Changes between Version 11 and Version 12 of SMWeinberg
- Timestamp:
- Mar 24, 2021, 4:46:09 PM (4 years ago)
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SMWeinberg
v11 v12 3 3 === Contact Author === 4 4 Richard Ruiz 5 * Universite Catholique de Louvain6 * r ichard.ruiz AT uclouvain.be5 * Institute of Nuclear Physics Polish Academy of Science (IFJ PAN) 6 * rruiz AT ifj.edu.pl (or richard.physics AT gmail.com) 7 7 8 8 In collaboration with … … 10 10 11 11 12 For additional instructions and examples on using the {{{SMWeinberg}}} UFO libraries, see B. Fuks, et al, arXiv:2012. abcde12 For additional instructions and examples on using the {{{SMWeinberg}}} UFO libraries, see B. Fuks, et al, arXiv:2012.09882 13 13 14 14 * If using the {{{SMWeinberg}}} UFO, please cite [ [#Fuks 1] ] along with the appropriate {{{FeynRules}}} and generator papers. … … 79 79 &-&\frac{g m_N}{2 M_W} h \sum_{\ell=e}^{\tau} \overline{N} P_{L}\nu_\ell 80 80 +{\rm H.c.} 81 \\ 82 &+& \text{Additional Higgs and Goldstone terms} 81 83 \end{eqnarray} 82 84 }}} 83 85 84 The new external parameters of the {{{SMWeinberg}}} UFO are the six Wilson coefficients and the effective field theory cutoff scale.86 The new external parameters of the {{{SMWeinberg}}} UFO are the six real-valued Wilson coefficients and the effective field theory cutoff scale. 85 87 86 88 … … 134 136 135 137 == Notes == 136 * For instructions on using the {{{SMWeinberg}}} UFO, see B. Fuks, et al, arXiv:20 20.abcde138 * For instructions on using the {{{SMWeinberg}}} UFO, see B. Fuks, et al, arXiv:2012.09882 137 139 138 140 * This model contains seven external parameters in addition to those in the SM: … … 164 166 165 167 [=#Fuks] [1] B. Fuks, J. Neundorf, K. Peters, R. Ruiz and M. Saimpert, 166 ''Probing the Weinberg Operator at Colliders,'' arXiv:2012. abcde[hep-ph]168 ''Probing the Weinberg Operator at Colliders,'' arXiv:2012.09882 [hep-ph] 167 169 168 170 [=#Fuks] [2] B. Fuks, J. Neundorf, K. Peters, R. Ruiz and M. Saimpert,