Living Long At the LHC G. WATTS (UW/SEATTLE/MARSEILLE) WG3: EXOTIC HIGGS FERMILAB MAY 21, 2015.

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Presentation transcript:

Living Long At the LHC G. WATTS (UW/SEATTLE/MARSEILLE) WG3: EXOTIC HIGGS FERMILAB MAY 21, 2015

What is long lived? G. Watts (UW/Seattle/CPPM) 2 Jets Flavor Further Displaced Vertices Lepton Jets # of leptons Lepton Flavor(s) For me, started with the worry we’d miss the Standard Model Higgs SM couplings still allow a lot of room for something new… But what!? Can’t be too driven by a model… but can’t ignore them completely! Be as final state and model independent as possible

How are we going to look for it? G. Watts (UW/Seattle/CPPM) 3 Two jet decays Single jet decays Topologies Final States Jets Where did it decay? Lepton Jets Additional cuts as needed to reduce background…

G. Watts (UW/Seattle/CPPM) 4

5 Hadronic Signatures Lepton Jets Miscellaneous Comments & Conclusions

Hadronic Jets G. Watts (UW/Seattle/CPPM) 6

ATLAS Displaced Jets G. Watts (UW/Seattle/CPPM) 7 Require evidence of two displaced jets Detector signature evolves with decay length Keep backgrounds under control Decay in each sub-detector is a new analysis

ATLAS Displaced Jets G. Watts (UW/Seattle/CPPM) 8 Displaced Vertex Trackless, low EMF Jet Jet of particles in the Muon Spectrometer

ATLAS Displaced Jets G. Watts (UW/CPPM) 9 Inner detector Vertexing, looser track impact parameter cuts than normal vertexing Sensitivity: 4 cm – 27 cm Calorimeter Muon Spectrometer Tracking & Jet veto, vertexing in the MS Sensitivity: 4.5 m – 14 m ATL-COM-PHYS Z’ ATL-COM-PHYS ATL-COM-PHYS Sensitivity: 1.75 m m

ATLAS Displaced Jets G. Watts (UW/Seattle/CPPM) 10 Look for associated production Can use standard triggers Take a hit in cross section! Custom trigger to look for the signal

ATLAS Displaced Jets G. Watts (UW/Seattle/CPPM) 11 Inner Detector Vertex Reconstruction

ATLAS Displaced Jets G. Watts (UW/Seattle/CPPM) 12 CalRatio Jet Finding Muon Spectrometer Vertexing Custom vertex finding algorithm Tracklets formed from MS hits Tracklets are fit to a vertex using a custom vertex finding algorithm Track and jet isolation similar to trigger level cuts

ATLAS Displaced Jets G. Watts (UW/Seattle/CPPM) 13 Displaced Trigger Topology (Vertex Locations) Yes-2 ID YesMSID + MS YesMS2 MS -CalRatio2 CalRatio Combined Limits are derived for each of the various senarios

ATLAS Displaced Jets G. Watts (UW/Seattle/CPPM) 14

ATLAS DV and 2 Lepton Search G. Watts (UW/Seattle/CPPM) 15 DV Jet DV DV+ Searches optimized for for RPV SUSY, split SUSY, GMSB Long lived: both decays to leptons and to jets!

ATLAS DV and 2 Lepton Search G. Watts (UW/Seattle/CPPM) 16 Displaced Vertex

ATLAS DV and 2 Lepton Search G. Watts (UW/Seattle/CPPM) 17 The vertex reconstruction efficiency Pixel Layers

ATLAS DV and 2 Lepton Search G. Watts (UW/Seattle/CPPM) 18 Complex background model (Control Regions simultaniously fit)

ATLAS DV and 2 Lepton Search G. Watts (UW/Seattle/CPPM) 19 Example limits

2 Jets from one Vertex Pro: Can do a mass cut G. Watts (UW/Seattle/CPPM) 20 Two jets coming from a single vertex Only requires a single LLP Mass cut possible in a way it isn’t in other search topologies

CMS 2-Jet Vertex Search G. Watts (UW/Seattle/CPPM) 21 All the models in the paper expect two of these displaced vertices “Nothing but b-tag”

CMS 2-Jet Vertex Search G. Watts (UW/Seattle/CPPM) 22

LHCb 2-Jet Vertex Search 7 TeV Result Mass Cut G. Watts (UW/Seattle/CPPM) 23

LHCb 2-Jet Vertex Search G. Watts (UW/Seattle/CPPM) 24

Lepton Jets G. Watts (UW/Seattle/CPPM) 25

CMS Displaced 2-Lepton Jets G. Watts (UW/Seattle/CPPM) 26 Both predict two displaced vertices Look for two leptons originating from a displaced vertex But only one required

CMS Displaced 2-Lepton Jets G. Watts (UW/Seattle/CPPM) 27

ATLAS Displaced Lepton Jets G. Watts (UW/CPPM) 28 (FRVZ, ) Dark photon decays to standard model leptons if it’s mass is MeV-GeV 4-8 leptons in these models An attempt to be as inclusive as possible:

ATLAS Displaced Lepton Jets G. Watts (UW/Seattle/CPPM) 29 Separate background issues for each LJ type!

ATLAS Displaced Lepton Jets G. Watts (UW/Seattle/CPPM) 30

Miscellaneous G. Watts (UW/Seattle/CPPM) 31

CMS LL Slow Particles Decaying to Photons G. Watts (UW/Seattle/CPPM) 32 Slow!

ATLAS Long Lived Charged Particle Search G. Watts (UW/Seattle/CPPM) 33 This is not an exotics Higgs search They are heavy and they are slow Cal Only

Ignored G. Watts (UW/Seattle/CPPM) 34

Conclusions WHY HAVE ONLY ONE SLIDE? G. Watts (UW/Seattle/CPPM) 35

Detectors Are Different G. Watts (UW/Seattle/CPPM) 36 CMS has amazing tracking ATLAS’ Muon Spectrometer can be used stand-alone

G. Watts (UW/Seattle/CPPM) 37 Side comment: Timing cuts exist: Explicit in the measurement, or The timing window for the experiment trigger Combinitorics: More than one LL particle in each event Start With: A limit at a single proper lifetime Range of actual lifetimes may be limited for distribution expected for long proper lifetimes! Toy-MC often used to extrapolate

Summary Plots G. Watts (UW/Seattle/CPPM) 38

The ATLAS combined plot G. Watts (UW/Seattle/CPPM) 39

The Reach of the experiments G. Watts (UW/Seattle/CPPM) 40 (old)

Run 2 G. Watts (UW/Seattle/CPPM) 41 Run 2 has enough luminosity we can really look at WH finally? Most LL analyses are not threshold analyses Detector Upgrades New sub-detectors have been added to both experiments New triggering capabilities

LHC Schedule G. Watts (UW/Seattle/CPPM) 42

13 TeV From Last Night!!! G. Watts (UW/Seattle/CPPM) 43 With new inner detector!!

Experiment’s Physics Schedule G. Watts (UW/Seattle/CPPM) 44 Conference LHC Results But, data will pour in until Winter Conference Cut off 50 ns to 25 ns transition

Conclusions  Thanks to everyone that has started to use these measurements  We are aware of the comments, and please keep them coming  We are designing the Run 2 versions of these analyses as we speak (well, already moving past that stage).  Detector design differences can make a real difference  The program is strong  Lots of current measurements. A huge amount of work by both theorists and experimentalists to get to this point!  We are still missing quite a bit… input on what is important to first fill out is always helpful (for Run 2 and beyond) G. Watts (UW/Seattle/CPPM) 45