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Kerstin Sonnabend, IKP, TU Darmstadt S-DALINAC - Nuclear Astrophysics Nuclear Astrophysics at the Darmstadt superconducting electron linear accelerator S-DALINAC N. Pietralla and K. Sonnabend for the SFB 634 Workshop on European Small-Scale Accelerator Facilities Aghios Nikolaos, Crete, Greece September 7 th to 8 th , 2007 supported by the DFG under grant No. SFB 634
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Kerstin Sonnabend, IKP, TU Darmstadt S-DALINAC - Nuclear Astrophysics Nuclear Astrophysics at the Darmstadt superconducting electron linear accelerator.

Mar 27, 2015

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Page 1: Kerstin Sonnabend, IKP, TU Darmstadt S-DALINAC - Nuclear Astrophysics Nuclear Astrophysics at the Darmstadt superconducting electron linear accelerator.

Kerstin Sonnabend, IKP, TU Darmstadt S-DALINAC - Nuclear Astrophysics

Nuclear Astrophysics at the Darmstadt superconducting electron linear accelerator

S-DALINAC

N. Pietralla and K. Sonnabendfor the SFB 634

Workshop on European Small-Scale Accelerator Facilities

Aghios Nikolaos, Crete, Greece

September 7th to 8th, 2007

supported by the DFG under grant No. SFB 634

Page 2: Kerstin Sonnabend, IKP, TU Darmstadt S-DALINAC - Nuclear Astrophysics Nuclear Astrophysics at the Darmstadt superconducting electron linear accelerator.

Kerstin Sonnabend, IKP, TU Darmstadt S-DALINAC - Nuclear Astrophysics

Accelerator hall of the S-DALINAC

– electron energies from 2 to 130 MeV available– cw and pulsed beam operation possible– source for polarized electron beams under construction

HIPS

Page 3: Kerstin Sonnabend, IKP, TU Darmstadt S-DALINAC - Nuclear Astrophysics Nuclear Astrophysics at the Darmstadt superconducting electron linear accelerator.

Kerstin Sonnabend, IKP, TU Darmstadt S-DALINAC - Nuclear Astrophysics

HIPS – High-intensity photon setup

photon energies up to 11 MeV available

electrons

Emax

0 ≤ E ≤ Emax

0 ≤ E ≤ Emax

n

Au/Re - target

n

11B - target

N ≈ 105 / (keV s cm2)

≈ 300 · N

collimator

radiator

Activation with continuous-energy bremsstrahlung

Page 4: Kerstin Sonnabend, IKP, TU Darmstadt S-DALINAC - Nuclear Astrophysics Nuclear Astrophysics at the Darmstadt superconducting electron linear accelerator.

Kerstin Sonnabend, IKP, TU Darmstadt S-DALINAC - Nuclear Astrophysics

LCS – Laboratory for counting and spectroscopy

– three low-energy photon spectrometers (LEPS)

– four 30% and 40% HPGe detectors

– setups with passive Cu and/or Pb shielding

Pb

Pb

Cu

Cu

LEPS LEPS

Pb Pb

Pb

HPGe

– complementation with x-ray detectors and electron counters

Determination of activation yield with -spectroscopy

Page 5: Kerstin Sonnabend, IKP, TU Darmstadt S-DALINAC - Nuclear Astrophysics Nuclear Astrophysics at the Darmstadt superconducting electron linear accelerator.

Kerstin Sonnabend, IKP, TU Darmstadt S-DALINAC - Nuclear Astrophysics

LCS – Laboratory for counting and spectroscopy

Sample decay spectra: LEPS versus HPGe

Page 6: Kerstin Sonnabend, IKP, TU Darmstadt S-DALINAC - Nuclear Astrophysics Nuclear Astrophysics at the Darmstadt superconducting electron linear accelerator.

Kerstin Sonnabend, IKP, TU Darmstadt S-DALINAC - Nuclear Astrophysics

NEPTUN – High-resolution photon tagger

High-resolution cross section measurements

detectorarray

Page 7: Kerstin Sonnabend, IKP, TU Darmstadt S-DALINAC - Nuclear Astrophysics Nuclear Astrophysics at the Darmstadt superconducting electron linear accelerator.

Kerstin Sonnabend, IKP, TU Darmstadt S-DALINAC - Nuclear Astrophysics

NEPTUN – High-resolution photon tagger

– 14 liquid scintillator neutron detectors

– 8 additional 10B enriched liquid scintillator detectors

– high-resolution cross section measurements

– determination of angular momentum of neutrons

– (,p) and (,) in preparation

Determine (,n) cross sections with 100 keV ≤ En ≤ 10 MeV

Page 8: Kerstin Sonnabend, IKP, TU Darmstadt S-DALINAC - Nuclear Astrophysics Nuclear Astrophysics at the Darmstadt superconducting electron linear accelerator.

Kerstin Sonnabend, IKP, TU Darmstadt S-DALINAC - Nuclear Astrophysics

QCLAM – Large-acceptance spectrometer

(e,e‘x) experiments of astrophysical interest

QCLAM

Page 9: Kerstin Sonnabend, IKP, TU Darmstadt S-DALINAC - Nuclear Astrophysics Nuclear Astrophysics at the Darmstadt superconducting electron linear accelerator.

Kerstin Sonnabend, IKP, TU Darmstadt S-DALINAC - Nuclear Astrophysics

QCLAM – Large-acceptance spectrometer

– clamshell dipole magnet (deflection angle: 120°)

– quadrupole magnet

– three multiwire drift chambers

– plastic scintillation and plexiglas Cherenkov counters

– momentum resolution: p/p = 2 10-4

– solid angle acceptance: 35 msr

– max. central momentum: 200 MeV/c

– momentum acceptance: ±10%

Page 10: Kerstin Sonnabend, IKP, TU Darmstadt S-DALINAC - Nuclear Astrophysics Nuclear Astrophysics at the Darmstadt superconducting electron linear accelerator.

Kerstin Sonnabend, IKP, TU Darmstadt S-DALINAC - Nuclear Astrophysics

QCLAM – Large-acceptance spectrometer

– momentum resolution: p/p = 2 10-4

– solid angle acceptance: 6.4 msr

– max. central momentum: 95 MeV/c

– momentum acceptance: -5% to +8%

Electron scattering at 180° deflection angle

Page 11: Kerstin Sonnabend, IKP, TU Darmstadt S-DALINAC - Nuclear Astrophysics Nuclear Astrophysics at the Darmstadt superconducting electron linear accelerator.

Kerstin Sonnabend, IKP, TU Darmstadt S-DALINAC - Nuclear Astrophysics

QCLAM – Large-acceptance spectrometer

Recent results on M1 deuteron break-up

– high energy resolution and high selectivity of M1 states

– precision test of modern theoretical models (potential model, EFT)

– prediction of p(n,)d cross section at Big Bang energies

Page 12: Kerstin Sonnabend, IKP, TU Darmstadt S-DALINAC - Nuclear Astrophysics Nuclear Astrophysics at the Darmstadt superconducting electron linear accelerator.

Kerstin Sonnabend, IKP, TU Darmstadt S-DALINAC - Nuclear Astrophysics

QCLAM – Large-acceptance spectrometer

Role of neutrino-induced reactions

properties of pre-collapse core supernova shock revivalexplosive nucleosynthesis

– branching ratios of 12C(e,e‘) electro-weak theory (,‘) cross sections

nucleosynthesis of 9Be and 10B

– high resolution (e,e‘) data M1 strength distribution GT0 from shell-model calc. -nucleus cross section

Shell-Modeltotal

Orbital

Spin

52CrS-DALINAC

excitation energy / MeV

K. Langanke et al., PRL 20 (2004) 202501

B(M

1) /

N

B(M

1) /

N

Page 13: Kerstin Sonnabend, IKP, TU Darmstadt S-DALINAC - Nuclear Astrophysics Nuclear Astrophysics at the Darmstadt superconducting electron linear accelerator.

Kerstin Sonnabend, IKP, TU Darmstadt S-DALINAC - Nuclear Astrophysics

Experimental hall of the S-DALINAC

QCLAM

NEPTUN

HIPS