CUSTODIAL SYMMETRY IN THE STANDARD MODEL AND BEYOND V. Pleitez Instituto de Física Teórica/UNESP Modern Trends in Field Theory João Pessoa ─ Setembro 2006.

Slides:



Advertisements
Similar presentations
Z’ Production in 331 models
Advertisements

THE FINE-TUNING PROBLEM IN SUSY AND LITTLE HIGGS
Effective Operators in the MSSM Guillaume Drieu La Rochelle, LAPTH.
Searching for Doubly-Charged Higgs at the LHC Sá Borges, Cieza Montalvo Mauro Tonasse Nelson Cortez Universidade do Estado do Rio de Janeiro - Instituto.
TeV scale see-saws from higher than d=5 effective operators Neutrino masses and Lepton flavor violation at the LHC Würzburg, Germany November 25, 2009.
Hep-ph/ , with M. Carena (FNAL), E. Pontón (Columbia) and C. Wagner (ANL) New Ideas in Randall-Sundrum Models José Santiago Theory Group (FNAL)
Chiral freedom and the scale of weak interactions.
The minimal B-L model naturally realized at TeV scale Yuta Orikasa(SOKENDAI) Satoshi Iso(KEK,SOKENDAI) Nobuchika Okada(University of Alabama) Phys.Lett.B676(2009)81.
The classically conformal B-L extended standard model Yuta Orikasa Satoshi Iso(KEK,SOKENDAI) Nobuchika Okada(University of Alabama) Phys.Lett.B676(2009)81.
Higgs Boson Mass In Gauge-Mediated Supersymmetry Breaking Abdelhamid Albaid In collaboration with Prof. K. S. Babu Spring 2012 Physics Seminar Wichita.
Higgs Quadruplet for Type III Seesaw and Implications for → e and −e Conversion Ren Bo Coauther : Koji Tsumura, Xiao - Gang He arXiv:
F. Richard Feb 2003 A Z’ within the ‘Little Higgs’ Scenario The LHC/LC Study group meeting CERN.
Chiral freedom and the scale of weak interactions.
Richard Howl The Minimal Exceptional Supersymmetric Standard Model University of Southampton UK BSM 2007.
Fermion Masses and Unification Steve King University of Southampton.
The Top Quark and Precision Measurements S. Dawson BNL April, 2005 M.-C. Chen, S. Dawson, and T. Krupovnikas, in preparation M.-C. Chen and S. Dawson,
4 th Generation Leptons in Minimal Walking Technicolor Theory Matti Heikinheimo University of Jyväskylä.
Chiral freedom and the scale of weak interactions.
Chiral freedom and the scale of weak interactions.
.. Particle Physics at a Crossroads Meenakshi Narain Brown University.
Aug 29-31, 2005M. Jezabek1 Generation of Quark and Lepton Masses in the Standard Model International WE Heraeus Summer School on Flavour Physics and CP.
 Collaboration with Prof. Sin Kyu Kang and Prof. We-Fu Chang arXiv: [hep-ph] submitted to JHEP.
Relating dark matter and radiative Seesaw neutrino mass scales without beyond SM gauge symmetry Xiao-Gang He 1. Introduction 2. Radiative seesaw and dark.
Seesaw Neutrino mass and U(1) symmetry Rathin Adhikari Centre for Theoretical Physics Jamia Millia Islamia Central University New Delhi : arXiv:
Fermion Masses and Unification Steve King University of Southampton.
Electroweak interaction
Center for theoretical Physics at BUE
A Composite Little Higgs ZACKARIA CHACKO UNIVERSITY OF MARYLAND, COLLEGE PARK Puneet Batra.
2. Two Higgs Doublets Model
Takehiro Nabeshima University of Toyama ILC physics general meeting 9 jun Phenomenology at a linear collider in a radiative seesaw model from TeV.
Hep-ph/ , with M. Carena (FNAL), E. Pontón (Columbia) and C. Wagner (ANL) Light KK modes in Custodially Symmetric Randall-Sundrum José Santiago Theory.
Wednesday, Apr. 23, 2003PHYS 5326, Spring 2003 Jae Yu 1 PHYS 5326 – Lecture #24 Wednesday, Apr. 23, 2003 Dr. Jae Yu Issues with SM picture Introduction.
Electroweak Precision Measurements and BSM Physics: (A) Triplet Models (B) The 3- and 4-Site Models S. Dawson (BNL) February, 2009 S. Dawson and C. Jackson,
1 Supersymmetry Yasuhiro Okada (KEK) January 14, 2005, at KEK.
1 THEORETICAL PREDICTIONS FOR COLLIDER SEARCHES “Big” and “little” hierarchy problems Supersymmetry Little Higgs Extra dimensions G.F. Giudice CERN.
Twin Higgs Theories Z. Chacko, University of Arizona H.S Goh & R. Harnik; Y. Nomura, M. Papucci & G. Perez.
WHAT BREAKS ELECTROWEAK SYMMETRY ?. We shall find the answer in experiments at the LHC? Most likely it will tells us a lot about the physics beyond the.
X ± -Gauge Boson Production in Simplest Higgs Matthew Bishara University of Rochester Meeting of Division of Particles and Fields August 11, 2011  Simplest.
Neutrino mass and DM direct detection Daijiro Suematsu (Kanazawa Univ.) Erice Sept., 2013 Based on the collaboration with S.Kashiwase PRD86 (2012)
Yukawa and scalar interactions induced by scalar relevant for neutrino masss generation are: Since is assumed to be an exact symmetry of the model has.
weak decays beta decay ofneutron problem energy and momentum not conserved e n p.
1 Prospect after discoveries of Higgs/SUSY Yasuhiro Okada (KEK) “Discoveries of Higgs and Supersymmetry to Pioneer Particle Physics in the 21 st Century”
H. Quarks – “the building blocks of the Universe” The number of quarks increased with discoveries of new particles and have reached 6 For unknown reasons.
Sally Dawson, BNL Standard Model and Higgs Physics FNAL LHC School, 2006 Introduction to the Standard Model  Review of the SU(2) x U(1) Electroweak theory.
Nobuchika Okada The University of Alabama Miami 2015, Fort Lauderdale, Dec , GeV Higgs Boson mass from 5D gauge-Higgs unification In collaboration.
QFTHEP – A.Beylin, V.Beylin, A.Pivovarov SFU, MIPT Scenarios of Higgs bosons and Z’ manifestations in the minimal gauge extension.
DYNAMICAL GENERATION OF FERMION MASSES AND ITS CONSEQUENCES Jiří Hošek Department of Theoretical Physics Nuclear Physics Institute Rez (Prague) Czech Republic.
? composite ? H. Fritzsch LMU Munich.
Supersymmetric B-L Extended Standard Model with Right-Handed Neutrino Dark Matter Nobuchika Okada Miami Fort Lauderdale, Dec , 2010 University.
1 Why Does the Standard Model Need the Higgs Boson ? II Augusto Barroso Sesimbra 2007.
Monday, Apr. 7, 2003PHYS 5326, Spring 2003 Jae Yu 1 PHYS 5326 – Lecture #20 Monday, Apr. 7, 2003 Dr. Jae Yu Super Symmetry Breaking MSSM Higgs and Their.
The Importance of the TeV Scale Sally Dawson Lecture 3 FNAL LHC Workshop, 2006.
BEYOND MFV IN FAMILY SYMMETRY THEORIES OF FERMION MASSES Work done with Zygmunt Lalak and Graham Ross Based on existing ideas but, hopefully, contributing.
Family Gauge Bosons with an Inverted Mass Hierarchy Yoshio Koide (Osaka University) in collaboration with Toshifumi Yamashita (Maskawa Insititute, KSU)
Renormalization of the Higgs Triplet Model Mariko Kikuchi ( Univ. of Toyama ) Collaborators M. Aoki ( Kanazawa Univ. ), S. Kanemura ( Univ. of Toyama ),
2 nd International Conference on Particle Physics in Memoriam Engin Arık and Her Colleagues Doğuş University, Istanbul, Turkey June nd International.
Lecture 7. Tuesday… Superfield content of the MSSM Gauge group is that of SM: StrongWeakhypercharge Vector superfields of the MSSM.
Physics 222 UCSD/225b UCSB Lecture 12 Chapter 15: The Standard Model of EWK Interactions A large part of today’s lecture is review of what we have already.
M. Frank, K. H., S.K. Rai (arXiv: ) Phys.Rev.D77:015006, 2008 D. Demir, M. Frank, K. H., S.K. Rai, I.Turan ( arXiv: ) Phys.Rev.D78:035013,
DIS2003 A.Tilquin Searches for Physics Beyond the Standard Model at LEP What is the Standard Model Why to go beyond and how Supersymmetry Higgs sector.
and what we unsuccessfully tried to explain (so far)
B-Anomalies related to leptons and LFUV
Classically conformal B-L extended Standard Model
Generating Neutrino Mass & Electroweak Scale Radiatively
The MESSM The Minimal Exceptional Supersymmetric Standard Model
Spontaneous breakdown (SB) of symmetry
Custodial SU(2) Symmetry
Lecture 12 Chapter 15: The Standard Model of EWK Interactions
Weak interactions.
Prospect after discoveries of Higgs/SUSY
Presentation transcript:

CUSTODIAL SYMMETRY IN THE STANDARD MODEL AND BEYOND V. Pleitez Instituto de Física Teórica/UNESP Modern Trends in Field Theory João Pessoa ─ Setembro 2006

OUTLINE  What is the Custodial Symmetry?  Standard Model  Models ...  Conclusions

Automatic or Accidental (Global) Symmetry, are not imposed, consequence of:  Lorentz invariance  Gauge invariance  Renormalizability  Representation content of the model Examples: Baryon number, Lepton number, and approximate chiral symmetries:

STANDARD MODEL’s THREE GENERATIONS:

The fermion mass problem:  Why do weak isospin partners have different masses?  Why are quark and lepton masses split?  Why there is a mass hierarchy between generations, and  Why is there a mixing angle hierarchy in quarks but not in leptons?

PDG 2004 Weak isospin partners u d

The SM answer: the gauge group permits a different Yukawa coupling constantto set each fermion mass and mixing angle. The SM accomodates the problem but does not explain it. this suggests that it should be correlated with the breakdown of a larger symmetry. Weak isospin partners have different masses because the left- and right-handed fields are not related by any symmetry. Before SSB: After SSB: ? u,d generic quarks

a few percent (At the tree level) (Radiative corrections)  -parameter in the SM

a few percent The first is a clear violation of isospin The second one is a consequence of isospin [SU(2)] conservation can be made compatible ? How the following experimental facts The accidental SU(2) (global) symmetry, for its protective functions is called: CUSTODIAL SYMMETRY. (It may, or not, be the isospin.)

STANDARD MODEL’s GAUGE SYMMETRIES: SSB

SSB: ONE SCALAR DOUBLET SCALAR POTENTIAL: 2-doublet:

Global and local: g’=0 (sin  W =0) Global

g’=0

(broken) (conserved) When g’≠0 At the tree level this is a zero order correction: g 0,g’ 0 W 1,W 2,W 3  Z are in a triplet of SU(2) L+R

Fermion loops Radiative correction due to gauge and Higgs bosons are proportional to g’ 2 (or sin 2  W ). For instance, loops of Higgs Due to unbroken SU(2) L+R in the limit g’→0 (sin 2  W =0) the custodial symmetry protects the tree level relation  =1. This correction vanishes in the limit m t =m b

Quark masses in the SM (Yukawa couplings) (we have omitted summation symbols) If all Yukawa couplings  ’s are different the generated Dirac masses in eachcharge sector (weak isospin partners) are different and arbitrary.

Defining the 2-doublets: in the quark sector and in the lepton sector Right-handed neutrinos are needed Extending the custodial symmetry to the Yukawa sector

The Yukawa interactions are now, manisfestly invariant under SU(2) L  SU(2) R, This is a consequence of the custodial SU(2) L+R symmetry

g’≠0 (sin  W ≠0), i.e, turn on the electromagnetic interactions and, as usual

or it is possible that the source of the breakdown of the SU(2) L+R symmetry in the gauge-Higgs bosons system is different from the breakdown of that symmetryin the fermion-Higgs sector. In the latter one, NEW PHYSIC may be at work. M&P (hep-ph/ ): Assume that

New Physics:  New quark singlets of SU(2) L  U(1) Y (generalized seesaw mechanism)  Multi-Higgs doublet extensions  Radiative corrections of a Z’ vector boson  The seesaw mechanism for neutrinos is mandatory (for details see hep-ph/ )

 generalized seesaw mechanism

 Multi-Higgs doublet extensions

Radiative corrections of a Z’ vector boson Breaks the deneracy of charged lepton and neutrino masses

Also in the context of the SM, multi-Higgs extensions The most general scalar structure which naturally (follows from the group structure and representation content... (Glashow-Weinberg)Added for unification at GeV Manohar & Wise, hep-ph/ And...

BEYOND THE STANDARD MODEL

In the context of the standard model: No attempt is made to explain the number of fermion generations from the viewpoint of anomaly cancelation: each generation is anomaly free. Also sin 2  W is a completely arbitrary parameter Among other open problems, the SM does not give an answer to the questions: Why three generations? Why sin 2  W is near ¼?

There are only three active sequential generations (LEP):

PDG 2004 sin 2  W (M Z )= (15) The history of the value of sin 2  W until 1989 Just an accident?

If sin 2  W  1/4 is not na accident there must be an SU(3) symmetry at the TeV scale sin 2  W (µ)=1/4 but sin 2  W (M Z )= (15) By choosing appropriately the representation content of the model: The anomaly cancelation plus the property of asymptotic freedom of QCD the number of generations allowed is three and only three Both problems have answers in the so called models. SU(3) C  SU(2) L  U(1) Y  SU(3) C  SU(3) L  U(1) X STANDARD MODEL3-3-1 MODELS SU(3) L symmetry at an energy scale v  of the order of TeV

New quarks have masses proportional to v  The neutral vector boson Z’ has a mass proportional to v  and also Z’ prime has a mixing with Z of the SM  v  at the TeV scale Goldberger-Treimam Relation valid in the m 2  =0 (chiral limit) D&M&P: PRD73, (2006); PL B637, 85 (2006) v   G F at the Fermi scale (weak interactions) models have an approximate SU(2) L+R custodial symemtry

Ths condition is valid if, and only if, At the tree level (v  >1 TeV), sin  <<1

ILC e+e-  H 1 H 2 (Cieza Montalvo-Tonasse, PRD71, ) ?

Little Higgs, 5D composite Higgs Higgsless models,Little Higgs and 5D composite models: SU(2) that protects  from radiative corrections can also protect the Zbbbar coupling. Agashe et al. hep-ph/ in a Randall-Sundrum scenarios the SU(2) L  SU(2) R and left-right symmetries can be used to make the tree level contributions to the T parameter and the anomalous couplings of the b-quark to the Z very small... M. Carena, et al., hep-ph/

Conclusions  The difference on the weak isospin partners’s masses may be a signal of NEW PHYSICS  Right-handed neutrinos have to added  The seesaw mechanism have to be implemented  Custodial symmetry is important, both in the SM and beyond

Muito obrigado!