Understanding the Standard Model of Physics

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Delve into the world of quantum field theory, gauge symmetry, Higgs mechanism, electroweak theory, and more with this detailed overview of the Standard Model. Explore classical mechanics, Noether's theorem, relativistic mechanics, quantum mechanics, and quantum field theory concepts. Discover how the uncertainty principle, particle localization, fields, and the Lorentz group play crucial roles in our understanding of the fundamental forces of nature.


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  1. Introduction to the Standard Model Cao Hoang Nam Phenikaa University The 26th Vietnam School of Physics, November 29 - December 11, 2020, Quy Nhon , Vietnam

  2. Plan of Lecture Lecture 1: Basics in Quantum Field Theory Lecture 2: Gauge Symmetry Lecture 3: Spontaneous symmetry breaking and Higgs mechanism Lecture 4,5: Weinberg Salam electroweak theory Lecture 6: Electroweak phenomenology Lecture 7: For solving exercises

  3. Lecture 1: Basics in Quantum Field Theory

  4. Classical Mechanics (Newtonian physics) Space and time in Newtonian physics The state of a (point) particle is described its position in space and its momentum (or velocity) as functions of time

  5. Lagrangian formalism: classical behavior is obtained by the least action principle Noether s Theorem: The conservation laws are consequences of symmetries

  6. Relativistic Mechanics Spacetime in SR

  7. (Non-relativistic) Quantum Mechanics

  8. Quantum Field Theory (QFT) When the uncertainty in momentum is bigger than ??, then uncertainty in energy is larger than ??2. Thus, there is enough energy to produce another particle of the same type. On the other hand, we can not localize a particle below its Compton wave length. This means that we would not find a single particle but with no well-defined number of particles. We need to have the objects which describe infinitely many degrees of freedom, at least one for each point in space: Fields 1. A classical field is a collection of an infinite number of harmonic oscillators numbered by space coordinates interacting with neighbourhood oscillators. 2. A classical field is a continuous (differential) function of spacetime coordinates. 3. A particle is defined as an energy quantum or vibration excitation of the field.

  9. Lorentz group Lie algebra of Lorentz group

  10. The representation of Lorentz group (algebra) can be labelled by two indexes (? ,?+) which take values 0, 1/2, 1, 3/2, The dimension of representation (? ,?+) is (2? +1)(2?++1). As addition of angular momentum in quantum mechanics, in the representation (? ,?+) we have states with all possible spin j in integer steps between |?+ ? | and ?++ ? . Scalar field Dirac spinor has four complex components Majorana spinor as real Dirac spinor

  11. Contravariant complex four-vectors Real four-vectors The fields with spin s (=0, 1/2, 1, 3/2, ) are representations of Lorentz (and Poincare) group which leaves invariant the line element of spacetime.

  12. The action principle

  13. Real scalar fields

  14. Complex scalar fields Dirac spinor field

  15. Vector field

  16. Interactions

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