First observation of bar Lambda p to K+ pi+ pi- pi0 and bar Lambda p to K+ pi+ pi- 2pi0 with cross sections 8.5 mb and 7.9 mb respectively.
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Relativistic mean-field calculations with asymmetric finite differences find that neutron-star inner-crust binding energies decrease with larger symmetry-energy slope L and larger nucleon effective mass, while quantum shell effects produce oscillatory densities and alter neutron properties.
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Observation of $\bar{\Lambda}p\to K^{+}\pi^{+}\pi^{-}\pi^{0}$ and $\bar{\Lambda}p\to K^{+}\pi^{+}\pi^{-}2\pi^{0}$
First observation of bar Lambda p to K+ pi+ pi- pi0 and bar Lambda p to K+ pi+ pi- 2pi0 with cross sections 8.5 mb and 7.9 mb respectively.
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Relativistic mean-field study of the neutron star inner crust using the asymmetric finite difference method
Relativistic mean-field calculations with asymmetric finite differences find that neutron-star inner-crust binding energies decrease with larger symmetry-energy slope L and larger nucleon effective mass, while quantum shell effects produce oscillatory densities and alter neutron properties.