Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aps..apro10006g&link_type=abstract
American Physical Society, April Meeting, Jointly Sponsored with the High Energy Astrophysics Division (HEAD) of the American As
Astronomy and Astrophysics
Astrophysics
Scientific paper
The measurements of ground state g factors using projectile fragmentation and beta-NMR have been hampered by the fact that the induced fragment spin polarization cannot be accurately predicted. A systematic behavior in the spin polarization as a function of target, beam energy and incident beam angle has previously been demonstrated. A Monte Carlo code developed to predict the induced fragment spin polarization from projectile fragmentation reactions reproduces the gross features of the spin polarization as a function of fragment momentum. We have made improvements to this model to correctly account for the observed absence of spin polarization when the incident beam angle is 0°. We are currently working to include this polarization model in an intermediate-energy fragmentation code similar to that done for high-energy fragmentation. This work has been supported in part by the National Science Foundation under Contract No. PHY-9528844.
Groh Daniel
Mantica Paul
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