Medium energy (ME) GENIE configurations (100 MeV - 100 GeV)

• The G00_* CMCs are attempts to preserve the historic but severely outdated model in GENIE v2 series (G00_00a is the "Default" model and G00_00b is the "Default+MEC" model of GENIE v2.12)
• The G18_01* CMCs are adiabatic evolutions of the historic model, updating some of the cross-section and FSI models and including missing processes (diffractive production of pions, hyperon production) but keeping the same basic model construction.
• The G18_02* CMCs are similar to G18_01* CMCs, but upgrade the resonance and coherent pion production models (RS → BS)
• The G18_10* CMCs keep G18_02* upgrades to the resonance and coherent pion production models, and add a consistent theory-based model of interactions around the quasi-elastic peak (NAV QE and NSV 2p2h model). There are variants of that model that use a simple dipole axial form factor, and other variants that employ the better motivated but multi-parameter z expansion of the axial form factor.
• The G21_11* CMCs, similarly to G18_10*, start from G18_02* and install an improved and consistent model of interactions around the quasi-elastic peak. G21_11* uses the SuSAv2 QE and 2p2h model.
• For each basic model construction, several CMC variants are produced by using different intranuclear hadron transport models: `a' demotes use of INTRANUKE/hA, `b' of INTRANUKE/hN, `c' of Liege/INCL and `d' of Geant4 Bertini cascade.

• opt.: Optional (needs to be enabled)
• RFG: Relativistic Fermi Gas model
• LFG: Local Fermi Gas model
• LS: Llewellyn-Smith quasi-elastic model
• RS: Rein and Sehgal models for resonance neutrino-production and coherent pion production
• BY: Bodek and Yang model
• ASAV: M. Rafi Alam, I. Ruiz Simo, M. Sajjad Athar and M.J. Vicente Vacas model of single-Kaon production
• NAV: J.Nieves, J. Enrique Amaro, and M. Valverde quasi-elastic interaction model
• NSV: J.Nieves, I. Ruiz Simo, and M.J. Vicente Vacas 2p2h model
• AGKY: C.Andreopoulos, H.Gallagher, P.Kehayias and T.Yang neutrino-induced hadronization model
• AG: C.Andreopoulos, and H.Gallagher charm hadronization model
• hA: Effective intranuclear transport model in INTRANUKE
• hN: Full intranuclear cascade (INC) model in INTRANUKE
• INCL: The Liege INC model
• G4B: Geant4 implementation of the Bertini INC model

• We use the following status labels for tunes: Outdated (O), Experimental (E), Production (P), Recommended Production (P*)
• The tune labels shown in red below, are the labels that can be accepted as --tune arguments in GENIE applications
• Tunes marked as `baseline' describe the original settings of each new CMC and include parameter values from a mixture of past GENIE tunes, external tunes, or reasonable first estimates for new modelling elements that is too complex to note in this summary table. Typically, they carry the label 00_000. They form the starting point for a branch of more refined and well-motivated GENIE tunes.
• The label 02_11b denotes the final version of the GENIE 2020 nucleon cross-section model re-tune using bubble chamber CCQE, CC1π, CC2π, and CC inclusive cross-section data, published in J.Tena-Vidal et al., Phys.Rev.D 104 (2021) 7, 072009. This tune was made available in v3.2.0. Please note that the label 02_11a denotes a Preliminary version of that fit, and not the published version.
• The GENIE 2021 hadronization tunes published in J.Tena-Vidal, Phys.Rev.D 105 (2022) 1, 012009 are not yet distributed as part of a tuned bundled in public GENIE release.
• The GENIE 2022 nuclear CC0π tunes published in J.Tena-Vidal, TBA are not yet distributed as part of a tuned bundled in public GENIE release.

High energy (HE) GENIE configurations (> 100 GeV)

Low energy (LE) GENIE configurations (<100 MeV)