.. _smatgc: Standard Model + ATGC --------------------- This model implements the Standard Model (SM) with the SM QCD sector renormalized and including anomalous triple gauge boson couplings in terms of the effective action :cite:`Chiesa:2018lcs`: .. math:: \mathcal{L}^{\mathrm{eff}.} = \mathcal{L}^{\mathrm{SM}} +\sum_i \frac{c_6^i}{\Lambda^2} \mathcal{O}_6^i +\sum_i \frac{c_8^i}{\Lambda^4} \mathcal{O}_8^i , The fields correspond to the ones in the :ref:`SM `. Parameters and power-counting ***************************** Besides the :ref:`usual power-counting ` Wilson coefficients carry the power :m:`\mathrm{LAM}` (similar to :m:`\mathrm{QED}`, :m:`\mathrm{QCD}`) corresponding to :m:`\Lambda^{-2}`. For the dimension 6 operators the following parameters can be set .. list-table:: :widths: 4 8 12 4 :header-rows: 1 :align: center * - Parameter - |recola| identifier - Operator - Order * - :m:`c_{WWW}/\Lambda^2` - ``'CWWWL2'`` - :m:`-\frac{g_\mathrm{W}^3}{4} \epsilon_{ijk} W^i_{\mu\nu}W^{\nu\rho\;j}W_\rho^{\;\mu\;k}` - :m:`\mathrm{LAM}^1` * - :m:`c_{W}/\Lambda^2` - ``'CWL2'`` - :m:`-\mathrm{i}g_\mathrm{W} \left(D_\mu \Phi\right)^\dagger \frac{\tau_k}{2} W^{\mu\nu\;k} \left(D_\nu \Phi\right)` - :m:`\mathrm{LAM}^1` * - :m:`c_{B}/\Lambda^2` - ``'CBL2'`` - :m:`+\mathrm{i}\frac{g_1}{2} \left(D_\mu \Phi\right)^\dagger B^{\mu\nu} \left(D_\nu \Phi\right)` - :m:`\mathrm{LAM}^1` * - :m:`c_{\tilde WWW}/\Lambda^2` - ``'CPWWWL2'`` - :m:`+\frac{g_\mathrm{W}^3}{4} \epsilon_{ijk} \tilde W^i_{\mu\nu}W^{\nu\rho\;j}W_\rho^{\;\mu\;k}` - :m:`\mathrm{LAM}^1` * - :m:`c_{\tilde W}/\Lambda^2` - ``'CPWL2'`` - :m:`+\mathrm{i}g_\mathrm{W} \left(D_\mu \Phi\right)^\dagger \frac{\tau_k}{2} \tilde W^{\mu\nu\;k} \left(D_\nu \Phi\right)` - :m:`\mathrm{LAM}^1` For the neutral sector the following Wilson coefficients associated to dimension 8 operators can be set .. list-table:: :widths: 4 8 12 4 :header-rows: 1 :align: center * - Parameter - |recola| identifier - Operator - Order * - :m:`c_{BW}/\Lambda^4` - ``'CBWL4'`` - :m:`-\mathrm{i} \Phi^\dagger B_{\mu\nu} \frac{\tau_i}{2} W^{\mu\rho\;i} \left\{D_\rho, D^\nu\right\}\Phi + \mathrm{h.c.}` - :m:`\mathrm{LAM}^2` * - :m:`c_{WW}/\Lambda^4` - ``'CWWL4'`` - :m:`\mathrm{i} \Phi^\dagger \frac{\tau_i}{2} \frac{\tau_j}{2} W^{i}_{\mu\nu} W^{\mu\rho\;j} \left\{D_\rho, D^\nu\right\}\Phi + \mathrm{h.c.}` - :m:`\mathrm{LAM}^2` * - :m:`c_{BB}/\Lambda^4` - ``'CBBL4'`` - :m:`\mathrm{i} \Phi^\dagger B_{\mu\nu} B^{\mu\rho} \left\{D_\rho, D^\nu\right\}\Phi + \mathrm{h.c.}` - :m:`\mathrm{LAM}^2` * - :m:`c_{\tilde BW}/\Lambda^4` - ``'CBtWL4'`` - :m:`-\mathrm{i} \Phi^\dagger \tilde B_{\mu\nu} \frac{\tau_i}{2} W^{\mu\rho\;i} \left\{D_\rho, D^\nu\right\}\Phi + \mathrm{h.c.}` - :m:`\mathrm{LAM}^2` The user has to make sure that no corrections other than pure QCD ones are selected. An example for diboson production is given below. See :file:`agc_test.py` under `tests` for a more complete example. Snippet code ************ .. tabs:: .. code-tab:: py from pyrecola import * set_output_file_rcl('*') set_print_level_squared_amplitude_rcl(2) define_process_rcl(1,'u u~ -> Z Z ','NLO') unselect_all_powers_LoopAmpl_rcl(1) unselect_all_powers_BornAmpl_rcl(1) select_power_BornAmpl_rcl(1, 'QCD', 0) select_power_BornAmpl_rcl(1, 'QED', 2) select_power_BornAmpl_rcl(1, 'LAM', 0) select_power_BornAmpl_rcl(1, 'LAM', 1) select_power_BornAmpl_rcl(1, 'LAM', 2) select_power_LoopAmpl_rcl(1, 'QCD', 2) select_power_LoopAmpl_rcl(1, 'QED', 2) select_power_LoopAmpl_rcl(1, 'LAM', 0) select_power_LoopAmpl_rcl(1, 'LAM', 1) select_power_LoopAmpl_rcl(1, 'LAM', 2) generate_processes_rcl() s = 1000. p1 = [s / 2, 0., 0., s / 2] p2 = [s / 2, 0., 0., - s / 2] psp = set_outgoing_momenta_rcl(1, [p1, p2]) compute_process_rcl(1, psp, 'NLO') reset_recola_rcl() Releases ^^^^^^^^ * :sm_atgc:`2.2.3` **newest** * :sm_atgc:`2.2.2` * :sm_atgc:`2.2.0` UFO model files ^^^^^^^^^^^^^^^ * :sm_atgc:`UFO` .. rubric :: References .. bibliography:: ../references.bib :filter: docname in docnames