Neutron rich nuclei in a new binding energy formula and the astrophysical $r-$process

Chirashree Lahiri; G. Gangopadhyay

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Neutron rich nuclei in a new binding energy formula and the astrophysical $r-$process

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arxiv 1207.2937 v1 pith:7LWDDGRW submitted 2012-07-12 nucl-th

Chirashree Lahiri , G. Gangopadhyay This is my paper · ORCID

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keywords massformulaneutrondifferentformulasfoundnucleir-process

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Neutron rich nuclei has been studied with a new phenomenological mass formula. Predictions of different mass formulas for the location of the neutron dripline are compared with those from the present calculation. The implications of the new mass formula for r-process nucleosynthesis are discussed. It is found that though the neutron drip line obtained from this formula differs substantially from other formulas, the r-process abundance upto mass 200 are unlikely to be significantly different. The errors inherent in the mass formula are found to play an insignificant role beyond mass A = 80.

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