Supersymmetry and other theories of Dark Matter Candidates

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Transcription:

Supersymmetry and other theories of Dark Matter Candidates Ellie Lockner 798G Presentation 3/1/07 798G 3/1/07 1

Overview Why bother with a new theory? Why is Supersymmetry a good solution? Basics of Supersymmetry Why this leads to Dark Matter Candidates Other theoretical basis for Dark Matter Candidates 798G 3/1/07 2

Obligatory Standard Model Slide 3 categories of particles: Quarks Leptons Bosons (force mediating) Lagragian for 3 of 4 fundamental forces Been supported by SIGNIFICANT experimental data Requires Scalar Boson (Higgs) as a mechanism to explain why Z, W massive 798G 3/1/07 3

Hierarchy Problem Quadratic divergence in Higgs loops Can t renormalize Higgs mass without significant cancelations Electroweak scale vs. Planck scale 798G 3/1/07 4

How does SUSY Help? Unification of Forces Energy dependent coupling parameters meet with SUSY Higgs Mass Divergences cancel due to opposite sign contributions Abundance of matter over antimatter, size and age of universe, proton decay, 798G 3/1/07 5

Basics of SuSy What is a symmetry? Lagrangian remains unchanged under a transformation of the fields Ex: SM Lagrangian doesn t change if fields are boosted (transformed to moving frame using Spec. Rel.) What is a SUPER symmetry? Transformation of fields include fields of opposite nature Terms cancel in Lagrangian when all fields transformed, leaving it changed by only a derivative 798G 3/1/07 6

The Mathematics Wess-Zumino Model 798G 3/1/07 7

Eliminating Quadratic Divergences 798G 3/1/07 8

Naming Scheme Fermions get an s in front Bosons get an -ino ino at the end Symbols get a ~ on top. 798G 3/1/07 9

A typical SuSy decay mode 798G 3/1/07 10

How could we see it? The Lightest Supersymmetric Particle (LSP) neutral, so only interact via weak force Very hard to detect, so seen as Missing Transverse Energy in decays 798G 3/1/07 11

Common Types of SuSy MSSM Minimal Supersymmetric Model Adds fewest number of new particles Adds new conserved quantum number: R = (-1)( msugra 1) 3(B-L)+2S Minimal Supergravity Decreases # of parameters from >100 to 5 by grouping some together and requiring they be equal 798G 3/1/07 12

Why is this a Dark Matter Candidate? Dark matter must interact only via the weak force If electrically or color charged would see it in Nuclear effects such as anomalously heavy ions, Very hard to hide Baryons. If R quantum # conserved the Lightest Supersymmetric Particle (LSP) would be stable LSP must be relatively massive since hasn t been detected yet 798G 3/1/07 13

What are the Candidates? Gravitino Very difficult to confirm or exclude Sneutrino In MSSM has been excluded by direct and indirect searches Neutralino Could be photino, bino,, or Higgsinos 798G 3/1/07 14

What if we don t see SUSY? There must be modifications to SM SUSY provides an EXTENSION of SM, leaving most of it intact Time to scrap SM and start over? New theories that avoid quadratic divergences (renormalization?), explain hierarchy problem, unify forces 798G 3/1/07 15

Other theories that provide DMC WIMPs Weakly Interacting Massive Particles Generic name for DMC that interacts only via weak force Could have not seen it yet due to lifetime, mass, small production cross section Axions Strong Lagrangian not unchanged under CP transformation, yet no CP violation seen Solution involves introduction of mechanism similar to Higgs, but with a MASSIVE Goldstone boson Axion. 798G 3/1/07 16

Summary Don t forget, there is very little if any evidence for SUSY so far. Provides solutions to many problems of the SM, but requires many arbitrary parameters Gives a clear prediction for mass ranges of spartners,, (m 2 B -m 2 F )<1 TeV,, so we ll know in a few years 798G 3/1/07 17

References http://universe-review.ca/f15 review.ca/f15-article.htm#supersymmetryarticle.htm#supersymmetry Olive, Keith, Introduction to Supersymmetry; ; Astrophysical and Phenomenological constraints,, arxiv/hep-ph:9911307, ph:9911307, Nov. 1999 Lyon, Adam, A search for squarks and gluinos using the jets and missing energy signature at D0,, Dissertation for PhD at UMD, 1997 Freund, Peter, Introduction to Supersymmetry,, Cambridge University Press, 1986 Kane, Gordon, Supersymmetry Unveiling the Ultimate Laws of Nature, Perseus Publishing, 2000 www.wikipedia.org/supersymmetry Particles books 798G 3/1/07 18