1 Why Does the Standard Model Need the Higgs Boson ? II Augusto Barroso Sesimbra 2007.

Slides:



Advertisements
Similar presentations
Higgs Physics at the Large Hadron Collider Markus Schumacher, Bonn University NRW Phenomenology Meeting 2006, Bad Honnef, January 2006.
Advertisements

5th May 2010Fergus Wilson, RAL1 Experimental Particle Physics PHYS6011 Looking for Higgs and SUSY at the LHC or...what can you get for $10,000,000,000.
Higgs physics theory aspects experimental approaches Monika Jurcovicova Department of Nuclear Physics, Comenius University Bratislava H f ~ m f.
THE FINE-TUNING PROBLEM IN SUSY AND LITTLE HIGGS
Extensions of the Standard Model (part 2) Prof. Jorgen DHondt Vrije Universiteit Brussel Inter-university Institute for High Energies Content: The Higgs.
What do we know about the Standard Model? Sally Dawson Lecture 4 TASI, 2006.
The search for the God Particle
Vertex Function of Gluon-Photon Penguin Swee-Ping Chia High Impact Research, University of Malaya Kuala Lumpur, Malaysia
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.
J. Hošek, in “Strong Coupling Gauge Theories in LHC Era”, World Scientific 2011 (arXiv: ) P. Beneš, J. Hošek, A. Smetana, arXiv: A.
Higgs Boson Mass In Gauge-Mediated Supersymmetry Breaking Abdelhamid Albaid In collaboration with Prof. K. S. Babu Spring 2012 Physics Seminar Wichita.
A model of soft mass generation Jiří Hošek Department of Theoretical Physics Nuclear Physics Institute Řež (Prague)
Chiral freedom and the scale of weak interactions.
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,
Smashing the Standard Model: Physics at the CERN LHC
Chiral freedom and the scale of weak interactions.
CUSTODIAL SYMMETRY IN THE STANDARD MODEL AND BEYOND V. Pleitez Instituto de Física Teórica/UNESP Modern Trends in Field Theory João Pessoa ─ Setembro 2006.
Chiral freedom and the scale of weak interactions.
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.
Masses For Gauge Bosons. A few basics on Lagrangians Euler-Lagrange equation then give you the equations of motion:
 Collaboration with Prof. Sin Kyu Kang and Prof. We-Fu Chang arXiv: [hep-ph] submitted to JHEP.
A model of flavors Jiří Hošek Department of Theoretical Physics NPI Řež (Prague) (Tomáš Brauner and JH, hep-ph/ )
Particle Physics Chris Parkes 5 th Handout Electroweak Theory 1.Divergences: cancellation requires.
Geneva, October 2010 Dark Energy at Colliders? Philippe Brax, IPhT Saclay Published papers :
What do we know about the Standard Model? Sally Dawson Lecture 2 SLAC Summer Institute.
Center for theoretical Physics at BUE
The Standard Model of Electroweak Physics Christopher T. Hill Head of Theoretical Physics Fermilab.
P Spring 2003 L12Richard Kass The properties of the Z 0 For about ten years the Z 0 was studied in great detail at two accelerator complexes: LEP.
Electroweak Theory Mr. Gabriel Pendas Dr. Susan Blessing.
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.
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.
Paweł Pachołek IFT UW Scalars 2011 Warsaw
05/07/06Standard Model 21 The Standard Model of Fundamental Interactions Achievements and Prospects Gilles Cohen-Tannoudji.
Sally Dawson, BNL Introduction to the Standard Model TASI, 2006 Introduction to the Standard Model –Review of the SU(2) x U(1) Electroweak theory –Experimental.
weak decays beta decay ofneutron problem energy and momentum not conserved e n p.
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.
Announcements 11/26 Tomorrow:10.1, 10.3 Wednesday: 10.4, 10.5, 10.7 Problem 10.5: diagram only Friday: 10.8, Error in eq Find the decay rate.
Standard Model III: Higgs and QCD Rogério Rosenfeld Instituto de Física Teórica UNESP Physics Beyond SM – 06/12/2006 UFRJ.
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.
Takaaki Nomura(Saitama univ)
The Search For Supersymmetry Liam Malone and Matthew French.
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.
Weak Interactions (continued)
Particle Physics Particle Physics Chris Parkes Feynman Graphs of QFT QED Standard model vertices Amplitudes and Probabilities Forces from particle exchange.
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.
Prof. M.A. Thomson Michaelmas Particle Physics Michaelmas Term 2011 Prof Mark Thomson Handout 3 : Interaction by Particle Exchange and QED X X.
Dirac Gauginos, Negative Supertraces and Gauge Mediation hep-th Linda Carpenter CERN 2011.
Monday, Apr. 11, 2005PHYS 3446, Spring 2005 Jae Yu 1 PHYS 3446 – Lecture #18 Monday, Apr. 11, 2005 Dr. Jae Yu Symmetries Local gauge symmetry Gauge fields.
Electroweak Theory Joint Belgian Dutch German School September 2007 Andrzej Czarnecki University of Alberta.
Some remarks on Higgs physics The Higgs mechanism Triviality and vacuum stability: Higgs bounds The no-Higgs option: strong WW scattering These are just.

Takaaki Nomura(Saitama univ)
Handout 3 : Interaction by Particle Exchange and QED
NGB and their parameters
Reference: “The Standard Model Higgs Boson” by Ivo van Vulpen,
Physics 222 UCSD/225b UCSB Lecture 10 Chapter 14 in H&M.
Handout 9 : The Weak Interaction and V-A
PHYS 5326 – Lecture #19 Wrapping up the Higgs Mechanism
Ultraviolet Complete Electroweak Model
P Spring 2002 L13 Richard Kass The properties of the Z0
Lecture 11 Spontaneous Symmetry Breaking
Higgs boson(s) Why do we need them? What do they look like?
Spontaneous breakdown (SB) of symmetry
Ultraviolet Complete Quantum Field Theory and Particle Model
Handout 13 : Electroweak Unification and the W and Z Bosons
Spontaneous symmetry breaking.
Lecture 12 Chapter 15: The Standard Model of EWK Interactions
Weak interactions.
Presentation transcript:

1 Why Does the Standard Model Need the Higgs Boson ? II Augusto Barroso Sesimbra 2007

2 Scattering  e-e- e+e+ W-W- W+W+ Incoming e- e+e+ Outgoing W-W- W+W+

3 Scattering  and Z s-channel Both terms grow as s. However, notice the cancelation between gamma and Z.

4 t-channel diagram It cancels with the similar contribution from the s-channel, i. e. Conclusion: All contributions that grow with s or cancel

5 Notice that: The previous results were obtained with m=0. Otherwise there would be an additional contribution to the t-channel diagram, namely:

6 Again the scalar exchange rescues the theory !

7 The Standard Model SU(3)xSU(2)xU(1) x Gravity Number of Parameters: 27 parameters. 23 are generated by the Higgs Sector. Another one, the Cosmological Constant, “does not like the Higgs sector”.

8 The Higgs Sector and The Higgs gives: The Higgs gives: Cosmology gives: Cosmology gives: =2x m -2

9 The Electroweak Sector

10 Example: only SU(2) But QFT is more than L g

11 Ex: Calculate the Self Energy is absorbed in the Wave Function renormalization. …=finite terms + +

12 Now, introduce fermions, F We don’t want to decide if F is left, right or whatever. Hence we use the coupling: There is another contribution to the gauge field self-energy. The new singular term requires a mass renormalization.

13 Renormalization of massless non- Abelian Gauge Theory Without Fermions Without Fermions –Simply With massive fermions axial coupled With massive fermions axial coupled –It requires This implies a mass term for the gauge bosons.

14 Loop Corrections Because the W and Z self energies are different we have a correction to . Because the W and Z self energies are different we have a correction to .

15 Summary: Parity conservation in QED Electron in Dirac Rep. Mass terms are Left-right Parity violation in Weak Int. The weak currents are left Bad behaviour of WW scattering Scalar boson couples to W Bad behaviour of e + e - WW The scalar couples to fermions Scalar is a doublet of SU(2)

16 Solution with Spontaneous symmetry breaking. Three degrees of freedom become the longitudinal polarizations of W and Z. The remaining is the Higgs Boson.

17 Higgs Boson From the value of G F one obtains: The parameter can be traded off with the Higgs mass. Inserting the LEP upper bound: M H < 144 GeV (95%CL) gives One can safely use perturbation theory.

18 FAQ The Higgs mechanism is a “clever trick”. Can we do it without ending up with an The Higgs mechanism is a “clever trick”. Can we do it without ending up with an Higgs Boson? Higgs Boson? NO. Cif. the example on WW scattering. NO. Cif. the example on WW scattering. Unless …

19 FAQ If we are not careful can we also break the electromagnetic gauge group and give the photon a mass? If we are not careful can we also break the electromagnetic gauge group and give the photon a mass? No, in the minimal model with a single doublet. No, in the minimal model with a single doublet.

20 Conclusion LEP results tested the SM in such a way that it is hard to believe that one is not checking the loop expansion of a QFT. LEP results tested the SM in such a way that it is hard to believe that one is not checking the loop expansion of a QFT. Then, the standard model is a QFT valid at the same level as, for instance, QED. Then, the standard model is a QFT valid at the same level as, for instance, QED. Hence, the Higgs boson ought to exist. Hence, the Higgs boson ought to exist.