From Lagrangian Density to Observable

Slides:



Advertisements
Similar presentations
Feynman Diagrams Feynman diagrams are pictorial representations of
Advertisements

What do we know about the Standard Model? Sally Dawson Lecture 4 TASI, 2006.
Jørgen Beck Hansen Particle Physics Basic concepts Particle Physics.
1 Top Production Processes at Hadron Colliders By Paul Mellor.
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.
Derivation of Electro-Weak Unification and Final Form of Standard Model with QCD and Gluons  1 W 1 +  2 W 2 +  3 W 3.
January 16, 2001Physics 8411 Introduction to Feynman Diagrams and Dynamics of Interactions All known interactions can be described in terms of forces forces:
Chiral freedom and the scale of weak interactions.
The Klein Gordon equation (1926) Scalar field (J=0) :
Chiral freedom and the scale of weak interactions.
1 Methods of Experimental Particle Physics Alexei Safonov Lecture #14.
What do we know about the Standard Model? Sally Dawson Lecture 2 SLAC Summer Institute.
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.
Cross section for potential scattering
Announcements Homework returned now 9/19 Switching to more lecture-style class starting today Good luck on me getting powerpoint lectures ready every day.
Monday, Jan. 27, 2003PHYS 5326, Spring 2003 Jae Yu 1 PHYS 5326 – Lecture #4 Monday, Jan. 27, 2003 Dr. Jae Yu 1.Neutrino-Nucleon DIS 2.Formalism of -N DIS.
Frontiers of particle physics II
Quantum Mechanical Cross Sections In a practical scattering experiment the observables we have on hand are momenta, spins, masses, etc.. We do not directly.
Threshold Resummation for Top- Quark Pair Production at ILC J.P. Ma ITP, CAS, Beijing 2005 年直线对撞机国际研讨会, Tsinghua Univ.
Nucleon Polarizabilities: Theory and Experiments
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.

1 Methods of Experimental Particle Physics Alexei Safonov Lecture #2.
M. Cobal, PIF 2006/7 Feynmann Diagrams. M. Cobal, PIF 2006/7 Feynman Diagrams 
Physics 842, February 2006 Bogdan Popescu Presentation based on “Introduction to Elementary Particles” by David Griffiths WEAK INTERACTION (1)
The Importance of the TeV Scale Sally Dawson Lecture 3 FNAL LHC Workshop, 2006.
Prof. M.A. Thomson Michaelmas Particle Physics Michaelmas Term 2011 Prof Mark Thomson Handout 3 : Interaction by Particle Exchange and QED X X.
Lecture 2 - Feynman Diagrams & Experimental Measurements
IFIC. 1/15 Why are we interested in the top quark? ● Heaviest known quark (plays an important role in EWSB in many models) ● Important for quantum effects.
New Physics effect on Higgs boson pair production processes at LHC and ILC Daisuke Harada (KEK, Graduate University for Advanced Studies) in collaboration.
Lecture 4 – Quantum Electrodynamics (QED)
Song He Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing.
Some remarks on Higgs physics The Higgs mechanism Triviality and vacuum stability: Higgs bounds The no-Higgs option: strong WW scattering These are just.
Advanced Algorithms Analysis and Design By Dr. Nazir Ahmad Zafar Dr Nazir A. Zafar Advanced Algorithms Analysis and Design.
WEAK DECAYS: ALL DRESSED UP
Spontaneous Symmetry Breaking and the
Quantum Mechanics for Applied Physics
Theory of Scattering Lecture 2.
Lagrange Formalism & Gauge Theories
Introduction to pQCD and TMD physics
Handout 3 : Interaction by Particle Exchange and QED
Chapter III Dirac Field Lecture 2 Books Recommended:
Classically conformal B-L extended Standard Model
NGB and their parameters
Chapter V Interacting Fields Lecture 1 Books Recommended:
Derivation of Electro-Weak Unification and Final Form of Standard Model with QCD and Gluons  1W1+  2W2 +  3W3.
Physics 222 UCSD/225b UCSB Lecture 10 Chapter 14 in H&M.
Lecture 2 Evolution and resummation
Lecture 10: Standard Model Lagrangian
Handout 9 : The Weak Interaction and V-A
Section VI - Weak Interactions
Announcements Exam Details: Today: Problems 6.6, 6.7
Ultraviolet Complete Electroweak Model
P Spring 2002 L13 Richard Kass The properties of the Z0
Chapter V Interacting Fields Lecture 7 Books Recommended:
Adaptive Perturbation Theory: QM and Field Theory
Adnan Bashir, UMSNH, Mexico
Lecture 2: Invariants, cross-section, Feynman diagrams
Radiative corrections FOR PYTHIA
Ultraviolet Complete Quantum Field Theory and Particle Model
Handout 4 : Electron-Positron Annihilation
It means anything not quadratic in fields and derivatives.
The energy dependence of saturation scale at next-to-leading order
Determination of Higgs branching ratio into
QCD at very high density
Y.Kitadono (Hiroshima ),
Can new Higgs boson be Dark Matter Candidate in the Economical Model
PHYS 3446 – Lecture #4 Monday, Sept. 11, 2006 Dr. Jae Yu
Leptonic Charged-Current Interactions
Examples of QED Processes
Presentation transcript:

From Lagrangian Density to Observable Roger Wolf 20. Mai 2015 Prof. Dr. Max Mustermann | Name of Faculty

Schedule for today Does a Feynman diagram have a time direction? If yes, what is it? 3 Intrinsic bounds on the Higgs boson mass in the SM 2 Discussion of higher order effects in perturbation theory 1 Completion of cross section calculation Prof. Dr. Max Mustermann | Name of Faculty

The perturbative series Prof. Dr. Max Mustermann | Name of Faculty

The perturbative series The integral equation can be solved iteratively: ( = solution of the homogeneous Dirac equation) 0th order perturbation theory: Just take as solution (→ boring). 1st order perturbation theory: Assume that is close enough to actual solution on RHS. 2nd order perturbation theory: Take as better approximation at RHS to solve inhomogene-ous equation. Prof. Dr. Max Mustermann | Name of Faculty

The perturbative series The integral equation can be solved iteratively: ( = solution of the homogeneous Dirac equation) 0th order perturbation theory: Just take as solution (→ boring). 1st order perturbation theory: Assume that is close enough to actual solution on RHS. 2nd order perturbation theory: Prof. Dr. Max Mustermann | Name of Faculty

The matrix element is obtained from the projection of the scattering wave on : “LO” “NLO” 1st order perturbation theory: For and respectively. cf. slide 7 cf. slide 28 NB: the time integration has already been carried out for the backward evolution from to to arrive at the equation of slide 28. Prof. Dr. Max Mustermann | Name of Faculty

The matrix element is obtained from the projection of the scattering wave on : “LO” “NLO” 1st order perturbation theory: (1st order matrix element) This corresponds exactly to the IA term in , including the multiplication by (cf. Lecture-05 slide 39). Prof. Dr. Max Mustermann | Name of Faculty

The photon propagator The evolution of happens according to the inhomogeneous wave equation of the photon field (in Lorentz gauge ) (++) We solve (++) again formally via the Green's function with the property: Prof. Dr. Max Mustermann | Name of Faculty

The photon propagator The evolution of happens according to the inhomogeneous wave equation of the photon field (in Lorentz gauge ) (++) We solve (++) again formally via the Green's function with the property: Prof. Dr. Max Mustermann | Name of Faculty

Green's function in Fourier space (fast forward) Check for the concrete form of the Green's function again first in Fourier space: (Fourier transform) In analogy to the fermion case the defining property of in Fourier space ! (omitting the discussion of integral paths) leads to (photon propagator) Prof. Dr. Max Mustermann | Name of Faculty

Green's function in Fourier space (fast forward) The Green's function can again be obtained from the inverse Fourier transform. We have now collected all pieces of the puzzle to complete the cross section calculation. Prof. Dr. Max Mustermann | Name of Faculty

On the way to completion... Ansatz for target current: Combination with photon propagator to get the evolution of : target Ansatz for projectile current: projectile Prof. Dr. Max Mustermann | Name of Faculty

On the way to completion... 1st order matrix element: projectile target Prof. Dr. Max Mustermann | Name of Faculty

The matrix element (complete picture) projectile virtual photon exchange target Prof. Dr. Max Mustermann | Name of Faculty

The matrix element (complete picture) projectile virtual photon exchange target Prof. Dr. Max Mustermann | Name of Faculty

The matrix element (complete picture) projectile virtual photon exchange target Prof. Dr. Max Mustermann | Name of Faculty

The matrix element (complete picture) projectile virtual photon exchange target Prof. Dr. Max Mustermann | Name of Faculty

Feynman Rules (QED) Feynman diagrams are a way to represent the elements of the matrix element calculation: Legs: Incoming (outgoing) fermion. Incoming (outgoing) photon. Vertices: Lepton-photon vertex. Propagators: Fermion propagator. Photon propagator. Four-momenta of all virtual particles have to be integrated out. Prof. Dr. Max Mustermann | Name of Faculty

Feynman Rules (QED) Feynman diagrams are a way to represent the elements of the matrix element calculation: A Feynman diagram: is not just a sketch, it has a strict mathematical correspondence. is drawn in momentum space. does not have a time direction. Only time information is introduced by choice of initial and final state by reader (e.g. t-channel vs s-channel processes). Prof. Dr. Max Mustermann | Name of Faculty

Higher order Prof. Dr. Max Mustermann | Name of Faculty

Fixed order calculations Scattering amplitude only known in perturbation theory. Works better the smaller the perturbation is: QED: QFD: QCD: If perturbation theory works well, the first contribution of the scattering amplitude is already sufficient to describe the main features of the scattering process. This contribution is of order . It is often called Tree Level, Born Level or Leading Order (LO) scattering amplitude. Any higher order of the scattering amplitude in perturbation theory appears at higher orders of . Prof. Dr. Max Mustermann | Name of Faculty

Order diagrams (QED) We have only discussed contributions to , which are of order in QED. (e.g. LO scattering) . Diagrams which contribute to order would look like this: Additional legs: Loops: (in propagators or legs) (in vertices) Prof. Dr. Max Mustermann | Name of Faculty

Order diagrams (QED) We have only discussed contributions to , which are of order in QED. (e.g. LO scattering) . Diagrams which contribute to order would look like this: Additional legs: Loops: (in propagators or legs) (in vertices) LO term for a process. NLO contrib. for the process. Opens phasespace. Prof. Dr. Max Mustermann | Name of Faculty

Order diagrams (QED) We have only discussed contributions to , which are of order in QED. (e.g. LO scattering) . Diagrams which contribute to order would look like this: Additional legs: Loops: (in propagators or legs) (in vertices) LO term for a process. NLO contrib. for the process. Opens phasespace. Modifies (effective) masses of particles (“running masses”). Prof. Dr. Max Mustermann | Name of Faculty

Order diagrams (QED) We have only discussed contributions to , which are of order in QED. (e.g. LO scattering) . Diagrams which contribute to order would look like this: Additional legs: Loops: (in propagators or legs) (in vertices) LO term for a process. NLO contrib. for the process. Opens phasespace. Modifies (effective) masses of particles (“running masses”). Modifies (effective) couplings of particles (“running couplings”). Prof. Dr. Max Mustermann | Name of Faculty

Examples for “running constants” Running of the constants can be predicted and are indeed observed. Coupling needs to be measured at least in one point. One usually gives the value at a reference scale (e.g. ). Prof. Dr. Max Mustermann | Name of Faculty

Effect of higher order corrections Change of over all normalization of cross sections (e.g. via change of coupling, but also by kinematic opening of phasespace – large effect). Change of kinematic distributions (e.g. harder or softer transverse momentum spectrum of particles) Prof. Dr. Max Mustermann | Name of Faculty

Effect of higher order corrections Change of over all normalization of cross sections (e.g. via change of coupling, but also by kinematic opening of phasespace – large effect). Change of kinematic distributions (e.g. harder or softer transverse momentum spectrum of particles) In QED effects are usually “small” (correction to LO is already at level). In QCD effects are usually “large” ( ). Therefore reliable QCD predictions almost always require (N)NLO calculations. Higher orders can be mixed (e.g. ). In concrete calculations the number of contributing diagrams quickly explodes for higher order calculations, which makes these calculations very difficult. Prof. Dr. Max Mustermann | Name of Faculty

Boundaries on Higgs mass within the SM Prof. Dr. Max Mustermann | Name of Faculty

Running of in the Higgs potential Like the couplings , and also the self-coupling in the Higgs potential is subject to higher order corrections: (Higgs potential) (Renormalization group equation at 1-loop accuracy) Higgs top quark Since the Higgs boson couples proportional to the mass the high energy behavior of will be dominated by the heaviest object in the loop. Prof. Dr. Max Mustermann | Name of Faculty

Running of in the Higgs potential First case: large Higgs mass ( ). Higgs top quark solution For we get and . For increasing will run into a pole and become non-perturbative. This pole is called Landau pole. From the pole an upper bound on can be obtained depending on the scale . Prof. Dr. Max Mustermann | Name of Faculty

Triviality bound The upper bound on due to the Landau pole is called triviality bound: (triviality bound) NB: here indicates up to which scale the SM should be applicable. Prof. Dr. Max Mustermann | Name of Faculty

The Running of in the Higgs Potential Second case: small Higgs mass ( ) Higgs potential w/ running . Higgs top quark solution (with: ) With increasing will turn negative and the Higgs potential will no longer be bound from below. The vacuum turns instable. From this turning point we obtain a lower bound on depending on the scale . Prof. Dr. Max Mustermann | Name of Faculty

Triviality bound & stability bound The upper bound on due to the Landau pole is called triviality bound: (triviality bound) The lower bound on is called stability bound: (stability bound) Indeed the later search window for the SM Higgs boson was in the range of , for these and other reasons. NB: here indicates up to which scale the SM should be applicable. Prof. Dr. Max Mustermann | Name of Faculty

Intrinsic bounds on Higgs potential w/ running . The SM in the stress field of vacuum stability. Running of . Prof. Dr. Max Mustermann | Name of Faculty

Intrinsic bounds on Higgs potential w/ running . Different levels of fine tuning in the SM. ~general reach of LHC What we have found and measured for . Prof. Dr. Max Mustermann | Name of Faculty

Concluding Remarks Reviewed Feynman rules and calculated cross section for simple QED scattering process. Briefly discussed effects of higher order corrections in perturbation theory. Discussed boundaries on Higgs boson mass immanent to the SM as an application of higher order effects on the Higgs self-coupling. Note: on Thursday next week will be holiday. On Friday next week there will be an Exercise session. The week after we will start with the experimental part of the lecture. Prof. Dr. Max Mustermann | Name of Faculty

Backup Prof. Dr. Max Mustermann | Name of Faculty