances in the 12C(α,γ)16O reaction
gamma-transmission coefficients are most uncertain values !!!
Calibration, Simulations, and “Remaining” Issues
LaBr3 Ball at HIE-ISOLDE
Carbon, From Red Giants to White Dwarfs
Satoshi Adachi Research Center for Nuclear Physics (RCNP),
L*(1520) Photoproduction off Proton and Neutron from CLAS eg3 data set
Study of the resonance states in 27P by using
Study of the resonance states in 27P by using
probability of surviving
Deeply Bound Mesonic States -Case of Kaon-
Photoproduction of poh pairs on the proton
Recoil charge state distributions in 12C(a,g)16O at DRAGON
e+e−→ J/ D(*)D(*) & ψ(4160) → DD
Comprehensive study of S = -1 hyperon resonances via the coupled-channels analysis of K- p and K- d reactions Hiroyuki Kamano (KEK) YITP Workshop on.
Study of K-p→Lp+p-, Lp0 and γn → K+Σ*-
The np -> d p0 reaction measured with g11 data
Presentation transcript:

E.C. Simpson C. Ugalde M. Heil P.J. LeBlank R.J. DeBoer H. Costantini E. Uberseder R.E. Azuma C.R. Brune J. Goerres M.M. Wiescher “ In addition, the authors are indebted To Fred C. Barker and (ANU, Canberra) and Erich Vogt (Triumf, Vancouver) for many discussions and their help in the AZURE R-matrix project.”

Differential Cross Section Lane and Thomas, Eqns. 2.7 and 2.8, p. 292 where Angle Integrated Cross section

24°

33°

38.0

43.9°

48.9

54°

58.9°

63.9°

68.9°

74.0°

75.8°

165.8°

Measurement of 16O Widths: Determination of 15N+p astrophysical reactions All reactions and data sets analyzed simultaneously (Including radiative direct capture) Reactions studied: 12C(α,α0)12C 12C(α,α1)12C 12C(α,p)15N 12C(α,γ)16O 15N(p,p0)15N 15N(p,α0)12C 15N(p,α1)12C 15N(p,γ)16O Data Sets: (a,a0) (a,a1) (a,p0) (a,g) Tischausser x Morris et al x Feng et al x Mitchel et al x Mitchel+Ophel x Schuerman et al x (p,p0) (p0,a0) (p,a1) (p,g) Hagedorn x Hagedorn+Marion x Bashkin et al x x Redder et al x Bray et al x LeBlank etal x

Alpha Entrance-Channel Reactions Above proton threshold 12C(α,α0)12C

167° 136° 104° 71°

165°

6.6 MeV6.99 MeV 7.4 MeV7.7 MeV

12c(α,α1)12C Above proton threshold

40° 90° 120°

12C(α,γ)16O and 12C(α,p0)15N Above proton threshold

Total Cross section

30° 40° 90° 120°

Proton Entrance-Channel Reactions Threshold Ex= MeV

25° 105°

0.888 MeV1.038 MeV MeV MeV

82° 159.9°

90° 125° 160°

16 O(  ) 20 Ne

Graphical representation of the related uncertainty between two of the R-matrix fit parameters for the broad resonance at 2.5 MeV. Here the change in chi2 would be on the z- axis. Since the shape is elliptical this signifies that the two parameters have very little correlation. That is, the alpha and gamma widths for this resonance are good (not redundant) fit parameters.

AZURE WEB SITE