SPIN QUACK ! QUACK ! Not all things that quack are ducks! We will - - PowerPoint PPT Presentation

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SPIN QUACK ! QUACK ! Not all things that quack are ducks! We will - - PowerPoint PPT Presentation

What is Discovering SUSY ? E.g. what makes Supersymmetry different to Universal Extra Dimensional models with Kaluza-Klein particles. One part of the answer: SPIN QUACK ! QUACK ! Not all things that quack are ducks! We will


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SLIDE 1

What is “Discovering SUSY” ?

  • E.g. – what makes Supersymmetry

different to Universal Extra Dimensional models with Kaluza-Klein particles.

  • One part of the answer:

SPIN

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SLIDE 2

QUACK ! QUACK !

Not all things that quack are ducks!

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SLIDE 3

We will see two important themes:

  • Mass measurements will

precede(*) spin determinations

  • “Spin measurement”(**) should not

be confused with “sensitivity to spin”

(*) or will at best be simultaneous with (**) Here “spin measurement” means “determining unambiguously the correct nature (scalar, fermion, vector) of one or more particles in a decay chain or model

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SLIDE 4

(more info at) A REVIEW OF SPIN DETERMINATION AT THE LHC

Lian-Tao Wang and Itay Yavin

arXiv:0802:2726

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SLIDE 5

Spin determination topics

  • Consistency checks
  • Spins in “QLL chain”

– A.Barr

hep-ph/0405052 – Smillie et al hep-ph/0605286 – Florida etc arXiv:0808.2472

– Biglietti et al

ATL-PHYS-PUB-2007-004

  • Slepton Spin (production)

– A.Barr

hep-ph/0511115

  • MAOS method

– Cho, Kong, Kim, Park arXiv:0810.4853

  • Gluino chain spin

– Alvez, Eboli, Plehn

hep-ph/0605067

  • Spins in chains with charginos

– Wang and Yavin

hep-ph/0605296

– Smillie

hep-ph/0609296

  • Spins in chains radiating photons

– Ehrenfeld et al arXiv:0904.1293

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SLIDE 6

Spin Consistency Check

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SLIDE 7

Spin Consistency Check

Di-Lepton Invariant Mass (GeV) Relative Frequency

Straight line

Consistent with:

  • Phase-space
  • Scalar slepton

(SFSF)

  • Fermion KK lepton

(FVFV)

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SLIDE 8

QL Spin Determination (A.Barr)

“NEAR” “FAR”

How can we tell from ?

2 problems:

How can we distinguish the „near‟ lepton from the „far‟ lepton?

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SLIDE 9

Quark+NearLepton

invariant mass distributions for:

sin ½θ*

Back to back in 2

0 frame

QL+ QL-

Phase space (spin-0) Probability density

QUARKS

L+ L-

and

sin ½θ*

Back to back in 2

0 frame

QL- QL+

Phase space (spin-0) Probability density

ANTI-QUARKS

L+ L-

and

_ _

hep-ph/0405052

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SLIDE 10

Experimental problem

  • Cannot reliably distinguish QUARKs from

ANTI-QUARKs

In experiment, can only distinguish RED(QL+,_ L+) from BLUE(QL-,_L-) Can only distinguish lepton charge RED(QL+,QL+) from BLUE(QL-,QL-)

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SLIDE 11

Expect QUARK and ANTI-QUARK contributions to cancel:

QL+ QL+

_

QL- QL-

_

SUM

jL+

SUM

jL-

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SLIDE 12

But LHC is Proton-Proton machine

  • More Quarks than Anti-Quarks! So get:

QL+ QL+

_

QL- QL-

_

SUM SUM

jL+ jL-

Asymmetry!

hep-ph/0405052

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SLIDE 13

“Far” Lepton washout?

“NEAR” “FAR”

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SLIDE 14

jL+

So define mjL+, mjL- asymmetry

parton-level detector-level Asymmetry “A” spin-0

MjL / GeV  sin ½θ*

where

jL-

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SLIDE 15

Different method altogether

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SLIDE 16

Direct slepton spin detection: qq→Zγ* →slepton slepton

1

~ 

1

~ 

R

l ~

R

l ~

l

l

hep-ph/0511115

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SLIDE 17

Look at slepton production angle in c.o.m.

hep-ph/0511115 ATL-PHYS-PUB-2005-023

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SLIDE 18

Have some access to desired angle

Distribution of is correlated with decay angle

hep-ph/0511115 ATL-PHYS-PUB-2005-023

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SLIDE 19

Direct slepton spin (A.Barr)

Signal only hep-ph/0511115 2 years high luminosity?

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SLIDE 20

Different again

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SLIDE 21

Spin Determination (T.Plehn et.al.)

  • What if we want to investigate chain from gluino?
  • Crucial to test gluino nature
  • Cannot rely on quark

charge asymmetry

“NEAR” “FAR” “NEAR” “FAR”

hep-ph/0605067

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SLIDE 22

Instead, rely on b-tag

B B _

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SLIDE 23

Instead, rely on b-tag

B B _

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SLIDE 24

MBL

BL+ and

and MBL

BL- distributions

distributions

SUSY UED

Room for an asymmetry!

hep-ph/0605067

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SLIDE 25

So define asymmetry

Signal, no cuts hep-ph/0605067

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SLIDE 26

After realistic cuts, SPS1A, 200 fb-1

Asymmetry still

  • bservable

Acceptance cuts: Cuts to reject Standard Model hep-ph/0605067

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SLIDE 27

Back to long chains

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SLIDE 28

Spin sensitivity elsewhere in the llq chain (Smillie et.al.) Later more general follow-up (Matchev, Kong, et al)

F F F F S F S

hep-ph/0605286 arXiv:0808.2472 Cannot distinguish:

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SLIDE 29

But masses matter

SPS1a mass spectrum: (GeV) UED-type mass spectrum: (GeV) (R-1 ~ 800 GeV)

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SLIDE 30

SPS1a masses UED type masses hep-ph/0605286

Maybe masses are not too important for mll distribution

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SLIDE 31

hep-ph/0605286

… but this fun ….

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SLIDE 32

…. is spoiled. 

MJL+ MJL- MJL- MJL+

hep-ph/0605286

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SLIDE 33

Example asymmetries:

(a big mix of spin and mass spectrum) 

SPS1a UED type

MJL MJL A A

hep-ph/0605286

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SLIDE 34

Yet another game one can play

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SLIDE 35

MT2-assisted (MAOS) spin determination

Use splitting for which leads to MT2 solution to assign 4-momenta to invisible particles:

Cho, Choi,Kim,Park, 0810.4853

qbar q

gluino gluino Then do conventional Dalitz plot for each side. Then do conventional Dalitz plot for each side.

Finds the spin

  • f these gluinos
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SLIDE 36

MT2-assisted (MAOS) spin determination

assign 4-momenta

SUSY SUSY UED UED

Cho, Choi,Kim,Park, 0810.4853

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SLIDE 37

Reminder: cross sections reveal spins

Datta, Kane, Toharia hep-ph/0510204

Higher spins mean higher cross sections (for given masses)

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SLIDE 38

End Notes

  • QLL chain

– Some spin “sensitivity” – but no strong UED/SUSY separation – Reduced discriminatory power when considering general couplings (Matchev/Kong).

  • Di-slepton production

– Better chance of separating UED/SUSY – Still model dependent

  • Both require large cross sections
  • Masses inextricably intertwined.
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SLIDE 39
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SLIDE 40

Backup slides

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SLIDE 41

43

Helicity dependence

Process 1 (SUSY) Process 1 (UED, transverse Z*: P /P = 2x) Both prefer high invariant mass

T L