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Intro to SUSY II: SUSY QFT

Archil Kobakhidze PRE-SUSY 2016 SCHOOL 27 JUNE -1 JULY 2016, MELBOURNE. Intro to SUSY II: SUSY QFT. Recap from the first lecture: N=1 SUSY algebra. Recap from the first lecture: 8-dimensional N=1 superspace Covariant derivatives Non-zero torsion. Recap from the first lecture:

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Intro to SUSY II: SUSY QFT

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  1. Archil Kobakhidze PRE-SUSY 2016 SCHOOL 27 JUNE -1 JULY 2016, MELBOURNE Intro to SUSY II: SUSY QFT

  2. Recap from the first lecture: • N=1 SUSY algebra A. Kobakhidze (U. of Sydney)

  3. Recap from the first lecture: • 8-dimensional N=1 superspace • Covariant derivatives • Non-zero torsion A. Kobakhidze (U. of Sydney)

  4. Recap from the first lecture: • Superspace integration Grassmannintegration is equivalent to differentiation A. Kobakhidze (U. of Sydney)

  5. Outline of Part II: SUSY QFT • Basic consequences of superalgebra • Superfields • Chiral superfield • Vector superfield. Super-gauge invariance • Nonrenormalisation theorems A. Kobakhidze (U. of Sydney)

  6. Basic consequences of the superalgebra • Inspect, P2is a quadratic Casimir operator of the super-Poincaré algebra with eigenvalues m2. That is, each irreducible representation of superalgebra contains fields that are degenerate in mass. A. Kobakhidze (U. of Sydney)

  7. Basic consequences of the superalgebra • Inspect, Since is an invertible operator, so is Then, the action implies one-to-one correspondence between fermionicand bosonicstates. Thus, each irreducible representation of superalgebracontains equal number of fermionicand bosonicstates. A. Kobakhidze (U. of Sydney)

  8. Basic consequences of the superalgebra • Take sum over spinor indices in A. Kobakhidze (U. of Sydney)

  9. Basic consequences of the superalgebra iiia. Total energy of an arbitrary supersymmetric system is positive definite: iiib The vacuum energy of a supersymmetric system is 0, iiic Supersymmetry is broken if A. Kobakhidze (U. of Sydney)

  10. Basic consequences of the superalgebra • Compute 1-loop vacuum energy of a system of particles with various spins S and corresponding masses mS: A. Kobakhidze (U. of Sydney)

  11. Basic consequences of the superalgebra • Compute 1-loop correction to the mass of a scalar field (SUSY adjustment of couplings is assumed): A. Kobakhidze (U. of Sydney)

  12. Basic consequences of the superalgebra • Cancellation of divergences follow automatically from superalgebra! The above examples follow from the general all-loop perturbativenon-renormalization theorem in quantum field theories with supersymmetry. • Absence of quadratic divergences in scalar masses is the main phenomenological motivation for supersymmetry: supersymmetry may ensure stability of the electroweak scale against quantum corrections (the hierarchy problem) A. Kobakhidze (U. of Sydney)

  13. Superfields • Superfield is a function of superspace coordinates. A generic scalar superfield can be expanded in a form of a Taylor series expansion with respect to Grassmannian coordinates: • This generic scalar superfield is in a reducible SUSY representation. We may impose covariant constraints to obtain irreducible superfields. A. Kobakhidze (U. of Sydney)

  14. Chiral superfield • Consider, e.g., the following covariant condition: • The solution to the above constraint is known as the (left-handed) chiral superfield. A. Kobakhidze (U. of Sydney)

  15. Chiral superfield • To solve the constraint let us introduce new bosonic coordinates: • One verifies that Exercise: Check this. A. Kobakhidze (U. of Sydney)

  16. Chiral superfield • Therefore, the solution is: • Taylor expansion of the chiral superfield reads: Exercise: Obtain this expansion A. Kobakhidze (U. of Sydney)

  17. Chiral superfield • Supersymmetry transformations: Exercise: Verify this • Thus, we have: A. Kobakhidze (U. of Sydney)

  18. Anti-chiral superfield • In similar manner, we can define anti-chiral superfield through the constraint: which posses the solution A. Kobakhidze (U. of Sydney)

  19. Chiral field Lagrangian - Superpotential • Superpotential is a holomorphic function of a chiral (anti-chiral) superfields • Superpotential itself is a (composite) chiral (anti-chiral) superfield: • Consider, A. Kobakhidze (U. of Sydney)

  20. Chiral field Lagrangian - Superpotential • Since F-terms transform as total derivatives under SUSY transformations, is SUSY invariant Lagrangian density! A. Kobakhidze (U. of Sydney)

  21. Chiral field Lagrangian – Kähler potential • Consider product of chiral and anti-chiral superfields, which is a generic scalar superfield with the reality condition imposed. • SUSY transformation of D-term A. Kobakhidze (U. of Sydney)

  22. Chiral field Lagrangian - Kähler potential • Hence, is SUSY invariant Lagrangian density! • Kähler potential A. Kobakhidze (U. of Sydney)

  23. Wess-Zumino model • A chiral superfield, which contains a complex scalar (2 dofs both on-shell and off-shell), Majorana fermion (2 dofs on-shell, 4-dofs off-shell), a complex auxiliary field (0 dof on-shell, 2 dofs off-shell) Exercise: Express WZ Lagrangian in component form J. Wess and B. Zumino, “Supergauge transformations in four Dimensions”, Nuclear Physics B 70 (1974) 39 A. Kobakhidze (U. of Sydney)

  24. Vector (real) superfield • Reality condition: • Solution is: A. Kobakhidze (U. of Sydney)

  25. Vector (real) superfield • Let’s use the vector superfield to describe a SUSY gauge theory, e.g. super-QED • Supergauge transformations • Arbitrary chiral superfield – • Standard gauge transformations A. Kobakhidze (U. of Sydney)

  26. Vector (real) superfield • We can fix to remove (Wess-Zumino gauge) • Note, in the Wess-Zumino gauge SUSY is not manifest. • We can generalize this construction to super-Yang-Mills: A. Kobakhidze (U. of Sydney)

  27. Strength tensor superfield Exercise: Prove that these are chiral and anti-chiral superfields, respectively. • In the WZ gauge: A. Kobakhidze (U. of Sydney)

  28. Super-QED Exercise: Rewrite this Lagrangian in component form. • Matter couplings: • Gauge and SUSY invariant ‘kinetic’ term A. Kobakhidze (U. of Sydney)

  29. Nonrenormalisation theorems M.T. Grisaru, W. Siegel and M. Rocek, ``Improved Methods for Supergraphs,’’ Nucl. Phys. B159 (1979) 429 • Kahler potential receives corrections order by order in perturbation theory • Only 1-loop corrections for • is not renormalised in the perturbation theory! A. Kobakhidze (U. of Sydney)

  30. Nonrenormalisation theorems N. Seiberg, ``Naturalness versus supersymmetric nonrenormalization theorems,’’Phys. Lett. B318 (1993) 469 • Consider just Wess-Zumino model: • R-symmetry and U(1) charges: A. Kobakhidze (U. of Sydney)

  31. Nonrenormalisation theorems N. Seiberg, ``Naturalness versus supersymmetric nonrenormalization theorems,’’Phys. Lett. B318 (1993) 469 • Quantum corrected superpotential: • Consider • Consider • Hence, A. Kobakhidze (U. of Sydney)

  32. Summary of Part II • Basic consequences of SUSY algebra • Chiral superfield. Superpotential and Kahler potential. Wess-Zumino model • Vector superfield. Wess-Zumino gauge. Super-QED and matter coupling • Nonrenormalisation theorems A. Kobakhidze (U. of Sydney)

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