Preparation for 44Ti(α ,p)47V experiment

at CERN ISOLDE

 
List of participants / interested 
    Alex Murphy (PI), Marialuisa Aliotta, Tom Davinson, Phil Woods (Edinburgh)
    Beyhan Bastin, Olivier Sorlin, François de Oliveira, Pierre Delahaye, 
        Emil Traykov , M.G. Saint Laurent, Thomas Rogers (GANIL)
    Dorothea Schumann, Ayranov Marin, Rugard Dressler, Maruta Bunka  (PSI)
    Nicolas de Sereville (Orsay)
    G H-T Wang (Aberdeen)
    D. Bemmerer (HZDR)
    J. Fallis, C. Ruiz (TRIUMF)
    Thierry Stora, Fredrik John Carl Wenander , Didier Voulot, Alexandre Dorsiva, Richard         
        Catherall, Peter Butler (Liverpool), Magdalena Kowalska, Thomas Elias Cocolios (CERN)
    Piet Van Duppen (KU Leuven)
    Alison Laird (York)

Relevant papers
    D. Hartmann et al. NPA 621(1997) 83-91
        On Flamsteeds Supernova Cas-A
    L.S. The, D. D. Clayton and L. Jin & B.S. Meyer  Astrophys J 504 (1998)
        Nuclear Reactions Governing the Nucleosynthesis of 44Ti
    Sonzogni et al. Phys.Rev.Lett. 84, 1651 (2000)
        The 44Ti(a,p) Reaction and its Implication on the 44Ti Yield in Supernovae sonzogni.pdf
    M. Horoi, et al. PRC 66 (2002) 015801
        45V(p,γ) thermonuclear reaction rate relevant to 44Ti production in core-collapse     
        supernovae: General estimates and shell model analysis
    L.S. The et al. Astronomy & Astrophysics A&A 450 (2006) 1037-1050
        Are 44Ti -Producing Supernovae Exceptional?  
    C.D. Ott et al. Physical Review Letters 96 (2006) 201102
        A New Mechanism for Gravitational-Wave Emission in Core-Collapse Supernovae
    J.J. He & A.StJ. Murphy PRC 75 (2007) 068801
        A Revised 45V(p,g)46Cr astrophysical reaction rate
    C. Vockenhuber et al. Phys.Rev. C 76, 035801 (2007)
        Measurement of the 40Ca(α, γ)44Ti reaction relevant for supernova nucleosynthesis
    C. Vockenhuber et al. J. Phys. G: Nucl. Part. Phys. (2008) 35 014034
        40Ca(α,γ)44Ti and the production of 44Ti in supernovae
    C. Tur, A. Heger. S. Austin, PoS, NIC XI (2010) Heidelberg
         Production of 26Al, 44Ti and 60Fe in Supernovae-sensitivity to the helium burning rates
    G. Magkotsios et al. Astrophys.J.Suppl.Ser. 191 (2010) 66
        Trends in 44Ti and 56Ni from Core-Collapse Supernovae Magkotsios.pdf
    G. Magkotsios F.X. Timmes and M. Wiescher ApJ 741 (2011) 78
        Freeze-out yields of radioactivities in core-collapse supernovae
    C. H-T Wang CERN Courier Nov 2011
        Scalar field could unlock supernova mystery
    C. H-T Wang Physics Letters B 705 (2011) 148
        Parametric instability induced scalar gravitational waves from a model pulsating neutron star
    A.C. Larsen et al. PRC 85 014320 (2012)
        Primary g-ray spectra in 44Ti of astrophysical interest


   
Proposals and LoIs
    2005-06-03 TRIUMF LOI loi.pdf
    2007-04-22 INTC ISOLDE LOI LoI-Murphy.pdf 
    2010-02-23 SPIRAL LoI Letter of Intent to SPIRAL.pdf
    2010-06-28 TRIUMF Proposal S1289_201007S_merged.pdf
    2012-01-06 CERN INTC 44tI prop2.pdf

Talks, Presentations & Reports
    10-2005 Experimental nuclear astrophysics relevant to supernovae 
            supernovae.ppt
    First ERAWAST Workshop, PSI talk.ppt 
    GANIL LoI PAC PAC-MurphyLOI-lite.pdf
    2005-07-08: Presentation of LOI to TRIUMF EEC: EEC-LI-XXXXI.ppt
    Nuclear Physics News meeting report npn-erawast-pub.pdf 
    Jennifer Fallis Erawast 2011 JennFallisERAWAST2011.ppt
    CERN Invited talk talk.pdf
    CERN INTC presentation The case for 44Ti.pdf

Useful images
    Survivor companion to SN1572:
       Website: http://hubblesite.org/newscenter/archive/releases/star/2004/34/results/100/
        Artists impression: sn1572.jpg 
    Chandra image of Tycho chandra.jpg

Proposed Set Up (as of 09-12-2011)
    setup.png
    

Calculations and Simulations




http://www.sciencedirect.com/science/article/pii/S0375947497002170http://iopscience.iop.org/0004-637X/504/1/500/44Ti_files/sonzogni.pdfhttp://prc.aps.org/abstract/PRC/v66/i1/e015801http://prc.aps.org/abstract/PRC/v66/i1/e015801http://www.aanda.org/index.php?option=com_article&access=doi&doi=10.1051/0004-6361:20054626&Itemid=129http://www.aanda.org/index.php?option=com_article&access=doi&doi=10.1051/0004-6361:20054626&Itemid=129http://prc.aps.org/pdf/PRC/v75/i6/e068801http://prc.aps.org/abstract/PRC/v76/i3/e035801http://iopscience.iop.org/0954-3899/35/1/014034/http://iopscience.iop.org/0954-3899/35/1/014034/http://pos.sissa.it/archive/conferences/100/046/NIC%20XI_046.pdf44Ti_files/Magkotsios.pdfhttp://iopscience.iop.org/0004-637X/741/2/78/http://cerncourier.com/cws/article/cern/47821http://www.sciencedirect.com/science/article/pii/S0370269311012111http://prc.aps.org/pdf/PRC/v85/i1/e01432044Ti_files/loi.pdf44Ti_files/LoI-Murphy.pdf44Ti_files/Letter%20of%20Intent%20to%20SPIRAL.pdf44Ti_files/S1289_201007S_merged.pdf44Ti_files/44tI%20prop2.pdf44Ti_files/supernovae.ppt44Ti_files/talk.ppt44Ti_files/PAC-MurphyLOI-lite.pdf44Ti_files/EEC-LI-XXXXI.ppt44Ti_files/npn-erawast-pub.pdf44Ti_files/JennFallisERAWAST2011.ppt44Ti_files/talk.pdf44Ti_files/The%20case%20for%2044Ti.pdfhttp://hubblesite.org/newscenter/archive/releases/star/2004/34/results/100/44Ti_files/607579main_hubble_supernova1200_946-710.jpg44Ti_files/chandra.jpg44Ti_files/setup.pnghttp://prl.aps.org/pdf/PRL/v96/i20/e201102shapeimage_1_link_0shapeimage_1_link_1shapeimage_1_link_2shapeimage_1_link_3shapeimage_1_link_4shapeimage_1_link_5shapeimage_1_link_6shapeimage_1_link_7shapeimage_1_link_8shapeimage_1_link_9shapeimage_1_link_10shapeimage_1_link_11shapeimage_1_link_12shapeimage_1_link_13shapeimage_1_link_14shapeimage_1_link_15shapeimage_1_link_16shapeimage_1_link_17shapeimage_1_link_18shapeimage_1_link_19shapeimage_1_link_20shapeimage_1_link_21shapeimage_1_link_22shapeimage_1_link_23shapeimage_1_link_24shapeimage_1_link_25shapeimage_1_link_26shapeimage_1_link_27shapeimage_1_link_28shapeimage_1_link_29shapeimage_1_link_30shapeimage_1_link_31shapeimage_1_link_32shapeimage_1_link_33