rare kaon physics from 30,000’ and other perspectives

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Rare kaon physics from 30,000’ and other perspectives L. Littenberg 29 April 2013

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Rare kaon physics from 30,000’ and other perspectives. L. Littenberg 29 April 2013. Outline. Some things can best be appreciated from 30,000 feet What do we have to do to get some respect ? What does N events buy us? Lightening review of K ® pnn experimental situation Real ghosts - PowerPoint PPT Presentation

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Page 1: Rare  kaon  physics from 30,000’ and other perspectives

Rare kaon physics from 30,000’ and other perspectives

L. Littenberg29 April 2013

Page 2: Rare  kaon  physics from 30,000’ and other perspectives

Outline

• Some things can best be appreciated from 30,000 feet• What do we have to do to get some respect?• What does N events buy us?• Lightening review of K ® pnn experimental situation• Real ghosts• Any alternatives?• A challenge• Cycling back to the beginning

Page 3: Rare  kaon  physics from 30,000’ and other perspectives

Some things you can only appreciate from 30,000’

Page 4: Rare  kaon  physics from 30,000’ and other perspectives

Like the Nasca lines in Peru

Page 5: Rare  kaon  physics from 30,000’ and other perspectives

It’s clear they were trying to perfect them

Page 6: Rare  kaon  physics from 30,000’ and other perspectives

Could have been a contender• Almost as old as the Nasca pix:

• Green dashed line is supposed to be the usual unitarity triangle• Red solid line is a triangle from rare kaon information alone• If SM is the whole story the vertices at the upper left should meet

Page 7: Rare  kaon  physics from 30,000’ and other perspectives

• Evolution in what qualifies as a discovery. • Now 5s demanded before people believe something.

– It’s kind of interesting, 3s means there’s a 1 in 770 chance of being wrong

– But that’s not good enough, we demand a 1 in 3.5M chance!– Note that in the US, there are 1.1 deaths/108 highway miles

• So if you drive 10,000 miles/year, your chance of dying is 1 in 9000.• So you will bet your life on 3.7s, much less than you demand of a physics

result!– Seems like we don’t trust our own systematic errors

• Let me pose the question – how close could one come to the Standard Model, and have a five sigma deviation from it?

What do we have to do to get some respect?

Even though we experimentalists couldn’t possibly make a >5s mistake!

Page 8: Rare  kaon  physics from 30,000’ and other perspectives

• Evolution in what qualifies as a discovery. • Now 5s demanded before people believe something.

– It’s kind of interesting, 3s means there’s a 1 in 770 chance of being wrong

– But that’s not good enough, we demand a 1 in 3.5M chance!– Note that in the US, there are 1.1 deaths/108 highway miles

• So if you drive 10,000 miles/year, your chance of dying is 1 in 9000.• So you will bet your life on 3.7s, much less than you demand of a physics

result!– Seems like we don’t trust our own systematic errors

• Let me pose the question – how close could one come to the Standard Model, and have a five sigma deviation from it?

What do we have to do to get some respect?

Page 9: Rare  kaon  physics from 30,000’ and other perspectives

How many events you need to have 5s?

Equivalent Events

Ratio

to S

M @

5s

Page 10: Rare  kaon  physics from 30,000’ and other perspectives

Zeroing in

D.M. Straub arXiv:1012.3893

Page 11: Rare  kaon  physics from 30,000’ and other perspectives

Zeroing in – 10 event experiments

Page 12: Rare  kaon  physics from 30,000’ and other perspectives

Zeroing in – 100 event experiments

Page 13: Rare  kaon  physics from 30,000’ and other perspectives

Zeroing in – 100 event experiments

Page 14: Rare  kaon  physics from 30,000’ and other perspectives

Zeroing in – 1000 event experiments

Page 15: Rare  kaon  physics from 30,000’ and other perspectives

More realistically …

A. Buras et al., General MSSM, tanb = 20 hep-ph/0408142

_

_

1000 evts

Page 16: Rare  kaon  physics from 30,000’ and other perspectives

More recent theory example

“Trivially Unitary Model” from A. Buras et al. arXiv:1301.5498v1

Page 17: Rare  kaon  physics from 30,000’ and other perspectives

Primary K ® pnn experimental technique

Page 18: Rare  kaon  physics from 30,000’ and other perspectives

Veto System

Page 19: Rare  kaon  physics from 30,000’ and other perspectives

Vetoed Event

Page 20: Rare  kaon  physics from 30,000’ and other perspectives

Ghosts of Experiments Past: E949 @ BNL

• Proved K+ ® p+nn could be done in the “traditional” way• Designed to be a 10-event experiment by my criterion• But killed in the prime of life so ended up a two-event experiment

Page 21: Rare  kaon  physics from 30,000’ and other perspectives

Ghosts of Experiments Past: E391a @ KEK

• First dedicated KL ® p0nn experiment• High energy approach performed at low energy• Need another factor 1000

Page 22: Rare  kaon  physics from 30,000’ and other perspectives

Ghosts of Experiments Present: KOTO @ J-PARC

• High energy technique for KL ® p0nn at even lower energy• Scheduled for 1st long physics run any minute• Much experience, improved technology• First stage is a 1.5 event experiment by my criterion• Step-by-step approach has a lot going for it• Next step, get rid of some unnecessary constraints

Page 23: Rare  kaon  physics from 30,000’ and other perspectives

Ghosts of Experiments Present: NA62@ CERN

• First to use in-flight technique for K+ ® p+nn • Physics run scheduled for 2014• Designed to leap 11 orders of magnitude in a single bound• 75-event class experiment

Page 24: Rare  kaon  physics from 30,000’ and other perspectives

Ghosts of Experiments Future: ORKA@FNAL

• Lineal descendent of previous K+ ® p+nn experiments• 10x the exposure of E949• 10x better acceptance • Scientific approval December 2011• Would be a 400-event experiment by my criterion

Page 25: Rare  kaon  physics from 30,000’ and other perspectives

Ghosts of Experiments Future: KOPIO-like experiment for Project-X2

• True 1000-event class experiment• Really requires 3 GeV Stage 2 of Project-X

Page 26: Rare  kaon  physics from 30,000’ and other perspectives

Once and future K experiments

E39

1a

KO

TO

E94

9

NA

62

OR

KA

P-X

K0

Even

tsEvents

LL Evts

Page 27: Rare  kaon  physics from 30,000’ and other perspectives

True Ghost Experiments

E949 - killed in its prime by DOE KOPIO – NSF pulled the plug on RSVP

CKM - murdered by P5 KaMI - rejected by the Fermilab PAC

Page 28: Rare  kaon  physics from 30,000’ and other perspectives

28

Another Look at KL®p0l+l-• KL®p0l+l- has several kinds of bad-luck and trouble.• NA48 observed KS®p0l+l- at higher end of expectation• & arguments for constructive interference between mixing &

direct CP-violating components strong as ever• SM expectation for KL®p0l+l- rather large:

– B(KL®p0e+e-) = (41)10-11

– B(KL®p0+-) = (1.50.3)10-11

• Compare with KL®l+l- background (worst one):KL®p0e+e- (‘99) KL®p0+- (‘97)

KTeV s.e.s.. 10.410-11 7.510-11

KL®l+l- evts 0.99 0.37

B(KL®l+l- )effective 10.310-11 2.810-11

S:B 1:2.5 1:1.9

Page 29: Rare  kaon  physics from 30,000’ and other perspectives

29

Motivation for KL®p0l+l-

Add to this, now we are interested in bigger game than Imt.

E.g., from Isidori, et al., hep-

ph/0404127

• Take KaMI as example of a next-generation experiment with sensitivity to KL®p0+-. In 3 years, KaMI would have reached a s.e.s of 410-13.

• In the example above, would collect 110±13 signal events (with 70 events of background) compared with a SM expectation of 37 events.

• KL®p0e+e- case left for homework

Page 30: Rare  kaon  physics from 30,000’ and other perspectives

Why not KL ® +-?K ® pnn

• BR ~ few 10-11

• Very poor signature

• Background 10% or worse

KL ® +-

• BR ~ 7 10-9

• Beautiful signature

• 1% background

Page 31: Rare  kaon  physics from 30,000’ and other perspectives

Here’s Why

The fundamental irony of rare kaon physics: The very interactions that make the the process detectable, introduce obfuscating long-distance effects!

The above process introduces an absorptive part that is many times larger than the short-distance contribution plus a dispersive part that can interfere with it.

Page 32: Rare  kaon  physics from 30,000’ and other perspectives

A long distance to go• We start off with what I’d classify as a 3700 event experiment.• The absorptive piece can be well-determined by measuring KL ®

– Subtracting it gives Bdisp(KL®+-)= (3.2±1.2) 10-10

– I.e. a number ~20 times smaller than the absorptive part– And ~3 times smaller than SM fits to the short-distance part!

• This corresponds to a 7 event experiment! Nature is a real killjoy.• And this is before trying to untangle the dispersive interference.

– Where there’s agreement from all sectors of the theory world that this is very difficult!

• What could possibly be done?• The experiment can be done better – I never imagined it would be worth it.• Could imagine 5 smaller errors, would correspond to a ~200 event

experiment for the dispersive part.• Then the theorists could do their part. If they were perfect, and the true

value was ~ the SM-predicted one, could get to 500 event equivalent. So it might be worth considering

– But theorists really have to do well. A 10% error on the dispersive amplitude degrades it to a 100 equivalent event experiment

Page 33: Rare  kaon  physics from 30,000’ and other perspectives

What about KS ® +-?

• In this case the short distance piece is CP-violating!– In the SM µh2.– BR = 1.7 10-13, exp as sensitive as the KL one would see 1.5 evts

• Moreover the long distance parts are tractable – Don’t interfere with the SM– Well-calculable – maybe the lattice could improve further

• But LD parts are still 25 bigger than SD (~510-12).• Note Isidori & Unterdorfer (hep-ph/0311084) point out that

K+ ® p+nn currently limits SD BR to ~10-11 in most BSM models. – So any sensitivity exceeding that limit is interesting.– Starts to limit K ® pnn, also Grossman-Nir bound

• Present limit, 9x10-9 @ 90%CL, is from LHCb! (arXiv 1209.4029)• How much better could a fixed-target experiment do?

Page 34: Rare  kaon  physics from 30,000’ and other perspectives

KS ® m+m-

Limits on the K unitarity triangle (Isidori & Unterdorfer)

Corresponds to B(KS® +-)<1.710-11

Evts

/0.1t S

KL®+-

KS + KL (SM)

K®+- events for a 10-13/evt experiment. At the SM level, KL dominates. Green curve corresponds to the BR at which KS®+- becomes a stronger constraint on KL®p0nn than the Grossman-Nir bound. Could get >6s separation from SM for green curve at this sensitivity.Time (tS)

Page 35: Rare  kaon  physics from 30,000’ and other perspectives

Is the Unitarity Triangle Melting?

Page 36: Rare  kaon  physics from 30,000’ and other perspectives

Is the Unitarity Triangle Melting?

For a 100 evt KL experiment this distance is >6s!

Page 37: Rare  kaon  physics from 30,000’ and other perspectives

Take-away Thoughts

• The virtue of the golden twins is safe for at least another generation. There’s a huge range of BR in which to prospect for BSM effects.

• If new physics shows up, can further refine its properties by studying other rare modes.

• But what’s really strange is that the golden twins may be essential for cleaning up what’s now considered the SM CKM triangle, for which they were proposed 25 years ago!

• Editorial: rare process experiments thrive in a programmatic, rather than a project environment.

• Homework: beat LHCb in KS ® +-

• Appreciate that your work may be have uses you never thought of…

Page 38: Rare  kaon  physics from 30,000’ and other perspectives

Limit on heavy photons from K+ ® p+X0

Page 39: Rare  kaon  physics from 30,000’ and other perspectives

Backup Slides

Page 40: Rare  kaon  physics from 30,000’ and other perspectives

What I mean by “equivalent events”

• If you had a perfect experiment, with no background and no systematic errors, a given number of events gives a fractional uncertainty = 1/sqrt(S), where S is the number of signal events.

• So I’m really talking about a certain sensitivity• If one had a perfectly determined background B, the equivalent

number of events would be S/(1+B/S).• If the background had an uncertainty sB, then the equivalent

number of events would be S/(1+B/S + sB2/S)

• This gets increasingly complicated as more realism is inserted, but the basic idea should be clear.