Physics with Exotic Nuclei

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1 Physics with Exotic Nuclei Hans-Jürgen Wollersheim NUclear STructure, Astrophysics and Reaction

2 Outline Projectile Fragmentation A Route to Exotic Nuclei Fragmentation Cross Sections Nuclear Reaction Rates In-Flight Separation of Radioactive Ion Beams FRagment Separator at GSI Comparison FRS Super-FRS Identification of RIBs Excited Fragments Gateway to Nuclear Structure Scattering Experiments with RIBs projectile projectile fragment target nucleus abrasion ablation

3 The Why and How of Radioactive-Beam Research

4 The Why and How of Radioactive-Beam Research Atomic nuclei are quantum systems with a finite number of strongly interacting fermions: protons and neutrons. Light nuclei up to A=12 are described by bare nucleon-nucleon interaction. In heavier nuclei the interactions between the nucleons are modified by the medium effective interactions are needed. range of nuclear force from Due to constant density, potential energy felt by is also constant Mean potential (effect from other nucleons) distance from the center of the nucleus How can collective phenomena be explained from individual motion?

5 The Nuclear Chart Our Road Map from Stable to Exotic Nuclei 126 doubly magic nuclei: 4 He, 16 O, 40 Ca, 48 Ca, 208 Pb protons instable: 48 Ni, 56 Ni, 78 Ni, 100 Sn, 132 Sn neutrons no 28 O!

6 Nuclear radii textbooks says: R=1.2 A 1/3 11 Li 208 Pb Prog. Part. Nucl. Phys. 59 (2007), 432

7 Nuclear shell structure Experimental evidence of magic numbers N=20 N=28 Z=20 40 Ca 42 Ca 44 Ca 46 Ca 48 Ca spherical Z=18 38 Ar 46 Ar Ca Z=16 36 S 44 S S Z=14 34 Si 42 Si Si deformed Z=12 32 Mg 40 Mg Z=10 30 Ne 38 Ne Indicators for nuclear shell model: high energies of state for nuclei with magic numbers

8 Solar abundances of elements Solar abundance (Si 28 = 10 6 ) Big Bang fusion reactions neutron reactions open questions: Why is Fe more common than Au? Why do the heavy elements exist and how are they produced? Can we explain the solar abundances of the elements? Mass number

9 The chart of nuclides

10 Spallation & Projectile Fragmentation Reactions A Route to Exotic Nuclei Spallation Fragmentation ISOL = Isotope Separator On Line

11 High-energy proton-induced nuclear reactions Some early high-energy proton accelerators: Facility Energy from year Bevatron (Berkeley) 6 GeV AGS (Brookhaven) 11 GeV Fermilab (Chicago) >300 GeV They were also used to bombard various stable target materials. These targets were analyzed with radiochemical methods, i.e. γ-spectroscopy with or without chemical separators Production cross sections and (some) kinematics for suitable radioactive isotopes

12 High-energy proton-induced nuclear reactions Important findings: Energy-independence of cross sections Bell-shaped Z-distribution for constant A E p [GeV] σ [mb] σ [mb] p+au Mass yields: exponential slope A

13 Proton- versus heavy-ion induced reactions Proton- and heavy-ion induced reactions give very similar isotope distribution: Na Target fragmentation: GeV p + A target A 8 GeV 48 Ca+Be Projectile fragmentation: GeV/u A proj + p A are equivalent 28 GeV p U

14 Projectile fragmentation reactions projectile projectile fragment target nucleus abrasion ablation At GeV energies nucleons can be regarded as a classical particles Nucleon-nucleon collisions can be treated classically using measured free nucleon-nucleon cross sections (intra-nuclear cascade). In these collisions very little transfer momentum is exchanged. After the cascade the residual nucleus is highly excited. Heavy-ion projectiles can be treated as a bag of individual nucleons. Physical models: Two-step approach Step 1: Intranuclear-cascade models or Abrasion models Step 2: Evaporation calculation

parameterization of fragmentation cross section: EPAX v.3 K.

15 Projectile fragmentation reactions projectile projectile fragment target nucleus abrasion ablation Empirical parameterization of fragmentation cross section: EPAX v.3 K. Sümmerer, Phys. Rev. C86 (2012)

16 The Accelerator Facility at GSI Experimental Areas Ion Sources all elements: p U Fragment Separator ESR FRS Linear-Accelerator 20% speed of light (20 AMeV) SIS Synchrotron SIS-18 90% speed of light (2 AGeV)

17 UNILAC Accelerator

18 The Accelerator Facility at GSI Experimental Areas Ion Sources all elements: p U Fragment Separator ESR FRS Linear-Accelerator 20% speed of light (20 AMeV) SIS Synchrotron SIS-18 90% speed of light (2 AGeV)

20 Where do we do the experiments?

21 Projectile fragmentation reactions Projectile Fragmentation Projectile Target Projectile Fragment Projectile Projectile Fission Target Projectile Fragments

Nuclear Reaction Rate nuclear reaction rate [s -1 ] = luminosity [atoms cm -2 s -1 ] * σ f [cm 2 ] abrasion ablation σ f [cm 2 ] for projectile fragmentation + fission luminosity [atoms cm -2 s -1 ]

22 Nuclear Reaction Rate nuclear reaction rate [s -1 ] = luminosity [atoms cm -2 s -1 ] * σ f [cm 2 ] abrasion ablation σ f [cm 2 ] for projectile fragmentation + fission luminosity [atoms cm -2 s -1 ] = projectiles [s -1 ] * target nuclei [cm -2 ] Ion SIS-18 (2008) SIS-100 (expected) 20 Ne Ne Ar Ar Ni Ni Kr Kr Xe Xe eeeeeeeeeeeeeeeeeeee 70% experiment 197 Au Au U U U U

23 Nuclear Reaction Rate 2 1 x Primary reaction rate: φ f [ s ] φ p[ s ] [ g / cm ] A t [ g] 23 σ f 2 [ cm ] (thin target) density ρ Example: 238 U (10 9 s -1 ) on 208 Pb (x=1g/cm 2 ) 132 Sn (σ f =15.4mb) reaction rate: [s -1 ] Example: 124 Xe (10 9 s -1 ) on 9 Be (x=1g/cm 2 ) 104 Sn (σ f =5.6μb) reaction rate: 375 [s -1 ] The optimum thickness of the production target is limited by the loss of fragments due to secondary reactions 1 Primary + secondary reaction rate: φ [ s ] = φ [ s ] 1,6 1,4 1,2 1 0,8 0,6 0,4 0, µ p x[ g / cm ] µ f x[ g / cm ] ( e e ) 2 µ µ f p max x [g/cm 2 ] f with σ 1 f p A µ = σ A 2 [ g] t [ g] reaction 2 [ cm ] 2 [ cm ] µ f 1 2 µ p x[ g / cm ] µ f x[ g / cm ] ( e e ) 2 µ Example: Xe on Be Sn, σ ( Xe+ Be) = 3.65[ b] µ p = 0.244[ cm / g] σ ( Sn+ Be) = 3.44[ b] µ = 0.230[ cm / g] φφ ff ss 1 = φφ pp ss 1 φφ ss 1 = φφ pp ss 1 1 ee NN tt cccc 2 σσ ff cccc 2 (thick target) p f

24 In-Flight Separation of Radioactive Ion Beams Primary (production) target Peripheral nuclear reactions Forward focused products Secondary (reaction) target Experimental area Electromagnetic separator Stable HI projectile source E ~ 1000 AMeV Selected radioactive beam E >> 20 AMeV

25 Fragmentation at Relativistic Energies projectile projectile fragment target nucleus abrasion ablation FRS FRS FRagment Separator

26 Radioactive Ion Beams at GSI 1GeV/u U + H About 1000 nuclear residues identified A/Z-resolution ~10-3

27 FRagment Separator at GSI 131 Sn 132 Sn in-flight A and Z selection energy resolution: ~ 1 GeV

28 Rare Isotope Selection at FRS: Bρ-ΔE-Bρ Selection primary beam 86 Kr ~700 AMeV fully striped fragments 20m secondary beam 78 Ni ~ 100 AMeV production target 9 Be

29 Rare Isotope Selection at FRS: Bρ-ΔE-Bρ Selection primary beam 86 Kr ~700 AMeV Transmission : % for fragmentation < 2 % for fission 20m secondary beam 78 Ni ~ 100 AMeV production target 9 Be magnetic dipoles Βρ βγ Α/Ζ degrader Ε Ζ 2 f(β) magnetic dipoles Βρ βγ Α/Ζ

30 Production, Separation, Identification SIS FRS abrasion ablation fragment FRagment Separator 56 Cr, 100MeV/u 86 Kr, 480MeV/u Standard FRS detectors TPC-x,y S2,S4 Plastic scintillator S4 MUSIC S4

31 Das Bild kann zurzeit nicht angezeigt werden. Production, Separation, Identification multiwire chamber or TPC; beam position 56 Cr, 100MeV/u 86 Kr, 480MeV/u MUSIC scintillator scintillator β ionization chamber; Z 56 Cr Y Z X A/Q

32 Production, Separation, Identification SIS FRS abrasion ablation fragment FRagment Separator

33 Comparison of FRS with Super-FRS FRS Super-FRS 150m

The Super-FRS Project at GSI

2 m A G A T A The Super-FRS Project at GSI FRS facility The concept of the new facility The Super-FRS and its branches Summary Martin Winkler for the Super-FRS working group CERN, 3.1.22 Energy Buncher