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Rev. C 81 (2010) 021301(R). [21] A. , Gamow-Teller Strengths in the A = 14 Multiplet: A Challenge to the Shell Model, Phys. Rev. Lett. 97, 062502 (2006). [22] S. Quaglioni and P. Navrátil, Phys. Rev. Lett. 101, 092501 (2008). [23] S. Quaglioni and P. Navrátil, Phys. Rev.

2001). Quantum field theories without infinities, Ann. , 292, 139. Weinberg, S. (1995). 1. Wentzel, G. (1949). Quantum Theory of Fields, Interscience, New York. 0 2 Ab Initio Hamiltonian Approach to Light-Front Quantum Field Theory James P. Vary Department of Physics and Astronomy, Iowa State University, Ames, Iowa USA 1. Introduction Non-perturbative solutions of quantum field theory represent opportunities and challenges that span particle physics and nuclear physics. Increasingly, it is also gaining attention in condensed matter physics.

Rev. C. 3420]. [13] A. C. Hayes, P. Navrátil and J. P. Vary, Neutrino-12C Scattering in the ab initio Shell Model with a Realistic Three-Body Interaction Phys. Rev. Lett. 91, 012502 (2003); nucl-th/0305072. [14] A. M. Shirokov, J. P. Vary, A. I. Mazur and T. A. Weber, Realistic Nuclear Hamiltonian: Ab exitu approach, Phys. Letts. B 644 (2007) 33 [nucl-th/0512105]. [15] P. Navratil, V. G. Gueorguiev, J. P. Vary, W. E. Ormand and A. Nogga, Structure of A = 10-13 nuclei with two- plus three-nucleon interactions from chiral effective field theory, Phys.

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