Changes between Version 2 and Version 3 of ZeeBabu

Timestamp:

Jun 30, 2022, 3:03:50 PM (2 years ago)

Author:

Richard Ruiz

Comment:

Added title and references

ZeeBabu

@@ -1 @@
-Come back Friday!
+= {{{SM_ZeeBabu}}}: The Standard Model + Zee-Babu scalars at NLO in QCD =
+
+=== Contact Author ===
+Richard Ruiz
+* Institute of Nuclear Physics Polish Academy of Science (IFJ PAN)
+* richard.physics AT gmail.com
+
+
+==== Usage resources ====
+
+* [[span(style=color: #FF0000, '''*New*''' )]] For detailed instructions and examples on using the SM_ZeeBabu UFO libraries, see R. Ruiz arXiv:2207.qwerty . 
+* See '''Validation''' section below for additional information
+
+==== Citation requests ====
+
+* For the Lagrangian, please cite the original papers by Zee [ [#Zee1 1], [#Zee2 2] ] and Babu  [ [#Babu 3] ].
+* If using any of the UFOs, please cite the companion paper [ [#Ruiz 4] ].
+
+== Model Description ==
+=== Majorana N ===
+This effective/simplified model extends the Standard Model (SM) field content by introducing three right-handed (RH) neutrinos, which are singlets under the SM gauge symmetry (no color, weak isospin, or weak hypercharge charges). Each RH neutrino possesses one RH Majorana mass. After electroweak symmetry breaking, the Lagrangian with three heavy Majorana neutrinos ''N''i (for i=1,2,3) is given by [ [#Atre 6] ]
+{{{ 
+#!latex 
+\begin{equation}
+\mathcal{L} = \mathcal{L}_{\rm SM} + \mathcal{L}_{N} + \mathcal{L}_{N~\text{Int.}}
+\end{equation}
+}}}
+The first term is the Standard Model Lagrangian. In the mass basis, i.e., after mixing with active neutrinos, the heavy Majorana neutrinos' kinetic and mass terms are
+{{{ 
+#!latex 
+\begin{equation}
+\mathcal{L}_{N} = \frac{1}{2}\overline{N_k} i\!\not\!\partial N_k - \frac{1}{2}m_{N_k} \overline{N_k}N_k, \quad k=1,\dots,3,
+\end{equation}
+}}}
+
+and its interactions with the Weak gauge and Higgs bosons are given by
+{{{ 
+#!latex 
+\begin{eqnarray}
+\mathcal{L}_{N~\text{Int}} = 
+&-&\frac{g}{\sqrt{2}} W_{\mu}^{+}\sum_{k=1}^{3}\sum_{\ell=e}^{\tau} \overline{N_k}V_{\ell k}^{*}\gamma^{\mu}P_{L}\ell^{-}
++{\rm H.c.}
+\\
+&-&\frac{g}{2\cos\theta_W}Z_{\mu}\sum_{k=1}^{3}\sum_{\ell=e}^{\tau} \overline{N_k}V_{\ell k}^{*}\gamma^{\mu}P_{L}\nu_\ell
++{\rm H.c.}
+\\
+&-&\frac{g m_N}{2 M_W}         h \sum_{k=1}^{3}\sum_{\ell=e}^{\tau} \overline{N_k}V_{\ell k}^{*}P_{L}\nu_\ell
++{\rm H.c.}
+\end{eqnarray}
+}}} 
+Neutrino masses (mNk) and mixing parameters (Vlk) between heavy mass eigenstate and (active) flavor eigenstates are taken to be independent, phenomenological parameters. This allows for maximum flexibility and model independence when calculating rates. Therefore, some care is required by the user. 
+The lepton number- and flavor-violating interactions of the Lagrangian allow for modeling of the Type I, Inverse, and Linear seesaw mechanisms at both lepton, hadron, and lepto-hadron colliders.
+
+=== Dirac N ===
+The Dirac variant of the HeavyN model file contains the same interaction Lagrangian as the Majorana case. The heavy Dirac neutrinos' kinetic and mass terms are [ [#Pascoli2 4] ]
+{{{ 
+#!latex 
+\begin{equation}
+\mathcal{L}_{N} = \overline{N_k} i\!\not\!\partial N_k - m_{N_k} \overline{N_k}N_k, \quad k=1,\dots,3.
+\end{equation}
+}}}
+
+=== [[span(style=color: #FF0000, '''*New*''' )]] vSMEFT at dimension six ===
+In the {{{HeavyN_vSMEFTdim6}}} UFO [ [#Cirigliano 5] ], the {{{HeavyN}}} (Majorana) Lagrangian is extended by the dimension-six EFT operator
+{{{ 
+#!latex 
+\begin{equation}
+\mathcal{L}_{H\nu e}^{(6)} = \frac{1}{\Lambda^2}   \left(i \tilde{\varphi}^{\dagger} D_{\mu} \varphi\right) \, \bar \nu_R \gamma^\mu \,C_{H\nu l} ~ l_R
++  \mathrm{H.c.}\, ,
+\end{equation}
+}}}
+where {{{D_\mu}}} is the usual SM covariant derivative. {{{\Lambda}}} is the EFT cutoff in GeV scale, {{{ C_{H\nu l} }}} is the dimensionless Wilson coefficient, and {{{$l=e,\mu,\tau$}}}. Note that in Ref. [ [#Cirigliano 5] ], {{{ C_{H\nu l} }}} has dimension {{{GeV^-2}}}. In the unitary gauge after and EW symmetry breaking, the leading contribution of this operator can be written in the neutrino mass basis as
+{{{ 
+#!latex 
+\begin{equation}
+\mathcal{L}_{H\nu e}^{(6)} \approx 
+\frac{g v^2}{2\sqrt{2}\Lambda^2}
+\sum_{\ell=e}^{\tau}
+\sum_{k=1}^{3} \,\overline{N_k}  
+ \left[\bar{C}_{H\nu l}\right]_{k \ell} \gamma^\mu P_R \ell_{R}\,W_\mu^+  
+\left(1+\frac{h}{v}\right)^2 +\text{H.c.}
+\end{equation}
+}}}
+Here {{{k=1,\dots,3}}} runs over all three heavy neutrino mass eigenstates and {{{$\ell=e,\mu,\tau$}}} runs over all lepton flavors. For the precise definition of the effective Wilson coefficient {{{$\bar{C}_{H\nu l}$}}}, see Ref. [ [#Cirigliano 5] ].
+
+
+== QCD Corrections ==
+The above Lagrangian with Goldstone boson couplings and in the Feynman Gauge was implemented into FeynRules  2.3.10. QCD renormalization and R2 rational counter terms were determined using NLOCT 1.02 and FeynArts 3.8. Feynman rules were collected into a single UFO, available below. 
+In the UFO file, five massless quarks are assumed as are zero off-diagonal CKM matrix entries.
+For additional details, see [ [#Degrande 2] ] and references therein.
+These additions permit tree-level calculations at LO and NLO in QCD and loop-induced calculations at LO in QCD using MadGraph_aMC@NLO.
+
+
+== Model Files ==
+'''Note:''' The only difference between NLO and LO libraries is the presence of additional (effective) O(a_s) Feynman rules. By definition the NLO libraries can compute tree-level processes at LO precision.
+
+
+==== Majorana ====
+ * [https://feynrules.irmp.ucl.ac.be/raw-attachment/wiki/HeavyN/SM_HeavyN_NLO_UFO.tgz SM_HeavyN_NLO_UFO.tgz]: Standalone UFO folder. Assumes massless bottom quark and tau lepton, diagonal CKM.
+
+ * [https://feynrules.irmp.ucl.ac.be/raw-attachment/wiki/HeavyN/SM_HeavyN_Gen3Mass_NLO.tgz SM_HeavyN_Gen3Mass_NLO.tgz]: Standalone UFO folder. Assumes massive bottom quark and tau lepton, diagonal CKM.
+
+ * [https://feynrules.irmp.ucl.ac.be/raw-attachment/wiki/HeavyN/SM_HeavyN_CKM_AllMasses_LO.tgz SM_HeavyN_CKM_AllMasses_LO.tgz]: Standalone UFO folder. Assumes LO in QCD, with CKM elements (in radians), and all particle masses. Majorana equivalent of SM_HeavyN_Dirac_CKM_Masses_LO_UFO.
+
+
+ * [https://feynrules.irmp.ucl.ac.be/raw-attachment/wiki/HeavyN/heavyN.fr heavyN.fr]: Main model file. Relies on sm.fr (default FR model file) being declared elsewhere. 
+
+ * [https://feynrules.irmp.ucl.ac.be/raw-attachment/wiki/HeavyN/heavyN_NLO.nb heavyN_NLO.nb]: Mathematica notebook file that generates UFO file from FeynRules model files. Allows user to also run quick sanity checks (optional) on model. 
+
+ * [https://feynrules.irmp.ucl.ac.be/raw-attachment/wiki/HeavyN/SM_HeavyN_Files.tgz SM_HeavyN_Files.tgz]: Standalone package containing heavyN.fr, heavyN_NLO.nb, massless.rst (default FR file), diagonalCKM.rst (default FR file), and sm.fr (default FR file). 
+
+ * [https://feynrules.irmp.ucl.ac.be/raw-attachment/wiki/HeavyN/SM_HeavyN_FilesWithUFO.tgz SM_HeavyN_FilesWithUFO.tgz]: Combination of SM_HeavyN_NLO_UFO.tgz and SM_HeavyN_Files.tgz.
+
+==== Dirac ====
+ * [https://feynrules.irmp.ucl.ac.be/raw-attachment/wiki/HeavyN/SM_HeavyN_Dirac_NLO_UFO.tgz SM_HeavyN_Dirac_NLO_UFO.tgz]: Standalone NLO UFO libraries
+
+ * [https://feynrules.irmp.ucl.ac.be/raw-attachment/wiki/HeavyN/SM_HeavyN_Dirac_NLO_UFO.tgz SM_HeavyN_Dirac_LO_UFO.tgz]: Standalone LO UFO libraries.
+
+ * [https://feynrules.irmp.ucl.ac.be/raw-attachment/wiki/HeavyN/SM_HeavyN_Dirac_CKM_Masses_LO_UFO.tgz SM_HeavyN_Dirac_CKM_Masses_LO_UFO.tgz]: Standalone LO UFO libraries, assuming non-diagonal CKM matrix, six quark masses, and three charged lepton masses
+
+ * [https://feynrules.irmp.ucl.ac.be/attachment/wiki/HeavyN/heavyN_Dirac.fr heavyN_Dirac.fr]: Main model file. Relies on sm.fr (default FR model file) being declared elsewhere. 
+
+==== [[span(style=color: #FF0000, '''*New*''' )]] vSMEFT ====
+* [https://feynrules.irmp.ucl.ac.be/raw-attachment/wiki/HeavyN/SM_HeavyN_vSMEFTdim6_NLO.tgz SM_HeavyN_vSMEFTdim6_NLO.tgz]: Standalone NLO UFO folder. Assumes massless bottom quark and tau lepton, diagonal CKM.
+
+* [https://feynrules.irmp.ucl.ac.be/raw-attachment/wiki/HeavyN/SM_HeavyN_vSMEFTdim6_XLO.tgz SM_HeavyN_vSMEFTdim6_XLO.tgz]: Standalone LO UFO folder. Assumes massless bottom quark and tau lepton, diagonal CKM.
+
+* [https://feynrules.irmp.ucl.ac.be/raw-attachment/wiki/HeavyN/heavyN_vSMEFTdim6.fr heavyN_vSMEFTdim6.fr]: Main model file. Relies on sm.fr (default FR model file) being declared elsewhere. 
+
+== Download and Unpack ==
+ * To download any of the packages and unpack via the terminal, use the commands:
+
+==== Majorana NLO ====
+~/Path $ wget http://feynrules.irmp.ucl.ac.be/raw-attachment/wiki/HeavyN/SM_HeavyN_NLO_UFO.tgz
+
+~/Path $ tar -zxvf SM_HeavyN_NLO_UFO.tgz
+
+==== Majorana LO ====
+~/Path $ wget http://feynrules.irmp.ucl.ac.be/raw-attachment/wiki/HeavyN/SM_HeavyN_FilesWithUFO.tgz
+
+~/Path $ tar -zxvf SM_HeavyN_FilesWithUFO.tgz
+
+==== Dirac NLO ====
+~/Path $ wget http://feynrules.irmp.ucl.ac.be/raw-attachment/wiki/HeavyN/SM_HeavyN_Dirac_NLO_UFO.tgz 
+
+~/Path $ tar -zxvf SM_HeavyN_Dirac_NLO_UFO.tgz
+
+==== Dirac LO ====
+~/Path $ wget http://feynrules.irmp.ucl.ac.be/raw-attachment/wiki/HeavyN/SM_HeavyN_Dirac_LO_UFO.tgz 
+
+~/Path $ tar -zxvf SM_HeavyN_Dirac_LO_UFO.tgz
+
+==== vSMEFT NLO ====
+~/Path $ wget https://feynrules.irmp.ucl.ac.be/raw-attachment/wiki/HeavyN/SM_HeavyN_vSMEFTdim6_NLO.tgz 
+
+~/Path $ tar -zxvf SM_HeavyN_vSMEFTdim6_NLO.tgz 
+
+==== vSMEFT LO ====
+~/Path $ wget http://feynrules.irmp.ucl.ac.be/raw-attachment/wiki/HeavyN/SM_HeavyN_vSMEFTdim6_XLO.tgz 
+
+~/Path $ tar -zxvf SM_HeavyN_vSMEFTdim6_XLO.tgz 
+
+
+
+== Notes ==
+ * For instructions on using the HeavyN UFO, see C. Degrande, et al, arXiv:1602.06957 and S. Pascoli, et al, arXiv:1812.08750
+
+ * The flagship {{{HeavyN}}} UFO model contains 15 free parameters:
+  * Three masses: mN1, mN2, mN3. Defaults are 300 GeV, 500 GeV, and 1 TeV, respectively.
+  * Three widths: WN1, WN2, WN3. Defaults are 0.303 GeV, 1.50 GeV, and 12.3 GeV, respectively.
+  * Nine real (no CP violation) mixing parameters: V''lk'' for ''l'' = ''e, mu, tau'' and ''k'' = 1,2,3. Default values are V''lk'' = Identity(3x3), i.e., {{{Ve1 = Vmu2 = Vta3 = 1}}} and all others zero.
+  * '''Note''': VlN are restricted to be real in the model file.
+  * '''Note''': Default parameters are set so "out-of-the-box" checks can be made with [ [#Alva 1] ] and [ [#Degrande 2] ].
+
+* For the Majorana file, particle identification (PID) codes for N1,...,N3, follow standard HEP MCPID codes: 9900012, 9900014, 9900016
+
+* For the Dirac file, to avoid conflict with Pythia8, where the above PIDs are reserved for Majorana fields, the nonstandard HEP MCPID codes for N1,...,N3 are:9990012, 9990014, 9990016
+
+* For the vSMEFT file, 10 additional model parameters are introduced: 
+  * One EFT cutoff scale {{{Lambda}}} in units of GeV.
+  * Nine Wilson coefficients coupling {{{N_k}}} to {{{l}}}: {{{CeN1, CeN2, CeN3, CmuN1, CmuN2, CmuN3, CtaN1, CtaN2, CtaN3}}}
+  * '''Note''': Default parameters are set such that {{{Lambda=1000}}} (GeV), {{{CeN1=CmuN2=CtaN3=1}}}, and all other coefficients are zero
+
+
+== Validation ==
+* The model file was validated at LO in  [ [#Alva 1] ]; see Tables 2 and 5 for further validation checks.
+* The model file was validated at NLO in [ [#Degrande 2] ]; see Table 1 for further validation checks.
+* For very large masses, this model has been constructed to satisfy the Goldstone Equivalence Theorem:
+{{{
+#!latex 
+\begin{eqnarray}
+\text{BR}(N_i \rightarrow W^+ \ell^-) &=& \text{BR}(N_i \rightarrow W^- \ell^+) =
+\\ 
+\text{BR}(N_i \rightarrow Z \nu_\ell + Z \overline{\nu_\ell} ) &=&
+\text{BR}(N_i \rightarrow h \nu_\ell + h \overline{\nu_\ell} ) = 25\%.
+\end{eqnarray}
+}}}
+* Helicity dependence of LNV and LNC decay rates of Majorana neutrino decays was validated in [ [#Ruiz 7] ]
+
+== Studies that have used the above model files ==
+Please email to update this space.
+* Golling, et al., ''Physics at a 100 TeV pp collider: beyond the Standard Model phenomena'', arXiv:1606.00947
+* CMS, ''Search for heavy neutral leptons in events with three charged leptons in proton-proton collisions at 13 TeV'', arXiv:1802.02965 [hep-ex]
+* CMS, ''Search for heavy Majorana neutrinos in same-sign dilepton channels in proton-proton collisions at 13 TeV'', arXiv:1806.10905 [hep-ex]
+
+== References ==
+* For studies of Majorana neutrinos, please consider citing [ 6 ] for the Lagrangian and [ 1-2 ] for the Majorana FR/UFO files.
+* For studies of heavy Dirac neutrinos, please also consider citing [ 4 ].
+* For studies of heavy neutrinos in vSMEFT, please consider citing [ 5 ].
+
+
+[ [#Zee1 1], [#Zee2 2] ] and Babu  [ [#Babu 3] ].
+* If using any of the UFOs, please cite the companion paper [ [#Ruiz 4] ]
+
+[=#Zee1] [1] A. Zee, ''Charged Scalar Field and Quantum Number Violations,'' Phys. Lett. '''B161''' (1985) 141, https://inspirehep.net/literature/214241
+
+[=#Zee2] [2] A. Zee, ''Charged Scalar Field and Quantum Number Violations,'' Nucl. Phys. '''B264''' (1986) 99, 
+https://inspirehep.net/literature/218115
+
+[=#Babu] [3] K. Babu, ``Model of 'Calculable' Majorana Neutrino Masses,''    Phys. Lett. '''B203''' (1988) 132, 
+https://inspirehep.net/literature/22952
+
+[=#Ruiz] [4] R. Ruiz, ``Doubly Charged Higgs Boson Production at Hadron Colliders II: A Zee-Babu Case Study,'' 
+arXiv:2207.qwerty [hep-ph]
+