J. Hinnefeld
Indiana University
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Featured researches published by J. Hinnefeld.
Nuclear Physics | 2013
S. Mosby; M. Gardner; G. Christian; J. Hinnefeld; J. Brown; Graham F. Peaslee; D. Bazin; M.J. Strongman; E.A. Hook; M. Thoennessen; Paul DeYoung; E. Lunderberg; D.A. Meyer; J. E. Finck; T. Baumann; J. K. Smith; A. Spyrou; B. Luther; M. Bennett; N.S. Badger; Warren F. Rogers; M. Mosby; J. Snyder
A search for the neutron-unbound nucleus
Journal of Physics G | 1998
A. N. Ostrowski; Alan C. Shotter; W. Bradfield-Smith; A.M. Laird; A. Di Pietro; Thomas Davinson; S. Morrow; Philip Woods; S. Cherubini; W. Galster; J.S. Graulich; P. Leleux; Laurent D. Michel; A. Ninane; Jean Vervier; M. Aliotta; C. Cali; F. Cappuzzello; A. Cunsolo; C. Spitalieri; J. Görres; M. Wiescher; J. Rahighi; J. Hinnefeld
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Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 1999
W. Bradfield-Smith; Thomas Davinson; A. DiPietro; A.M. Laird; A. N. Ostrowski; Alan C. Shotter; Philip Woods; S. Cherubini; W. Galster; J.S. Graulich; P. Leleux; Luc Michel; A. Ninane; Jean Vervier; J. Görres; M. Wiescher; J. Rahighi; J. Hinnefeld
C was performed via the single proton removal reaction from a beam of 22 N at 68 MeV/u. Neutrons were detected with the Modular Neutron Array (MoNA) in coincidence with
Nuclear Physics | 2001
S. Cherubini; W. Galster; J.S. Graulich; P. Leleux; Marc Loiselet; A. Musumarra; A. Ninane; G. Ryckewaert; Jean Vervier; M. Aliotta; P. Figuera; M. Lattuada; M. G. Pellegriti; C. Spitaleri; T. Davinson; A. Di Pietro; A. M. Laird; A. N. Ostrowski; A.C. Shotter; P. J. Woods; J. Hinnefeld; S. Typel; H.H. Wolter
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Physical Review C | 2013
Z. Kohley; E. Lunderberg; P. A. DeYoung; Alexander Volya; T. Baumann; D. Bazin; G. Christian; N. L. Cooper; N. Frank; A. Gade; C. Hall; J. Hinnefeld; B. Luther; S. Mosby; W. A. Peters; J. K. Smith; J. Snyder; A. Spyrou; M. Thoennessen
C fragments. No evidence for a low-lying state was found, and the reconstructed
Physical Review C | 2013
Z. Kohley; E. Lunderberg; P. A. DeYoung; Alexander Volya; T. Baumann; D. Bazin; G. Christian; N. L. Cooper; N. Frank; A. Gade; C. Hall; J. Hinnefeld; B. Luther; S. Mosby; W. A. Peters; J. K. Smith; J. Snyder; A. Spyrou; M. Thoennessen
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Physical Review C | 2011
D. Albertson; B. Luther; J. Bailey; M. Kasperczyk; A. Smith; T. Baumann; D. Bazin; A. Schiller; B. A. Brown; A. Gade; W. A. Peters; J. Brown; P. A. DeYoung; J. E. Finck; J. Hinnefeld; R. Howes; J. A. Tostevin
C+n decay energy spectrum could be described with an s-wave line shape with a scattering length limit of |as| < 2.8 fm, consistent with shell model predictions. A comparison with a renormalized zero-range three-body model suggests that
Physical Review C | 2010
C. Hall; E. Lunderberg; P. A. DeYoung; Deborah H. Denby; T. Baumann; D. Bazin; G. Blanchon; Angela Bonaccorso; B. A. Brown; G. Christian; N. Frank; A. Gade; S. Mosby; W. A. Peters; A. Spyrou; J. Brown; J. E. Finck; J. Hinnefeld
^{22}
arXiv: Nuclear Experiment | 2008
N. Frank; T. Baumann; D. Bazin; A. Gade; J.-L. Lecouey; W. A. Peters; Heiko Scheit; A. Schiller; M. Theonnessen; J. Brown; Paul DeYoung; J. E. Finck; J. Hinnefeld; R. Howes; B. Luther
C is bound by less than 70 keV.
Physical Review C | 2007
J. J. Kolata; H. Amro; F. D. Becchetti; J. Brown; P. A. DeYoung; Michael Hencheck; J. Hinnefeld; Graham F. Peaslee; A. L. Fritsch; C. Hall; U. Khadka; Patrick J. Mears; P. O'Rourke; D. Padilla; J. Rieth; Tabatha Spencer; T Williams
Low-energy post-accelerated radioactive ion beams have been used to study nuclear reactions addressing important nuclear structure and nuclear astrophysics questions. A high-granularity, large-solid-angle silicon strip detector array has been used to account for the low reaction products yields. First experiments using a He-6 beam on thin C-12 targets show the feasibility of direct reaction studies with good angular resolution and a detection limit in access of 0.1 mb sr(-1) cross sections. The measurement of the six alpha-decay channel in a N-13-induced reaction on a B-11 target shows the capabilities of this experimental technique even for sophisticated reaction studies. The study of stellar properties in ground-based experiments, in particular break-out reactions from the hot-CNO, i.e. O-15(alpha, gamma) Ne-19, can be pursued using these beams. Experiments are being performed to study these reactions by measurement of d(Ne-18, p) Ne-19*(alpha)O-15 and alpha(Ne-18, p), which might provide an alternative breakout route.