14O Level Information - Experimental


** We would like to advise the reader that data provided in these Update Lists have not been evaluated by the TUNL Nuclear Data Evaluation Project. The reader should consult the original papers before using any values provided in the Update Lists.


1991DE25: P. Decrock, Th. Delbar, P. Duhamel, W. Galster, M. Huyse, P. Leleux, I. Licot, E. Lienard, P. Lipnik, M. Loiselet et al, Phys. Rev. Lett. 67 (1991) 808
Studied 13N(p, g)14O reaction, obtained partial g width of the 5.17 MeV state of 14O to be 3.8 ± 1.2 eV; compared result with other measurements.

1991MO20: T. Motobayashi, T. Takei, S. Kox, C. Perrin, F. Merchez, D. Rebreyend, K. Ieki, H. Murakami, Y. Ando, N. Iwasa et al, Phys. Lett. B264 (1991) 259
Studied reaction 13N(p, g)14O using Coulomb dissociation, obtained partial g width of the 5.17 MeV state of 14O to be 3.1 ± 0.6 eV; compared result with other measurements.

1991WI12: D.H. Wilkinson, Nucl. Phys. A527 (1991) 689C
Discusses superallowed b decay of eight nuclei, including 14O.

1992DE19: Th Delbar, W. Galster, P. Leleux, E. Lienard, P. Lipnik, C. Michotte, J. Vervier, P. Duhamel, J. Vanhorenbeeck, P. Decrock et al, Nucl. Phys. A542 (1992) 263
Studied 13N + p elastic scattering; obtained resonance energy 526.0 ± 1.0 keV and width 37.0 ± 1.1 keV for 1- state of 14O; the resonance energy differs from previous accepted value.

1993DE02: Th. Delbar, Phys. Rev. C47 (1993) R14
Discusses several measurements of the g partial width of the 5.17 MeV state of 14O; compares with theoretical result.

1993DE13: P. Decrock, Th. Delbar, W. Galster, M. Huyse, P. Leleux, I. Licot, E. Lienard, P. Lipnik, C. Michotte, P. Van Duppen et al, Phys. Lett. B304 (1993) 50
Studied 13N(p, g)14O reaction; obtained resonance energy, width, partial g width, spectroscopic factor for 13N(d, p)14O reaction, astrophysical S factor in 1- resonance region.

1993DE25: P. Decrock, M. Gaelens, M. Huyse, G. Reusen, G. Vancraeynest, P. Van Duppen, J. Wauters, Th. Delbar, W. Galster, P. Leleux et al, Phys. Rev. C48 (1993) 2057
Studied 13N(d, p)14O reaction; obtained spectroscopic factor and compared with previous results, also obtained astrophysical S factor.

1993DE34: Th. Delbar, W. Galster, P. Leleux, I. Licot, E. Lienard, P. Lipnik, M. Loiselet, C. Michotte, G. Ryckewaert, J. Vervier et al, Phys. Rev. C48 (1993) 3088
Used radioactive 13N beams to study 13N(p, g)14O reaction; obtained partial g width and compared with previous results, astrophysical S factor in 1- resonance region.

1993KI06: J. Kiener, A. Lefebvre, P. Aguer, C.O. Bacri, R. Bimbot, G. Bogaert, B. Borderie, F. Clapier, A. Coc, D. Disdier ET AL, Nucl. Phys. A552 (1993) 66
Studied 13N(p, g)14O reaction by Coulomb break-up of radioactive 14O beam; obtained radiative width of 5.17 MeV level in 14O to be 2.4 ± 0.9 eV; astrophysical aspects discussed.

1993SM04: M.S. Smith, P.V. Magnus, K.I. Hahn, R.M. Curley, P.D. Parker, T.F. Wang, K.E. Rehm, P.B. Fernandez, S.J. Sanders, A. Garcia et al, Phys. Rev. C47 (1993) 2740
Determined g decay width of 5.17 MeV state of 14O to be 12 ± 7 eV; calculated stellar reaction rate for 13N(p, g)14O.

1993WI21: D.H. Wilkinson, Nucl. Instrum. Meth. Phys. Res. A335 (1993) 172
Methodology for superallowed Fermi b decay, including 14O; Part I.

1993WI22: D.H. Wilkinson, Nucl. Instrum. Meth. Phys. Res. A335 (1993) 182
Methodology for superallowed Fermi b decay, including 14O; Part II.

1993WI23: D.H. Wilkinson, Nucl. Instrum. Meth. Phys. Res. A335 (1993) 201
Methodology for superallowed Fermi b decay, including 14O; Part III.

1994CA03: A.S. Carnoy, J. Deutsch and P. Quin, Nucl. Phys. A568 (1994) 265
Studied superallowed b decay, including 14O; set limits on possible scalar coupling.

1994MA14: P.V. Magnus, E.G. Adelberger and A. Garcia, Phys. Rev. C49 (1994) R1755
Obtained excitation energy, resonance energy and width of 5.17 MeV state of 14O to be 5156.8 ± 2.0 keV, 528.8 ± 2.0 keV, 37 ± 3 keV respectively; compared with previous results.

1994WI05: D.H. Wilkinson, Z. Phys. A348 (1994) 129
Analyzes superallowed Fermi b decay, including 14O; recommends values for coupling constants.

1995FO18: H.T. Fortune, Phys. Rev. C52 (1995) 2261
Studied energy differences between 1d5/2 and 2s1/2 states in light nuclei, including 14O.

1995WI17: D.H. Wilkinson, Nucl. Phys. A587 (1995) 421
Studied nuclear mismatch in superallowed Fermi b decay, including 14O.

1996BA29: C.R. Bain, P.J. Woods, R. Coszach, T. Davinson, P. Decrock, M. Gaelens, W. Galster, M. Huyse, R.J. Irvine, P. Leleux et al, Phys. Lett. B373 (1996) 35
Used radioactive 13N beam to study 7.77 MeV 2+ state of 14O; observed sequential emission of two protons with width of 125 ± 20 eV and set limit for 2He emission width to be less than 6 eV; compared with theory.

1996OZ01: A. Ozawa, I. Tanihata, T. Kobayashi, Y. Sugahara, O. Yamakawa, K. Omata, K. Sugimoto, D. Olson, W. Christie and H. Wieman, Nucl. Phys. A608 (1996) 63
Measured interaction cross section and matter radii of several light nuclei, including 14O; isospin dependence discussed.

1998BA83: P.H. Barker and P.A. Amundsen, Phys. Rev. C58 (1998) 2571
Revised Q value for the superallowed b decay of 14O.


Last modified: 18 November 2001