Version 2 (modified by 5 years ago) ( diff ) | ,
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Heavy Scalar Effective Model
Authors
- Yongcheng Wu (contact for inquiries)
- ycwu -at- physics.carleton.ca, Carleton University
- Yue Xu
- yue.xu -at- cern.ch, Tsinghua University
- Xin Chen
- xin.chen -at- cern.ch, Tsinghua University
Model Description
In addition to the SM particle contents, we add one heavy scalar which might come from the second doublet etc. We focus on the effective couplings to the vector bosons, which are related to EWSB, and add following operators with both dim-6 and dim-4:
\begin{align*} \mathcal{L}_6 =& g_{6,H}^{WW} (\partial_\nu H)W^{\dagger}_{\mu} W^{\mu\nu} + h.c. + g_{6,H}^{\prime WW} H W^{\mu\nu}W^\dagger_{\mu\nu} \nonumber \\ & + g_{6,H}^{ZZ} (\partial_\nu H) Z_\mu Z^{\mu\nu} + h.c. + g_{6,H}^{\prime ZZ} H Z^{\mu\nu}Z_{\mu\nu} +\nonumber \\ & + g_{6,H}^{Z\gamma} (\partial_\nu H) Z_\mu F^{\mu\nu} + g_{6,H}^{\prime Z\gamma} F^{\mu\nu}Z_{\mu\nu} \nonumber \\ & + g_{6,H}^{\gamma\gamma} H F^{\mu\nu}F_{\mu\nu} \end{align*}
and
\begin{align*} \mathcal{L}_4 = g_{4,H}^{WW}g^{\mu\nu} H W^+_\mu W^-_\nu + g_{4,H}^{ZZ}g^{\mu\nu} H Z_\mu Z_\nu \end{align*}
For more details, please check the document here and the references listed below.
Model Files
FeynRules Model Files
UFO Model Files
References
- Y.-P. Kuang, H.-Y. Ren, L.-H. Xia, Phys. Rev. D90(2014) 115002 arXiv:1404.6367
- Y.-P. Kuang, H.-Y. Ren, L.-H. Xia, Chin.Phys.C40(2) (2016) 023101 arXiv:1506.08007
- X. Chen, Y. Xu, Y. Wu, Y.-P. Kuang, Q. Wang, H. Chen, S.-C. Hsu, Z. Hu, C. Li, arXiv:1905.05421
Attachments (2)
-
HeavyScalar_EFT_FR.tar.gz
(10.6 KB
) - added by 5 years ago.
FeynRules model files, used to generate the UFO model file
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HeavyScalar_EFT_UFO.tar.gz
(13.9 KB
) - added by 5 years ago.
The UFO model file
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