NucleoSynthesis of Galactic 26 Al 26 Al gs +p, 26 Al m +p, 25 Al+p Resonances Peter Parker, Yale University Catherine Deibel, Rachel Lewis, Anuj Parikh,

Slides:



Advertisements
Similar presentations
The 26g Al(p, ) 27 Si Reaction at DRAGON Heather Crawford Simon Fraser University TRIUMF Student Symposium July 27, 2005.
Advertisements

An overview of the S1105 experiment at TRIUMF. 1 Martin Jones The University of Liverpool
Advanced GAmma Tracking Array
Structure of the ECEC candidate daughter 112 Cd P.E. Garrett University of Guelph TRIUMF Excellence Cluster “Universe”, Technische Universität München.
Progress on the 40 Ca(α,  ) 44 Ti reaction using DRAGON Chris Ouellet Supervisor: Alan Chen Experiment leader: Christof Vockenhuber ● Background on the.
Owned and operated as a joint venture by a consortium of Canadian universities via a contribution through the National Research Council Canada Propriété.
NucleoSynthesis of Galactic 26 Al 25 Al+p Resonances Peter Parker, Yale University Catherine Deibel, Rachel Lewis, Anuj Parikh, Christopher Wrede Jac Caggiano,
The Role of 12 C( 12 C,n) in the Astrophysical S-Process Brian Bucher University of Notre Dame.
Classical novae, type I x-ray bursts, and ATLAS Alan Chen Department of Physics and Astronomy McMaster University.
Low energy radioactive beams Carmen Angulo, CRC Louvain-la-Neuve, Belgium FINUPHY meetingLouvain-la-Neuve, Belgium3-4 May 2004 Recent highlights on nuclear.
Studying the  p-process at ATLAS Catherine M. Deibel Joint Institute for Nuclear Astrophysics Michigan State University Physics Division Argonne National.
Reaction rates in the Laboratory Example I: 14 N(p,  ) 15 O stable target  can be measured directly: slowest reaction in the CNO cycle  Controls duration.
Status of TACTIC: A detector for nuclear astrophysics Alison Laird University of York.
GAMMA-PARTICLE ARRAY FOR DIRECT REACTION STUDIES SIMULATIONS.
1 An Introduction to Ion-Optics Series of Five Lectures JINA, University of Notre Dame Sept. 30 – Dec. 9, 2005 Georg P. Berg.
1107 Series of related experiments; first for transfer with TIGRESS Nuclear structure motivation for 25,27 Na beams Nuclear astrophysics motivation for.
Reaction rates in the Laboratory Example I: 14 N(p,  ) 15 O stable target  can be measured directly: slowest reaction in the CNO cycle  Controls duration.
Reaction rates in the Laboratory Example I: 14 N(p,  ) 15 O stable target  can be measured directly: slowest reaction in the CNO cycle  Controls duration.
Anuj Parikh Universitat Politècnica de Catalunya The search for “important” nuclear reactions in astrophysical environments.
ANASEN - Array for Nuclear Astrophysics Studies with Exotic Nuclei Silicon-strip detector array backed with 2-cm-thick CsI Gas proportional counter for.
Astrophysics with DRAGON: The 26g Al (p,γ) 27 Si Reaction Heather Crawford a,1 for the DRAGON Collaboration b a Simon Fraser University, Burnaby, B.C.,
Nuclear astrophysics with the Munich Q3D spectrograph
Abstract The 13 N(p,γ) 14 O reaction is very important for our understanding of explosive astrophysical sites, such as novae and supernovae. This reaction.
Recoil Separator Techniques J.C. Blackmon, Physics Division, ORNL RMS - ORNL WF QT QD Q D Target FP ERNA - Bochum WF Target D QT FP DRS ORNL QD VF D VAMOS.
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.
Absolute resonance strength measurements of the 22 Na(p,  ) reaction Chris Wrede Center for Experimental Nuclear Physics and Astrophysics University of.
Nuclear Astrophysics with the PJ Woods, University of Edinburgh.
Mats Lindroos Measuring difficult reaction rates involving radioactive beams: A new approach John D’Auria, Mats Lindroos, Jordi Jose and Lothar Buchmann.
Proton resonance scattering of 7 Be H. Yamaguchi, Y. Wakabayashi, G. Amadio, S. Kubono, H. Fujikawa, A. Saito, J.J. He, T. Teranishi, Y.K. Kwon, Y. Togano,
Study of the 40 Ca(  ) 44 Ti reaction at stellar temperatures with DRAGON Christof Vockenhuber for the DRAGON collaboration Vancouver, B.C., Canada.
Depth Profiling with Low-Energy Nuclear Resonances H.-W. Becker, IAEA May 2011 CRP: Reference Database for Particle Induced Gamma-ray Emission (PIGE) Ruhr-University.
Constraining the astrophysical S-factor of the 3 He(  ) 7 Be reaction Constraining the astrophysical S-factor of the 3 He(  ) 7 Be reaction Mariano.
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.
TRIUMF Canada’s national laboratory for nuclear and particle physics Direct Measurement of the 21 Na(p,γ) 22 Mg Reaction: Resonance Strengths and γ-γ Analysis.
B.MOUGINOT IPNO PHD director : F. AZAIEZ, S. FRANCHOO Giant Pairing Vibration : Experimental Overview.
B.MOUGINOT IPNO PHD director : F. AZAIEZ, S. FRANCHOO Search of Giant Pairing Vibration in nuclei.
The neutron source for the weak component of the s-process: latest experimental results Claudio Ugalde University of North Carolina at Chapel Hill and.
Proton emission from deformed rare earth nuclei: A possible AIDA physics campaign Paul Sapple PRESPEC Decay Physics Workshop Brighton 12 January 2011.
Zagreb IP: Experimental nuclear physics inputs for thermonuclear runaway - NuPITheR Neven Soić, Ru đ er Bošković Institute, Zagreb, Croatia EuroGENESIS.
Measurement of the 26 Al(d,p) 27 Al reaction to constrain the 26 Al(p,  ) 27 Si reaction rate Steven D. Pain Oak Ridge National Laboratory NS12, Argonne,
Study of the Destruction of 18 F in Novae with an Inverse (d,p) Reaction at the HRIBF Introduction/Motivation Experiment and Results Astrophysical Significance.
Hidetoshi Yamaguchi ( 山口英斉 ) T. Hashimoto, S. Hayakawa, D. Kahl, and S. Kubono Center for Nuclear Study, Univ. of Tokyo Hidetoshi Yamaguchi ( 山口英斉 ) T.
Surface Characterization of 14 N Implanted Targets Abhijit Bisoi Saha Institute of Nuclear Physics 1/AF Bidhannagar, Kolkata-64.
CAWONAPS - Dec 10th, S(p,  ) 34 Cl Constraining nova observables: Direct measurement of 33 S(p,  ) 34 Cl in inverse kinematics Jennifer Fallis,
Experimental Nuclear Physics Some Recent Activities 1.Development of a detector for low-energy neutrons a. Hardware -- A Novel Design Idea b. Measure the.
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,
Measurements of the 27 Al(d,  ) 25 Mg excitation functions A. Gurbich Institute of Physics and Power Engineering Obninsk, Russia.
 ( E ) = S(E) e –2   E -1 2      m  m   m   m   Reaction Rate(star)    (E)  (E) dE Gamow Peak  Maxwell Boltzmann.
 ( E ) = S(E) e –2   E -1 2       m  m   m   m   Reaction Rate(star)    (E)  (E) dE Gamow Peak  Maxwell Boltzmann.
1 Hypernuclear  -ray spectroscopy via the (K -,  0 ) reaction K. Shirotori Tohoku Univ.
Direct measurement of the 18 Ne( , p) 21 Na reaction with a GEM – MSTPC Takashi Hashimoto CNS, University of Tokyo Collaborators CNS S. Kubono, H. Yamaguchi,
Measurement of 7 Be(n,  ) and 7 Be(n,p) cross sections for the Cosmological Li problem in Addendum to CERN-INTC /INTC-P-417 Spokepersons:
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.
Nuclear Astrophysics ARUNA Workshop, Notre Dame, IN Carl R. Brune Ohio University, Athens Ohio June 12-13, 2014.
Beginning of 0˚ mode for K600 at iTL
REQUIREMENTS for Zero-Degree Ion Selection in TRANSFER Wilton Catford University of Surrey, UK & SHARC collabs.
Study of isomeric states using gamma spectroscopy around N=40 C. Petrone 1,2, J. M. Daugas 3, M. Stanoiu 1, F. Negoita 1, G. Simpson 4, C. Borcea 1, R.
EUROPEAN ORGANIZATION FOR NUCLEAR RESEARCH Proposal to the ISOLDE and Neutron Time-of-Flight Committee Study of the beta delayed particle emission from.
Activities and Opportunities at the accelerator lab in Bochum H.-W. Becker, NUPECC Small Scale Facilities workshop, 7./8. Sep
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,
PJ Woods University of Edinburgh In-ring detector systems.
Studies on alpha-induced astrophysical reactions using the low-energy RI beam separator CRIB Studies on alpha-induced astrophysical reactions using the.
Anuj Parikh Universitat Politècnica de Catalunya
Nuclear Reaction Studies for Explosive Nuclear Astrophysics
Recoil charge state distributions in 12C(a,g)16O at DRAGON
Naohito Iwasa Dept. Phys., Tohoku Univ.
A Study in Garnet & Gold – Unveiling mysteries with the SE-SPS
Presentation transcript:

NucleoSynthesis of Galactic 26 Al 26 Al gs +p, 26 Al m +p, 25 Al+p Resonances Peter Parker, Yale University Catherine Deibel, Rachel Lewis, Anuj Parikh, Christopher Wrede, Jac Caggiano, Jason Clark 2006 Mitchell Symposium

Wasserburg, et al. e.g., T.Lee & D.Papanastassiou, Geophys.Res.Lett. 1(1974) 225. J,G,Bradley et al., J.Geophys.Res. 83(1978)547.

HEAO-3 (1979) :

26 Al (1809 keV) map of our Galaxy GRO-Comptel

R.Diehl et al., Nature 439(2006) Al 1809-keV  -ray Line - SPI-INTEGRAL

R.Diehl et al., Nature 439(2006) Al 1809-keV  -ray Line Doppler Shift vs. Galactic Longitude - SPI-INTEGRAL

25 Al Branch Point: (p,  ) 26 Si(   ) 26m Al(   ) 26 Mg GS 24 Mg(p,  ) 25 Al (   ) 25 Mg(p,  ) 26 Al(   ) 26* Mg(  26 Mg GS

25 Al(p,  ) 26 Si  Resonance Searches: 29 Si( 3 He, 6 He) 26 Si 26 Al( 3 He,t) 26 Si(p) 25 Al Direct Measurement: TRIUMF DRAGON E922 Yale TRIUMF E1O71 26g Al(p,  ) 27 Si  Direct Measurement: TRIUMF DRAGON E989 26m Al(p,  ) 27 Al  Resonance Search: 27 Al( 3 He,t) 27 Si(p) 26m Al Yale

25 Al(p,  ) Reaction Rates 29 Si( 3 He, 6 He) 27 Si J.A.Caggiano, et al. Phys.Rev.C65(2002)055801

25 Al(p,  ) 26 Si  Resonance Searches: 29 Si( 3 He, 6 He) 26 Si 26 Al( 3 He,t) 26 Si(p) 25 Al Direct Measurement: TRIUMF DRAGON E922 Yale TRIUMF E1O71 26g Al(p,  ) 27 Si  Direct Measurement: TRIUMF DRAGON E989 26m Al(p,  ) 27 Al  Resonance Search: 27 Al( 3 He,t) 27 Si(p) 26m Al Yale

26 Al Implanted Target: ( TRIUMF-ISAC Proposal E1071) HRMS   4  Al/sec at an energy of 51 keV  Al/cm 2 rastered into a 3-mm diameter circle in 4 to 7 days, into a 40 μg/cm 2 carbon foil  Contamination: About 1 to 10% 26 Na(  - ) 26 Mg,  But  no 27 Al With this target, in conjunction with the Yale split-pole spectrograph and the YLSA silicon array, we project a 26 Al( 3 He,t) 26 Si * (p) 25 Al coincidence rate of 1/hour.

500-  thick Silicon 5 Sectors; 16 strips each Covering 131°  lab  166° 80-energy and 80-time signals Yale LampShade Array - YLSA

26 Al( 3 He,t) 26 Si*(p) 25 Al E YLSA vs. Focal Plane

25 Al(p,  ) 26 Si  Resonance Searches: 29 Si( 3 He, 6 He) 26 Si 26 Al( 3 He,t) 26 Si(p) 25 Al Direct Measurement: TRIUMF DRAGON E922 Yale TRIUMF E1O71 26g Al(p,  ) 27 Si  Direct Measurement: TRIUMF DRAGON E989 26m Al(p,  ) 27 Al  Resonance Search: 27 Al( 3 He,t) 27 Si(p) 26m Al Yale

25 Al(p,  ) 26 Si  Resonance Searches: 29 Si( 3 He, 6 He) 26 Si 26 Al( 3 He,t) 26 Si(p) 25 Al Direct Measurement: TRIUMF DRAGON E922 Yale TRIUMF E1O71 26g Al(p,  ) 27 Si  Direct Measurement: TRIUMF DRAGON E989 26m Al(p,  ) 27 Al  Resonance Search: 27 Al( 3 He,t) 27 Si(p) 26m Al Yale

Low-Energy 26 Al(p,  ) Measurements : (E res  600 keV) E res = 277, 363 keV Buchmann, Rolfs, et al. Nucl.Phys. A415 (1984) E res = 188, 238, 277, 363 keV Vogelaar, Kavanagh, et al. Ph.D. Thesis Al( 3 He,d) (E res = 188, 277 keV) Vogelaar, Champagne, et al. Phys.Rev.C 53 (1996) `

26 Al(p,  ) 27 Si DRAGON TOF vs. Focal Plane Energy E 989

26 Al(p,  ) 27 Si DRAGON TOF Projection

ISAC-DRAGON Gas Target and BGO Array E 989

Primary BGO Hit Position (mm) E 989

26 Al(p,  ) TRIUMF - DRAGON E989 Chris Ruiz (Simon Fraser) PI Anuj Parikh (Yale) - PhD Thesis E cm = 184±1 keV resonance. E( 26 Al) = 5.2 MeV 2-4  Al/second Hydrogen gas target: 6 torr, 12 cm   35 ± 7  eV

25 Al(p,  ) 26 Si  Resonance Searches: 29 Si( 3 He, 6 He) 26 Si 26 Al( 3 He,t) 26 Si(p) 25 Al Direct Measurement: TRIUMF DRAGON E922 Yale TRIUMF E1O71 26g Al(p,  ) 27 Si  Direct Measurement: TRIUMF DRAGON E989 26m Al(p,  ) 27 Al  Resonance Search: 27 Al( 3 He,t) 27 Si(p) 26m Al Yale

27 Al( 3 He,t) 27 Si*(p) 26 Al

27 Al( 3 He,t) 27 Si*(p) 26 Al* Rachel Lewis (Yale, 2005)

27 Al( 3 He,t) 27 Si

Collaborations at TRIUMF E Al(p,  ) 26 DRAGON Alan Chen (McMaster) - P.I. E989 26g Al(p,  ) 27 DRAGON Chris Ruiz (Simon Fraser) - P.I. E Al implanted HRMS Catherine Deibel (Yale) - P.I.

Yale – Nuclear Astrophysics Group Faculty and Post Doc: Peter Parker Jason Clark Current Graduate Students: Anuj Parikh (5 th year) Catherine Deibel (4 th year) Christopher Wrede (3 rd year) Most Recent PhDs: Rachel Lewis (‘05), Univ.of York Dale Visser (’03), ORNL Alan Chen (’00), McMaster Dan Bardayan (’99 DNP ), Wigner ORNL Recent PostDocs: Will Univ.Western Ontario Jac TRIUMF- DRAGON