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Exascale computing could soon enable a predictive theory of nuclear structure and reactions rooted in the Standard Model, with quantifiable and systematically improvable uncertainties.
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Nucleon axial, tensor, and scalar charges and σ \sigma -terms in lattice QCD,
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N. Kaiser, · 1910
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Λ Λ \Lambda\Lambda and N Ξ \Xi interactions from Lattice QCD near the physical point,
K. Sasaki, et al., · 1912
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N π N\pi states and the projection method for the nucleon axial and pseudoscalar form factors,
O. Bar, · 1912
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A N I C E R NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation,
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G. Raaijmakers, T. E. Riley, A. L. Watts, S. K. Greif, S. M. Morsink, K. Hebeler, A. Schwenk, T. Hinderer, S. Nissanke, S. Guillot, Z. Arzoumanian, S. Bogdanov, D. Chakrabarty, K. C. Gendreau, W. C. G. Ho, J. M. Lattimer, R. M. Ludlam, M. T. Wolff, · 1912
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Meson-Baryon Scattering Lengths from Mixed-Action Lattice QCD,
A. Torok, S. R. Beane, W. Detmold, T. C. Luu, K. Orginos, A. Parreno, M. J. Savage, A. Walker-Loud, · 1913
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The maximum mass and radius of neutron stars and the nuclear symmetry energy,
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J. Martin Camalich, L. S. Geng, M. J. Vicente Vacas, · 1929
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Perhaps a Stable Dihyperon,
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A New Algorithm for Adaptive Multidimensional Integration,
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