New Physics Searches at CMS Claudio Campagnari UC

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New Physics Searches at CMS Claudio Campagnari UC Santa Barbara 1

New Physics Searches at CMS Claudio Campagnari UC Santa Barbara 1

What this talk is not A comprehensive summary of New Physics (NP) potential/reach at

What this talk is not A comprehensive summary of New Physics (NP) potential/reach at CMS Because: 1. You have probably seen it before 2. Many public NP CMS results are quite old • CMS now finalizing approval of a many results for the Physics TDR • • Better, more realistic, treatment Happy reading! 3. I am not an expert on most of these searches 2

What this talk is trying to do • Give you a sense of how

What this talk is trying to do • Give you a sense of how searches for New Physics are carried out • Give you some rules-of-thumb to help you think about them • Point out issues on theoretical side 3

Outline • Parton-parton luminosities, cross sections • Ingredients for discoveries • Different type of

Outline • Parton-parton luminosities, cross sections • Ingredients for discoveries • Different type of searches – examples – comments on theoretical issues 4

Parton-Parton luminosities • LHC opens up new energy regime – obvious • A way

Parton-Parton luminosities • LHC opens up new energy regime – obvious • A way to think about this and develop a semiquantitative intuition: Look at parton-parton luminosities • Hadron collider = collisions of two broadband beams of partons (q, q, and gluons) • Define "effective luminosity" for parton-parton collisions as a function of the ECM of the parton-parton system 5

Parton-Parton luminosities (2) • Parton-parton x-section, i+j X: EHLQ RMP 56 579 (1984) •

Parton-Parton luminosities (2) • Parton-parton x-section, i+j X: EHLQ RMP 56 579 (1984) • pp (or pp) x-section, pp X or pp X: (the sum is over all the i's and j's that result in X) • Rewrite it as: Luminosity for parton-parton collisions as a function of parton-parton ECM 6

Parton-Parton luminosities (3) gg luminosity @ LHC qq luminosity @ LHC gg luminosity @

Parton-Parton luminosities (3) gg luminosity @ LHC qq luminosity @ LHC gg luminosity @ Tevatron qq luminosity @ Tevatron 7

Zooming-in on the < 1 Te. V region gg luminosity @ LHC qq luminosity

Zooming-in on the < 1 Te. V region gg luminosity @ LHC qq luminosity @ LHC gg luminosity @ Tevatron qq luminosity @ Tevatron 8

Ratio of LHC and Tevatron parton luminosities LHC vs Tevatron gg qq 1 st

Ratio of LHC and Tevatron parton luminosities LHC vs Tevatron gg qq 1 st (simplistic) rule of thumb: – For 1 Te. V gg processes, 1 fb-1 at FNAL is like 1 nb-1 at LHC – For 1 Te. V qq processes, 1 fb-1 at FNAL is like 1 pb-1 at LHC 9

Another rule of thumb: d. L/d falls steeply with ECM • In multi-Te. V

Another rule of thumb: d. L/d falls steeply with ECM • In multi-Te. V region, ~ by factor 10 every 600 Ge. V • New states produced near threshold • Suppose you have a limit on some pair-produced object, M > 1 Te. V • How does your sensitivity improve with more data? LHC gg qq Answer: by ~ (600/2)=300 Ge. V = 30% for 10 times more lumi 10 Improving sensitivity with lumi is tough. . but you might turn a hint into discovery

T. Han Tev 4 LHC SM Cross Sections Good to keep these in mind

T. Han Tev 4 LHC SM Cross Sections Good to keep these in mind when thinking about NP • (bb, high PT) ~ 1 b • (W l ) ~ 60 nb • (WW) ~ 200 pb • (tt) ~ 1 nb Jet rates are enormous ~ 10 b/Ge. V @ 100 Ge. V ~ 0. 1 pb/Ge. V @ 1 Te. V Also, another useful rule of thumb: (X+1 jet) ~ 1/10 (X) for moderate (~ 30 Ge. V) PT jet 11

NP discoveries at the LHC 3 + 1 ingredients 0. Detector and machine: If

NP discoveries at the LHC 3 + 1 ingredients 0. Detector and machine: If they don't work, forget it • I assume (hope? pray? ) that they will 1. Trigger: If you didn't trigger on it, it never happened • See Sridhara's talk 2. Backgrounds: It's the background, stupid • Need to understand SM and instrumental backgrounds • • • Instrumental BG: us (experimentalists, mostly) Physics BG: you (theorists, mostly) There are exceptions. . 3. Searches: If you look for something, you may not find it. But if you don't look, you will never find it • Model independent vs model dependent searches 12

NP discovery ingredients • Carefully crafted combinations of – photons – electrons – muons

NP discovery ingredients • Carefully crafted combinations of – photons – electrons – muons – taus – jets – b-tagged jets – missing transverse energy (MET) • A quick look at these ingredients to develop intuition about them – particularly the questions of BG & fake rates 13

Jets • Jets are everywhere • Jets can fake isolated high PT , e,

Jets • Jets are everywhere • Jets can fake isolated high PT , e, , signatures D 0 Lauer Ph. D Thesis Iowa State – Probability of jet faking a : ~ few 10 -4. – Probability of faking e or ~ 1 order of magnitude smaller • But some jets have real lepton, e. g. , b-jets – Probability of faking a : ~ few 10 -3 • Light quark or gluon jets fake b-quark signature at the % level Wen (Rutgers) DPF 2004 CDF Jeans (Rome) LHC Symposium 05 14 All of these to be measured on data (not MC)

Missing Transverse Energy • Fake MET mostly from jets, resolutions and tails 1 min

Missing Transverse Energy • Fake MET mostly from jets, resolutions and tails 1 min bias event contribution to MET component in a given direction ~ 6 Ge. V • Also from missed muons • Also from "underlying event" CMS And the tails don't come without some work. . D 0 15

 • A little bit of intuition/knowledge of – cross-sections – triggers – fake

• A little bit of intuition/knowledge of – cross-sections – triggers – fake rates is necessary to estimate whether something is feasible or not • You should try to develop it • Hardest intuition is on MET tails • Have easy to use tools to calculate x-section, kinematical distribution for many LO processes 16 e. g. , COMPHEP

New Physics discoveries @ LHC Broadly speaking, three possibilities 1. Self Calibrating • e.

New Physics discoveries @ LHC Broadly speaking, three possibilities 1. Self Calibrating • e. g. , a mass peak 2. Counting experiments • The number of observed events of some type is >> than the SM prediction 3. Distributions • The distribution of some kinematical quantity is inconsistent with the SM prediction NB: the distinction is not always clean, but still 17 useful to think in these terms

Self Calibrating Signals (SCS) • A NP signal that stands out and punches you

Self Calibrating Signals (SCS) • A NP signal that stands out and punches you in the face – where you do not need to know the SM BG very precisely • or do you? • watch out for irrational exuberance • For example: – A mass peak – A huge distortion to some kinematical distribution 18

SCS example: Z' What a 100 pb-1 expt might look like Cousins, Mumford, Valuev

SCS example: Z' What a 100 pb-1 expt might look like Cousins, Mumford, Valuev UCLA 19

Another SCS example: di-jet resonances e. g. , excited quarks, axigluons, E 6 di-quarks,

Another SCS example: di-jet resonances e. g. , excited quarks, axigluons, E 6 di-quarks, Z', W', . . . Rules of thumb: • If produced strongly about same cross section as QCD at same mass, fairly easy to see • If produced weakly, tougher CMS 20

Di-jet resonances (cont. ) 95% CL Sensitivity to Dijet Resonances CMS Published Exclusion (Dijets)

Di-jet resonances (cont. ) 95% CL Sensitivity to Dijet Resonances CMS Published Exclusion (Dijets) CMS 100 pb-1 CMS 1 fb-1 CMS 10 fb-1 E 6 Diquark Excited Quark Axigluon or Coloron Color Octet Technirho W’ RS Graviton Esen and Harris (FNAL) Gumus and Akchurin (Texas Tech) Z’ 0 1 2 3 4 5 6 Mass (Te. V) 21

(Yet) Another SCS example: di-jet mass distribution • Distorts angular distributions • More scatters

(Yet) Another SCS example: di-jet mass distribution • Distorts angular distributions • More scatters at high angles – More jets at high PT – More di-jets at high mass • Like Rutherford scattering, but with quarks! Quark Compositeness New Interactions q q M~L q q Dijet Mass << L Quark Contact Interaction q q d / d. M or d /d. PT L QCD Background QCD + Signal q q If the "edge" is low enough, this could be a relatively easy discovery (Self-calibrating variety) 22 Dijet Mass or jet PT

Di-jet mass distribution distortion • Ratio of events at high-low is a sensitive variable

Di-jet mass distribution distortion • Ratio of events at high-low is a sensitive variable that eliminates many syst uncertaintes CMS Left-Handed Quark Contact Interaction + for 100 pb-1 (Te. V) + for 1 fb-1 (Te. V) + for 10 fb-1 (Te. V) 95% CL Exclusion 6. 2 10. 4 14. 8 5σ Discovery 4. 7 7. 8 12. 0 Esen and Harris (FNAL) Gumus and Akchurin (Texas Tech) 23

SCS: Edges 10 fb-1 M(l+l-) 24

SCS: Edges 10 fb-1 M(l+l-) 24

Not all that glitters is gold Pentaquarks z(8. 3) Leptoquarks 40 Ge. V top

Not all that glitters is gold Pentaquarks z(8. 3) Leptoquarks 40 Ge. V top Buyer beware. Especially in the tails of distributions 25

An aside Tail of the jet ET distribution. Definitely not a self calibrating signal

An aside Tail of the jet ET distribution. Definitely not a self calibrating signal (SCS) CDF PRL 77 438 (1996) • Data in the tail not consistent with QCD + (then) existing sets of parton distribution functions (PDFs) • Looks like contact term ~ 1. 6 Te. V • Further PDF analysis found that the discrepancy could be absorbed by modifying gluon distribution – without conflicting with other data – even though all existing PDF fits were "low" • Modern PDFs include uncertainties • A great step forward Example of careful, not-so-glamorous, phenomenological work that has a major impact 26

Counting experiments, distributions • Not all NP signals are as dramatic as a mass

Counting experiments, distributions • Not all NP signals are as dramatic as a mass peak • Need to establish whether data is or is not compatible with SM Need the SM prediction • In some cases the SM prediction can come entirely from the experiment (data driven) • Robust • In other cases the SM prediction relies heavily on theory • Not so robust • A couple of examples to understand typical issues 27

Example 1: CDF search for NP in lep + + MET • www-cdf. fnal.

Example 1: CDF search for NP in lep + + MET • www-cdf. fnal. gov/physics/exotic/r 2 a/20050714. loginov. Lep. Photon. X/ • A fairly simple final state • Motivated by a few weird events in Run 1 • Select events, then compare with SM – both number of events and kinematical distributions • Requires careful accounting of SM sources • A lot of work! – typical for this type of searches – painstaking accounting of many BG sources – you don't just "run the Monte Carlo" • this is not e+e 28

SM contributions to lep+ +MET (1) • pp W+jet, W lep , jet fakes

SM contributions to lep+ +MET (1) • pp W+jet, W lep , jet fakes – estimated from observed rate of W+jet and measured probability for jet to fake a – difficult (100% uncertainty), but data driven • Drell-Yan e+e- pairs with hard brehmstrahlung, where the electron is lost and looks like a and the MET fluctuates high – estimated from observed rate of Z ee and Z e" " and observed MET distribution – data driven • pp jets, jets fake leptons – estimated from data by relaxing the lepton quality requirements, and extrapolating 29

SM contributions to lep+ +MET (2) • pp W or Z – This turns

SM contributions to lep+ +MET (2) • pp W or Z – This turns out to be the main background – Need theoretical input – Tools are: • LO parton level event generators, interfaced to Pythia – yes: more than one • NLO calculation – Good case because the NLO calculation exist • Often it doesn't • The NLO/LO K-factor is ~ 1. 5, but it varies across phase space • The LO MC is then "fudged" to account for that 30

Baur, Han, and Ohnemus. PRD 57 (1998) 2823 NLO changes shape of distributions 31

Baur, Han, and Ohnemus. PRD 57 (1998) 2823 NLO changes shape of distributions 31

Results of CDF lep + + MET search Decent agreement in shape and normalization

Results of CDF lep + + MET search Decent agreement in shape and normalization Without NLO, SM prediction ~ 26 ± ? What would you have concluded? 32

Example 2: UA 2 W tb search (1989) • Ancient, but an example of

Example 2: UA 2 W tb search (1989) • Ancient, but an example of a search based on a shape analysis that is independent of theoretical assumptions – yes, sometimes this happens! • Signal is W tb, t e b – M(e ) < MW • BG is W+jets, W e – M(e ) = MW Z. Phys. C 46, 179 1990 33

Example 3: CDF tt evidence (1994) • Also ancient, but example of counting expt

Example 3: CDF tt evidence (1994) • Also ancient, but example of counting expt independent of theoretical assumptions • Signal: lep + MET + ≥ 3 jets (≥ 1 of them b-tagged) • Background: W+jets (fake b-tag), or Wbb (real b-tag) • Background estimate, entirely data-driven: – measure b-tagging rate per jet in pp jets • includes fake and real tags – apply to jets in W + jets sample • conservative • b-content of pp jets >> pp W+jets) PRD 50 2966 1994 34

Comments • Often purely data driven BG estimates do not work • SM BG

Comments • Often purely data driven BG estimates do not work • SM BG to LO have large normalization uncertainties – Makes counting experiments difficult • SM LO event generators can have large shape uncertainties – Makes shape analyses difficult • What are the uncertainties at LO? at NLO? – Often can get handle from data, e. g. , W+jets vs Z+jets • Where is the smoking gun? – As an experimentalist, more comfortable if uncertainties are under my control – As a theorist, you might feel differently – Don't ask how sausages are made 35

What can you do for us? Slides from Z. Bern at LBNL LHC West

What can you do for us? Slides from Z. Bern at LBNL LHC West Coast Theory Network meeting And don't forget to implement them in a MC so that we can actually use them Now that we are about to get data, nuts-and-bolts contributions can be more useful than suggestions for another beyond the SM theory 36

Model dependent vs. model independent searches • Can search for generic NP signatures e.

Model dependent vs. model independent searches • Can search for generic NP signatures e. g. , the lep + + MET CDF search described earlier • Or, for very specific, complicated signatures e. g. , pp TT, T t. Z T b. W, t e b Z , W • Because we do not know what the NP is, generic searches are very powerful • But in a generic search worry about missing complicated signature • With O(1000) physicists both approaches will be pursued 37

Ba. Bar Palano (Bari) Ds. J(2317) DS 0 PRL 90 242001 (2003) This huge

Ba. Bar Palano (Bari) Ds. J(2317) DS 0 PRL 90 242001 (2003) This huge signal had been in various data sets for many years. – What is hiding in the Tevatron data sets? – What was missed by the Tevatron triggers? 38

A case study: tt at the Tevatron • The high PT discovery at Tevatron

A case study: tt at the Tevatron • The high PT discovery at Tevatron • Not NP, the ultimate known unknown • Complicated signature, search narrowly focused on expected SM properties Would it have been seen in generic search? • In the high statistics lep+jets channel probably not for a long time – Lots of BG, theoretical tools (W+multijet & Wbb calculations/MC) developed specifically for the search • In the dilepton channel would have slowly emerged as excess of events with jets (and eventually, b-jets) Power of multi-lepton searches 39

If we see NP, can we tell what it is? • Great question –

If we see NP, can we tell what it is? • Great question – Supersymmetry and the LHC inverse problem (hep-ph/0512190) • Great fun (Olympics. . . ) • But give me a break – Let's 1 st find a NP signal, and celebrate • Emphasis shifts to "Given that you see X, if the NP is Y, you should see Z" – suggestions with Z experimentally impossible not very useful • but do not underestimate your experimental colleagues! – a well developed feel for experimental issues could make a difference 40

Conclusion • After a long wait, exploration of the Te. V scale is about

Conclusion • After a long wait, exploration of the Te. V scale is about to start in earnest • There are many ideas about NP, but we don't know what it is – That's why they play the games • Nuts-and-bolts contributions from theory community extremely important and perhaps underappreciated 41