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Dive into the research topics where C. Hutter is active.

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Featured researches published by C. Hutter.


Physics Letters B | 2000

Experimental simulation of a stellar photon bath by bremsstrahlung: the astrophysical gamma-process

Peter Mohr; Karsten Vogt; Mario Babilon; J. Enders; T. Hartmann; C. Hutter; T. Rauscher; S. Volz; A. Zilges

The nucleosynthesis of heavy proton-rich nuclei in a stellar photon bath at temperatures of the astrophysical


Physical Review C | 2001

Measurement of the (y,n) reaction rates of the nuclides 190Pt, 192Pt, and 198Pt in the astrophysical y process

Karsten Vogt; P. Mohr; Mario Babilon; J. Enders; T. Hartmann; C. Hutter; T. Rauscher; S. Volz; A. Zilges

\gamma


Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 2002

Polarization sensitivity of a segmented HPGe detector up to 10 MeV

C. Hutter; Mario Babilon; W. Bayer; D. Galaviz; T. Hartmann; Peter Mohr; S. Müller; W. Rochow; D. Savran; K. Sonnabend; Karsten Vogt; S. Volz; A. Zilges

-process was investigated where the photon bath was simulated by the superposition of bremsstrahlung spectra with different endpoint energies. The method was applied to derive (


Nuclear Physics | 2001

(γ,n) reactions in a quasi-thermal photon bath

Peter Mohr; Mario Babilon; J. Enders; T. Hartmann; C. Hutter; Karsten Vogt; S. Volz; A. Zilges

\gamma


European Physical Journal A | 2000

Half-lives of platinum isotopes from photoactivation

Peter Mohr; C. Hutter; Karsten Vogt; J. Enders; T. Hartmann; S. Volz; A. Zilges

,n) cross sections and reaction rates for several platinum isotopes.The nucleosynthesis of heavy proton-rich nuclei in a stellar photon bath at temperatures of the astrophysical gamma-process was investigated where the photon bath was simulated by the superposition of bremsstrahlung spectra with different endpoint energies. The method was applied to derive (gamma,n) cross sections and reaction rates for several platinum isotopes


Nuclear Physics | 2001

Nuclear structure and nuclear astrophysics at a 10 MeV bremsstrahlung facility

Mario Babilon; W. Bayer; K. Denefleh; J. Enders; D. Galaviz; T. Hartmann; C. Hutter; P. Mohr; Karsten Vogt; S. Volz; A. Zilges

The nucleosynthesis of heavy neutron-deficient nuclei in a stellar photon bath at the temperatures relevant for the astrophysical gamma process was investigated. In order to derive (gamma,n) cross sections and reaction rates, the stellar photon bath was simulated by the superposition of several bremsstrahlung spectra with different endpoint energies. As a first test for this method, the (gamma,n) reaction rates of the platinum isotopes 190Pt, 192Pt, and 198Pt were derived. The results are compared to other experimental data and theoretical calculations.


Archive | 2001

Measurement of the (gamma,n) reaction rates of the nuclides Pt-190, Pt-192, and Pt-198 in the astrophysical gamma process

Karsten Vogt; Peter Mohr; Mario Babilon; J. Enders; T. Hartmann; C. Hutter; T. Rauscher; S. Volz; A. Zilges

Abstract Linear γ-ray polarization can be measured using segmented germanium detectors. The polarization sensitivity of the Compton scattering process leads to asymmetries in the signals of a segmented detector. We have measured the polarization sensitivity of a four-fold segmented large volume germanium detector up to photon energies of approximately 10 MeV for the first time. The detector and its performance are compared to smaller Compton polarimeters which have been analyzed in previous work. A possible application of the described Compton polarimeter will be parity assignments in photon scattering experiments.


Archive | 2003

Zerfallstruktur von Niedrigspinzuständen unterhalb von 8 MeV in 140 Ce

T. Hartmann; Mario Babilon; M. A. Caprio; R. F. Casten; A. Hamamoto; A. A. Hecht; C. Hutter; Peter Mohr; S. Müller; Jennifer J. Ressler; Victor Zamfir; A. Zilges


Proceedings of the International Symposium | 2002

PHOTOREACTIONS IN NUCLEAR ASTROPHYSICS

Peter Mohr; Mario Babilon; W. Bayer; D. Galaviz; T. Hartmann; C. Hutter; K. Sonnabend; Karsten Vogt; S. Volz; A. Zilges


Physical Review C | 2002

Resonance strengths for the reaction 28 Si (alpha, gamma) 32 S at low energies

Mario Babilon; Wolfgang Bayer; Daniel Galaviz Redondo; T. Hartmann; C. Hutter; Peter Mohr; W. Rochow; K. Sonnabend; Karsten Vogt; S. Volz; A. Zilges

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T. Hartmann

Technische Universität Darmstadt

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A. Zilges

University of Cologne

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Karsten Vogt

Technische Universität Darmstadt

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Mario Babilon

Technische Universität Darmstadt

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Peter Mohr

Technische Universität Darmstadt

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S. Volz

Technische Universität Darmstadt

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J. Enders

Technische Universität Darmstadt

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D. Galaviz

Technische Universität Darmstadt

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K. Sonnabend

Technische Universität Darmstadt

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W. Rochow

University of Tübingen

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