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1. dia

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Nothing tends so much to the advancement of knowledge as the ... GR studies with magnetic spectrographs. A split-pole magnetic spectrograph as a present ... – PowerPoint PPT presentation

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Title: 1. dia


1
GIANT RESONANCES, NEUTRON SKIN
  • Krasznahorkay, M. Csatlós, J. Gulyás, M. Hunyadi,
    Z. Máté,
  • B.M. Nyakó, D. Sohler, L. Zolnai
  • for the ATOMKI, KVI, RCNP, INFN collaboration

Nothing tends so much to the advancement of
knowledge as the application of a new instrument.
-- Sir Humphrey Davy
2
History of the collaboration
  • Postdoctoral position at KVI (AK, 1989,1990)
  • GR studies with magnetic spectrographs
  • A split-pole magnetic spectrograph as a present
  • NWO OTKA support
  • Study of HD states in Debrecen, collaboration
    also with LMU
  • Postdoc position at KVI (MH, 2000,2001)
  • NWO-OTKA (1994-2002, 49 publications)
  • 2002-2007 30 common publications.

3
Electric Giant Resonances
Isoscalar
Isovector
1977
1983
Monopole
Dipole
1948
1971
1980
Quadrupole
4
Experimental determination of the neutron-skin
thickness
neutrons protons
5
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6
The GDR method
?
?
?
Hatáskeresztmetszet számolások a GT és SJ modell
alapján
7
The experimental setup
8
Final state spectra
9
Final state spectra for the 208Pb(?, ??)
reaction
NaI det.
Clover det.
10
Determination of the neutron-skin thickness of
208Pb
GDR results 0.120.07 fm G.W. Hoffmann et al.,
Phys. Rev C21 (1980) 1488 0.140.04
fm Trzcinska et al., Phys. Rev. Lett. 87 (2001)
82501 0.150.03
11
Trzcinska et al., Phys. Rev. Lett. 87 (2001) 82501
12
Vibrations in the spin-isospin space Sum rule
for the SDR strength
A. Krasznahorkay et al., Phys. Rev. Lett. 82
(1999) 3216.
13
114-124Sn(3He,t) at E 400 MeVat RCNP, Osaka
14
(p,p) GDR SDR
A. Krasznahorkay et al., Phys. Rev. Lett. 82
(1999) 3216.
15
Experimental methods
BBS
E177 MeV ?3.2o
16
Differential cross sections
17
Our results obtained with the SDR method
18
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19
Isovector GRs in unstable nuclei
  • - The physics case
  • Macroscopic microscopic info
  • Neutron skin
  • SDR sum-rule
  • Ex(GTR)-Ex(IAS)
  • astrophysics e.g. ?-process
  • Experimental considerations ((p,n) in inverse
    kinematics)
  • High cross sections (10mb/sr)
  • Complete kinematics (use FRS)
  • low-En, no energy loss in target
  • Neutron detection
  • aim 1 MeV resolution in Ex
  • required ???10 ?En /En 10 flight path 1
    m, Timing resolution 1 ns

20
(p,n) in inverse kinematics p(132Sn,n) E400 AMeV
21
The ELENA setup
  • Type of the scintillator UPS-89 NE102A
  • Syze of the scintillator 10x45x1000 mm
  • PMTs XP2262 active dividers

22
Monte-Carlo simulations
23
Conclusions
  • GR studies in stable beams
  • GR studies in RIBs
  • Challenges for the detectors
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