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| Paper IPM / P / 7339 |
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We calculate the two-body relativistic boost interaction corrections as well as relativistic one-body and two-body kinetic energy corrections in cluster expansion of energy with AV18 and the new charge dependent Reid93 potentials within the lowest order constrained variational(LOCV) method. The equation of state of symmetric nuclear matter and pure neutron matter are calculated using the non-relativistic (HNR), non-relativistic plus boost interaction corrections (H*NR) and H*NR plus kinetic energy corrections (H*R) Hamiltonians. The relativistic boost interaction effects reduce the binding energies of symmetric nuclear matter for AV18 interaction by ∼ 3MeV.
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