Accurate predictions ! for Higgs Characterisation
Transcripción
Accurate predictions ! for Higgs Characterisation
Accurate predictions ! for Higgs Characterisation ! ! Marco Zaro, LPTHE - UPMC Paris VI ! based on! Artoisenet, de Aquino, Demartin, Frederix, Frixione, Maltoni, Mandal, Mathews, ! Mawatari, Ravindran, Seth, Torrielli, MZ, arXiv:1306.6464! Maltoni, Mawatari, MZ, arXiv:1311.1829! Demartin, Maltoni, Mawatari, Page, MZ, arXiv:1407.5089! ! HEFT 2014 @IFT Madrid! September 30, 2014 1 LHCPhenoNet Any major discovery is the ! beginning of a new journey… Marco Zaro, 30-09-2014 2 LHCPhenoNet Any major discovery is the ! beginning of a new journey… What is that peak?? Marco Zaro, 30-09-2014 2 LHCPhenoNet Is it THE Higgs boson! as expected in the SM? NAME ! Higgs boson! DATE OF BIRTH! Jul 4th 2012 (presumed)! SPIN 0! CP even! FERMIONIC COUPLING! mf/v! BOSONIC COUPLING! 2mv2/v! SELF COUPLING! λ=MH2/2v2 Marco Zaro, 30-09-2014 3 LHCPhenoNet How to answer the question(s)? • (at least) Two approaches can be used: Anomalous couplings (AC) e.g JHU (arXiv: 1001.3396, 1208.4018)! ✔ Only requirement is Lorentz symmetry! ✔ Agnostic on new physics! ✘ Non renormalizable! ✘ Large number of extra couplings! ✘ Possibly violate unitarity, yet can include model dependent form factors Marco Zaro, 30-09-2014 Effective field theory (EFT) ! ✔ Based on SM symmetries! ✘ Valid only up to a scale Λ! ✔/✘ New physics heavier than the resonance itself! ✔ Renormalizable (order by order in 1/Λ) ➝ can include QCD corrections! ✔ Reduce number of extra couplings by using symmetries and dimensional analyses 4 LHCPhenoNet The HC-EFT approach • Use the Higgs dim-6 effective Lagrangian and implement it in FeynRules → UFO model! • Add missing pieces needed for NLO QCD corrections UV/R2! • SM + Hgg! • Include QCD corrections in the MadGraph5_aMC@NLO framework → events (rates & distributions) at NLO in QCD! • Study different production and decay channels, keeping spincorrelations! • Disclaimer: we assume the EFT approach to be valid in all the phase-space Marco Zaro, 30-09-2014 5 LHCPhenoNet ! The MadGraph5_aMC@NLO framework Alwall, Frederix, Frixione, Maltoni, Mattelaer, Shao, Stelzer, Torrielli, Hirschi, MZ, arXiv:1405.0301 FKS MadGraph MadGraph5_aMC@NLO MC@NLO CutTools Marco Zaro, 30-09-2014 6 LHCPhenoNet Above the EW scale: Introduction HEFT in FEYNRULES Phenomenological examples Summary D6 Higgs Effective Lagrangian slide from K. Mawatari@MC4BSM 2014 Marco Zaro, The30-09-2014 model file ✦ Wyler, Nucl.Phys.B177 [ from Contino,Buchmuller, Ghezzi, Grojean, Muhlleitner, Spira (JHEP(1986)! ’13) ] Grzadkowski, Iskrzynski, Misiak, Rosiek, arXiv:1008.4884! [ Alloul, Fuks, Sanz (1310.5150) ] Contino, Ghezzi, Grojean, Muhlleitner, Spira, arXiv:1303.3876! Alloul, Fuks, Sanz, arXiv:1310.5150 7 LHCPhenoNet is publicly available. (https://feynrules.irmp.ucl.ac.be/wiki/HEL) Below the EW scale: Mapping between the D6 and D5 operators slide from K. Mawatari@MC4BSM 2014 HC [arXiv: 1306.6464] HEL [arXiv: 1310.5150] The two approaches are equivalent! Two approaches equivalent as they can be mapped intoextendible one another.to HEL NLO implementation Marco Zaro, 12-06-2014 8 LHCPhenoNet atari, M. Zaro: Higgs characterisation via VBF and VH production refs. [13, 32] (see e.g. eq. (3.46) of ref. [32]) not including the terms in LF1 and LF hich modify four-point gXyy interactions, ⇥v ZZ/W W and equivalent toZeq. (3) of ref. [26]. For a CP -odd physics interactions 2m2Z/W of ref. 47↵ [32]. /18⇡ C(94c2W 13)/9⇡ an automatically atebethis is equivalentXto= H eq. (A.98) X=A 0 4↵ /3⇡ 2C(8c2W 5)/3⇡ raph5 aMC@NLO Let us start the interaction lagrangian relevant to fermions which, while bein acterisation can alsowith Table 2. Values in units of vqtaken by the couplings gXyy for tion channel [46], all illustrates our philosophy ↵ G m tremely simple, well. p . Such a lagrangian is: the EW gauge bosons. C = 8 2⇡ are covered. X dies in VBF and VH f ¯f c↵ Hf f gHf f + is↵ Af f gAf f 5 f X0 , (2.2 in H ! ZZ/W W L0 = 0 The Lagrangian:! Spin-0! EM EM EM F 2 Z 0 in ref. [37]): ges in the VBF and is (eq. (2.4) f =t,b,⌧ rvables, e.g., the az⇢ ⇥1 ⇤ tagging jets V µ + µ jj in L0 = c↵ SM gHZZ Zµ Z + gHW W Wµ W here we Higgs use the on of the res- notation: 2 ween the Z and W ⇤ 1⇥ µ⌫ µ⌫ e c↵ H gH Aµ⌫ A + s↵ A gA Aµ⌫ A s study, we focus on c↵ ⌘ cos ↵ , s↵ ⌘ sin ↵ , (2.3 4 Higgs VBF and VH ⇤ 1⇥ µ⌫ µ⌫ e c↵ HZ gHZ Zµ⌫ A + s↵ AZ gAZ Zµ⌫ A ecay. nd denote by secgHf f = m21f ⇥/v (gAf f = mf /v) the strength of⇤ the scalar (pseudoscalar In the following a a,µ⌫ a e a,µ⌫ grangian of ref. [37], c + s ↵ Hgg gHgg Gµ⌫ G ↵ Agg gAgg Gµ⌫ G upling in the SM (in a 2HDM with tan = 1). We point out that the constants i can b 4 to illustrate the phe⇤ 1⇥ µ⌫ µ⌫ e we present the VBF any loss1of ken real without generality, except in eq. (2.4). For simplicity, we hav c↵ HZZ Zµ⌫ Z + s↵ AZZH@W Zµ⌫ Z 4⇤ f key observables in sumed that only the third-generation of fermions couple to ⇤the scalar state; extension 1 1⇥ + µ⌫ + f µ⌫ dedicated VBF cuts, c↵ HW W Wµ⌫ W + s↵ AW W Wµ⌫ W 2⇤ H andother ZH producthe families and flavour-changing structures are trivial to implement, which can ⇥ 1 gs in the concluding µ⌫ µ⌫ c Z @ A Z @ Z ↵ H@ ⌫ µ H@Z ⌫ µ directly done by users of⇤ FeynRules. As mentioned above, the interaction of eq. (2.2 dim=6 = ( † )Q ⇤ ˜tR operator. Note also that al n also parametrise the e↵ects of a L + µ⌫ L + H@W W⌫Y @µ W + h.c. X0 , (1) quirements listed above are satisfied at the price of a small redundancy in the number o Marco Zaro, 30-09-2014 9 tensors are defined as where the (reduced) field strength LHCPhenoNet atari, M. Zaro: Higgs characterisation via VBF and VH production refs. [13, 32] (see e.g. eq. (3.46) of ref. [32]) not including the terms in LF1 and LF hich modify four-point gXyy interactions, ⇥v ZZ/W W and equivalent toZeq. (3) of ref. [26]. For a CP -odd physics interactions 2m2Z/W of ref. 47↵ [32]. /18⇡ C(94c2W 13)/9⇡ an automatically atebethis is equivalentXto= H eq. (A.98) X=A 0 4↵ /3⇡ 2C(8c2W 5)/3⇡ raph5 aMC@NLO Let us start the interaction lagrangian relevant to fermions which, while bein acterisation can alsowith Table 2. Values in units of vqtaken by the couplings gXyy for tion channel [46], all illustrates our philosophy ↵ G m tremely simple, well. p . Such a lagrangian is: the EW gauge bosons. C = 8 2⇡ are covered. X dies in VBF and VH f ¯f c↵ Hf f gHf f + is↵ Af f gAf f 5 f X0 , (2.2 in H ! ZZ/W W L0 = 0 The Lagrangian:! Spin-0! EM EM EM F 2 Z 0 in ref. [37]): ges in the VBF and is (eq. (2.4) f =t,b,⌧ rvables, e.g., the az⇢ ⇥1 ⇤ tagging jets V µ + µ jj in L0 = c↵ SM gHZZ Zµ Z + gHW W Wµ W here we Higgs use the on of the res- notation: 2 ween the Z and W ⇤ 1⇥ µ⌫ µ⌫ e c↵ H gH Aµ⌫ A + s↵ A gA Aµ⌫ A s study, we focus on c↵ ⌘ cos ↵ , s↵ ⌘ sin ↵ , (2.3 4 Higgs VBF and VH ⇤ 1⇥ µ⌫ µ⌫ e c↵ HZ gHZ Zµ⌫ A + s↵ AZ gAZ Zµ⌫ A ecay. nd denote by secgHf f = m21f ⇥/v (gAf f = mf /v) the strength of⇤ the scalar (pseudoscalar In the following a a,µ⌫ a e a,µ⌫ grangian of ref. [37], c + s ↵ Hgg gHgg Gµ⌫ G ↵ Agg gAgg Gµ⌫ G upling in the SM (in a 2HDM with tan = 1). We point out that the constants i can b 4 to illustrate the phe⇤ 1⇥ µ⌫ µ⌫ e we present the VBF any loss1of ken real without generality, except in eq. (2.4). For simplicity, we hav c↵ HZZ Zµ⌫ Z + s↵ AZZH@W Zµ⌫ Z 4⇤ f key observables in sumed that only the third-generation of fermions couple to ⇤the scalar state; extension 1 1⇥ + µ⌫ + f µ⌫ dedicated VBF cuts, c↵ HW W Wµ⌫ W + s↵ AW W Wµ⌫ W 2⇤ H andother ZH producthe families and flavour-changing structures are trivial to implement, which can ⇥ 1 gs in the concluding µ⌫ µ⌫ c Z @ A Z @ Z ↵ H@ ⌫ µ H@Z ⌫ µ directly done by users of⇤ FeynRules. As mentioned above, the interaction of eq. (2.2 dim=6 = ( † )Q ⇤ ˜tR operator. Note also that al n also parametrise the e↵ects of a L + µ⌫ L + H@W W⌫Y @µ W + h.c. X0 , (1) SM quirements listed above are satisfied at the price of a small redundancy in the number o Marco Zaro, 30-09-2014 9 tensors are defined as where the (reduced) field strength LHCPhenoNet atari, M. Zaro: Higgs characterisation via VBF and VH production refs. [13, 32] (see e.g. eq. (3.46) of ref. [32]) not including the terms in LF1 and LF hich modify four-point gXyy interactions, ⇥v ZZ/W W and equivalent toZeq. (3) of ref. [26]. For a CP -odd physics interactions 2m2Z/W of ref. 47↵ [32]. /18⇡ C(94c2W 13)/9⇡ an automatically atebethis is equivalentXto= H eq. (A.98) X=A 0 4↵ /3⇡ 2C(8c2W 5)/3⇡ raph5 aMC@NLO Let us start the interaction lagrangian relevant to fermions which, while bein acterisation can alsowith Table 2. Values in units of vqtaken by the couplings gXyy for tion channel [46], all illustrates our philosophy ↵ G m tremely simple, well. p . Such a lagrangian is: the EW gauge bosons. C = 8 2⇡ are covered. X dies in VBF and VH f ¯f c↵ Hf f gHf f + is↵ Af f gAf f 5 f X0 , (2.2 in H ! ZZ/W W L0 = 0 The Lagrangian:! Spin-0! EM EM EM F 2 Z 0 in ref. [37]): ges in the VBF and is (eq. (2.4) f =t,b,⌧ rvables, e.g., the az⇢ ⇥1 ⇤ tagging jets V µ + µ jj in L0 = c↵ SM gHZZ Zµ Z + gHW W Wµ W here we Higgs use the on of the res- notation: 2 ween the Z and W ⇤ 1⇥ µ⌫ µ⌫ e c↵ H gH Aµ⌫ A + s↵ A gA Aµ⌫ A s study, we focus on c↵ ⌘ cos ↵ , s↵ ⌘ sin ↵ , (2.3 4 Higgs VBF and VH ⇤ 1⇥ µ⌫ µ⌫ e c↵ HZ gHZ Zµ⌫ A + s↵ AZ gAZ Zµ⌫ A ecay. nd denote by secgHf f = m21f ⇥/v (gAf f = mf /v) the strength of⇤ the scalar (pseudoscalar In the following a a,µ⌫ a e a,µ⌫ grangian of ref. [37], c + s ↵ Hgg gHgg Gµ⌫ G ↵ Agg gAgg Gµ⌫ G upling in the SM (in a 2HDM with tan = 1). We point out that the constants i can b 4 to illustrate the phe⇤ 1⇥ µ⌫ µ⌫ e we present the VBF any loss1of ken real without generality, except in eq. (2.4). For simplicity, we hav c↵ HZZ Zµ⌫ Z + s↵ AZZH@W Zµ⌫ Z 4⇤ f key observables in sumed that only the third-generation of fermions couple to ⇤the scalar state; extension 1 1⇥ + µ⌫ + f µ⌫ dedicated VBF cuts, c↵ HW W Wµ⌫ W + s↵ AW W Wµ⌫ W 2⇤ H andother ZH producthe families and flavour-changing structures are trivial to implement, which can ⇥ 1 gs in the concluding µ⌫ µ⌫ c Z @ A Z @ Z ↵ H@ ⌫ µ H@Z ⌫ µ directly done by users of⇤ FeynRules. As mentioned above, the interaction of eq. (2.2 dim=6 = ( † )Q ⇤ ˜tR operator. Note also that al n also parametrise the e↵ects of a L + µ⌫ L + H@W W⌫Y @µ W + h.c. X0 , (1) SM HD quirements listed above are satisfied at the price of a small redundancy in the number o Marco Zaro, 30-09-2014 9 tensors are defined as where the (reduced) field strength LHCPhenoNet atari, M. Zaro: Higgs characterisation via VBF and VH production refs. [13, 32] (see e.g. eq. (3.46) of ref. [32]) not including the terms in LF1 and LF hich modify four-point gXyy interactions, ⇥v ZZ/W W and equivalent toZeq. (3) of ref. [26]. For a CP -odd physics interactions 2m2Z/W of ref. 47↵ [32]. /18⇡ C(94c2W 13)/9⇡ an automatically atebethis is equivalentXto= H eq. (A.98) X=A 0 4↵ /3⇡ 2C(8c2W 5)/3⇡ raph5 aMC@NLO Let us start the interaction lagrangian relevant to fermions which, while bein acterisation can alsowith Table 2. Values in units of vqtaken by the couplings gXyy for tion channel [46], all illustrates our philosophy ↵ G m tremely simple, well. p . Such a lagrangian is: the EW gauge bosons. C = 8 2⇡ are covered. X dies in VBF and VH f ¯f c↵ Hf f gHf f + is↵ Af f gAf f 5 f X0 , (2.2 in H ! ZZ/W W L0 = 0 The Lagrangian:! Spin-0! EM EM EM F 2 Z 0 in ref. [37]): ges in the VBF and is (eq. (2.4) f =t,b,⌧ rvables, e.g., the az⇢ ⇥1 ⇤ tagging jets V µ + µ jj in L0 = c↵ SM gHZZ Zµ Z + gHW W Wµ W here we Higgs use the on of the res- notation: 2 ween the Z and W ⇤ 1⇥ µ⌫ µ⌫ e c↵ H gH Aµ⌫ A + s↵ A gA Aµ⌫ A s study, we focus on c↵ ⌘ cos ↵ , s↵ ⌘ sin ↵ , (2.3 4 Higgs VBF and VH ⇤ 1⇥ µ⌫ µ⌫ e c↵ HZ gHZ Zµ⌫ A + s↵ AZ gAZ Zµ⌫ A ecay. nd denote by secgHf f = m21f ⇥/v (gAf f = mf /v) the strength of⇤ the scalar (pseudoscalar In the following a a,µ⌫ a e a,µ⌫ + grangian of ref. [37], c + s ↵ Hgg gHgg Gµ⌫ G ↵ Agg gAgg Gµ⌫ G upling in the SM (in a 2HDM with tan = 1). We point out that the constants i can b 4 to illustrate the phe⇤ 1⇥ µ⌫ µ⌫ e we present the VBF any loss1of ken real without generality, except in eq. (2.4). For simplicity, we hav c↵ HZZ Zµ⌫ Z + s↵ AZZH@W Zµ⌫ Z 4⇤ f key observables in sumed that only the third-generation of fermions couple to ⇤the scalar state; extension 1 1⇥ + µ⌫ + f µ⌫ dedicated VBF cuts, c↵ HW W Wµ⌫ W + s↵ AW W Wµ⌫ W 2⇤ H andother ZH producthe families and flavour-changing structures are trivial to implement, which can ⇥ 1 gs in the concluding µ⌫ µ⌫ c Z @ A Z @ Z ↵ H@ ⌫ µ H@Z ⌫ µ directly done by users of⇤ FeynRules. As mentioned above, the interaction of eq. (2.2 dim=6 = ( † )Q ⇤ ˜tR operator. Note also that al n also parametrise the e↵ects of a L + µ⌫ L + H@W W⌫Y @µ W + h.c. X0 , (1) SM HD 0 quirements listed above are satisfied at the price of a small redundancy in the number o Marco Zaro, 30-09-2014 9 tensors are defined as where the (reduced) field strength LHCPhenoNet atari, M. Zaro: Higgs characterisation via VBF and VH production refs. [13, 32] (see e.g. eq. (3.46) of ref. [32]) not including the terms in LF1 and LF hich modify four-point gXyy interactions, ⇥v ZZ/W W and equivalent toZeq. (3) of ref. [26]. For a CP -odd physics interactions 2m2Z/W of ref. 47↵ [32]. /18⇡ C(94c2W 13)/9⇡ an automatically atebethis is equivalentXto= H eq. (A.98) X=A 0 4↵ /3⇡ 2C(8c2W 5)/3⇡ raph5 aMC@NLO Let us start the interaction lagrangian relevant to fermions which, while bein acterisation can alsowith Table 2. Values in units of vqtaken by the couplings gXyy for tion channel [46], all illustrates our philosophy ↵ G m tremely simple, well. p . Such a lagrangian is: the EW gauge bosons. C = 8 2⇡ are covered. X dies in VBF and VH f ¯f c↵ Hf f gHf f + is↵ Af f gAf f 5 f X0 , (2.2 in H ! ZZ/W W L0 = 0 The Lagrangian:! Spin-0! EM EM EM F 2 Z 0 in ref. [37]): ges in the VBF and is (eq. (2.4) f =t,b,⌧ rvables, e.g., the az⇢ ⇥1 ⇤ tagging jets V µ + µ jj in L0 = c↵ SM gHZZ Zµ Z + gHW W Wµ W here we Higgs use the on of the res- notation: 2 ween the Z and W ⇤ 1⇥ µ⌫ µ⌫ e c↵ H gH Aµ⌫ A + s↵ A gA Aµ⌫ A s study, we focus on c↵ ⌘ cos ↵ , s↵ ⌘ sin ↵ , (2.3 4 Higgs VBF and VH ⇤ 1⇥ µ⌫ µ⌫ e c↵ HZ gHZ Zµ⌫ A + s↵ AZ gAZ Zµ⌫ A ecay. nd denote by secgHf f = m21f ⇥/v (gAf f = mf /v) the strength of⇤ the scalar (pseudoscalar In the following a a,µ⌫ a e a,µ⌫ + grangian of ref. [37], c + s ↵ Hgg gHgg Gµ⌫ G ↵ Agg gAgg Gµ⌫ G upling in the SM (in a 2HDM with tan = 1). We point out that the constants i can b 4 to illustrate the phe⇤ 1⇥ µ⌫ µ⌫ e we present the VBF any loss1of ken real without generality, except in eq. (2.4). For simplicity, we hav c↵ HZZ Zµ⌫ Z + s↵ AZZH@W Zµ⌫ Z 4⇤ f key observables in sumed that only the third-generation of fermions couple to ⇤the scalar state; extension 1 1⇥ + µ⌫ + f µ⌫ dedicated VBF cuts, c↵ HW W Wµ⌫ W + s↵ AW W Wµ⌫ W 2⇤ H andother ZH producthe families and flavour-changing structures are trivial to implement, which can ⇥ 1 gs in the concluding µ⌫ µ⌫ c Z @ A Z @ Z ↵ H@ ⌫ µ H@Z ⌫ µ directly done by users of⇤ FeynRules. As mentioned above, the interaction of eq. (2.2 dim=6 = ( † )Q ⇤ ˜tR operator. Note also that al n also parametrise the e↵ects of a L + µ⌫ L + H@W W⌫Y @µ W + h.c. X0 , (1) SM HD 0 0 quirements listed above are satisfied at the price of a small redundancy in the number o Marco Zaro, 30-09-2014 9 tensors are defined as where the (reduced) field strength LHCPhenoNet atari, M. Zaro: Higgs characterisation via VBF and VH production refs. [13, 32] (see e.g. eq. (3.46) of ref. [32]) not including the terms in LF1 and LF hich modify four-point gXyy interactions, ⇥v ZZ/W W and equivalent toZeq. (3) of ref. [26]. For a CP -odd physics interactions 2m2Z/W of ref. 47↵ [32]. /18⇡ C(94c2W 13)/9⇡ an automatically atebethis is equivalentXto= H eq. (A.98) X=A 0 4↵ /3⇡ 2C(8c2W 5)/3⇡ raph5 aMC@NLO Let us start the interaction lagrangian relevant to fermions which, while bein acterisation can alsowith Table 2. Values in units of vqtaken by the couplings gXyy for tion channel [46], all illustrates our philosophy ↵ G m tremely simple, well. p . Such a lagrangian is: the EW gauge bosons. C = 8 2⇡ are covered. X dies in VBF and VH f ¯f c↵ Hf f gHf f + is↵ Af f gAf f 5 f X0 , (2.2 in H ! ZZ/W W L0 = 0 The Lagrangian:! Spin-0! EM EM EM F 2 Z 0 in ref. [37]): ges in the VBF and is (eq. (2.4) f =t,b,⌧ rvables, e.g., the az⇢ ⇥1 ⇤ tagging jets V µ + µ jj in L0 = c↵ SM gHZZ Zµ Z + gHW W Wµ W here we Higgs use the on of the res- notation: 2 ween the Z and W ⇤ 1⇥ µ⌫ µ⌫ e c↵ H gH Aµ⌫ A + s↵ A gA Aµ⌫ A s study, we focus on c↵ ⌘ cos ↵ , s↵ ⌘ sin ↵ , (2.3 4 Higgs VBF and VH ⇤ 1⇥ µ⌫ µ⌫ e c↵ HZ gHZ Zµ⌫ A + s↵ AZ gAZ Zµ⌫ A ecay. nd denote by secgHf f = m21f ⇥/v (gAf f = mf /v) the strength of⇤ the scalar (pseudoscalar In the following a a,µ⌫ a e a,µ⌫ + grangian of ref. [37], c + s ↵ Hgg gHgg Gµ⌫ G ↵ Agg gAgg Gµ⌫ G upling in the SM (in a 2HDM with tan = 1). We point out that the constants i can b 4 to illustrate the phe⇤ 1⇥ µ⌫ µ⌫ e we present the VBF any loss1of ken real without generality, except in eq. (2.4). For simplicity, we hav c↵ HZZ Zµ⌫ Z + s↵ AZZH@W Zµ⌫ Z 4⇤ f key observables in sumed that only the third-generation of fermions couple to ⇤the scalar state; extension 1 1⇥ + µ⌫ + f µ⌫ dedicated VBF cuts, c↵ HW W Wµ⌫ W + s↵ AW W Wµ⌫ W 2⇤ H andother ZH producthe families and flavour-changing structures are trivial to implement, which can ⇥ 1 gs in the concluding µ⌫ µ⌫ c Z @ A Z @ Z ↵ H@ ⌫ µ H@Z ⌫ µ directly done by users of⇤ FeynRules. As mentioned above, the interaction of eq. (2.2 dim=6 = ( † )Q ⇤ ˜tR operator. Note also that al n also parametrise the e↵ects of a L + µ⌫ L + H@W W⌫Y @µ W + h.c. X0 , (1) SM HD 0 0 quirements listed above are satisfied at the price of a small redundancy in the number o Marco Zaro, 30-09-2014 +Der 9 0 where the (reduced) field strength tensors are defined as LHCPhenoNet The Lagrangian:! Spin-1! [K. Hagiwara, R.D. Peccei, D. Zeppenfeld, Nuclear Physics B282 (1987)] Marco Zaro, 30-09-2014 10 LHCPhenoNet The Lagrangian:! Spin-1! [K. Hagiwara, R.D. Peccei, D. Zeppenfeld, Nuclear Physics B282 (1987)] ‣ 1- in parity-conserving scenarios Marco Zaro, 30-09-2014 10 LHCPhenoNet The Lagrangian:! Spin-1! [K. Hagiwara, R.D. Peccei, D. Zeppenfeld, Nuclear Physics B282 (1987)] ‣ 1- in parity-conserving scenarios Marco Zaro, 30-09-2014 ‣ 1+ in parity-conserving scenarios 10 LHCPhenoNet The Lagrangian:! Spin-2! 1 L2 = ⇤ X i=V, ,g, i ki Tµ⌫ X µ⌫ The minimal spin-2 particle is graviton like (2+)! Higher dimension operators and 2- available Marco Zaro, 30-09-2014 11 LHCPhenoNet HC in the various ! production channels gluo n vecto r VH ttH fusi boso n fusi pro du c pro du cti on on tio n on 125 Marco Zaro, 30-09-2014 12 LHCPhenoNet Chapter 1: ! spin/CP analysis in gg→X→… Artoisenet, de Aquino, Demartin, Frederix, Frixione, Maltoni, Mandal, Mathews, Mawatari, Ravindran, Seth, Torrielli, MZ, arXiv:1306.6464 are due to the different dominant initial • Differences in shape 1 0 2 • state (qq̄ for X , gg for X , X ) ! MLM distributions are harder (as expected), otherwise agreement is quite good Marco Zaro, 30-09-2014 13 LHCPhenoNet Results:! decay into V V→4l at LO! ! 0.2 1 pp → X(0±) → 4l at the LHC8 pp → X(0±) → 4l at the LHC8 0.8 + 0.15 0 : κ SM=1 0+: κ HZZ=1 0+: κ H∂Z=1 0 : κ AZZ=1 0.1 0.6 0.4 0.05 0 0 0.2 20 40 60 80 100 m1,2 (GeV) 0 -1 -0.5 0 0.5 1 cosθ* 0.3 1 pp → X(0±) → 4l at the LHC8 pp → X(0±) → 4l at the LHC8 0.8 0.2 0.6 0.4 0.1 0.2 0 -1 -0.5 0 0.5 1 cosθ1 0 0 2 4 6 ∆φ Figure 1. Normalised distributions in pp ! X0 ! µ+ µ e+ e for di↵erent choices of X0 ZZ couplings: the invariant masses of the two lepton pairs m1 , m2 (with m1 > m2 ), cos ✓⇤ , cos ✓1 , and , as defined in ref. [10]. Event simulation performed at the leading order, parton level only (no Marco Zaro, 30-09-2014 14 shower/hadronisation). Angles defined in Bolognesi et al. arXiv:1208.4018 LHCPhenoNet Results:! decay into V V→4l /2l2ν at NLO+PS! ! Figure of the in transverse X(! W W ⇤ ) ! µ ⌫¯µ e+ ⌫e : (a) the transverse momentum n X(! ZZ ⇤ ) 8. ! Distributions µ+ µ e+ e : (a) andleptons (b) the Z2 + 1 the muon, pµT , (b) the invariant mass of the two leptons m(µ e ). st andoflowest reconstructed mass, pZ and p , (c) and T T m`` corresponding to Z1 and Z2 . largest invariant mass) for the di↵erent spin and parity hypotheses. As already noted in thewhile literature [10, 92] the lowest pair invariant proach, aMC@NLO may be limited by the mass is particularly sensitive to both spin parity assignments. Finally, the transverse leptons ments. However, spin 0 is obviously a trivial case (a Marcoand Zaro, 30-09-2014 15 momentum of one of the charged LHCPhenoNet ⇤ raph5 aMC@NLO acterisation can also tion channel [46], all are covered. dies in VBF and VH in H ! ZZ/W W ges in the VBF and rvables, e.g., the aztagging jets jj in on of the Higgs resween the Z and W s study, we focus on Higgs VBF and VH decay. In the following secgrangian of ref. [37], to illustrate the phewe present the VBF f key observables in dedicated VBF cuts, ± H and ZH producgs in the concluding X=A 0 4↵EM /3⇡ 2C(8c2W 5)/3⇡ Table 2. Values in units of vqtaken by the couplings gXyy0 for ↵EM GF m2 Z p . the EW gauge bosons. C = 8 2⇡ Chapter 2:! HD iseffects in the VVH interactions (eq. (2.4) in ref. [37]): l setup, from the lak Marco scenarios, to event Zaro, 30-09-2014 LV0 0+ = ⇢ Maltoni, Mawatari, MZ, arXiv:1311.1829 ⇥1 c↵ SM gHZZ Zµ Z µ + gHW W Wµ+ W 2 µ ⇤ SM ⇤ 1⇥ µ⌫ µ⌫ e c↵ H gH Aµ⌫ A + s↵ A gA Aµ⌫ A 4 ⇤ 1⇥ µ⌫ µ⌫ e c↵ HZ gHZ Zµ⌫ A + s↵ AZ gAZ Zµ⌫ A 2 ⇤ 1⇥ a a,µ⌫ a e a,µ⌫ c↵ Hgg gHgg Gµ⌫ G + s↵ Agg gAgg Gµ⌫ G 4 ⇤ 1 1⇥ µ⌫ µ⌫ e c↵ HZZ Zµ⌫ Z + s↵ AZZ Zµ⌫ Z 4⇤ ⇤ 1 1⇥ + µ⌫ + f µ⌫ c↵ HW W Wµ⌫ W + s↵ AW W Wµ⌫ W 2⇤ 1 ⇥ c↵ H@ Z⌫ @µ Aµ⌫ H@Z Z⌫ @µ Z µ⌫ ⇤ ⇤ + µ⌫ + H@W W⌫ @µ W + h.c. X0 , (1) HD 0- 0 Der + strength tensors are defined as where the (reduced) field Vµ⌫ = @µ V⌫ @⌫ Vµ (V = A, Z, W ± ) , Gaµ⌫ = @µ Ga⌫ @⌫ Gaµ + gs f16abc Gbµ Gc⌫ , (2) (3) LHCPhenoNet ! VBF ! pp→X0jj (VBF) at the LHC8, NLO+PS pp→X0jj (VBF) at the LHC8, NLO+PS + 0 (SM) + 0 (HD) -1 0+ (HDder) 10 0+ (SM+HD) + 0 (SM) + 0 (HD) -1 0+ (HDder) 10 0 (HD) 0- (HD) 0± (HD) 0± (HD) 10-3 aMC@NLO+HERWIG6 NLO+PS / NLO NLO+PS / LO pT • • 400 500 (GeV) X 600 700 10-2 10-3 aMC@NLO+HERWIG6 300 0+ (SM+HD) 0 (HD) 10-3 200 + 0+ (HDder) 0± (HD) 10-2 100 + 0 (SM) 0 (HD) 10 - 10-2 0 pp→X0jj (VBF) at the LHC8, NLO+PS 0+ (SM+HD) - 10-4 1.2 1 0.8 0.6 1.2 1 0.8 0.6 -1 10-4 1.2 NLO+PS / NLO 1 0.8 0.6 1.2 NLO+PS / LO 1 0.8 0.6 800 0 100 200 aMC@NLO+HERWIG6 300 pT 400 500 (GeV) j1 600 700 10-4 1.2 NLO+PS / NLO 1 0.8 0.6 1.2 NLO+PS / LO 1 0.8 0.6 800 0 500 1000 1500 2000 m(j1,j2) (GeV) 2500 300 SM case shows a softer behaviour (not for Mjj)! NLO and PS effects are important (in particular for jetrelated observables) Marco Zaro, 30-09-2014 17 LHCPhenoNet PS 0+ (SM) ! + 0 (HD) VBF ! 0+ (HDder) + 0 (SM+HD) 0- (HD) ± 0 (HD) pp→X0jj (VBF) at the LHC8, NLO+PS pp→X0jj (VBF) at the LHC8, NLO+PS + 0 (SM) + 0 (HD) -1 0+ (HDder) 10 0+ (SM+HD) + 0 (SM) + 0 (HD) -1 0+ (HDder) 10 0 (HD) 0- (HD) 0± (HD) 0± (HD) 10-3 aMC@NLO+HERWIG6 NLO+PS / NLO NLO+PS / LO pT • • 400 500 (GeV) X 600 700 10-2 10-3 aMC@NLO+HERWIG6 300 0+ (SM+HD) 0 (HD) 10-3 200 + 0+ (HDder) 0± (HD) 10-2 100 + 0 (SM) 0 (HD) 10 - 10-2 0 pp→X0jj (VBF) at the LHC8, NLO+PS 0+ (SM+HD) - 10-4 1.2 1 0.8 0.6 1.2 1 0.8 0.6 -1 10-4 1.2 NLO+PS / NLO 1 0.8 0.6 1.2 NLO+PS / LO 1 0.8 0.6 800 0 100 200 aMC@NLO+HERWIG6 300 pT 400 500 (GeV) j1 600 700 10-4 1.2 NLO+PS / NLO 1 0.8 0.6 1.2 NLO+PS / LO 1 0.8 0.6 800 0 500 1000 1500 2000 m(j1,j2) (GeV) 2500 300 SM case shows a softer behaviour (not for Mjj)! NLO and PS effects are important (in particular for jetrelated observables) Marco Zaro, 30-09-2014 17 LHCPhenoNet VBF 0.08 pp→X0jj (VBF) at the LHC8, NLO+PS 0.1 0+ (SM) pp→X0jj (VBF) at the LHC8, NLO+PS + 0+ (HD) 0 (HD) 0+ (HDder) 0+ (HDder) 0.08 + 0.06 + 0 (SM+HD) 0 (SM+HD) 0.06 pp→X0jj (VBF) at the LHC8, NLO+PS 0+ (SM) 0- (HD) 0- (HD) 0± (HD) 0± (HD) 0.06 0+ (SM) 0+ (HD) 0.04 + 0 (HDder) 0.04 0+ (SM+HD) 0- (HD) 0.04 0.02 0.02 aMC@NLO+HERWIG6 aMC@NLO+HERWIG6 0 1.2 1 0.8 0.6 1.2 1 0.8 0.6 0± (HD) 0.02 0 1.2 1 0.8 0.6 1.2 1 0.8 0.6 NLO+PS / NLO NLO+PS / LO -4 -3 -2 -1 0 η • • j1 1 2 3 4 aMC@NLO+HERWIG6 0 1.2 1 0.8 0.6 1.2 1 0.8 0.6 NLO+PS / NLO NLO+PS / LO 0 1 2 3 4 |∆η(j1, j2)| 5 6 7 8 NLO+PS / NLO NLO+PS / LO 0 0.5 1 1.5 |∆φ(j1, j2)| 2 2.5 3 In SM case jets are more forward: HD scenarios feature a different signature! Jet correlations Δɸ, Δη are sensitive to the HVV structure Marco Zaro, 30-09-2014 18 LHCPhenoNet VBF ! (with extra Mjj cut): 0.08 0.1 pp→X0jj (VBF) at the LHC8, NLO+PS 0 (SM) m(j1,j2)>500 GeV 0 (HD) + + 0+ (HDder) 0.08 0+ (SM+HD) 0.06 pp→X0jj (VBF) at the LHC8, NLO+PS 0 (SM) m(j1,j2)>500 GeV 0 (HD) pp→X0jj (VBF) at the LHC8, NLO+PS + + 0+ (HDder) m(j1,j2)>500 GeV 0.06 0+ (SM+HD) - 0 (HD) 0- (HD) 0± (HD) 0± (HD) 0.06 0+ (SM) 0+ (HD) 0.04 + 0 (HDder) 0.04 0+ (SM+HD) 0- (HD) 0.04 0.02 0.02 aMC@NLO+HERWIG6 0 1.2 1 0.8 0.6 1.2 1 0.8 0.6 0± (HD) 0.02 aMC@NLO+HERWIG6 0 1.2 1 0.8 0.6 1.2 1 0.8 0.6 NLO+PS / NLO NLO+PS / LO -4 -3 -2 -1 0 η • • j1 1 2 3 4 aMC@NLO+HERWIG6 0 1.2 1 0.8 0.6 1.2 1 0.8 0.6 NLO+PS / NLO NLO+PS / LO 0 1 2 3 4 |∆η(j1, j2)| 5 6 7 8 NLO+PS / NLO NLO+PS / LO 0 0.5 1 1.5 |∆φ(j1, j2)| 2 2.5 3 The extra Mjj cut pushes jets to be more separated! No dramatic effects on angular correlations Marco Zaro, 30-09-2014 19 LHCPhenoNet ZX0: pp→X0Z (Z→e+e-) at the LHC8, NLO+PS + 0 (HD) 0+ (HDder) 10-1 pp→X0Z (Z→e+e-) at the LHC8, NLO+PS + 0 (SM) 0+ (SM+HD) 0.03 + + 0 (HD) 0+ (HDder) 10-1 0+ (SM+HD) 0 (HD) 0- (HD) 0± (HD) 0± (HD) - 10-2 10-2 pp→X0Z (Z→e+e-) at the LHC8, NLO+PS 0 (SM) 0.02 0+ (SM) 0.01 0+ (HD) 0+ (HDder) 0+ (SM+HD) 0- (HD) aMC@NLO+HERWIG6 10-3 1.4 1.2 1 10-3 1.4 1.2 1 NLO+PS / NLO NLO+PS / LO 1.4 1.2 1 0 100 • • • 1.4 1.2 1 200 300 pT 400 500 (GeV) X 600 700 800 aMC@NLO+HERWIG6 0 1.4 1.2 1 NLO+PS / NLO NLO+PS / LO 50 NLO+PS / NLO NLO+PS / LO 1.4 1.2 1 100 0± (HD) aMC@NLO+HERWIG6 150 200 250 lep,hard pT (GeV) 300 350 400 -1 -0.5 0 cosθlep 0.5 1 SM is softer, HD harder, HDder much harder (contact interaction)! QCD effects are less important than for VBF! Similar features for WH Marco Zaro, 30-09-2014 20 LHCPhenoNet approximation as long is not sensibly larger EFT approach for the 1 limit, the resulting production have been been used by Powheg O results matched with NLO+PS predictions ] for the one-loop ma@NLO [35], that em37], are also available. are for the SM Higgs roduction for the CPO, yet with the exact r we present NLO reroduction of a generic sociation with one or arton shower. twodimensions. independentThe realcomplete quantities are at needed to parametrise the ing basis dimension six has been most general CP violating this parametrisation known for a long time [47, interaction), 48] and recently reconsidered in has several practical advantages, among which possibility more detail in the context of the Higgs boson, seethe e.g., [49–51]. of easily interpolating CP-even (c↵ = [52] 1, s↵imple= 0) This approach has beenbetween followed the in the FeynRules and CP-odd 0, swhere assignments. ↵ = ↵ = 1)the mentation of (c ref. [53], e↵ective lagrangian is written The Higgs interaction with the top-quarks inducesbreaking a (nonin terms of fields above the electroweak symmetry decoupling) e↵ective couplings to photons, gluons, and photon(EWSB) scale and then expressed in terms of gauge eigenDemartin, Maltoni, Mawatari, Page, MZ, arXiv:1407.5089 Z gauge bosons through a top-quark loop. In the HC framestates. work, e↵ective lagrangian such loop-induced interacAs the already mentioned above,for in ref. [14] we have followed an tions with vector bosons (eq.equivalent (2.4) in ref. alternative approach (andreads yet fully in [14]): the context of ⇢ the phenomenological applications of this paper, as explicitly ⇥ 1 loop a a,µ⌫ + the EFT seenLin tables 1 and 3 of ref. [53]) and implemented = c g G G ↵ Hgg Hgg µ⌫ 0 4 from the mass eigenstates, so below the lagrangian starting a e a,µ⌫ ⇤ P EWSB scale, and for spin-parity assignments (X(J ) + svarious g G G ↵ Agg Agg µ⌫ with J P = 0± , 1±1, ⇥2+ ). We have also used FeynRules, whose µ⌫ c↵ H gH Aµ⌫ A output in the UFO 4 format [54, 55] can be directly passed to MadGraph5 aMC@NLO [35]. We stress µ⌫ ⇤ that this procedure e + scomputations Aµ⌫atALO, while at NLO the ↵ A gA is fully automatic for µ⌫ UFO model has 1to⇥c be supplemented with suitable countert↵ HZ gHZ Zµ⌫ A erms, as it will be2recalled in Sect. 2.2, a procedure that in this work has been performed by hand. µ⌫ ⇤ e +s g Zµ⌫ A X0 , (2) The term of interest↵ inAZthe AZ e↵ective lagrangian can be written as (see eq. (2.2) in ref. [14]): wheret the (reduced) field strength tensors are defined as L0 = ¯t c↵ Htt gHtt + is↵ Att gAtt 5 t X0 , (1) a a a abc b c G = @ G @ G + g f (3) s µ ⌫the scalar ⌫ µ boson, cGµ ⌫ , ↵ and s ⌘ sin ↵ can whereµ⌫ X labels ⌘Gcos Chapter 3:! CP properties of the top Yukawa or arbitrary CP coule NLO corrections in or quite some time [38, done only recently, for MC@NLO [40] and in case only. The spinay products have been th the help of Madections have been also respectively. The pheMarco Zaro, 30-09-2014 0 0 this can be ach e.g. the dimens HC model. Fin grangian the lo parametrized b tribution to th In order to we also write t massive gauge LZ,W = 0 ⇢ c 1 1⇥ c 4⇤ 1 1⇥ c 2⇤ 1 ⇥ c↵ ⇤ where gHZZ = plings, and ⇤ is summarised in 0 ↵ ↵ In table 3 w ± be thought parameters, are the dimenHtt,Att Vµ⌫ = @asµ V“CP-mixing” @ V (V = A, Z, W ) , (4) ⌫ ⌫ µ sionless real coupling parameters, and gHtt = gAtt = mt /v (= use for illustrat corresponds to 21 and the dual tensor is LHCPhenoNet 0 (VBF, HD) 0.20 0 (VBF, HD) ± 0 (VBF, HD) 0.25 0.15 0.20 0.10 0.10 0.00 0.05 GF vs VBF pp→X0jj at the LHC13 MG5_aMC@NLO + HERWIG6 0.00 0.35 GF uncertainties, NLO+PS 0+ 0.30 0.20 0.10 0.00 -0.10 -0.20 0.30 0.20 0.10 0.00 -0.10 -0.20 0.30 0.20 0.10 0.00 -0.10 -0.20 PDF+αS µR,F µR,F PDF+αS 0± µR,F PDF+αS GF m(j1uncertainties, ,j2) > 500 GeV NLO+PS 0+ 0.30 0.30 0.20 0.10 0.00 0.25 -0.10 -0.20 0.20 0.30 0.20 0.10 0.15 0.00 -0.10 -0.20 0.10 0.30 0.20 0.10 0.05 0.00 -0.10 -0.20 0.00 - NLO+PS (µ+PDF+αS) LO+PS (µ+PDF) 0.30 0.20 2.00 0.10 0.00 1.50 -0.10 1.00 -0.20 2.00 1.50 1.00 µR,F 0- µR,F PDF+αs 0± µR,F PDF+αs 0.50 0.30 0.20 2.00 0.10 0.00 1.50 -0.10 -0.20 1.00 00- NLO+PS (µ+PDF+αs) 0± 0± NLO+PS (µ+PDF+αs) 1.00 0.50 0.30 0.20 2.00 0.10 0.00 1.50 -0.10 -0.20 1.00 0.50 0.50 0.50 0 2.00 LO+PS (µ+PDF) 1.50 1.00 0.50 ± NLO+PS (µ+PDF+αS) 0 2.00 LO+PS (µ+PDF) 1.50 0 1 2 3 4 | ∆η(j1,j2) | Marco Zaro, 30-09-2014 5 6 0 7 2.00 1.50 1.00 0- (GF, SM) 0 (GF) 0± (GF) 0+ (VBF, SM)s PDF+α + 0- (VBF, HD) 0± (VBF, HD) 0 (VBF, HD) GF uncertainties, NLO+PS GF NLO+PS/LO+PS (with total uncertainties) µR,F PDF+α ++ 0 NLO+PS (µ+PDF+αs) LO+PS (µ+PDF)s 0 GF NLO+PS/LO+PS (with total uncertainties) NLO+PS (µ+PDF+αS) + NLO+HERWIG6 0- 0+ (shape comparison) µR,F PDF+αs LO+PS (µ+PDF) µR,F PDF+αs LO+PS (µ+PDF) • VBF-like cuts enhance the MadGraph5_aMC@NLO 0.05 MadGraph5_aMC@NLO Jet correlations in X0jj 0.15 t-channel gluon exchange, which is more sensitive to CP Hagiwara, Li, Mawatari, arXiv:0915.4314 • NLO corrections are large, (~30%) and not flat GF NLO+PS/LO+PS (with total uncertainties) π/2 π NLO+PS (µ+PDF+αs) LO+PS (µ+PDF) 0+ | ∆φ(j1,j2) | 22 LHCPhenoNet 0 (VBF, HD) 0.20 0 (VBF, HD) ± 0 (VBF, HD) 0.25 0.15 0.20 0.10 0.10 0.00 0.05 GF vs VBF pp→X0jj at the LHC13 MG5_aMC@NLO + HERWIG6 0.00 0.35 GF uncertainties, NLO+PS 0+ 0.30 0.20 0.10 0.00 -0.10 -0.20 0.30 0.20 0.10 0.00 -0.10 -0.20 0.30 0.20 0.10 0.00 -0.10 -0.20 PDF+αS µR,F µR,F PDF+αS 0± µR,F PDF+αS GF m(j1uncertainties, ,j2) > 500 GeV NLO+PS 0+ 0.30 0.30 0.20 0.10 0.00 0.25 -0.10 -0.20 0.20 0.30 0.20 0.10 0.15 0.00 -0.10 -0.20 0.10 0.30 0.20 0.10 0.05 0.00 -0.10 -0.20 0.00 - NLO+PS (µ+PDF+αS) LO+PS (µ+PDF) 0.30 0.20 2.00 0.10 0.00 1.50 -0.10 1.00 -0.20 2.00 1.50 1.00 µR,F 0- µR,F PDF+αs 0± µR,F PDF+αs 0.50 0.30 0.20 2.00 0.10 0.00 1.50 -0.10 -0.20 1.00 00- NLO+PS (µ+PDF+αs) 0± 0± NLO+PS (µ+PDF+αs) 1.00 0.50 0.30 0.20 2.00 0.10 0.00 1.50 -0.10 -0.20 1.00 0.50 0.50 0.50 0 2.00 LO+PS (µ+PDF) 1.50 1.00 0.50 ± NLO+PS (µ+PDF+αS) 0 2.00 LO+PS (µ+PDF) 1.50 0 1 2 3 4 | ∆η(j1,j2) | Marco Zaro, 30-09-2014 5 6 0 7 2.00 1.50 1.00 0- (GF, SM) 0 (GF) 0± (GF) 0+ (VBF, SM)s PDF+α + 0- (VBF, HD) 0± (VBF, HD) 0 (VBF, HD) GF uncertainties, NLO+PS GF NLO+PS/LO+PS (with total uncertainties) µR,F PDF+α ++ 0 NLO+PS (µ+PDF+αs) LO+PS (µ+PDF)s 0 GF NLO+PS/LO+PS (with total uncertainties) NLO+PS (µ+PDF+αS) + NLO+HERWIG6 0- 0+ (shape comparison) µR,F PDF+αs LO+PS (µ+PDF) µR,F PDF+αs LO+PS (µ+PDF) • VBF-like cuts enhance the MadGraph5_aMC@NLO 0.05 MadGraph5_aMC@NLO Jet correlations in X0jj 0.15 t-channel gluon exchange, which is more sensitive to CP Hagiwara, Li, Mawatari, arXiv:0915.4314 • NLO corrections are large, (~30%) and not flat GF NLO+PS/LO+PS (with total uncertainties) π/2 π NLO+PS (µ+PDF+αs) LO+PS (µ+PDF) 0+ | ∆φ(j1,j2) | 22 LHCPhenoNet pT(X0) > 200 GeV pT(X0) > 200 GeV 0± 0 0± 0 0.09 0.16 0.08 0.14 Spin correlation effects ! in t tX ̄ 0 0.07 0.12 0.06 0.10 0.04 0.02 0.20 pp→ttX0 at the LHC13 0.00 0.18 NLO+HERWIG6 µR,F 0+ (SM) 0-± 0 PDF+αs 0- µR,F -0.10 1.00 -0.20 0.50 0.20 2.00 0.10 1.50 0.00 -0.10 1.00 -0.20 0.50 0.20 2.00 0.10 1.50 0.00 -0.10 1.00 -0.20 0.50 2.00 0.00 0.10 NLO+HERWIG6 0± µR,F PDF+αs NLO+PS/LO+PS (with total uncertainties) ttX0 uncertainties, NLO+PS + PDF+αs NLO+PS (µ+PDF+αs) µR,F LO+PS (µ+PDF) 0 0- 0 NLO+PS (µ+PDF+αs) ± 0± 0 NLO+PS (µ+PDF+αs) µR,F µR,F PDF+αs LO+PS (µ+PDF) PDF+αs LO+PS (µ+PDF) 0 ttX0 NLO+PS/LO+PS 1 2 (with total uncertainties) 3 4 5 + NLO+PS |(µ+PDF+α LO+PS (µ+PDF) 0 ∆η(jb,jb-s)) | 1.50 Marco Zaro, 30-09-2014 -0.20 0.06 PDF+αs 0.20 0.04 0.10 0.00 0.02 -0.10 0.00 -0.20 0.20 2.00 0.10 1.50 0.00 pp→ttX0 at the LHC13 pT(X0) > 200 GeV ttX0 uncertainties, NLO+PS 0+ (shape comparison) decay products kept with MadSpin! 0+ (SM) 0-± 0 PDF+αs µR,F • Spin correlations of the top 0.00 0.07 -0.10 MadGraph5_aMC@NLO 0.10 0.20 0.10 0.08 0.00 -0.10 0.06 -0.20 0.01 0.11 0.09 0.20 0.08 0.10 0.10 0.14 0.00 -0.10 0.12 -0.20 0.02 0.20 0.05 0.10 0.00 0.04 -0.10 -0.20 0.03 0- µR,F PDF+αs 0± µR,F PDF+αs 0.20 0.02 0.10 0.00 0.01 -0.10 0.00 -0.20 0.20 2.00 0.10 1.50 0.00 -0.10 1.00 -0.20 0.50 0.20 2.00 0.10 1.50 0.00 -0.10 1.00 -0.20 0.50 0.20 2.00 0.10 1.50 0.00 -0.10 1.00 -0.20 0.50 -1.0 2.00 1.50 1.00 Artoisenet, Frederix, Mattelaer, Rietkerk, arXiv:1212.3460 MadGraph5_aMC@NLO 0.16 0.20 pT(X0) > 200 GeV ttX0 uncertainties, NLO+PS 0+ (shape comparison) 0.03 NLO+PS/LO+PS (with total uncertainties) ttX0 uncertainties, NLO+PS + PDF+αs NLO+PS (µ+PDF+αs) µR,F LO+PS (µ+PDF) 0 • Requiring a boosted Higgs • reduces CP sensitivity for angular correlations! NLO effects of ~20%, not flat 0.11 pp→ttX0 at the LHC13 0.10 NLO+HERWIG6 (shape comparison) 0+ (SM) 0-± 0 acceptance cuts only 0.09 0- 0 NLO+PS (µ+PDF+αs) µR,F PDF+αs LO+PS (µ+PDF) 0.08 0.07 0.06 MadGraph5_aMC@NLO 0.06 0.04 MadGraph5_aMC@NLO 0.08 MadGraph5_aMC@NLO 0.05 0.05 ± 0± 0 NLO+PS (µ+PDF+αs) µR,F PDF+αs LO+PS (µ+PDF) 0.04 0.03 0.02 0.01 ttX0 NLO+PS/LO+PS (with0.0 total uncertainties) -0.5 0.5 1.0 + + s_) NLO+PS (µ+PDF+α LO+PS (µ+PDF) 0 cos θ(l ,l ) 23 0.00 -1.0 -0.5 0.0 _ cos θ(l+,l ) 0.5 1.0 LHCPhenoNet ! Do it yourself! • The code for the shown processes can be automatically generated with MadGraph5_aMC@NLO (available at http://amcatnlo.cern.ch )! • The HC-NLO model (with UV/R2 counterterms) is publicly available on the FeynRules database https://feynrules.irmp.ucl.ac.be/wiki/HiggsCharacterisation! • E.g. t tX ̄ 0: Marco Zaro, 30-09-2014 24 LHCPhenoNet Do it yourself! • The code for the shown processes can be automatically generated with MadGraph5_aMC@NLO (available at http://amcatnlo.cern.ch )! • The HC-NLO model (with UV/R2 counterterms) is publicly available on the FeynRules database https://feynrules.irmp.ucl.ac.be/wiki/HiggsCharacterisation! • E.g. t tX ̄ 0: > import model HC-NLO! > generate p p > X0 t t~ [QCD] Marco Zaro, 30-09-2014 24 LHCPhenoNet Conclusions • After the discovery of the Higgs boson, huge efforts have been set up in order to tell wether it is the SM Higgs! • EFT is a powerful tool for understanding the spin/CP/ coupling nature of the Higgs! • No hypotheses on the NP! • Can be improved beyond the LO! • HC-EFT approach applied to all the main Higgs production channels, including NLO+PS QCD corrections! • Model publicly available and easy to use with MadGraph5_aMC@NLO ! • The best is yet to come! (aka let’s wait for LHC13 data) Marco Zaro, 30-09-2014 25 LHCPhenoNet Thank you for your attention! Marco Zaro, 30-09-2014 26 LHCPhenoNet Backup slides Marco Zaro, 30-09-2014 27 LHCPhenoNet NLO: how to? Marco Zaro, 30-09-2014 28 LHCPhenoNet NLO: how to? d Marco Zaro, 30-09-2014 n N LO = d n LO + d 28 n V + Z d 1 d n+1 R LHCPhenoNet NLO: how to? d n N LO = d n LO + d n V + Z d 1 d n+1 R • Warning! Real emission ME is divergent!! • Divergences cancel with those from virtuals (in D=4-2eps)! • Need to cancel them before numerical integration (in D=4) Marco Zaro, 30-09-2014 28 LHCPhenoNet NLO: how to? d n N LO = d n LO + d n V + Z d 1 d n+1 R • Warning! Real emission ME is divergent!! • Divergences cancel with those from virtuals (in D=4-2eps)! • Need to cancel them before numerical integration (in D=4) • Structure of divergences is universal: (p + k) = 2Ep Ek (1 cos ✓pk ) p + k p 2 k lim |Mn+1 |2 ' |Mn |2 P AP (z) p//k 2 lim |Mn+1 | ' k!0 Marco Zaro, 30-09-2014 28 X ij |Mnij |2 p i pj pi k p j k LHCPhenoNet NLO: how to? d Marco Zaro, 30-09-2014 n N LO = d n LO + d 29 n V + Z d 1 d n+1 R LHCPhenoNet NLO: how to? d d n N LO n N LO =d = n LO d n LO +d n V + Z d d 1 Z n+1 + d 1d R Z C + d 1 C +d n V n+1 R • Add local counterterms in the singular regions and subtract its integrated finite part (poles will cancels against the virtuals)! • The n and n+1 body integral now are finite in 4 dimension! • Can be integrated numerically Marco Zaro, 30-09-2014 29 LHCPhenoNet NLO: how to? d d n N LO n N LO =d = n LO d n LO +d n V + Z d d 1 Z n+1 + d 1d R Z C + d 1 C +d n V n+1 R • Add local counterterms in the singular regions and subtract its integrated finite part (poles will cancels against the virtuals)! • The n and n+1 body integral now are finite in 4 dimension! • Can be integrated numerically How to do this in an efficient way? Marco Zaro, 30-09-2014 29 LHCPhenoNet The FKS subtraction Frixione, Kunszt, Signer, arXiv:hep-ph/9512328 • Soft/collinear singularities arise in many PS regions! • Find parton pairs i, j that can give collinear singularities! • Split the phase space into regions with one collinear sing! are split into the collinear ones! • Soft singularities X X X ! ! ! 2 |M | = 2 ij Sij |M | = Sij ! 1 if ki · kj ! 0 ij 2 |M |ij Sij = 1 Sij ! 0 if km6=i · kn6=j ! 0 • Integrate them independently! • Parallelize integration! • Choose ad-hoc phase space parameterization! • Advantages:! • # of contributions ~ n^2! • Exploit symmetries: 3 contributions for X Marco Zaro, 30-09-2014 30 Y > ng LHCPhenoNet Loops: the OPP Method Ossola, Papadopoulos, Pittau, arXiv:hep-ph/0609007 & arXiv:0711.3596 • Passarino & Veltman reduction:! • Write the amplitude at the integral level as linear combination of 1-...-4-point scalar integrals! A(q) m X1 = d(i0 i1 i2 i3 )D0 (i0 i1 i2 i3 ) m X1 + c(i0 i1 i2 )C0 (i0 i1 i2 ) kn i0 <i1 <i2 + m X1 i0 <i1 + m X1 q + k1 q D0 Dm b(i0 i1 )B0 (i0 i1 ) k2 k1 i0 <i1 <i2 <i3 1 D1 .. D2 . D3 k3 k4 q + . . . + k5 ! ! ! ! ! ! ! ! k5 a(i0 )A0 (i0 ) i0 + R • Do this at the integrand level Marco Zaro, 30-09-2014 31 LHCPhenoNet Loops: the OPP Method Ossola, Papadopoulos, Pittau, arXiv:hep-ph/0609007 & arXiv:0711.3596 • Sample the numerator at complex values of the loop momenta in • • order to reconstruct the a,b,c,d coefficients and part of the rational terms (R1)! Use CutTools: fed with the loop numerator outputs the coefficients of the scalar integrals and CC rational terms (R1)! Add R2-rational terms/UV counterterms ! • Model dependent but process-independent Marco Zaro, 30-09-2014 32 LHCPhenoNet Loop ME evaluation: MadLoop Hirschi et al. arXiv:1103.0621 • Load the NLO UFO model! • Generate Feynman diagrams to evaluate the loop ME! • Add R2/UV renormalisation counter terms! • Interface to CutTools or to tensor reduction programs (in progress)! if needed)! • Check PS point stability (and switch to QP Cascioli, Maierhofer, Pozzorini Improved with the OpenLoops method! • arXiv:1111.5206 • And much more (can be used as standalone or external OLP via the BLHA, handle loop-induced processes, …) Marco Zaro, 30-09-2014 33 LHCPhenoNet Matching in ! MC@NLO • Use suitable counterterms to avoid double counting the emission from shower and ME, keeping the correct rate at order αs:! !d ! M C@N LO dO ! = ✓ B+V + Z d 1M C ◆ d n n IM C (O) + (R S-events ! ⌅ tM C , z M C , ⇤ MC = ⌅ 1 1 tM C n d 1 n+1 IM C (O) H-events • MC depends on the PSMC’s Sudakov:! ! M C) d 1 P zM C B 2⇥ 2⇥ s • Available for Herwig6, Pythia6 (virtuality-ordered), Herwig++, Pythia8 (in the new release)! • MC acts as local counterterm! • Some weights can be negative (unweighting up to sign)! • Only affects statistics Marco Zaro, 30-09-2014 34 LHCPhenoNet