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Fermilab Users Meeting Fermilab Users Meeting Fermilab Users - - PowerPoint PPT Presentation

Fermilab Users Meeting Fermilab Users Meeting Fermilab Users Meeting Fermilab Users Meeting CMS Physics from Early LHC Running Dan Green Fermilab For the CMS Collaboration FNAL Users Meeting June 2010 1 Outline Outline


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SLIDE 1

FNAL Users’ Meeting– June 2010 1

Fermilab Users’ Meeting Fermilab Users’ Meeting Fermilab Users’ Meeting Fermilab Users’ Meeting CMS Physics from Early LHC Running

Dan Green Fermilab For the CMS Collaboration

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SLIDE 2

FNAL Users’ Meeting– June 2010 2

Outline Outline Outline Outline

  • Status of the LHC accelerator and the

detectors.

  • The 7 TeV startup of data taking.
  • Future plans for the accelerator
  • perations.
  • New physics opportunities in 2010, and

then 2011.

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SLIDE 3

FNAL Users’ Meeting– June 2010 3

US HEP and the LHC US HEP and the LHC US HEP and the LHC US HEP and the LHC

Very significant US participation, 1/3 on CMS, ¼ in ATLAS. Fermilab is the host lab for US CMS – E892.

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SLIDE 4

FNAL Users’ Meeting– June 2010 4

The ATLAS and CMS Experiments The ATLAS and CMS Experiments – Status Status The ATLAS and CMS Experiments The ATLAS and CMS Experiments – Status Status

Each detector is like a 100 megapixel camera which takes 40 million pictures per second The experiments have been designed, built, assembled and commissioned over the last 15 years. Using test beams, cosmic rays and lower energy data (0.9 TeV, Nov 2009 and 2.36 TeV Dec. 2009) they were initially aligned and calibrated before the 7 TeV startup,

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SLIDE 5

FNAL Users’ Meeting– June 2010 5

First CMS Publication First CMS Publication First CMS Publication First CMS Publication

Data taken in Dec., 2009. Published in Feb., 2010. Years of preparation pay off with prompt physics

  • results. Good agreement with previous data. The

“re-discovery” of the SM was well launched.

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SLIDE 6

FNAL Users’ Meeting– June 2010 6

March 30 March 30 – First 7 First 7 TeV TeV Collisions Collisions March 30 March 30 – First 7 First 7 TeV TeV Collisions Collisions

CMS is now 2 months into the 7 TeV run

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SLIDE 7

FNAL Users’ Meeting– June 2010 7

CMS has been Efficient CMS has been Efficient CMS has been Efficient CMS has been Efficient

First month of operation – log > 1 nb-1 of data. Rise is “exponential” – L doubling time is ~ 1 week, CMS has operated at ~ 90% efficiency.

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SLIDE 8

FNAL Users’ Meeting– June 2010 8

Plan for 2010, 2011 Plan for 2010, 2011 Plan for 2010, 2011 Plan for 2010, 2011

Integrated L SM Object SM Use Search Strategy

mb-1 ( 1) UE, MB Tune MC ub-1 (103) Jets, Heavy flavor

  • Align. dE/dx

Calib, trigger valid, MET c, b tag leptons nb-1 (106) W Z Cross section, charge Mass scale, resolution 1 pb-1 (109) Top pairs Leptons + J + true MET Black holes 10 pb-1 Dijet M > 2 TeV HSCP, leptoquarks 100 pb-1 (2010) M > TeV W’ , Z’ New range for SUSY 1000 pb-1 (2011) (1012) SUSY – TeV mass scale Higgs @ 95% CL, (140,190) GeV

*

, , , , ,

s

K K    

,

 ,  

CMS will start by rediscovering the Standard Model and then launch searches, starting with strongly produced final states.

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SLIDE 9

FNAL Users’ Meeting– June 2010 9

7 7 TeV TeV – Heavy Flavor Heavy Flavor 7 7 TeV TeV – Heavy Flavor Heavy Flavor

Note error ellipses on the primary and secondary vertices. B tagging is being commissioned. That establishes the fact that CMS tracking is well commissioned.

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SLIDE 10

FNAL Users’ Meeting– June 2010 10

Commissioning of Triggers Commissioning of Triggers with Millions of MB Events with Millions of MB Events Commissioning of Triggers Commissioning of Triggers with Millions of MB Events with Millions of MB Events

By taking millions

  • f MB events, with

the triggers in “mark and pass”, the low Pt triggers can be validated. Then when they are implemented at higher luminosity, the higher Pt triggers will, in turn, be put in mark and pass - bootstrap.

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SLIDE 11

FNAL Users’ Meeting– June 2010 11

MET is Being Commissioned MET is Being Commissioned MET is Being Commissioned MET is Being Commissioned

CMS has made a special effort to commission MET as soon as possible since it is crucial to many searches for new physics, e.g. SUSY. In dijet events there is ~ no true MET and there is a ~ 6 order of magnitude smooth fall of the observed

  • MET. The tails are

being explored and a successful “cleaning” strategy is in train – in time for ICHEP in July.

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SLIDE 12

FNAL Users’ Meeting– June 2010 12

Dilepton Dilepton Resonances Resonances Dilepton Dilepton Resonances Resonances

As the integrated luminosity goes up, dilepton resonances begin to be observed. The J/psi into di- electrons has been

  • seen. The Upsilon will

be next, followed by the Z. This is a “candelabra” of known “standard candle” resonances to be used for calibration – checking the momentum scale and the momentum resolution.

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SLIDE 13

FNAL Users’ Meeting– June 2010 13

W to Electron and W to Electron and Muon Muon W to Electron and W to Electron and Muon Muon

Very recently, > 10 nb-1 has been delivered. CMS will now move from candidate events to kinematic distributions.

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SLIDE 14

FNAL Users’ Meeting– June 2010 14

Z to Di Z to Di-electron electron Z to Di Z to Di-electron electron

Dilepton Z candidates are beginning to

  • appear. More

luminosity is needed to go beyond candidate event searches. New publications are submitted to PRL. Many abstracts have been submitted to ICHEP

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SLIDE 15

FNAL Users’ Meeting– June 2010 15

Z Decays into Lepton Pairs Z Decays into Lepton Pairs Z Decays into Lepton Pairs Z Decays into Lepton Pairs

In the near future CMS will complete the rediscovery of the SM. The dilepton Z “tag and probe” – extract data driven efficiencies for leptons – e.g. e trigger

  • efficiency. Backgrounds

are small so purity for clean tagging is very high. Then look in the high mass tail of the Z and transverse mass for the W…. W, Z recurrence ?

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SLIDE 16

FNAL Users’ Meeting– June 2010 16

Top Top – Jets + Leptons + MET Jets + Leptons + MET Top Top – Jets + Leptons + MET Jets + Leptons + MET

Check jet energy scale with hadronic decay of the W. Check b tag efficiency with 2 b in final state. Establish absolute MET scale. Studying this process largely completes the “rediscovery”

  • f the SM. Top pairs are a

pervasive background to searches BSM.

MW Mt

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SLIDE 17

FNAL Users’ Meeting– June 2010 17

Advancing the Energy Advancing the Energy Frontier Frontier - 2010 2010 Advancing the Energy Advancing the Energy Frontier Frontier - 2010 2010

The parton luminosity ratio is > 10 at a mass of many

  • f the present

Tevatron mass limits. At the TeV mass scale the ratio is large, all else being equal. Truly, the LHC is a machine for discovery and the focus will be

  • n states with ~ (0.5,

1.0) TeV mass scale where the ratio is most favorable.

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SLIDE 18

FNAL Users’ Meeting– June 2010 18

Heavy Stable Charged Heavy Stable Charged Particles Particles Heavy Stable Charged Heavy Stable Charged Particles Particles

Use dE/dx from tracker and timing in CMS detectors to look for HSCP. At 100 pb-1 the explored mass scale is > 0.5

  • TeV. Gluino

(stop) production is a strong process.

pb-1

95% C.L.

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SLIDE 19

FNAL Users’ Meeting– June 2010 19

Dijet Angular Ratios Dijet Angular Ratios Dijet Angular Ratios Dijet Angular Ratios

The di-jet mass searches for excited quarks or contact interactions or ? will be one of the earliest (2010) LHC searches – with fairly low luminosity. The angular ratio has some spin

  • discrimination. The dijet spectrum

already extends to ~ 1 TeV mass.

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SLIDE 20

FNAL Users’ Meeting– June 2010 20

Sequential W Sequential W – Tail of W BW Tail of W BW Sequential W Sequential W – Tail of W BW Tail of W BW

In the SM there are no states beyond the W and the Z

  • > look in

the BW tails. At 100 pb-1 the 95% C.L. for > 1.5 TeV sequential W is reached.

W’

100 pb-1

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SLIDE 21

FNAL Users’ Meeting– June 2010 21

Sequential Z in DY + BW Tail Sequential Z in DY + BW Tail Sequential Z in DY + BW Tail Sequential Z in DY + BW Tail

A 100 pb-1 the mass reach is > 1 TeV for a sequential Z resonance for a 5 s.d. The discovery. reach is longer for a 95 % C.L. exclusion.

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SLIDE 22

FNAL Users’ Meeting– June 2010 22

SUSY Reach in J + MET SUSY Reach in J + MET SUSY Reach in J + MET SUSY Reach in J + MET

Starting in late 2010 the LHC experiments will open up new regions of discovery potential for SUSY. The reach will be greatly extended in 2011.

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SLIDE 23

FNAL Users’ Meeting– June 2010 23

CMS @ 7 TeV, Reach for CMS @ 7 TeV, Reach for Higgs Higgs - 2011 2011 CMS @ 7 TeV, Reach for CMS @ 7 TeV, Reach for Higgs Higgs - 2011 2011

In 2011 CMS will delve deeper into the > TeV mass range and begin to make contributions to the Higgs search.

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SLIDE 24

FNAL Users’ Meeting– June 2010 24

Setting Out into Deep Waters Setting Out into Deep Waters Setting Out into Deep Waters Setting Out into Deep Waters

“The real voyage of discovery consists… in having new eyes” Marcel Proust We have built a magnificent new set of eyes. We have explored the shallows and visited the known islands. Now we will set

  • ut into deep and unknown waters.

The “take home message” is that 2010 and 2011 will be a great ride for the LHC experiments with “exponentially” increasing integrated luminosity. Buckle up.

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SLIDE 25

FNAL Users’ Meeting– June 2010 25

Dijet Masses Dijet Masses Dijet Masses Dijet Masses

With ~ 1 nb-1 of logged data, the dijet mass spectrum is approaching ~ 1 TeV. Strongly produced “new physics” processes will be the first to be searched for – e.g. composite quarks.