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Add CNMSSM and CE6SSM model files for testing
but currently they are incomplete and still need modifications
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Dylan Harries
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Jan 22, 2017
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FSModelName = "@CLASSNAME@"; | ||
FSEigenstates = SARAH`EWSB; | ||
FSDefaultSARAHModel = E6SSM; | ||
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(* CE6SSM input parameters *) | ||
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MINPAR = { | ||
{3, TanBeta} | ||
}; | ||
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EXTPAR = { | ||
{61, LambdaInput}, | ||
{62, KappaInput}, | ||
{63, MuPrimeInput}, | ||
{64, BMuPrimeInput}, | ||
{65, vsInput}, | ||
{66, Lambda12Input} | ||
}; | ||
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FSAuxiliaryParameters = { | ||
{m0Sq, {1}}, | ||
{m12, {1}}, | ||
{Azero, {1}} | ||
}; | ||
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EWSBOutputParameters = { m0Sq, m12, Azero }; | ||
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SUSYScale = Sqrt[Product[M[Su[i]]^(Abs[ZU[i,3]]^2 + Abs[ZU[i,6]]^2), {i,6}]]; | ||
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SUSYScaleFirstGuess = vsInput; | ||
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SUSYScaleInput = { | ||
{vs, vsInput} | ||
}; | ||
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HighScale = g1 == g2; | ||
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HighScaleFirstGuess = 1.0 10^16; | ||
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HighScaleMinimum = 1.0 10^4; | ||
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HighScaleMaximum = 5.0 10^17; | ||
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HighScaleInput = { | ||
{gN, g1}, | ||
{T[Ye], Azero*Ye}, | ||
{T[Yd], Azero*Yd}, | ||
{T[Yu], Azero*Yu}, | ||
{mq2, UNITMATRIX[3] m0Sq}, | ||
{ml2, UNITMATRIX[3] m0Sq}, | ||
{md2, UNITMATRIX[3] m0Sq}, | ||
{mu2, UNITMATRIX[3] m0Sq}, | ||
{me2, UNITMATRIX[3] m0Sq}, | ||
{mDx2, UNITMATRIX[3] m0Sq}, | ||
{mDxbar2, UNITMATRIX[3] m0Sq}, | ||
{mH1I2, UNITMATRIX[2] m0Sq}, | ||
{mH2I2, UNITMATRIX[2] m0Sq}, | ||
{msI2, UNITMATRIX[2] m0Sq}, | ||
{mHp2, m0Sq}, | ||
{mHpbar2, m0Sq}, | ||
{\[Kappa], UNITMATRIX[3] KappaInput}, | ||
{\[Lambda]12, UNITMATRIX[2] Lambda12Input}, | ||
{\[Lambda], LambdaInput}, | ||
{T[\[Kappa]], UNITMATRIX[3] Azero KappaInput}, | ||
{T[\[Lambda]12], UNITMATRIX[2] Azero Lambda12Input}, | ||
{T[\[Lambda]], Azero LambdaInput}, | ||
{MassB, m12}, | ||
{MassWB,m12}, | ||
{MassG,m12}, | ||
{MassBp,m12}, | ||
{\[Mu]Pr, MuPrimeInput}, | ||
{B[\[Mu]Pr], BMuPrimeInput} | ||
}; | ||
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LowScale = LowEnergyConstant[MZ]; | ||
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LowScaleFirstGuess = LowEnergyConstant[MZ]; | ||
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LowScaleInput = { | ||
{Yu, Automatic}, | ||
{Yd, Automatic}, | ||
{Ye, Automatic}, | ||
{vd, 2 MZDRbar / Sqrt[GUTNormalization[g1]^2 g1^2 + g2^2] Cos[ArcTan[TanBeta]]}, | ||
{vu, 2 MZDRbar / Sqrt[GUTNormalization[g1]^2 g1^2 + g2^2] Sin[ArcTan[TanBeta]]} | ||
}; | ||
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InitialGuessAtLowScale = { | ||
{vd, LowEnergyConstant[vev] Cos[ArcTan[TanBeta]]}, | ||
{vu, LowEnergyConstant[vev] Sin[ArcTan[TanBeta]]}, | ||
{vs, vsInput}, | ||
{Yu, Automatic}, | ||
{Yd, Automatic}, | ||
{Ye, Automatic} | ||
}; | ||
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InitialGuessAtHighScale = {}; | ||
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UseHiggs2LoopNMSSM = True; | ||
EffectiveMu = \[Lambda] vs / Sqrt[2]; | ||
EffectiveMASqr = T[\[Lambda]] vs / Sqrt[2] (vu^2 + vd^2) / (vu vd); | ||
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PotentialLSPParticles = { Chi, Sv, Su, Sd, Se, Cha, Glu }; | ||
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DefaultPoleMassPrecision = MediumPrecision; | ||
HighPoleMassPrecision = {hh, Ah, Hpm}; | ||
MediumPoleMassPrecision = {}; | ||
LowPoleMassPrecision = {}; |
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Block MODSEL # Select model | ||
# 12 1000 # DRbar parameter output scale (GeV) | ||
Block FlexibleSUSY | ||
0 1.000000000e-04 # precision goal | ||
1 0 # max. iterations (0 = automatic) | ||
2 0 # algorithm (0 = two_scale, 1 = lattice) | ||
3 0 # calculate SM pole masses | ||
4 2 # pole mass loop order | ||
5 2 # EWSB loop order | ||
6 2 # beta-functions loop order | ||
7 2 # threshold corrections loop order | ||
8 1 # Higgs 2-loop corrections O(alpha_t alpha_s) | ||
9 1 # Higgs 2-loop corrections O(alpha_b alpha_s) | ||
10 1 # Higgs 2-loop corrections O((alpha_t + alpha_b)^2) | ||
11 1 # Higgs 2-loop corrections O(alpha_tau^2) | ||
12 0 # force output | ||
13 1 # Top pole mass QCD corrections (0 = 1L, 1 = 2L, 2 = 3L) | ||
14 1.000000000e-11 # beta-function zero threshold | ||
15 0 # calculate observables (a_muon, ...) | ||
16 0 # force positive majorana masses | ||
17 0 # pole mass renormalization scale (0 = SUSY scale) | ||
18 0 # pole mass renormalization scale in the EFT (0 = min(SUSY scale, Mt)) | ||
19 0 # EFT matching scale (0 = SUSY scale) | ||
20 2 # EFT loop order for upwards matching | ||
21 1 # EFT loop order for downwards matching | ||
22 0 # EFT index of SM-like Higgs in the BSM model | ||
23 1 # calculate BSM pole masses | ||
Block SMINPUTS # Standard Model inputs | ||
1 1.279340000e+02 # alpha^(-1) SM MSbar(MZ) | ||
2 1.166370000e-05 # G_Fermi | ||
3 1.176000000e-01 # alpha_s(MZ) SM MSbar | ||
4 9.118760000e+01 # MZ(pole) | ||
5 4.200000000e+00 # mb(mb) SM MSbar | ||
6 1.733000000e+02 # mtop(pole) | ||
7 1.777000000e+00 # mtau(pole) | ||
8 0.000000000e+00 # mnu3(pole) | ||
9 80.404 # MW pole | ||
11 5.109989020e-04 # melectron(pole) | ||
12 0.000000000e+00 # mnu1(pole) | ||
13 1.056583570e-01 # mmuon(pole) | ||
14 0.000000000e+00 # mnu2(pole) | ||
21 4.750000000e-03 # md(2 GeV) MS-bar | ||
22 2.400000000e-03 # mu(2 GeV) MS-bar | ||
23 1.040000000e-01 # ms(2 GeV) MS-bar | ||
24 1.270000000e+00 # mc(mc) MS-bar | ||
Block MINPAR # Input parameters | ||
3 6 # TanBeta | ||
Block EXTPAR | ||
61 0.1 # LambdaInput | ||
62 0.2 # KappaInput | ||
63 10000 # MuPrimeInput | ||
64 10000 # BMuPrimeInput | ||
65 8000 # vsInput | ||
66 0.3 # Lambda12Input |
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FSModelName = "@CLASSNAME@"; | ||
FSEigenstates = SARAH`EWSB; | ||
FSDefaultSARAHModel = NMSSM; | ||
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FSBVPSolvers = { SemiAnalyticSolver }; | ||
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(* CNMSSM input parameters *) | ||
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MINPAR = { | ||
{2, m12}, | ||
{3, TanBeta}, | ||
{4, Sign[vS]}, | ||
{5, Azero} | ||
}; | ||
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EXTPAR = { | ||
{61, LambdaInput} | ||
}; | ||
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FSAuxiliaryParameters = { | ||
{m0Sq, {1}} | ||
}; | ||
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EWSBOutputParameters = { \[Kappa], vS, m0Sq }; | ||
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EWSBInitialGuess = { | ||
{m0Sq, LowEnergyConstant[MZ]^2} | ||
}; | ||
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SUSYScale = Sqrt[Product[M[Su[i]]^(Abs[ZU[i,3]]^2 + Abs[ZU[i,6]]^2), {i,6}]]; | ||
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SUSYScaleFirstGuess = Sqrt[14 m12^2 - 3 m12 Azero + Azero^2]; | ||
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SUSYScaleInput = {}; | ||
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HighScale = g1 == g2; | ||
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HighScaleFirstGuess = 2.0 10^16; | ||
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HighScaleInput={ | ||
{T[Ye], Azero*Ye}, | ||
{T[Yd], Azero*Yd}, | ||
{T[Yu], Azero*Yu}, | ||
{mq2, UNITMATRIX[3] m0Sq}, | ||
{ml2, UNITMATRIX[3] m0Sq}, | ||
{md2, UNITMATRIX[3] m0Sq}, | ||
{mu2, UNITMATRIX[3] m0Sq}, | ||
{me2, UNITMATRIX[3] m0Sq}, | ||
{mHu2, m0Sq}, | ||
{mHd2, m0Sq}, | ||
{ms2, m0Sq}, | ||
{\[Lambda], LambdaInput}, | ||
{T[\[Kappa]], Azero \[Kappa]}, | ||
{T[\[Lambda]], Azero LambdaInput}, | ||
{MassB, m12}, | ||
{MassWB,m12}, | ||
{MassG,m12} | ||
}; | ||
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LowScale = LowEnergyConstant[MZ]; | ||
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LowScaleFirstGuess = LowEnergyConstant[MZ]; | ||
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LowScaleInput = { | ||
{Yu, Automatic}, | ||
{Yd, Automatic}, | ||
{Ye, Automatic}, | ||
{vd, 2 MZDRbar / Sqrt[GUTNormalization[g1]^2 g1^2 + g2^2] Cos[ArcTan[TanBeta]]}, | ||
{vu, 2 MZDRbar / Sqrt[GUTNormalization[g1]^2 g1^2 + g2^2] Sin[ArcTan[TanBeta]]} | ||
}; | ||
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InitialGuessAtLowScale = { | ||
{vd, LowEnergyConstant[vev] Cos[ArcTan[TanBeta]]}, | ||
{vu, LowEnergyConstant[vev] Sin[ArcTan[TanBeta]]}, | ||
{\[Lambda], LambdaInput}, | ||
{\[Kappa], 0.1}, | ||
{vS, 1000}, | ||
{Yu, Automatic}, | ||
{Yd, Automatic}, | ||
{Ye, Automatic} | ||
}; | ||
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InitialGuessAtHighScale = {}; | ||
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UseHiggs2LoopNMSSM = True; | ||
EffectiveMu = \[Lambda] vS / Sqrt[2]; | ||
EffectiveMASqr = (T[\[Lambda]] vS / Sqrt[2] + 0.5 \[Lambda] \[Kappa] vS^2) (vu^2 + vd^2) / (vu vd); | ||
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PotentialLSPParticles = { Chi, Sv, Su, Sd, Se, Cha, Glu }; | ||
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DefaultPoleMassPrecision = MediumPrecision; | ||
HighPoleMassPrecision = {hh, Ah, Hpm}; | ||
MediumPoleMassPrecision = {}; | ||
LowPoleMassPrecision = {}; | ||
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ExtraSLHAOutputBlocks = { | ||
{FlexibleSUSYOutput, NoScale, | ||
{{0, Hold[HighScale]}, | ||
{1, Hold[SUSYScale]}, | ||
{2, Hold[LowScale]} } }, | ||
{EWSBOutputs, NoScale, | ||
{{1, \[Kappa]}, | ||
{2, vS}, | ||
{3, m0Sq} } }, | ||
{FlexibleSUSYLowEnergy, | ||
{{0, FlexibleSUSYObservable`aMuon} } }, | ||
{EFFHIGGSCOUPLINGS, NoScale, | ||
{{1, FlexibleSUSYObservable`CpHiggsPhotonPhoton}, | ||
{2, FlexibleSUSYObservable`CpHiggsGluonGluon}, | ||
{3, FlexibleSUSYObservable`CpPseudoScalarPhotonPhoton}, | ||
{4, FlexibleSUSYObservable`CpPseudoScalarGluonGluon} } }, | ||
{NMSSMRUN, | ||
{{1, \[Lambda]}, | ||
{2, \[Kappa]}, | ||
{3, T[\[Lambda]] / \[Lambda]}, | ||
{4, T[\[Kappa]] / \[Kappa]}, | ||
{5, \[Lambda] vS / Sqrt[2]}, | ||
{10, ms2} } } | ||
}; |
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Original file line number | Diff line number | Diff line change |
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@@ -0,0 +1,55 @@ | ||
Block MODSEL # Select model | ||
6 0 # flavour violation | ||
# 12 1000 # DRbar parameter output scale (GeV) | ||
Block FlexibleSUSY | ||
0 1.000000000e-04 # precision goal | ||
1 0 # max. iterations (0 = automatic) | ||
2 0 # algorithm (0 = two_scale, 1 = lattice) | ||
3 0 # calculate SM pole masses | ||
4 2 # pole mass loop order | ||
5 2 # EWSB loop order | ||
6 2 # beta-functions loop order | ||
7 2 # threshold corrections loop order | ||
8 1 # Higgs 2-loop corrections O(alpha_t alpha_s) | ||
9 1 # Higgs 2-loop corrections O(alpha_b alpha_s) | ||
10 1 # Higgs 2-loop corrections O((alpha_t + alpha_b)^2) | ||
11 1 # Higgs 2-loop corrections O(alpha_tau^2) | ||
12 0 # force output | ||
13 1 # Top pole mass QCD corrections (0 = 1L, 1 = 2L, 2 = 3L) | ||
14 1.000000000e-11 # beta-function zero threshold | ||
15 0 # calculate observables (a_muon, ...) | ||
16 0 # force positive majorana masses | ||
17 0 # pole mass renormalization scale (0 = SUSY scale) | ||
18 0 # pole mass renormalization scale in the EFT (0 = min(SUSY scale, Mt)) | ||
19 0 # EFT matching scale (0 = SUSY scale) | ||
20 2 # EFT loop order for upwards matching | ||
21 1 # EFT loop order for downwards matching | ||
22 0 # EFT index of SM-like Higgs in the BSM model | ||
23 1 # calculate BSM pole masses | ||
Block FlexibleSUSYInput | ||
0 0.00729735 # alpha_em(0) | ||
1 125.09 # Mh pole | ||
Block SMINPUTS # Standard Model inputs | ||
1 1.279340000e+02 # alpha^(-1) SM MSbar(MZ) | ||
2 1.166370000e-05 # G_Fermi | ||
3 1.176000000e-01 # alpha_s(MZ) SM MSbar | ||
4 9.118760000e+01 # MZ(pole) | ||
5 4.200000000e+00 # mb(mb) SM MSbar | ||
6 1.733000000e+02 # mtop(pole) | ||
7 1.777000000e+00 # mtau(pole) | ||
8 0.000000000e+00 # mnu3(pole) | ||
9 80.404 # MW pole | ||
11 5.109989020e-04 # melectron(pole) | ||
12 0.000000000e+00 # mnu1(pole) | ||
13 1.056583570e-01 # mmuon(pole) | ||
14 0.000000000e+00 # mnu2(pole) | ||
21 4.750000000e-03 # md(2 GeV) MS-bar | ||
22 2.400000000e-03 # mu(2 GeV) MS-bar | ||
23 1.040000000e-01 # ms(2 GeV) MS-bar | ||
24 1.270000000e+00 # mc(mc) MS-bar | ||
Block MINPAR # Input parameters | ||
2 200 # m12 | ||
3 10 # TanBeta | ||
5 -500 # Azero | ||
Block EXTPAR # Input parameters | ||
61 0.1 # LambdaInput |