symmetries 3
play

Symmetries + ... (3) Yuval Grossman Cornell Y. Grossman SM and - PowerPoint PPT Presentation

Symmetries + ... (3) Yuval Grossman Cornell Y. Grossman SM and flavor (3) ICTP, June 12, 2019 p. 1 Symmetries: Yesterday and today Yesterday: How to built invariants L has to be invariant For U (1) we explain what is a charge For SU ( N )


  1. Symmetries + ... (3) Yuval Grossman Cornell Y. Grossman SM and flavor (3) ICTP, June 12, 2019 p. 1

  2. Symmetries: Yesterday and today Yesterday: How to built invariants L has to be invariant For U (1) we explain what is a charge For SU ( N ) we explain what is a representation Today: Different kind of symmetries Imposed vs accidental Lorentz vs internal Global vs local Y. Grossman SM and flavor (3) ICTP, June 12, 2019 p. 2

  3. More on symmetries Y. Grossman SM and flavor (3) ICTP, June 12, 2019 p. 3

  4. Accidental symmetries A symmetry that is an output, and only due to the truncation Example: The symmetry that makes the period independent of the amplitude Example: U (1) with X ( q = 1) and Y ( q = − 4) V ( XX ∗ , Y Y ∗ ) ⇒ U (1) X × U (1) Y X 4 Y breaks this symmetry Y. Grossman SM and flavor (3) ICTP, June 12, 2019 p. 4

  5. Lorentz invariants Unlike symmetries in the internal space of the field, Lorentz is the symmetry of space-time We always impose it The representations we care about are Singlet: Spin zero (scalars, denote by φ ) LH and RH fields: Spin half (fermions, ψ L , ψ R ) Vector: Spin one (gauge boson, denote by A µ ) Fermions are more complicated than scalars Y. Grossman SM and flavor (3) ICTP, June 12, 2019 p. 5

  6. Fermions Under Lorentz, the basic fields are left-handed and right-handed We define the complex conjugation as ¯ ψ The kinetic term is different, only one derivative L kin ∼ ¯ ψ L ∂ µ γ µ ψ L The mass term is also different, it involves LH and RH field L m ∼ ¯ ψ L ψ R Why it is? We can also have Majorana mass What are the conditions to have a mass term? Y. Grossman SM and flavor (3) ICTP, June 12, 2019 p. 6

  7. Dimension In mechanics we count with dim [ x ] = 1 Here it is a bit more complicated. We use � = c = 1 and dim [ E ] = 1 that implies dim [ x ] = − 1 What are the dim of S L φ ψ Y. Grossman SM and flavor (3) ICTP, June 12, 2019 p. 7

  8. C , P , CP , CPT There are also discrete transformation on space-time C P T All Lorentz invariant QFT have CPT C and P take you from LH to RH fermion They are “easy” to break CP is the difference between matter and anti-matter. Breaking arises from phases in L Y. Grossman SM and flavor (3) ICTP, June 12, 2019 p. 8

  9. Local symmetires Y. Grossman SM and flavor (3) ICTP, June 12, 2019 p. 9

  10. Local symmetry Basic idea: rotations depend on x and t local φ ( x µ ) → e iqθ ( x µ ) φ ( x µ ) φ ( x µ ) → e iqθ φ ( x µ ) − − → It is kind of logical and we think that all imposed symmetries in Nature are local The kinetic term | ∂ µ φ | 2 is not invariant We want a kinetic term (why?) We can save the kinetic term if we add a field that is Massless Spin 1 Adjoint representation: q = 0 for U (1) , triplet for SU (2) , and octet for SU (3) Y. Grossman SM and flavor (3) ICTP, June 12, 2019 p. 10

  11. Gauge boson kinetic term Generalization of that of a scalar We know how it is in classical E & M L ∝ F µν F µν F µν = ∂ µ A ν − ∂ ν A µ For non-Abelian there is a modification. For SU(2) F a µν = ∂ µ G a ν − ∂ ν G a µ − igǫ abc G b G c We get gauge boson self interaction ∼ gG 3 + g 2 G 4 F a µν F µν a Y. Grossman SM and flavor (3) ICTP, June 12, 2019 p. 11

  12. Gauge symmetry New field A µ . How we couple it? Recall classical electromagnetism H = p 2 2 m ⇒ H = ( p − qA i ) 2 2 m In QFT, for a local U (1) symmetry and a field with charge q ∂ µ → D µ D µ = ∂ µ + iqA µ We get interaction from the kinetic term ¯ / ψ ∼ ¯ ψ ( ∂ µ + iqA µ ) γ µ ψ → q ¯ ψγ µ ψA µ ψD The interaction ∝ q (for SU ( N ) to matrices) Y. Grossman SM and flavor (3) ICTP, June 12, 2019 p. 12

  13. The two aspects of symmetries Thinking about E & M Charge conservation The force proportional to the charge Q: Which of these come from the “global” aspect and which from the “local” aspect of the symmetry? Y. Grossman SM and flavor (3) ICTP, June 12, 2019 p. 13

  14. More on masses To summarize masses There is no symmetry that forbids generic scalar masses Chiral symmetry forbid fermion Dirac masses Gauge symmetry forbid gauge boson masses Y. Grossman SM and flavor (3) ICTP, June 12, 2019 p. 14

  15. SSB Y. Grossman SM and flavor (3) ICTP, June 12, 2019 p. 15

  16. Breaking a symmetry Y. Grossman SM and flavor (3) ICTP, June 12, 2019 p. 16

  17. SSB A situation that we have when the Ground state is degenerate By choosing a ground state we break the symmetry We choose to expend around a point that does not respect the symmetry PT only works when we expand around a minimum What is the difference between a broken symmetry and no symmetry? SSB implies relations between parameters Y. Grossman SM and flavor (3) ICTP, June 12, 2019 p. 17

  18. SSB Symmetry is x → − x and we keep up to x 4 f ( x ) = a 2 x 4 − 2 b 2 x 2 x min = ± b/a We choose to expand around + b/a and use u → x − b/a f ( x ) = 4 b 2 u 2 + 4 bau 3 + a 2 u 4 No u → − u symmetry The x → − x symmetry is hidden A general function has 3 parameters c 2 u 2 + c 3 u 3 + c 4 u 4 SSB implies a relation between them c 2 3 = 4 c 2 c 4 Y. Grossman SM and flavor (3) ICTP, June 12, 2019 p. 18

  19. Partial SSB Think about a vector in 3d. What symmetry is broken by it? Y. Grossman SM and flavor (3) ICTP, June 12, 2019 p. 19

  20. SSB in QFT When we expand the field around a minimum that is not invariant under a symmetry φ ( x µ ) → v + h ( x µ ) It breaks the symmetries that φ is not a singlet under Then we can get masses that were protected by the broken symmetry Fermions yφ ¯ ψ L ψ R → y ( v + h ) ¯ ψ L ψ R , m ψ = yv Gauge fields of the broken symmetries | D µ φ | 2 = | ∂ µ φ + iqA µ φ | 2 ∋ A 2 φ 2 → v 2 A 2 Y. Grossman SM and flavor (3) ICTP, June 12, 2019 p. 20

  21. Model buildings Y. Grossman SM and flavor (3) ICTP, June 12, 2019 p. 21

  22. Building Lagrangians Choosing the generalized coordinates (fields) Imposing symmetries and how fields transform (input) The Lagrangian is the most general one that obeys the symmetries We truncate it at some order, usually fourth Y. Grossman SM and flavor (3) ICTP, June 12, 2019 p. 22

  23. The general L We write L = L kin + L ψ + L Yuk + L φ Always have a kinetic term The task is to find the other terms and see what they lead to Y. Grossman SM and flavor (3) ICTP, June 12, 2019 p. 23

Download Presentation
Download Policy: The content available on the website is offered to you 'AS IS' for your personal information and use only. It cannot be commercialized, licensed, or distributed on other websites without prior consent from the author. To download a presentation, simply click this link. If you encounter any difficulties during the download process, it's possible that the publisher has removed the file from their server.

Recommend


More recommend