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Gauged Axions

Gauged Axions. Claudio Coriano’ Physics Department University of Salento, INFN Lecce. Outline I will describe the general features of anomalous models which are characterized by the presence of gauged axions in their spectra. These models have been studied in the

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Gauged Axions

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  1. Gauged Axions Claudio Coriano’ Physics Department University of Salento, INFN Lecce

  2. Outline I will describe the general features of anomalous models which are characterized by the presence of gauged axions in their spectra. These models have been studied in the context of intersecting branes, but can have a rather general (and independent) origin, if the decoupling of chiral fermions from an anomaly free theory, which takes to these models, follows a specific path. (Guzzi, C.C., 2009) In this sense, the lagrangeans that I will describe are rather general and summarize all the basic features of a “universality class” of models which provide a generalization of the Peccei-Quinn theory. The PQ axion Gauged axions and anomalous U(1)’s Gauged axions from intersecting branes Gauged axions from decoupled fermions Local and non-local versions of the anomaly cancellation mechanism. Conformal and gauge anomalies.

  3. Nikos Irges INFN Lecce, Roberta Armillis, Marco Guzzi Luigi Delle Rose Antonio Mariano Simone Morelli Irges, Kiritsis, C.C. 2005 (Crete)

  4. 1) Stuckelberg axions and the effective action of anomalous Abelian models. 1. A Unitarity analysis of the Higgs-axion mixing. JHEP 0707:008,2007. 68 pp 2) Stuckelberg Axions and the Effective Action of Anomalous Abelian Models 2. A SU(3)C x SU(2)W x U(1)Y x U(1)B model and its signature at the LHC. 72 pp Nucl.Phys.B789:133-174,2008. 3) Trilinear Anomalous Gauge Interactions from Intersecting Branes and the Neutral Currents Sector. 68pp. Published in JHEP 0805:015,2008. with Armillis, Guzzi 4) Unitarity Bounds for Gauged Axionic Interactions and the Green-Schwarz Mechanism. 50pp.Published in Eur.Phys.J.C55:629-652,2008. with Guzzi and Morelli 5) Axions and Anomaly-Mediated Interactions: The Green-Schwarz and Wess-Zumino Vertices at Higher Orders and g-2 of the muon. Lecce) . Aug 2008. 52pp. Published in JHEP 0810:034,2008, with Armillis, Guzzi and Morelli 6) An Anomalous Extra Z Prime from Intersecting Branes with Drell-Yan and Direct Photons at the LHC. Sep 2008. 46pp.Published in Nucl.Phys.B814:15679,2009. With Armillis, Guzzi and Morelli

  5. 7) A Light Supersymmetric Axion in an Anomalous Abelian Extension of the Standard Model. 46 pp. (2008) Phys. Rev. D 2009, with Guzzi, Mariano and Morelli 8) Axions from Intersecting Branes and Decoupled Chiral Fermions at the Large Hadron Collider. Claudio Coriano, Marco Guzzi . e-Print: arXiv:0905.4462 [hep-ph], with M. Guzzi 9 ) Anomalous U(1) Models in Four and Five Dimensions and their Anomaly Poles. Roberta Armillis, Claudio Coriano, Luigi Delle Rose, Marco Guzzi .. e-Print: arXiv:0905.0865 [hep-ph] , with Armillis, Guzzi and Delle Rose Connection between gauge and conformal anomalies in these models 10) “Conformal Anomalies and the Gauge Contributions To the Gravitational effective action “ Armillis, Delle Rose, C.C., to appear

  6. ….Plenty of U(1)’s also in anomaly-free constructions The question is: if we find extra neutral currents at the LHC how do we discover if a different mechanism of anomaly cancelation is at work?

  7. Goal: to study the effective field theory of • a class of brane models containing a gauge structure of the form • SM x U(1) x U(1) x U(1) • SU(3) x SU(2) x U(1)Y x U(1)….. • corresponding to a certain class of vacua in string theory • These models are the object of an intense scrutiny by • many groups working on intersecting branes. • See. E. Kiritsis’ review on Phys. Rep. • These analysis focused on general (mostly geometrical) features of these models. • One has to be careful though: these axions are not necessarily physical fields. • First identification of a physical Axion in these models in the • non-supersymmetric case is in (Irges, Kiritsis, C.C., 2005). • The physical axion was called “The Axi Higgs” and the model • Minimal Low Scale Orientifold Model (MLSOM). • In the supersymmetric case, the construction • Needs a special form of superpotential, typical of the NMSSM. The model is called • the USSM-A (Mariano, Irges, Guzzi, C.C.) • Another SUSY extension is in Anastasopoulos,Fucito, Lionetto, Racioppi, Stanev. • based on previous formulations by Zagermann and Coll.

  8. Standard Model Anomalies As we have mentioned, one of the most interesting realizations of the class of anomalous theories contining anomalous U(1)’s are obtained from intersecting branes.

  9. Widths are small for small coupling (Faraggi, Guzzi, C.C., PRD 2008) We need extra information in order to capture the nature of the Extra Z prime (if it exists).

  10. Neutral current sector Why it is important and how to detect it at the LHC Guzzi, Cafarella, C.C. To discover neutral currents at the LHC, we need to know the QCD background with very high accuracy. Much more so if the resonance is in the higher-end in mass (5 TeV). NNLO in the parton model pp -> lepton +anti-lepton Excellent statistics. Theoretical error larger than exp.

  11. Withs are quite small g has to be O(1) Guzzi, Morelli, C.C.

  12. CANDIA, can be downloded www.le.infn.it/~candia NNLO evolution in x-space

  13. Gauged axions are naturally associated to anomalous symmetries. We can consider U(1) extensions of the Standard Model and compensate the anomalous variation of the effective action with Wess Zumino counterterms SIGNATURES at the LHC New trilinear gauge interactions Anomalous Extra Z prime’s One gauged axion In the supersymmetric case (UMSSM-A) We have axions and neutralinos as possible dark matter candidates. These models provide an extension of the (NMSSM) with an anomalous U(1) symmetry, a Stuckelberg multiplet, possible kinetic mixing etc.

  14. Wess-Zumino case. Trilinear gauge interaction CS terms

  15. Excellent domain: 4-fermion processes LO NLO

  16. The Peccei-Quinn axion Peccei and Quinn  U(1)PQ symmetry the axion as a pseudo Goldstone boson The mass and the coupling of the axion to photons depend on the SAME scale fa Astrophysical constraint linked to the stellar evolution Cosmological constraint given by the dark energy amount

  17. Solution of the strong CP problem Total lagrangean: axion + theta term Anomalous contribution due to U(1)_PQ Axion field is driven by the instanton potential

  18. The “gauged” axion We obtain a “gauged” axion by promoting the U(1)PQ global symmetry to a local one The mass and the coupling of the gauged axion are independent. This may allow to evade the constraints from CAST and other experiments and/or astrophysical bounds However: The presence of an axion-like particle is an indication of of a different mechanism of anomaly cancelation at work. At field theory level we have two possible versions of this “mechanism” 1) a local subtraction via a Wess-Zumino term 2) a nonlocal subtraction (subtraction of an anomaly pole)

  19. One or two axions? with Guzzi and Morelli

  20. anomaly cancellation mechanism(s) 1) Fermion charge assignment (anomaly free) 2) Wess-Zumino (anomalous) + physical axion (axion-like particle) 3) Green Schwarz (physical/unphysical axion ? Is it consistent with unitarity?) (GS involves a re-definition of the anomalous vertices of a given theory) Wess Zumino: axion Subtraction of an anomaly pole Armillis, Guzzi, C.C., Armillis, Delle Rose, Guzzi, C.C.

  21. This cancellation is identical only for special kinematics BIM amplitudes. Use these amplitudes to detect The non-unitary behaviour of the theory

  22. Re-defined vertex Redefined BIM amplitude. It is zero only for on-shell scattering of massless gauge bosons Digrammatic expansion The re-definition removes the anomaly pole from the vertex. In the UV this is always possible, but is an over subtraction in the IR

  23. Description with two axions This description renders the lagrangean local but at a costt

  24. The cost: a ghost Negative kinetic energy term (Federbush) Similar results in the case of the conformal anomaly Two pseudoscalars to re-express the conformal anomalous contribution in Gravity (Giannotti and Mottola, PRD 2009). In this case the authors claim consistency of this reformulation, wth the two field interpreted as collinear fermion antifermion states. I believe that these local formulations always have a ghost in the spectrum.

  25. Is there a way to unitarize the amplitude? Yes, but at a cost. The example The subtraction, however, is well defined in the UV, but leaves, In some cases an infrared pole coupled In the infrared. (Armillis, Delle Rose, Guzzi, C.C.)

  26. Similar situation in gravity To see the poles (the virtual axion) you need to keep all the terms in the effective Action Armillis, Delle Rose, C.C.

  27. 1/m captures the correct physics Euler Heisenberg In the anomalous case this is not true any longer

  28. But there is neverthless a pole The extra terms are given In our paper Armillis et al

  29. Gravity: same story (Conformal anomaly) Riegert The anomaly pole is here

  30. Linearized gravity Mottola, Giannotti, 2009 Anomaly poles from the loops of TJJ

  31. Specify the realization of the “anomaly cancellation mechanism” Pole subtraction Wess Zumino Asymptotic axion

  32. The effective actions in the two cases are rather different. The only actions which have been studied so far are of type 1). (MLSOM) They involve WZ terms and are characterized by a unitarity bound which is strongly sensitive on the coupling of the anomalous U(1) (anomalous) symmetry. In general, each anomalous U(1) symmetry requires an axion which acquires a kinetic term via a Stuckelberg mass term for the corresponding anomalous gauge boson

  33. The MLSOM

  34. Counterterms can be fixed using BRST invariance. JHEP 2008 Armillis, Guzzi, CC

  35. The SU(3)xSU(2)xU(1)xU(1) Model kinetic Higgs doublets L/R fermion CS GS Higgs-axion mixing Irges, Kiritsis, C. Stueckelberg

  36. No v/M corrections on first row SM-like 1/M O(M)

  37. CP even CP odd

  38. Some properties of the axi-Higgs: Yukawa couplings Induces the decay of the Axi-Higgs, similar to Higgs decay

  39. 1 physical axion, The Axi-Higgs GS Axions N Nambu-Goldstone modes

  40. The Stuckelberg are NOT necessarily physical fields. Their nature is identified after electroweak symmetry breaking When the anomalous gauge boson acquires an additional Mass correction due to the Higgs vev

  41. (Guzzi, Morelli, C.C.) Unitarity Bounds Bouchiat-Iliopoulos-Meyer amplitudes (BIM amplitudes) The WZ mechanism does not protect the theory from the non-unitary behaviour of these amplitudes

  42. Unitarity bound in the WZ case: gluon-gluon to gamma gamma

  43. Same behaviour for a varying Tan-beta

  44. CP-odd sector in the WZ mechanism (MLSOM) SU(3) x SU(2) x U(1)_Y x U(1)_B

  45. Models can be built without any string construction. Phenomenologically The specific charges are not relevant (Guzzi, C.C.) Combine axion countertemrs (C’s) Anomaly cancellation conditions And gauge invariance to fix the model We obtain 10 eqs. That allows a clas sof charge assignments

  46. Difference of the Higgs charges under the anomallous U(1)_B WZ counterterms fixed in terms of charge difference Guzzi, C.C.

  47. The Madrid model is a special case of this general approach

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