We’ve worked through 2 MATHEMATICAL MECHANISMS

Slides:



Advertisements
Similar presentations
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.
Advertisements

Higgs physics theory aspects experimental approaches Monika Jurcovicova Department of Nuclear Physics, Comenius University Bratislava H f ~ m f.
The search for the God Particle
The Standard Model and Beyond [Secs 17.1 Dunlap].
£ With  real, the field  vanishes and our Lagrangian reduces to introducing a MASSIVE Higgs scalar field, , and “getting” a massive vector gauge field.
Lecture 10: Standard Model Lagrangian The Standard Model Lagrangian is obtained by imposing three local gauge invariances on the quark and lepton field.
Section IX Electroweak Unification. 221 Electroweak Unification  Weak Charged Current interactions explained by W  exchange.  W bosons are charged,
THE SEARCH FOR THE HIGGS BOSON Aungshuman Zaman Department of Physics and Astronomy Stony Brook University October 11, 2010.
P461 - particles VII1 Glashow-Weinberg-Salam Model EM and weak forces mix…or just EW force. Before mixing Bosons are massless: Group Boson Coupling Quantum.
V (  )  ½    2 + ¼  4 A translation  (x) =  0 + u(x) → u(x) ≡  (x) –  0 V (  )  V (u +   )  ½   (u +   ) 2 + ¼ (u +   ) 4 selects.
Smashing the Standard Model: Physics at the CERN LHC
Chiral freedom and the scale of weak interactions.
Chiral freedom and the scale of weak interactions.
Let’s recap: We’ve worked through 2 MATHEMATICAL MECHANISMS for manipulating Lagrangains Introducing SELF-INTERACTION terms (generalized “mass” terms)
J. Nielsen1 The ATLAS experiment at the Large Hadron Collider Jason Nielsen UC Santa Cruz VERTEX 2004 July 28, 2010.
P Spring 2003 L12Richard Kass Weak Interactions & Neutral Currents Until the the mid-1970 ’ s all known weak interaction processes could be described.
Masses For Gauge Bosons. A few basics on Lagrangians Euler-Lagrange equation then give you the equations of motion:
Monday, Apr. 2, 2007PHYS 5326, Spring 2007 Jae Yu 1 PHYS 5326 – Lecture #12, 13, 14 Monday, Apr. 2, 2007 Dr. Jae Yu 1.Local Gauge Invariance 2.U(1) Gauge.
Particle Physics J4 Leptons and the standard model.
Joseph Haley Joseph Haley Overview Review of the Standard Model and the Higgs boson Creating Higgs bosons The discovery of a “Higgs-like” particle.
August 22, 2002UCI Quarknet The Higgs Particle Sarah D. Johnson University of La Verne August 22, 2002.
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.
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.
The Higgs Boson Observation (probably) Not just another fundamental particle… July 27, 2012Purdue QuarkNet Summer Workshop1 Matthew Jones Purdue University.
weak decays beta decay ofneutron problem energy and momentum not conserved e n p.
DISCOVERY OF THE NEUTRON
M. Cobal, PIF 2003 Weak Interactions Take place between all the quarks and leptons (each of them has a weak charge) Usually swamped by the much stronger.
1 Methods of Experimental Particle Physics Alexei Safonov Lecture #6.
Wednesday, Jan. 15, 2003PHYS 5396, Spring 2003 Jae Yu 1 PHYS 5396 – Lecture #2 Wednesday, Jan. 15, 2003 Dr. Jae Yu 1.What is a neutrino? 2.History of neutrinos.
1 Why Does the Standard Model Need the Higgs Boson ? II Augusto Barroso Sesimbra 2007.
Particle Physics II Chris Parkes Top Quark Discovery Decay Higgs Searches Indirect mW and mt Direct LEP & LHC searches 2 nd Handout.
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.
H Y P A T I A HYbrid Pupil’s Analysis Tool for Interactions in Atlas
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.
Higgs in the Large Hadron Collider Joe Mitchell Advisor: Dr. Chung Kao.
The Standard Model T. Kawamoto The University of Tokyo FAPPS08 Les Houches September 2008.
Today’s plan Reminder: Final Exam (Friday May 5, time 13:30-15:30).
Introduction to the Standard Model
The precise dynamical behavior of a system of particles
CMS Masterclasses 2017 S’Cool LAB
Today’s plan Collect homework QCD leftovers Weak Interaction.
Nuclear Physics: Mossbauer Effect
Reference: “The Standard Model Higgs Boson” by Ivo van Vulpen,
Introduction to CERN Activities
Countries that signed the nuclear arms treaty with Iran
Lecture 10: Standard Model Lagrangian
User Guide Tutorial of ISpy and CIMA
PHYS 5326 – Lecture #1 Class specifications and plans
G. Arnison et al., UA1 Collaboration
Lecture 14 – Neutral currents and electroweak unification
Generating Neutrino Mass & Electroweak Scale Radiatively
PHYS 5326 – Lecture #19 Wrapping up the Higgs Mechanism
The Standard Model strong nuclear force electromagnetic force
Section VI - Weak Interactions
H Y P A T I A HYbrid Pupil’s Analysis Tool for Interactions in Atlas
P Spring 2002 L13 Richard Kass The properties of the Z0
Lecture 11 Spontaneous Symmetry Breaking
Elementary particles Spring 2005, Physics /24/2018 Lecture XXV.
Particle Physics Part 1 -James Joyce Contents: Particle Accelerators
Electroweak bosons  .
Higgs boson(s) Why do we need them? What do they look like?
Radiation Shield Design by UA
Section XI - The Standard Model
CMS Masterclass 2017.
Methods of Experimental Particle Physics
Lecture 12: Electroweak Kaon Regeneration & Oscillation
£ introducing a MASSIVE Higgs scalar field, ,
Lecture 12 Chapter 15: The Standard Model of EWK Interactions
Weak interactions.
Presentation transcript:

We’ve worked through 2 MATHEMATICAL MECHANISMS Let’s recap: We’ve worked through 2 MATHEMATICAL MECHANISMS for manipulating Lagrangains Introducing SELF-INTERACTION terms (generalized “mass” terms) showed that a specific GROUND STATE of a system need NOT display the full available symmetry of the Lagrangian Effectively changing variables by expanding the field about the GROUND STATE (from which we get the physically meaningful ENERGY values, anyway) showed The scalar field ends up with a mass term; a 2nd (extraneous) apparently massless field (ghost particle) can be gauged away. Any GAUGE FIELD coupling to this scalar (introduced by local inavariance) acquires a mass as well!

We then applied these techniques by introducing the scalar Higgs fields through a weak iso-doublet (with a charged and uncharged state) +  0 v+H(x) Higgs= = which, because of the explicit SO(4) symmetry, the proper gauge selection can rotate us within the1, 2, 3, 4 space, reducing this to a single observable real field which we we expand about the vacuum expectation value v.

The “mass-generating” interaction is identified by simple constants With the choice of gauge settled: +  0 Higgs= v+H(x) = Let’s try to couple these scalar “Higgs” fields to W, B which means replace: which makes the 1st term in our Lagrangian: † The “mass-generating” interaction is identified by simple constants providing the coefficient for a term simply quadratic in the gauge fields so let’s just look at: † where Y =1 for the coupling to B

† ( ) ( ) ( ) ( 2g22W+W+ + (g12+g22) ZZ ) ( ) 0 1 1 0 0 -i i 0 1 0 recall that → → 0 1 1 0 0 -i i 0 1 0 0 -1 W3 W1-iW2 W1+iW2 -W3 τ ·W = W1 + W2 + W3 = 2 W1-iW2 H + v 1 2 † ( ) = 0 H +v W1+iW2 2 H + v 1 8 † ( ) = 0 H +v 1 8 † † ( ) ( 2g22W+W+ + (g12+g22) ZZ ) ( ) = H +v H +v

( ) ( 2g22W+W+ + (g12+g22) ZZ ) ( ) v22g22W+ W+ (g12+g22 )Z Z 8 † † ( ) ( 2g22W+W+ + (g12+g22) ZZ ) ( ) = H +v H +v No AA term has been introduced! The photon is massless! But we do get the terms 1 8 † 1 2 v22g22W+ W+ MW = vg2 1 8 1 2 (g12+g22 )Z Z MZ = v√g12 + g22 At this stage we may not know precisely the values of g1 and g2, but note: MW MZ 2g2 = √g12 + g22

( ) g12+g12 and we do know THIS much about g1 and g2 -g1g2 = e to extraordinary precision! from other weak processes: m- e- +e +m N  p + e- +e u e e- W - d m e e- W - m- ( ) 2 2 e sinθW lifetimes (decay rate cross sections) ~gW = give us sin2θW

Notice = cos W according to this theory. MW MZ Notice = cos W according to this theory. where sin2W=0.2325 +0.0015 -9.0019 We don’t know v, but information on the coupling constants g1 and g2 follow from lifetime measurements of b-decay: neutron lifetime=886.7±1.9 sec and a high precision measurement of muon lifetime=2.19703±0.00004 msec measurements (sometimes just crude approximations perhaps) of the cross-sections for the inverse reactions: e- + p  n + e electron capture e + p  e+ + n anti-neutrino absorption as well as e + e-  e- + e neutrino scattering

Fine work for theorists, but drew very little attention All of which can be compared in ratios to similar reactions involving well-known/ well-measured simple QED scattering (where the coupling is simply e2=1/137). Fine work for theorists, but drew very little attention from the rest of the high energy physics community Until 1973 all observed weak interactions were consistent with only a charged boson. 1973 (CERN): first neutral current interaction observed ν + nucleus → ν + p + π- + πo _ _ Suddenly it became very urgent to observe W±, Zo bosons directly to test electroweak theory.

The first example of the neutral-current process νμ + e- →νμ + e-. The electron is projected forward with an energy of 400 MeV at an angle of 1.5 ± 1.5° to the beam, entering from the right. _ _ _ _ ν + nucleus → ν + p + π- + πo The Gargamelle heavy-liquid bubble chamber, installed into the magnet coils at CERN(1970)

Current precision measurements give: By early 1980s had the following theoretically predicted masses: MZ = 92  0.7 GeV MW = cosWMZ = 80.2  1.1 GeV Late spring, 1989 Mark II detector, SLAC August 1989 LEP accelerator at CERN discovered opposite-sign lepton pairs with an invariant mass of MZ=92 GeV and lepton-missing energy (neutrino) invariant masses of MW=80 GeV Current precision measurements give: MW = 80.482  0.091 GeV MZ = 91.1885  0.0022 GeV

Z→e+e-

Z→e+e-

Z→e+e-

Z→e+e-

Z→+-

Z → jet + jet

Also notice the threshold for W+W- pair production! Among the observed resonances in e+e- collisions we now add the clear, well- defined Z peak! Also notice the threshold for W+W- pair production!

Z peak in e+e- invariant mass distribution

Z peak in  invariant mass distribution

W peak in e+e- transverse mass distribution

Z → jets cross section LEP (CERN)

Higgs= Gv[eLeR + eReL] + GH[eLeR + eReL] Can the mass terms of the regular Dirac particles in the Dirac Lagrangian also be generated from “first principles”? Theorists noted there is an additional gauge-invariant term we could try adding to the Lagrangian: A Yukawa coupling which, for electrons, for example, would read Higgs= v+H(x) which with becomes _ _ _ _ Gv[eLeR + eReL] + GH[eLeR + eReL]

Gv[eLeR + eReL] + GH[eLeR + eReL] _ _ _ _ Gv[eLeR + eReL] + GH[eLeR + eReL] _ _ e e e e from which we can identify: me = Gv or