Ab initio elastic scattering from light nuclei based on different chiral two-nucleon forces
ORAL
Abstract
Effective interactions (`optical potentials') derived from first principles to describe the elastic
scattering of nucleons from nuclei can be formulated consistently within the spectator expansion of
multiple scattering theory. In its leading order, the NN force enters into the description of the nucleus
as nonlocal one-body density obtained from NCSM structure calculations as well as in the reaction itself
by folding the NN amplitudes with the one-body densities. For consistency, the spin of the struck nucleon
must be taken into account on the same footing as the spin of the projectile nucleon.
In this contribution, we study nucleon-nucleus observables for proton (neutron) elastic scattering and their energy dependence
between 60 and 160 MeV projectile energy based on 3 different chiral NN interactions.
We will look at the effective potentials specifically for cases where the underlying interactions
differ more than the truncation errors of one of the underlying chiral NN interactions would suggest. Our
studies concentrate on elastic NA observables for 12C and 16O.
scattering of nucleons from nuclei can be formulated consistently within the spectator expansion of
multiple scattering theory. In its leading order, the NN force enters into the description of the nucleus
as nonlocal one-body density obtained from NCSM structure calculations as well as in the reaction itself
by folding the NN amplitudes with the one-body densities. For consistency, the spin of the struck nucleon
must be taken into account on the same footing as the spin of the projectile nucleon.
In this contribution, we study nucleon-nucleus observables for proton (neutron) elastic scattering and their energy dependence
between 60 and 160 MeV projectile energy based on 3 different chiral NN interactions.
We will look at the effective potentials specifically for cases where the underlying interactions
differ more than the truncation errors of one of the underlying chiral NN interactions would suggest. Our
studies concentrate on elastic NA observables for 12C and 16O.
*Supported in part by US DoE DE-FG02-93ER40756, DE-SC0018223, and resources underDE-AC02-05CH11231.
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Presenters
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Charlotte Elster
- Ohio University