Kern(e) der Materie, Brennstoff der Sterne.... zum Schunck-Fest...
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1 Kern(e) der Materie, Brennstoff der Sterne... zum Schunck-Fest...
2
3 Entwicklung des Universums 15 Milliarden Jahre 3 K 1 Milliarde Jahre 20 K Jahre 3 Minuten Zeit Temperatur K 10 9 K 1 Tausendstel Sekunde K Entfernung
4 Atom Atomhülle Atomkern Elektron Proton Neutron
5 Proton Neutron
6
7
8
9 Die Landschaft der Atomkerne
10 QGP Hadrons QCD Vacuum
11 Transition from the perturbative to to the non-perturbative regime of of Quantum-Chromodynamics (QCD) perturbative: QCD: a S << 1 non-perturbative: QCD: a S 1 q q q Gluon (g) q Quarks, Gluons One-Gluon Exchange Hadrons: Baryons, Mesons Models, Lattice QCD
12 Probing for Quarks
13 QCD Glueballs... C.J. Morningstar and M. Peardon, PRD60 (1999)
14 QGP Hadrons QCD Vacuum Nucleon-Nucleon / Meson Systems
15
16 Properties of neutron stars
17 QGP Nuclei Hadrons QCD Vacuum Nucleon-Nucleon / Meson Systems
18 The Nuclear Landscape Nuclear Binding at the Superheavy Front Nuclear Binding at and near the Neutron Drip Line
19
20 Festschrift Taufe von Element 110
21 Struktur der schwersten Atome Superschwere Elemente und die Chemie von Hassium - Element 108 Proton/Atomic Number Neutron Number Relative Ausbeute [%] Temperatur [ C] DeteKtor(rel. Flüchtigkeit Kollaboration Bern, Berkeley, Dubna, GSI, Lanzhou, Mainz, Rossendorf, PSI Villingen
22 The Nuclear Landscape Nuclear Binding at the Superheavy Front Nuclear Binding at and near the Neutron Drip Line
23 Secondary Beams of Short-Lived Nuclei Fragment Separator Production Target
24 P. Armbruster et al.; Phys. Rev. Letters, Jan. 05 About 1000 nuclear residues identified 1GeV/u U + H A/Z-resolution ~10-3
25 A.V. Dobrovolsky et al., unpublished P.Egelhof, private communication
26 ??? tin isotopes Neutron number
27 Giant Resonances in Exotic Nuclei
28 Dipolstärken in neutronenreichen Zinnisotopen Electromagnetic-excitation cross section Photo-neutron cross section P. Adrich et al., Phys. Rev. Lett.
29 Nuclear Physics in the Universe... Accreting White Dwarf Chemical Elements in the Solar System Number Proton number of Protons Z Nova Cygni 1992 Neutron Star Sun Neutron Number number of Neutrons N
30 Electron-Beam Cooled Ion Beams electron collector electron collector electron gun high voltage platform electron gun magnetic field electron beam ion beam high voltage platform magnetic field electron beam ion beam G.I. Budker, At. En. 22 (1967) 346 G.I. Budker, A.N. Skrinsky et al., IEEE NS-22 (1975) 2093
31 The GSI Electron Cooler at the ESR Elektronenkollektor Elektronenkanone Hochspannungsplattform Magnetisches Feld Elektronenstrahl Ionenstrahl
32 Ion Beam Cooling... before cooling after cooling ion intensity relative ion velocity v/v 0
33 Schottky Frequency Spectrum
34 Nuclear Matter QGP Nuclei Hadrons QCD Vacuum Nucleon-Nucleon / Meson Systems
35 1?? neutron excess (N-Z)/A neutron halos & skins finite nuclei 78 Ni crust neutron stars neutron drip line supernovae heavy-ion collisions protron drip line Pethik & Ravenhall (1996) 45 Ni Local matter density
36 Quark Matter Hadrons QGP Hadrons QCD Vacuum Nuclear Matter Nuclei Nucleon-Nucleon / Meson Systems Deconfinement & chiral transition GSI SIS300 RHIC & LHC
37
38 SPS RHIC QGP T
39
40 Quark Matter Deconfinement & chiral transition Nuclear Matter RHIC & LHC Hadrons GSI SIS300 QGP SPS RHIC LHC Condensate Nuclei Hadrons QCD Vacuum Nucleon-Nucleon / Meson Systems
41 Quark Matter Deconfinement & chiral transition Nuclear Matter RHIC & LHC Hadrons GSI SIS300 QGP Nuclear Astrophysics SPS RHIC LHC Condensate Nuclei Hadrons QCD Vacuum Nucleon-Nucleon / Meson Systems
42 Quark Matter RHIC & LHC Deconfinement & chiral transition Hadrons GSI SIS300 QGP Nuclear Matter S y m m e t r i e s Nuclear Astrophysics SPS RHIC LHC Condensate Nuclei Hadrons QCD Vacuum Nucleon-Nucleon / Meson Systems
43 ISOL Roadmap EURISOL E U R I S O L EUROPE FAIR NORTH AMERICA J-Lab NORTH AMERICA JAPAN RIA HIRFL JPARK RIBF RCNP ISAC II ALICE / LHC RHIC CHINA BRIF SIAP
44 FAIR Facility for Antiproton and Ion Research Existing UNILAC SIS 18 SIS 100/300 Future Project HESR Super FRS CR Beams now: Z RESR = (protons to to uranium) up up to to GeV/nucleon m Some beam cooling NESR Beams in in the thefuture: Intensity: fold fold Species: Z = (anti-protons to to uranium) Energies: up up to to GeV/u Precision: full fullbeam cooling
45
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