Conformal Standard Model
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1 K.A. Meissner, Conformal Standard Model p. 1/13 Conformal Standard Model Krzysztof A. Meissner University of Warsaw AEI Potsdam HermannFest, AEI,
2 K.A. Meissner, Conformal Standard Model p. 2/13 Hierarchy Problem Standard Model is conformally invariant except for the tree level Higgs mass term m 2 Φ Φ
3 K.A. Meissner, Conformal Standard Model p. 2/13 Hierarchy Problem Standard Model is conformally invariant except for the tree level Higgs mass term m 2 Φ Φ Quantum corrections m 2 Λ 2 why m M P? (with UV cutoff Λ = scale of new physics )
4 K.A. Meissner, Conformal Standard Model p. 2/13 Hierarchy Problem Standard Model is conformally invariant except for the tree level Higgs mass term m 2 Φ Φ Quantum corrections m 2 Λ 2 why m M P? (with UV cutoff Λ = scale of new physics ) Most popular proposal: SM (N)MSSM (but LHC does not seem to pointedly like it...)
5 Hierarchy Problem Standard Model is conformally invariant except for the tree level Higgs mass term m 2 Φ Φ Quantum corrections m 2 Λ 2 why m M P? (with UV cutoff Λ = scale of new physics ) Most popular proposal: SM (N)MSSM (but LHC does not seem to pointedly like it...) conformal symmetry also solves the HP: only 2 new parameters (MSSM 116) built-in breaking (conf. anomaly, Coleman-Weinberg) K.A. Meissner, Conformal Standard Model p. 2/13
6 Conformal Standard Model assumptions K.A. Meissner, Conformal Standard Model p. 3/13 K.A.M., H. Nicolai, Phys.Lett. B648 (2007) 312 Classical conformal symmetry in SM, all masses from conformal anomaly
7 Conformal Standard Model assumptions K.A. Meissner, Conformal Standard Model p. 3/13 K.A.M., H. Nicolai, Phys.Lett. B648 (2007) 312 Classical conformal symmetry in SM, all masses from conformal anomaly see-saw mechanism for neutrinos
8 Conformal Standard Model assumptions K.A. Meissner, Conformal Standard Model p. 3/13 K.A.M., H. Nicolai, Phys.Lett. B648 (2007) 312 Classical conformal symmetry in SM, all masses from conformal anomaly see-saw mechanism for neutrinos the model viable up to M Pl, no GUTs, no new scales, no low energy SUSY
9 Conformal Standard Model assumptions K.A. Meissner, Conformal Standard Model p. 3/13 K.A.M., H. Nicolai, Phys.Lett. B648 (2007) 312 Classical conformal symmetry in SM, all masses from conformal anomaly see-saw mechanism for neutrinos the model viable up to M Pl, no GUTs, no new scales, no low energy SUSY classical conformal symmetry Ward Ids all corrections logarithmic (Bardeen) K.A.M, H. Nicolai, Phys. Lett. B660 (2008) 260
10 K.A. Meissner, Conformal Standard Model p. 4/13 Nonconformal conformal? we expect at M Pl a non-conformal theory is it possible to get at low energies a (classically) conformal FT + gravity?
11 K.A. Meissner, Conformal Standard Model p. 4/13 Nonconformal conformal? we expect at M Pl a non-conformal theory is it possible to get at low energies a (classically) conformal FT + gravity? example: gauged N = 4 supergravity with κ 0 supergravity + conformal N = 4 SYM K.A.M., H. Nicolai, Phys.Rev. D80:086005,2009
12 K.A. Meissner, Conformal Standard Model p. 5/13 The Model Conformally invariant L = L kin +L : L := ( Li ΦYij E Ej + Q i ǫφ Yij D Dj + Q i ǫφ Yij U Uj + ) + L i ǫφ Yij ν νj R +ϕνit R CY ij M νj R +h.c. λ 1 4 (Φ Φ) 2 λ 2 2 ϕ 2 (Φ Φ) λ 3 4 ϕ 4
13 K.A. Meissner, Conformal Standard Model p. 5/13 The Model Conformally invariant L = L kin +L : L := ( Li ΦYij E Ej + Q i ǫφ Yij D Dj + Q i ǫφ Yij U Uj + ) + L i ǫφ Yij ν νj R +ϕνit R CY ij M νj R +h.c. λ 1 4 (Φ Φ) 2 λ 2 2 ϕ 2 (Φ Φ) λ 3 4 ϕ 4 Y M ij O(1), Y ν ij O(10 6 ) (see-saw)
14 K.A. Meissner, Conformal Standard Model p. 5/13 The Model Conformally invariant L = L kin +L : L := ( Li ΦYij E Ej + Q i ǫφ Yij D Dj + Q i ǫφ Yij U Uj + ) + L i ǫφ Yij ν νj R +ϕνit R CY ij M νj R +h.c. λ 1 4 (Φ Φ) 2 λ 2 2 ϕ 2 (Φ Φ) λ 3 4 ϕ 4 Y M ij O(1), Y ν ij O(10 6 ) (see-saw) new (complex) scalar necessary!
15 K.A. Meissner, Conformal Standard Model p. 6/13 The Model Standard Model + very light neutrinos + heavy neutrinos ( 1 TeV)) + complex new scalar
16 K.A. Meissner, Conformal Standard Model p. 6/13 The Model Standard Model + very light neutrinos + heavy neutrinos ( 1 TeV)) + complex new scalar Calculation of the CW effective action numerical analysis (no 2 loops...)
17 K.A. Meissner, Conformal Standard Model p. 6/13 The Model Standard Model + very light neutrinos + heavy neutrinos ( 1 TeV)) + complex new scalar Calculation of the CW effective action numerical analysis (no 2 loops...) BEH mechanism for EW symm. Φ 0 SSB of the lepton number symm. ϕ 0
18 K.A. Meissner, Conformal Standard Model p. 6/13 The Model Standard Model + very light neutrinos + heavy neutrinos ( 1 TeV)) + complex new scalar Calculation of the CW effective action numerical analysis (no 2 loops...) BEH mechanism for EW symm. Φ 0 SSB of the lepton number symm. ϕ 0 axion (pseudo)gb of global lepton number symmetry L i e iα L i, E i e iα E i, ν i R e iα ν i R, ϕ e 2iα ϕ
19 K.A. Meissner, Conformal Standard Model p. 7/13 Results At the minimum Higgs and the new scalar mix H = Hcosβ+φsinθ, φ = Hsinβ+φcosθ of masses M 1 and M 2. K.A.M., H. Nicolai, Phys.Lett. B648 (2007) 312
20 Results At the minimum Higgs and the new scalar mix H = Hcosβ+φsinθ, φ = Hsinβ+φcosθ of masses M 1 and M 2. K.A.M., H. Nicolai, Phys.Lett. B648 (2007) 312 propagator { icos 2 θ p 2 M1 2 +im 1Γ SM (M 1 )cos 2 θ + cosθ sinθ M 1 M 2 } in cross section there should be two bumps : heights as for Higgs widths smaller by cos 2 (sin 2 )θ K.A. Meissner, Conformal Standard Model p. 7/13
21 K.A. Meissner, Conformal Standard Model p. 8/13 Phenomenology no other new particles at LHC except standard Higgs and new scalar
22 K.A. Meissner, Conformal Standard Model p. 8/13 Phenomenology no other new particles at LHC except standard Higgs and new scalar LHC has announced the mass 125 GeV (M 1?)
23 K.A. Meissner, Conformal Standard Model p. 8/13 Phenomenology no other new particles at LHC except standard Higgs and new scalar LHC has announced the mass 125 GeV (M 1?) CDF has seen a 5σ excess of events 2Z l + l l + l at the same invariant mass 325 GeV we conjecture that it is a narrow resonance corresponding to φ (M 2 = 325 GeV?) K.A.M., H. Nicolai, arxiv: [hep-ph]
24 CDF 4 lepton cases K.A. Meissner, Conformal Standard Model p. 9/13
25 K.A. Meissner, Conformal Standard Model p. 10/13 Axion K.A.M., H. Nicolai, Eur.Phys.J.C57:493,2008 axion: phase of the new scalar φ Goldstone boson of spontaneously broken lepton number symmetry
26 K.A. Meissner, Conformal Standard Model p. 10/13 Axion K.A.M., H. Nicolai, Eur.Phys.J.C57:493,2008 axion: phase of the new scalar φ Goldstone boson of spontaneously broken lepton number symmetry the aγγ coupling is calculable and very small (because of small neutrino masses!) α wαm ν 8π 2 M 2 W a E B GeV 1 a E B
27 K.A. Meissner, Conformal Standard Model p. 10/13 Axion K.A.M., H. Nicolai, Eur.Phys.J.C57:493,2008 axion: phase of the new scalar φ Goldstone boson of spontaneously broken lepton number symmetry the aγγ coupling is calculable and very small (because of small neutrino masses!) α wαm ν 8π 2 M 2 W a E B GeV 1 a E B agg coupling (calculable) non-local, for small momenta anomaly solution of the strong CP problem
28 Axion K.A.M., H. Nicolai, Eur.Phys.J.C57:493,2008 axion: phase of the new scalar φ Goldstone boson of spontaneously broken lepton number symmetry the aγγ coupling is calculable and very small (because of small neutrino masses!) α wαm ν 8π 2 M 2 W a E B GeV 1 a E B agg coupling (calculable) non-local, for small momenta anomaly solution of the strong CP problem a very good candidate for CDM K.A. Meissner, Conformal Standard Model p. 10/13
29 K.A. Meissner, Conformal Standard Model p. 11/13 Axion coupling to gluons g p 1 u L W ν L /ν R u L d L e L q a g p 2 u L W ν L /ν R A. Latosiński, K.A.M., H. Nicolai, arxiv: [hep-ph]
30 K.A. Meissner, Conformal Standard Model p. 12/13 Summary assumption of classical CS solves problems of SM (hierarchy, strong CP,...)
31 K.A. Meissner, Conformal Standard Model p. 12/13 Summary assumption of classical CS solves problems of SM (hierarchy, strong CP,...) the model has 1 more parameter than SM (MSSM 116) and uses quantum symmetry breaking (conformal anomaly)
32 K.A. Meissner, Conformal Standard Model p. 12/13 Summary assumption of classical CS solves problems of SM (hierarchy, strong CP,...) the model has 1 more parameter than SM (MSSM 116) and uses quantum symmetry breaking (conformal anomaly) it has a definite (unique) prediction for LHC 2 scalars with SM Higgs cross sections scaled by cos 2 (sin 2 )θ, no other particles
33 K.A. Meissner, Conformal Standard Model p. 12/13 Summary assumption of classical CS solves problems of SM (hierarchy, strong CP,...) the model has 1 more parameter than SM (MSSM 116) and uses quantum symmetry breaking (conformal anomaly) it has a definite (unique) prediction for LHC 2 scalars with SM Higgs cross sections scaled by cos 2 (sin 2 )θ, no other particles there is an extremely light and weakly coupled particle (axion)
34 Summary assumption of classical CS solves problems of SM (hierarchy, strong CP,...) the model has 1 more parameter than SM (MSSM 116) and uses quantum symmetry breaking (conformal anomaly) it has a definite (unique) prediction for LHC 2 scalars with SM Higgs cross sections scaled by cos 2 (sin 2 )θ, no other particles there is an extremely light and weakly coupled particle (axion) if true the CSM is a theory descending directly from the Planck scale K.A. Meissner, Conformal Standard Model p. 12/13
35 HAPPY BIRT HDAY! K.A. Meissner, Conformal Standard Model p. 13/13
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