fyst11 lecture 12 bsm ii - particle physics · 2016. 2. 23. · susy cross section versus sparticle...

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FYST11 Lecture 12 BSM II Thanks to G. Brooijmans, T. Rizzo, L. Covi 1 1

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Page 1: FYST11 Lecture 12 BSM II - Particle Physics · 2016. 2. 23. · SUSY cross section versus sparticle mass 1000 events produced in 2011 100 events produced in 2011 . Unification of

FYST11 Lecture 12 BSM II

Thanks to G. Brooijmans, T. Rizzo, L. Covi

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Page 2: FYST11 Lecture 12 BSM II - Particle Physics · 2016. 2. 23. · SUSY cross section versus sparticle mass 1000 events produced in 2011 100 events produced in 2011 . Unification of

This week’s topics

• Why go Beyond the SM?

– What are the problems with the SM?

– What direct measurements points to physics BSM

• Some attempts at solutions

– Supersymmetry

– Extended Higgs sector

– Extra dimensions

– A few others

• Searches for DM

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Supersymmetry (SUSY)

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Idea New symmetry fermions bosons

This symmetry is the most general extension of Lorentz invariance

• To create supermultiplets, we need to

add one superpartner to each SM particle

• Superpartners have opposite spin

statistics but otherwise equal quantum

numbers

• Need to introduce an additional Higgs

doublet to the non-SUSY side 5 Higgs

bosons

But where are these partners?! Supersymmetry must be broken (if realized)

SUSY has: Ndof (bosons) = Ndof (fermions) [cf. SM: Ndof (bosons) << Ndof (fermions)]

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Page 5: FYST11 Lecture 12 BSM II - Particle Physics · 2016. 2. 23. · SUSY cross section versus sparticle mass 1000 events produced in 2011 100 events produced in 2011 . Unification of

Particle spectrum (minimal!)

In reality the new states would mix

Several ideas of how the supersymmetry is broken – intimately connected with EWK symmetry breaking

Since we don’t know the mechanism, have to introduce 𝒪(100) new parameters ….

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Page 6: FYST11 Lecture 12 BSM II - Particle Physics · 2016. 2. 23. · SUSY cross section versus sparticle mass 1000 events produced in 2011 100 events produced in 2011 . Unification of

SUSY and the hierachy problem

But as m(𝑡 ) m(𝑡) they do not quite cancel, instead just a suppression This still gives a decent result if |m(fermion) – m(boson)| < 𝒪(TeV)

If Supersymmetry not broken we would have perfect cancellation in the loops!

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Page 7: FYST11 Lecture 12 BSM II - Particle Physics · 2016. 2. 23. · SUSY cross section versus sparticle mass 1000 events produced in 2011 100 events produced in 2011 . Unification of

Once mass spectrum fixed, all cross sections predicted Spin structure of SUSY spectrum: lower s than other BSM models, harder to find !

Gluino & squark

production (examples)

Direct squark pair

production (example)

Direct

gaugino/slepton

pair production (example)

SUSY cross section versus sparticle mass

1000 events produced in 2011

100 events produced in 2011

Page 8: FYST11 Lecture 12 BSM II - Particle Physics · 2016. 2. 23. · SUSY cross section versus sparticle mass 1000 events produced in 2011 100 events produced in 2011 . Unification of

Unification of coupling constants with supersymmetry

“minimal

supersymmetric

(extension of) SM”

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Page 11: FYST11 Lecture 12 BSM II - Particle Physics · 2016. 2. 23. · SUSY cross section versus sparticle mass 1000 events produced in 2011 100 events produced in 2011 . Unification of
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Page 14: FYST11 Lecture 12 BSM II - Particle Physics · 2016. 2. 23. · SUSY cross section versus sparticle mass 1000 events produced in 2011 100 events produced in 2011 . Unification of

Extended Higgs sector

In the Standard Model single Higgs doublet, often

written as 𝜑+

𝜑0 or 0

𝑣2

Extended: Many choices but a few constraints,

for instance suppression of FCNC and 𝑀𝑊

𝑀𝑍= cos 𝜃𝑊

• Most successful: 2 Higgs doublet models (2HDMs)

– Supersymmetry uses this

• See-saw models predict Higgs triplet with 𝜑0, 𝜑+ − , 𝜑++ − −

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Page 15: FYST11 Lecture 12 BSM II - Particle Physics · 2016. 2. 23. · SUSY cross section versus sparticle mass 1000 events produced in 2011 100 events produced in 2011 . Unification of

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5 Higgs bosons! h, H, A, H 16

Page 17: FYST11 Lecture 12 BSM II - Particle Physics · 2016. 2. 23. · SUSY cross section versus sparticle mass 1000 events produced in 2011 100 events produced in 2011 . Unification of

Examples of searches for extra Higgs bosons

Singly-charged Doubly-charged

Limits around 𝒪(200 GeV ) 600 GeV

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Page 19: FYST11 Lecture 12 BSM II - Particle Physics · 2016. 2. 23. · SUSY cross section versus sparticle mass 1000 events produced in 2011 100 events produced in 2011 . Unification of

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T. Rizzo, hep-ph/0610104

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Dijets

• SM background obviously much larger

– But single source

– And opens the door to strongly interacting objects

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Page 22: FYST11 Lecture 12 BSM II - Particle Physics · 2016. 2. 23. · SUSY cross section versus sparticle mass 1000 events produced in 2011 100 events produced in 2011 . Unification of

W’ / e

Another very simple selection: lepton + MET

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Page 23: FYST11 Lecture 12 BSM II - Particle Physics · 2016. 2. 23. · SUSY cross section versus sparticle mass 1000 events produced in 2011 100 events produced in 2011 . Unification of

Extra Dimensions

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Page 24: FYST11 Lecture 12 BSM II - Particle Physics · 2016. 2. 23. · SUSY cross section versus sparticle mass 1000 events produced in 2011 100 events produced in 2011 . Unification of

ADD extra dimensions

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Page 25: FYST11 Lecture 12 BSM II - Particle Physics · 2016. 2. 23. · SUSY cross section versus sparticle mass 1000 events produced in 2011 100 events produced in 2011 . Unification of

ADD signatures

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Page 27: FYST11 Lecture 12 BSM II - Particle Physics · 2016. 2. 23. · SUSY cross section versus sparticle mass 1000 events produced in 2011 100 events produced in 2011 . Unification of

Warped extra dimensions

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Graviton excitations

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Page 29: FYST11 Lecture 12 BSM II - Particle Physics · 2016. 2. 23. · SUSY cross section versus sparticle mass 1000 events produced in 2011 100 events produced in 2011 . Unification of

Example The infamous bump is an example of a search for RS gravitons:

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Gauge boson excitations

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Page 31: FYST11 Lecture 12 BSM II - Particle Physics · 2016. 2. 23. · SUSY cross section versus sparticle mass 1000 events produced in 2011 100 events produced in 2011 . Unification of

(super)Strings

Avoid infinities from point-like particles

Different vibration modes = different particles

One fundamental parameter: string size

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Great idea but we have not yet understood how to test it at current ”low” energies Extra dimensions a must Supersymmetry a plus

Page 32: FYST11 Lecture 12 BSM II - Particle Physics · 2016. 2. 23. · SUSY cross section versus sparticle mass 1000 events produced in 2011 100 events produced in 2011 . Unification of

Dark Matter Searches

Lots of models, this is not a unique search!

Typically divided in two ”classes”:

WIMP: weakly interacting massive particle ( elementary particle)

MACHO: Massive Compact Halo Objects (planets, dwarf stars, something large)

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Page 33: FYST11 Lecture 12 BSM II - Particle Physics · 2016. 2. 23. · SUSY cross section versus sparticle mass 1000 events produced in 2011 100 events produced in 2011 . Unification of

33 or even black holes ~10000 x MSun

(MACHOs) (WIMPS)

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Underground searches (experiments: DAMA, Xenon etc WIMP scatters off nuclei Looking for annual modulation / DM ”wind”

Cross section depends on exchange particle: Z exchange ruled out Now looking for H exchange

Page 36: FYST11 Lecture 12 BSM II - Particle Physics · 2016. 2. 23. · SUSY cross section versus sparticle mass 1000 events produced in 2011 100 events produced in 2011 . Unification of

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Look for annihilation signals! Measure decay products

Experiments: FERMI, PAMELA, AMS etc

Page 37: FYST11 Lecture 12 BSM II - Particle Physics · 2016. 2. 23. · SUSY cross section versus sparticle mass 1000 events produced in 2011 100 events produced in 2011 . Unification of

At the LHC

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No Dark Matter interaction with the detector signature is missing energy Use initial state radiation (ISR) to detect it! (e.g jets, , W, Z, H)

Page 38: FYST11 Lecture 12 BSM II - Particle Physics · 2016. 2. 23. · SUSY cross section versus sparticle mass 1000 events produced in 2011 100 events produced in 2011 . Unification of

Summary/outlook

• Many problems with current Standard model

• Many new models to take over

Some important models not mentioned, for instance: – GUT models

– Technicolor

– Hidden valleys

• The LHC energy scale is tuned to be sensitive to many of these, complementary to other current searches

• Several potential signatures requires new ”objects”, ie lepton-jets, long-lived heavy particles, ”quirks” etc

• Several good ideas but Nature decides which (if any) are true!

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