Pregled bibliografske jedinice broj: 15159
Implications of the space-star anomaly in nd breakup
Implications of the space-star anomaly in nd breakup // Nuclear physics. A, 631 (1998), C 692-C 696 doi:10.1016/S0375-9474(98)00093-1 (međunarodna recenzija, članak, znanstveni)
CROSBI ID: 15159 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
Naslov
Implications of the space-star anomaly in nd breakup
Autori
Howell, C.R. ; Setze, H.R. ; Tornowa, W. ; Braun, R.T. ; Gloeckle, W. ; Hussein, A.H. ; Lambert, J.M. ; Mertens, G. ; Roper, C.D. ; Salinas, F. ; Šlaus, Ivo ; Gonzalez Trotter, D.E. ; Vlahović, Branislav ; Walter, R.L. ; Witala, H.
Izvornik
Nuclear physics. A (0375-9474) 631
(1998);
C 692-C 696
Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni
Ključne riječi
3-nucleon
Sažetak
Cross-section measurements of six exit-channel configurations in nd breakup at 13.0 MeV are reported and compared to rigorous calculations. Except for the coplant-star configuration, our data are consistent with previous data. The present data for all configurations, with the exception of the space star, are in good agreement with theoretical predictions. The previously observed large discrepancy between theory and data for the space-star configuration is confirmed in the present work. The inclusion of the Tucson-Melbourne 2pi exchange three-nucleon force with a cutoff parameter that correctly binds the triton only changes the predicted cross section by 2percent, a factor of 10 smaller than the amount needed to bring theory into agreement with data.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
POVEZANOST RADA
Ustanove:
Institut "Ruđer Bošković", Zagreb
